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Pulsar Astronomy Pulsar Astronomy
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Published online by Cambridge University Press:  21 July 2022

Andrew Lyne ,
Francis Graham-Smith  and
Benjamin Stappers
Andrew Lyne
Affiliation:
University of Manchester
Francis Graham-Smith
Affiliation:
University of Manchester
Benjamin Stappers
Affiliation:
University of Manchester
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Pulsar Astronomy , pp. 364 - 402
Publisher: Cambridge University Press
Print publication year: 2022

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References

Abbott, B. P., Abbott, R., Abbott, T. D., and 1153 others. 2017. GW170817: Observation of gravitational waves from a binary neutron star inspiral. Phys. Rev. Lett., 119(16), 16.Google ScholarPubMed
Abbott, B. P., Abbott, R., Abbott, T. D., and 1149 others. 2018. GW170817: Measurements of neutron star radii and equation of state. Phys. Rev. Lett., 121(16), 16.CrossRefGoogle ScholarPubMed
Abdo, A. A., Allen, B., Berley, D., and 31 others. 2007. TeV gamma-ray sources from a survey of the Galactic plane with Milagro. ApJ, 664(Aug.), L91–L94.CrossRefGoogle Scholar
Abdo, A. A., Ackermann, M., Ajello, M., and 177 others. 2009a. Detection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT. Science, 325(Aug.), 840—844.CrossRefGoogle ScholarPubMed
Abdo, A. A., Ackermann, M., Ajello, M., and 199 others. 2009b. A population of gammaray millisecond pulsars seen with the Fermi Large Area Telescope. Science, 325, 848.CrossRefGoogle Scholar
Abdo, A. A., Ackermann, M., Ajello, M., and 232 others. 2010a. Fermi Large Area Telescope first source catalog. ApJS, 188, 405–436.CrossRefGoogle Scholar
Abdo, A. A., Ackermann, M., Ajello, M., and 189 others. 2010b. Fermi Large Area Telescope observations of the Crab Pulsar and Nebula. ApJ, 708, 1254–1267.CrossRefGoogle Scholar
Abdo, A. A., Ackermann, M., Ajello, M., and 214 others. 2010c. The first Fermi Large Area Telescope catalog of gamma-ray pulsars. ApJS, 187, 460–494.CrossRefGoogle Scholar
Abdo, A. A., Ajello, M., Allafort, A., and 208 others. 2013. The Second Fermi Large Area Telescope catalog of gamma-ray pulsars. ApJS, 208(2), 2.CrossRefGoogle Scholar
Acciari, V. A., Aliu, E., Arlen, T., and 79 others. 2010. Discovery of very high energy γ -ray emission from the SNR G54.1+0.3. ApJ, 719(1), L69–L73.CrossRefGoogle Scholar
Ackermann, M., Ajello, M., Allafort, A., and 166 others. 2013. Detection of the characteristic pion-decay signature in supernova remnants. Science, 339(6121), 807–811.CrossRefGoogle ScholarPubMed
Aharonian, F., Akhperjanian, A. G., Aye, K.-M., and 96 others. 2005. Discovery of extended VHE gamma-ray emission from the asymmetric pulsar wind nebula in MSH 15-52 with HESS. A&A, 435, L17–L20.Google Scholar
Aharonian, F., Akhperjanian, A. G., Bazer-Bachi, A. R., and 103 others. 2006. First detection of a VHE gamma-ray spectral maximum from a cosmic source: HESS discovery of the Vela X nebula. A&A, 448, L43.Google Scholar
Aharonian, F., Akhperjanian, A. G., Bazer-Bachi, A. R., and 125 others. 2007. Discovery of two candidate pulsar wind nebulae in very-high-energy gamma rays. A&A, 472(2), 489–495.Google Scholar
Akgün, T., Link, B., and Wasserman, I. 2006. Precession of the isolated neutron star PSR B1828-11. MNRAS, 365, 653–672.CrossRefGoogle Scholar
Alam, Md F., Arzoumanian, Z., Baker, P. T., and 67 others. 2020. The NANOGrav 12.5year data set: Wideband timing of 47 millisecond pulsars. arXiv e-prints, May, arXiv:2005.06495.Google Scholar
Allen, B., Knispel, B., Cordes, J. M., and 43 others. 2013. The Einstein@Home search for radio pulsars and PSR J2007+2722 discovery. ApJ, 773(Aug.), 91.CrossRefGoogle Scholar
Alpar, M. A., Anderson, P. W., Pines, D., and Shaham, J. 1981. Giant glitches and the pinned vorticity in the Vela and other pulsars. ApJ, 249, L29–L33.CrossRefGoogle Scholar
Alpar, M. A., Cheng, A. F., Ruderman, M. A., and Shaham, J. 1982. A new class of radio pulsars. Nature, 300, 728–730.CrossRefGoogle Scholar
Alpar, M. A., Cheng, K. S., and Pines, D. 1989. Vortex creep and the internal temperature of neutron stars: Linear and nonlinear response to a glitch. ApJ, 346, 823–832.CrossRefGoogle Scholar
Alpar, M. A., Chau, H. F., Cheng, K. S., and Pines, D. 1996. Postglitch relaxation of the Crab Pulsar after its first four glitches. ApJ, 459, 706–716.CrossRefGoogle Scholar
Andersen, B. C., and Ransom, S. M. 2018. A Fourier domain “Jerk” search for binary pulsars. ApJ, 863(1), L13–L18.CrossRefGoogle Scholar
Andersen, B. C., Bandura, K. M., Bhardwaj, M., and 68 others. 2020. A bright millisecondduration radio burst from a Galactic magnetar. Nature, 587(7832), 54–58.Google Scholar
Anderson, P. W., and Itoh, N. 1975. Pulsar glitches and restlessness as a hard superfluidity phenomenon. Nature, 256, 25–27.CrossRefGoogle Scholar
Anderson, S. B. 1993 (Jan.). A Study of Recycled Pulsars in Globular Clusters. Ph.D. thesis, California Institute of Technology, Pasadena.Google Scholar
Antoniadis, J., Freire, P. C. C., Wex, N., and 19 others. 2013. A massive pulsar in a compact relativistic binary. Science, 340(6131), 6131.CrossRefGoogle Scholar
Antonopoulou, D., Espinoza, C. M., Kuiper, L., and Andersson, N. 2018. Pulsar spin-down: The glitch-dominated rotation of PSR J0537-6910. MNRAS, 473(2), 1644–1655.CrossRefGoogle Scholar
Archibald, A. M., Stairs, I. H., Ransom, S. M., and 15 others. 2009. A radio pulsar/X-ray binary link. Science, 324(5933), 5933.CrossRefGoogle ScholarPubMed
Archibald, R. F., Kaspi, V. M., Tendulkar, S. P., and Scholz, P. 2016. A magnetar-like outburst from a high-B radio pulsar. ApJ, 829(1), L21.CrossRefGoogle Scholar
Arendt, P. N., and Eilek, J. A. 2002. Pair creation in the pulsar magnetosphere. ApJ, 581, 451–469.CrossRefGoogle Scholar
Armstrong, J. W., Rickett, B. J., and Spangler, S. R. 1995. Electron density power spectrum in the local interstellar medium. ApJ, 443, 209–221.CrossRefGoogle Scholar
Arons, J., and Barnard, J. J. 1986. Wave propagation in pulsar magnetospheres: Dispersion relations and normal modes of plasmas in superstrong magnetic fields. ApJ, 302, 120.CrossRefGoogle Scholar
Arzoumanian, Z., Nice, D. J., Taylor, J. H, and Thorsett, S. E. 1994. Timing behavior of 96 radio pulsars. ApJ, 422, 671–680.CrossRefGoogle Scholar
Arzoumanian, Z., Joshi, K., Rasio, F. A., and Thorsett, S. E. 1996. Orbital parameters of the PSR B1620-26 triple system. PASP Conf. Ser., 105, 525–530.Google Scholar
Ash, M. E., Shapiro, I. I., and Smith, W. B. 1967. Astronomical constants and planetary ephemerides deduced from radar and optical observations. AJ, 72, 338–350.CrossRefGoogle Scholar
Ashton, G., Lasky, P. D., Graber, V., and Palfreyman, J. 2019. Rotational evolution of the Vela pulsar during the 2016 glitch. Nature Astronomy, 3, 1143–1148.CrossRefGoogle Scholar
Ashworth, M. 1982. The Emission Mechanism of Radio Pulsars. Ph.D. thesis, The University of Manchester.Google Scholar
Asseo, E., Pellat, R., and Sol, H. 1983. Radiative or two-stream instability as a source for pulsar radio emission. ApJ, 266, 201–214.CrossRefGoogle Scholar
Atwood, W. B., Ziegler, M., Johnson, R. P., and Baughman, B. M. 2006. A time-differencing technique for detecting radio-quiet gamma-ray pulsars. ApJ, 652(1), L49–L52.CrossRefGoogle Scholar
Atwood, W. B., Abdo, A. A., Ackermann, , and 237 others. 2009. The Large Area Telescope on the Fermi Gamma-Ray Space Telescope mission. ApJ, 697(2), 1071–1102.CrossRefGoogle Scholar
Baade, W. 1942. The Crab Nebula. ApJ, 96, 188–198.CrossRefGoogle Scholar
Baade, W., and Zwicky, F. 1934. On super-novae. Proc. Nat. Acad. Sci., 20, 254–259.CrossRefGoogle ScholarPubMed
Bachetti, M., Harrison, F. A., Walton, D. J., and 21 others. 2014. An ultraluminous X-ray source powered by an accreting neutron star. Nature, 514(7521), 202–204.CrossRefGoogle ScholarPubMed
Backer, D. C. 1970. Pulsar nulling phenomena. Nature, 228, 42–43.CrossRefGoogle ScholarPubMed
Backer, D. C. 1976. Pulsar average wave forms and hollow-cone beam models. ApJ, 209, 895–907.CrossRefGoogle Scholar
Backer, D. C., and Hellings, R. W. 1986. Pulsar timing and general relativity. Ann. Rev. Astr. Ap., 24, 537–575.CrossRefGoogle Scholar
Backer, D. C., Rankin, J. M., and Campbell, D. B. 1976. Orthogonal mode emission in geometric models of pulsar polarisation. Nature, 263, 202–207.CrossRefGoogle Scholar
Backer, D. C., Kulkarni, S. R., Heiles, C., Davis, M. M., and Goss, W. M. 1982. A millisecond pulsar. Nature, 300, 615–618.CrossRefGoogle Scholar
Bailes, M., Manchester, R. N., Kesteven, M. J., Norris, R. P., and Reynolds, J. E. 1990. The proper motion of six southern radio pulsars. MNRAS, 247, 322–326.Google Scholar
Baldo, M., and Burgio, G. F. 2012. Properties of the nuclear medium. Reports on Progress in Physics, 75(2), 2.CrossRefGoogle ScholarPubMed
Bamba, A., Mori, K., and Shibata, S. 2010. Chandra view of pulsar wind nebula tori. ApJ, 709, 507–511.CrossRefGoogle Scholar
Barat, C., Chambon, G., Hurley, K., Niel, M., Vedrenne, G., Estulin, I. V., Kurt, V. G., and Zenchenko, V. M. 1979. Evidence for periodicity in a gamma ray burst. A&A, 79, L24–L25.Google Scholar
Barnard, J. J. 1986. Probing the magnetic field of radio pulsars: A reexamination of polarization position angle swings. ApJ, 303, 280–291.CrossRefGoogle Scholar
Barr, E. D., Champion, D. J., Kramer, M., and 13 others. 2013. The Northern High Time Resolution Universe pulsar survey – I. Setup and initial discoveries. MNRAS, 435(3), 2234–2245.CrossRefGoogle Scholar
Bartel, N., Sieber, W., and Wolszczan, A. 1980. Pulse to pulse intensity modulation from radio pulsars with particular reference to frequency dependence. A&A, 90, 58–60.Google Scholar
Bartel, N., Morris, D., Sieber, W., and Hankins, T. H. 1982. The mode-switching phenomenon in pulsars. ApJ, 258, 776–789.CrossRefGoogle Scholar
Bartel, N., Chandler, J. F., Ratner, M. I., Shapiro, I. I., Pan, R., and Capallo, R. J. 1996. Towards a frame-tie via millisecond pulsar VLBI. AJ, 112, 1690–1696.CrossRefGoogle Scholar
Bassa, C. G., Pleunis, Z., Hessels, J. W. T., Ferrara, E. C., Kondratiev, V. I., Sanidas, S., Lyne, A. G., Stappers, B. W., Ransom, S. M., and Fermi Pulsar Search Consortium. 2018 (Aug.). Targeted millisecond pulsar surveys of Fermi γ -ray sources with LOFAR. Pages 33–36 of: Weltevrede, P., Perera, B. B. P., Preston, L. L., and Sanidas, S. (eds), Pulsar Astrophysics the Next Fifty Years, vol. 337.Google Scholar
Bastian, T. S. 1994. Angular scattering of solar radio emission by coronal turbulence. ApJ, 426(May), 774.CrossRefGoogle Scholar
Basu, R., and Mitra, D. 2019. Radio emission features in different modes of PSR J0826+2637 (B0823+26). MNRAS, 487(4), 4536–4549.CrossRefGoogle Scholar
Basu, R., Mitra, D., Melikidze, G. I., Maciesiak, K., Skrzypczak, A., and Szary, A. 2016. Meterwavelength Single-pulse Polarimetric Emission Survey. II. The phenomenon of drifting subpulses. ApJ, 833(1), 1.Google Scholar
Baym, G., Pethick, C. J., and Sutherland, P. 1971. The ground state of matter at high densities: Equation of state and stellar models. ApJ, 170, 299–317.CrossRefGoogle Scholar
Baym, G., Hatsuda, T., Kojo, T., Powell, P. D., Song, Y., and Takatsuka, T. 2018. From hadrons to quarks in neutron stars: A review. Reports on Progress in Physics, 81(5), 5.CrossRefGoogle ScholarPubMed
Baym, G., Furusawa, S., Hatsuda, T., Kojo, T., and Togashi, H. 2019. New neutron star equation of state with quark-hadron crossover. ApJ, 885(1), 1.Google Scholar
Beck, R. 2009 (Apr.). Measuring interstellar magnetic fields by radio synchrotron emission. Pages 3–14 of: Strassmeier, K. G., Kosovichev, A. G., and Beckman, J. E. (eds), Cosmic Magnetic Fields: From Planets, to Stars and Galaxies. IAU Symposium, vol. 259.Google Scholar
Beck, R. 2015. Magnetic fields in spiral galaxies. Astron. Astrophys. Rev., 24(Dec.), 4.CrossRefGoogle Scholar
Becker, W., and Trümper, J. 1997. The X-ray luminosity of rotation-powered neutron stars. A&A, 326, 682–691.Google Scholar
Belian, R. D., Conner, J. P., and Evans, W. D. 1976. The discovery of X-ray bursts from a region in the constellation Norma. ApJ, 206, L135–L138.CrossRefGoogle Scholar
Bell, J. F. 1998. Radio pulsar timing. Adv. Space Res., 21, 137–147.CrossRefGoogle Scholar
Bell, J. F., and Bailes, M. 1996. A new method for obtaining binary pulsar distances and its implications for tests of general relativity. ApJ, 456, L33–L36.Google Scholar
Bell, J. F., Bailes, M., Manchester, R. N., Weisberg, J. M., and Lyne, A. G. 1995. The proper motion and wind nebula of the nearby millisecond pulsar J0437-4715. ApJ, 440, L81–L83.CrossRefGoogle Scholar
Bergeron, P., Dufour, P., Fontaine, G., Coutu, S., Blouin, S., Genest-Beaulieu, C., Bédard, A., and Rolland, B. 2019. On the measurement of fundamental parameters of white dwarfs in the Gaia era. ApJ, 876(1), 1.Google Scholar
Bertotti, B., Carr, B. J., and Rees, M. J. 1983. Limits from the timing of pulsars on the cosmic gravitational wave background. MNRAS, 203, 945–954.CrossRefGoogle Scholar
Bertotti, B., Iess, L., and Tortora, P. 2003. A test of general relativity using radio links with the Cassini spacecraft. Nature, 425, 374–376.CrossRefGoogle ScholarPubMed
Beskin, V. S. 1999. Radio pulsars. Physics Uskpekhi, 42, 1071.CrossRefGoogle Scholar
Beskin, V. S., Gurevich, A. V., and Istomin, Ya. N. 1993. Physics of the Pulsar Magnetosphere. Cambridge University Press.Google Scholar
Beuermann, K., Kanbach, G., and Berkhuijsen, E. M. 1985. Radio structure of the Galaxy – Thick disk and thin disk at 408 MHz. A&A, 153, 17–34.Google Scholar
Bhandari, S., Sadler, E. M., Prochaska, J. X., and 16 others. 2020. The host galaxies and progenitors of fast radio bursts localized with the Australian Square Kilometre Array Pathfinder. ApJ, 895(2), L37.CrossRefGoogle Scholar
Bhat, N. D. R., Cordes, J. M., Camilo, F., Nice, D. J., and Lorimer, D. R. 2004. Multifrequency observations of radio pulse broadening and constraints on interstellar electron density microstructure. ApJ, 605(2), 759–783.CrossRefGoogle Scholar
Bhat, N. D. R., Gupta, Y., Kramer, M., Karastergiou, A., Lyne, A. G., and Johnston, S. 2007. Simultaneous single-pulse observations of radio pulsars. V. On the broadband nature of the pulse nulling phenomenon in PSR B1133+16. A&A, 462(1), 257–268.Google Scholar
Bhattacharya, D., Wijers, R. A. M. J., Hartman, J. W., and Verbunt, F. 1992. On the decay of magnetic fields of single radio pulsars. A&A, 254, 198–212.Google Scholar
Bhattacharya, B., Gupta, Y., and Gil, J. 2009 (Sept.). Wide profile drifting pulsars: An elegant way to probe pulsar magnetospheres. Page 313 of: Saikia, D. J., Green, D. A., Gupta, Y., and Venturi, T. (eds), The Low-Frequency Radio Universe. Astronomical Society of the Pacific Conference Series, vol. 407.Google Scholar
Bietenholz, M. F., Kassim, N., and Weiler, K. 2002. The radio spectral index of 3C58. Proc. IAU Symp. 199, 303.Google Scholar
Biggs, J. D. 1990. Meridional compression of radio pulsar beams. MNRAS, 245, 514–521.Google Scholar
Biggs, J. D., Hamilton, P. A., McCulloch, P. M., and Manchester, R. N. 1985a. The drifting subpulses of PSR 0148-06. MNRAS, 214, 47P–52P.CrossRefGoogle Scholar
Biggs, J. D., McCulloch, P. M., Hamilton, P. A., Manchester, R. N., and Lyne, A. G. 1985b. A study of PSR0826-34 – A remarkable pulsar. MNRAS, 215, 281–294.CrossRefGoogle Scholar
Bignall, H. E., Jauncey, D. L., Lovell, J., Macquart, J.-P., Kedziora-Chudczer, L., and Tzioumis, A. K. 2003 (Jan.). The rapidly scintillating quasar, PKS 1257-326. Page E12 of: IAU Joint Discussion. IAU Joint Discussion.Google Scholar
Bignami, G. F., Caraveo, P. A., De Luca, A., and Mereghetti, S. 2003. Discovery of X-ray cyclotron absorption lines measures the magnetic field of an isolated neutron star. Nature, 423, 725–727.CrossRefGoogle Scholar
Bilous, A. V., Pennucci, T. T., Demorest, P., and Ransom, S. M. 2015. A broadband radio study of the average profile and giant pulses from PSR B1821-24A. ApJ, 803(2), 2.Google Scholar
Bilous, A. V., Watts, A. L., Harding, A. K., Riley, T. E., Arzoumanian, Z., Bogdanov, S., Gendreau, K. C., Ray, P. S., Guillot, S., Ho, W. C. G., and Chakrabarty, D. 2019. A NICER view of PSR J0030+0451: Evidence for a global-scale multipolar magnetic field. ApJ, 887(1), L23.CrossRefGoogle Scholar
Bjoernsson, C.-I. 1998. A direct method to determine the geometry of the hollow cones in pulsars. A&A, 338, 971–976.Google Scholar
Blaauw, A. 1985. The progenitors of the local pulsar population. Pages 211–224 of: Boland, W., and van Woerden, H. (eds), Birth and Evolution of Massive Stars and Stellar Groups. Dordrecht: Reidel.CrossRefGoogle Scholar
Blandford, R., and Teukolsky, S. A. 1976. Arrival-time analysis for a pulsar in a binary system. ApJ, 205, 580–591.CrossRefGoogle Scholar
Blaskiewicz, M., Cordes, J. M., and Wasserman, I. 1991. A relativistic model of pulsar polarization. ApJ, 370, 643–669.CrossRefGoogle Scholar
Bochenek, C. D., Ravi, V., Belov, K. V., Hallinan, G., Kocz, J., Kulkarni, S. R., and McKenna, D. L. 2020. A fast radio burst associated with a galactic magnetar. Nature, 587(7832), 59–62.CrossRefGoogle ScholarPubMed
Bogdanov, S., Rybicki, G. B., and Grindlay, J. E. 2007. Constraints on neutron star properties from X-ray observations of millisecond pulsars. ApJ, 670(1), 668–676.CrossRefGoogle Scholar
Boldt, E. A., Desai, U. D., Holt, S. S., Serlemitsos, P. J., and Silverberg, R. F. 1969. Pulsed X-ray emission of NP 0532 in March 1968. Nature, 223, 280–281.CrossRefGoogle Scholar
Bolton, J. G., Stanley, G. J., and Slee, O. B. 1949. Positions of three discrete sources of galactic radio-frequency radiation. Nature, 164, 101–102.CrossRefGoogle Scholar
Boriakoff, V., Ferguson, D. C., and Slater, G. 1981. Pulsar microstructure quasi-periodicity. Pages 199–204 of: Sieber, W., and Wielebinski, R. (eds), Pulsars, IAU Symposium 95. Dordrecht: Reidel.CrossRefGoogle Scholar
Boriakoff, V., Buccheri, R., and Fauci, F. 1983. Discovery of a 6.1-ms binary pulsar, PSR1953+29. Nature, 304, 417–419.CrossRefGoogle Scholar
Bradt, H., Rappaport, S., Mayer, W., Nather, R. E., Warner, B., Macfarlane, M., and Kristian, J. 1969. X-ray and optical observations of the pulsar NP 0532 in the Crab Nebula. Nature, 222, 728–730.CrossRefGoogle Scholar
Bradt, H. V. D., and McClintock, J. E. 1983. The optical counterparts of compact galactic X-ray sources. Ann. Rev. Astr. Ap., 21, 13–66.CrossRefGoogle Scholar
Brambilla, G., Kalapotharakos, C., Timokhin, A., Harding, A., and Kazanas, D. 2018. Electron-positron pair flow and current composition in the pulsar magnetosphere. ApJ, 858(2), 2.Google Scholar
Breton, R. P., Kaspi, V. M., Kramer, M., McLaughlin, M. A., Lyutikov, M., Ransom, S. M., Stairs, I. H., Ferdman, R. D., Camilo, F., and Possenti, A. 2008. Relativistic spin precession in the Double Pulsar. Science, 321, 104.CrossRefGoogle ScholarPubMed
Brisken, W. F., Benson, J. M., Goss, W. M., and Thorsett, S. E. 2002. Very Long Baseline Array measurement of nine pulsar parallaxes. ApJ, 571, 906–917.CrossRefGoogle Scholar
Brisken, W. F., Macquart, J.-P., Gao, J. J., Rickett, B. J., Coles, W. A., Deller, A. T., Tingay, S. J., and West, C. J. 2010. 100 as resolution VLBI imaging of anisotropic interstellar scattering toward pulsar B0834+06. ApJ, 708, 232–243.CrossRefGoogle Scholar
Bühler, R., and Blandford, R. 2014. The surprising Crab pulsar and its nebula: A review. Rep. Prog. Phys., 77(6), 6.CrossRefGoogle ScholarPubMed
Burgay, M., D’Amico, N., Possenti, A., and 10 others. 2003. An increased estimate of the merger rate of double neutron stars from observations of a highly relativistic system. Nature, 426, 531–533.CrossRefGoogle ScholarPubMed
Burgay, M., Joshi, B. C., D’Amico, N., Possenti, A., Lyne, A. G., Manchester, R. N., McLaughlin, M. A., Kramer, M., Camilo, F., and Freire, P. C. C. 2006. The Parkes High-Latitude pulsar survey. MNRAS, 368(May), 283–292.CrossRefGoogle Scholar
Burgay, M., Keith, M. J., Lorimer, D. R., and 11 others. 2013. The Perseus Arm pulsar survey. MNRAS, 429(1), 579–588.CrossRefGoogle Scholar
Burgay, M., Stappers, B., Bailes, M., and 21 others. 2019. The High Time Resolution Universe pulsar survey – XV. Completion of the intermediate-latitude survey with the discovery and timing of25 further pulsars. MNRAS, 484(4), 5791–5801.CrossRefGoogle Scholar
Cadelano, M., Ransom, S. M., Freire, P. C. C., Ferraro, F. R., Hessels, J. W. T., Lanzoni, B., Pallanca, C., and Stairs, I. H. 2018. Discovery of three new millisecond pulsars in Terzan 5. ApJ, 855(2), 2.Google Scholar
Cairns, I. H., Johnston, S., and Das, P. 2004. Intrinsic variability and field statistics for pulsars B1641-45 and B0950+08. MNRAS, 353(1), 270–286.CrossRefGoogle Scholar
Cameron, A. D., Champion, D. J., Kramer, M., and 27 others. 2018. The High Time Resolution Universe pulsar survey – XIII. PSR J1757-1854, the most accelerated binary pulsar. MNRAS, 475(1), L57–L61.CrossRefGoogle Scholar
Camilo, F., Thorsett, S. E., and Kulkarni, S. R. 1994. The magnetic fields, ages and original spin periods of millisecond pulsars. ApJ, 421, L15–L18.CrossRefGoogle Scholar
Camilo, F., Nice, D. J., and Taylor, J. H. 1996a. A search for millisecond pulsars at galactic latitudes −50° <b < −20°. ApJ, 461, 812–819.CrossRefGoogle Scholar
Camilo, F., Nice, D. J., Shrauner, J. A., and Taylor, J. H. 1996b. Princeton-Arecibo all-sky survey for millisecond pulsars. I. ApJ, 469, 819–827.CrossRefGoogle Scholar
Camilo, F., Lorimer, D. R., Freire, P., Lyne, A. G., and Manchester, R. N. 2000. Observations of 20 millisecond pulsars in 47 Tucanae at 20 cm. ApJ, 535, 975–990.CrossRefGoogle Scholar
Camilo, F., Lorimer, D. R., Bhat, N. D. R., Gotthelf, E. V., Halpern, J. P., Wang, Q. D., Lu, F. J., and Mirabal, N. 2002a. Discovery of a 136 millisecond radio and X-ray pulsar in supernova remnant G54.1+0.3. ApJ, 574, L71–L74.CrossRefGoogle Scholar
Camilo, F., Manchester, R. N., Gaensler, B. M., Lorimer, D. L., and Sarkissian, J. 2002b. PSR J1124-5916: A young and energetic pulsar in supernova remnant G292.0+1.8. ApJ, 567, L71–L75.CrossRefGoogle Scholar
Camilo, F., Stairs, I. H., Lorimer, D. R., Backer, D. C., Ransom, S. M., Klein, B., Wielebinski, R., Kramer, M., McLaughlin, M. A., Arzoumanian, Z., and Müller, P. 2002c. Discovery of radio pulsations from the X-ray pulsar J0205+6449 in supernova remnant 3C 58 with the Green Bank Telescope. ApJ, 571, L41–L44.CrossRefGoogle Scholar
Camilo, F., Ransom, S. M., Gaensler, B. M., Slane, P. O., Lorimer, D. R., Reynolds, J., Manchester, R. N., and Murray, S. S. 2006a. PSR J1833-1034: Discovery of the central young pulsar in the supernova remnant G21.5-0.9. ApJ, 637, 456–465.CrossRefGoogle Scholar
Camilo, F., Ransom, S. M., Halpern, J. P., Reynolds, J., Helfand, D. J., Zimmerman, N., and Sarkissian, J. 2006b. Transient pulsed radio emission from a magnetar. Nature, 442, 892–895.CrossRefGoogle ScholarPubMed
Camilo, F., Reynolds, J., Johnston, S., Halpern, J. P., and Ransom, S. M. 2008. The magnetar 1E 1547.0-5408: Radio spectrum, polarimetry, and timing. ApJ, 679(May), 681–686.CrossRefGoogle Scholar
Camilo, F., Ransom, S. M., Gaensler, B. M., and Lorimer, D. R. 2009a. Discovery of the energetic pulsar J1747-2809 in the supernova remnant G0.9+0.1. ApJ, 700, L34–L38.CrossRefGoogle Scholar
Camilo, F., Ray, P. S., Ransom, S. M., and 24 others. 2009b. Radio detection of LAT PSRs J1741-2054 and J2032+4127: No longer just gamma-ray pulsars. ApJ, 705(Nov.), 1–13.CrossRefGoogle Scholar
Camilo, F., Ransom, S. M., Chatterjee, S., Johnston, S., and Demorest, P. 2012. PSR J1841- 0500: A radio pulsar that mostly is not there. ApJ, 746(Feb.), 63.CrossRefGoogle Scholar
Campana, R., Massaro, E., Mineo, T., and Cusumano, G. 2009. The multi-component model of the Crab Pulsar at energies above 25 GeV. A&A, 499, 847–850.Google Scholar
Caswell, J. L., Murray, J. D., Roger, R. S., Cole, D. J., and Cooke, D. J. 1975. Neutral hydrogen absorption measurements yielding kinematic distances for 42 continuum sources in the Galactic plane. A&A, 45, 239–258.Google Scholar
Cerutti, B., and Beloborodov, A. M. 2017. Electrodynamics of pulsar magnetospheres. Space Sci. Rev., 207(1-4), 111–136.CrossRefGoogle Scholar
Chakrabarty, D., and Morgan, E. H. 1998. The two-hour orbit of a binary millisecond X-ray pulsar. Nature, 394, 346–348.CrossRefGoogle Scholar
Chakrabarty, D., Morgan, E. H., Muno, M. P., Galloway, D. K., Wijnands, R., van der Klis, M., and Markwardt, C. B. 2003. Nuclear-powered millisecond pulsars and the maximum spin frequency of neutron stars. Nature, 424, 42–44.CrossRefGoogle ScholarPubMed
Chakraborty, A., and Bagchi, M. 2020. Understanding the Galactic population of normal pulsars: A leap forward. arXiv e-prints, Dec., arXiv:2012.13243.Google Scholar
Champion, D. J., Lorimer, D. R., McLaughlin, M. A., Cordes, J. M., Arzoumanian, Z., Weisberg, J. M., and Taylor, J. H. 2004. PSR J1829+2456: A relativistic binary pulsar. MNRAS, 350, L61–L65.CrossRefGoogle Scholar
Chandrasekhar, S. 1931. The maximum mass of ideal white dwarfs. ApJ, 74, 81–82.CrossRefGoogle Scholar
Chatterjee, S., and Cordes, J. M. 2002. Bow shocks from neutron stars: Scaling laws and HST observations of the Guitar Nebula. ApJ, 575, 407–418.CrossRefGoogle Scholar
Chatterjee, S., Brisken, W. F., Vlemmings, W. H. T., Goss, W. M., Lazio, T. J. W., Cordes, J. M., Thorsett, S. E., Fomalont, E. B., Lyne, A. G., and Kramer, M. 2009. Precision astrometry with the Very Long Baseline Array: Parallaxes and proper motions for 14 pulsars. ApJ, 698, 250–265.CrossRefGoogle Scholar
Chau, H. F., Cheng, K. S., and Ding, K. Y. 1992. Implications of 3P2 superfluidity in the interior of neutron stars. ApJ, 399, 213.CrossRefGoogle Scholar
Chen, J. L., and Wang, H. G. 2014. Frequency dependence of pulse width for 150 radio normal pulsars. ApJS, 215(1), 1.CrossRefGoogle Scholar
Cheng, A. F., and Ruderman, M. 1979. A theory of subpulse polarization patterns from radio pulsars. ApJ, 229, 348–360.CrossRefGoogle Scholar
Chevalier, R. A. 1977. Was SN 1054 a type II supernova? Pages 53–61 of: Schramm, D. N. (ed), Supernovae. Dordrecht: Reidel.CrossRefGoogle Scholar
Chevalier, R. A. 1992. Early expansion and luminosity evolution of supernovae. ApJ, 394, 599–602.CrossRefGoogle Scholar
Chiang, J., and Romani, R. W. 1994. An outer gap model of high-energy emission from rotation-powered pulsars. ApJ, 436, 754–761.CrossRefGoogle Scholar
Chiu, H. Y., and Salpeter, E. E. 1964. Surface X-ray emission from neutron stars. Phys. Rev. Lett., 12, 413.CrossRefGoogle Scholar
Chung, C. T. Y., and Melatos, A. 2011. Stokes tomography of radio pulsar magnetospheres – I. Linear polarization. MNRAS, 411, 2471–2529.CrossRefGoogle Scholar
Cieslar, M., Bulik, T., and Oslowski, S. 2018. Markov chain Monte Carlo population synthesis of single radio pulsars in the Galaxy. arXiv e-prints, Mar., arXiv:1803.02397.Google Scholar
Clark, C. J., Wu, J., Pletsch, H. J., and Guillemot, L. 2018. The Einstein@Home Survey for Gamma-ray Pulsars. Pages 21–24 of: Weltevrede, P., Perera, B. B. P., Preston, L. L., and Sanidas, S. (eds), Pulsar Astrophysics the Next Fifty Years, vol. 337.Google Scholar
Clark, D. H., and Caswell, J. L. 1976. A study of Galactic supernova remnants, based on Molonglo-Parkes observational data. MNRAS, 174, 267–305.CrossRefGoogle Scholar
Clark, D. H., and Stephenson, F. R. 1977. Do all Galactic supernovae produce long-lived remnants? MNRAS, 179, 87P–92P.CrossRefGoogle Scholar
Clemence, G. M., and Szebehely, V. 1967. Annual variation of an atomic clock. AJ, 72, 1324–1326.CrossRefGoogle Scholar
Clifton, T. R., and Lyne, A. G. 1986. High-radio-frequency survey for young and millisecond pulsars. Nature, 320, 43–45.CrossRefGoogle Scholar
Clifton, T. R., Lyne, A. G., Jones, A. W., McKenna, J., and Ashworth, M. 1992. A high frequency survey of the Galactic plane for young and distant pulsars. MNRAS, 254, 177–184.CrossRefGoogle Scholar
Cocke, W. J., Disney, M. J., and Taylor, D. J. 1969. Discovery of optical signals from pulsar NP 0532. Nature, 221, 525–527.CrossRefGoogle Scholar
Cognard, I., Bourgois, G., Lestrade, J.-F., Biraud, F., Aubry, D., Darchy, B., and Drouhin, J.-P. 1996. High-precision timing observations of the millisecond pulsar PSR 1821-24 at Nancay. A&A, 311, 179–188.Google Scholar
Cognard, I., Freire, P. C. C., Guillemot, L., and 10 others. 2017. A massive-born neutron star with a massive white dwarf companion. ApJ, 844(2), 2.Google Scholar
Cohen, M. H., Gunderman, E. J., Handebeck, H. E., and Sharp, L. E. 1967. Interplanetary scintillations. II. Observations. ApJ, 147, 449–466.CrossRefGoogle Scholar
Cole, T. W. 1970. Pulsar subpulses and the emission process. Nature, 227, 788–791.CrossRefGoogle Scholar
Coles, W. A., Rickett, B. J., Gao, J. J., Hobbs, G., and Verbiest, J. P. W. 2010. Scattering of pulsar radio emission by the interstellar plasma. ApJ, 717, 1206–1221.CrossRefGoogle Scholar
Comella, J. M., Craft, H. D., Lovelace, R. V. E., Sutton, J. M., and Tyler, G. L. 1969. Crab Nebula pulsar NP 0532. Nature, 221, 453–454.CrossRefGoogle Scholar
Cordes, J. M. 1986. Space velocities of radio pulsars from interstellar scintillations. ApJ, 311, 183–196.CrossRefGoogle Scholar
Cordes, J. M. 2002. Pulsar Observations I. – Propagation Effects, Searching Distance Estimates, Scintillations and VLBI. Astronomical Society of the Pacific Conference Series, vol. 278. Pages 227–250.Google Scholar
Cordes, J. M., and Chatterjee, S. 2019. Fast radio bursts: An extragalactic enigma. Ann. Rev. Astr. Ap., 57(Aug.), 417–465.CrossRefGoogle Scholar
Cordes, J. M., and Chernoff, D. F. 1997. Neutron star population dynamics. I. Millisecond pulsars. ApJ, 482, 971–992.CrossRefGoogle Scholar
Cordes, J. M., and Lazio, T.J. W. 2002. NE2001. I. A new model for the Galactic distribution of free electrons and its fluctuations. preprint (arXiv:astro-ph/0207156).Google Scholar
Cordes, J. M. 2004. NE2001: A new model for the Galactic electron density and its fluctuations. ASP Conf. Ser., 317, 211.Google Scholar
Cordes, J. M., and Lazio, T. J. W. 2003. NE2001. II. Using radio propagation data to construct a model for the Galactic distribution of free electrons. preprint (arXiv:astro- ph/0301598).Google Scholar
Cordes, J. M., and McLaughlin, M. A. 2003. Searches for fast radio transients. ApJ, 596, 1142–1154.CrossRefGoogle Scholar
Cordes, J. M., Romani, R. W., and Lundgren, S. C. 1993. The Guitar Nebula: A bow-shock from a slow-spin, high-velocity neutron star. Nature, 362, 133–135.CrossRefGoogle Scholar
Cordes, J. M., Freire, P. C. C., Lorimer, D. R., and 21 others. 2006a. Arecibo pulsar survey using ALFA. I. Survey strategy and first discoveries. ApJ, 637, 446–455.CrossRefGoogle Scholar
Cordes, J. M., Rickett, B. J., Stinebring, D. R., and Coles, W. A. 2006b. Theory of parabolic arcs in interstellar scintillation spectra. ApJ, 637, 346–365.CrossRefGoogle Scholar
Cordes, J. M., Shannon, R. M., and Stinebring, D. R. 2016. Frequency-dependent dispersion measures and implications for pulsar timing. ApJ, 817(1), 1.Google Scholar
Crossley, J. H., Eilek, J. A., Hankins, T. H., and Kern, J. S. 2010. Short-lived radio bursts from the Crab Pulsar. ApJ, 722, 1908–1920.CrossRefGoogle Scholar
Crusius-Waetzel, A. R., and Lesch, H. 2002 (Jan.). Emission mechanisms in high energy pulsars: From gamma rays to infrared. Page 162 of: Becker, W., Lesch, H., and Trümper, J. (eds), Neutron Stars, Pulsars, and Supernova Remnants.Google Scholar
Dai, S., Hobbs, G., Manchester, R. N., and 23 others. 2015. A study of multifrequency polarization pulse profiles of millisecond pulsars. MNRAS, 449(3), 3223–3262.CrossRefGoogle Scholar
Damashek, M., Taylor, J. H., and Hulse, R. A. 1978. Parameters of 17 newly discovered pulsars in the northern sky. ApJ, 225, L31.CrossRefGoogle Scholar
Damashek, M., Backus, P. R., Taylor, J. H., and Burkhardt, R. K. 1982. Northern hemisphere pulsar survey: A third radio pulsar in a binary system. ApJ, 253, L57–L60.CrossRefGoogle Scholar
D’Amico, N., Lyne, A. G., Manchester, R. N., Possenti, A., and Camilo, F. 2001. Discovery of short-period binary millisecond pulsars in four globular clusters. ApJ, 548, L171–L174.CrossRefGoogle Scholar
Damour, T., and Esposito-Farèse, G. 1998. Gravitational-wave versus binary-pulsar tests of strong-field gravity. Phys. Rev. D, 58, 1–12.CrossRefGoogle Scholar
Damour, T., and Esposito-Farèse, G. 1992. Testing local Lorentz invariance of gravity with binary pulsar data. Phys. Rev. D, 46, 4128–4132.CrossRefGoogle ScholarPubMed
Damour, T., and Taylor, J. H. 1991. On the orbital period change of the binary pulsar PSR1913+16. ApJ, 366, 501–511.CrossRefGoogle Scholar
Damour, T., and Taylor, J. H. 1992. Strong-field tests of relativistic gravity and binary pulsars. Phys. Rev. D, 45, 1840–1868.CrossRefGoogle ScholarPubMed
Davies, J. G., Horton, P. W., Lyne, A. G., Rickett, B. J., and Smith, F. G. 1968. Pulsating radio source at α = 19h19m, δ = +22°. Nature, 217, 910–913.CrossRefGoogle Scholar
Davies, J. G., Lyne, A. G., and Seiradakis, J. H. 1973. Thirteen new pulsars. Nature Phys. Sci., 244, 84–85.CrossRefGoogle Scholar
De, K., Gupta, Y., and Sharma, P. 2016. Detection of polarized quasi-periodic microstructure emission in millisecond pulsars. ApJ, 833(1), L10.CrossRefGoogle Scholar
de Jager, G., Lyne, A. G., Pointon, L., and Ponsonby, J. E. B. 1968. Measurement of the distance of pulsar CP 0328. Nature, 220, 128–129.CrossRefGoogle Scholar
de Plaa, J., Kuiper, L., and Hermsen, W. 2003. Hard X-ray timing and spectral properties of PSR B0540-69. A&A, 400(Mar.), 1013–1019.Google Scholar
de Vaucouleurs, G., and Corwin, H. G. 1985. S. Andromedae 1885: A centennial review. ApJ, 295, 287–304.CrossRefGoogle Scholar
Degenaar, N., and Suleimanov, V. F. 2018 (Jan.). Testing the equation of state with electromagnetic observations. Page 185 of: Rezzolla, L., Pizzochero, P., Jones, D. I., Rea, N., and Vidana, I. (eds), Astrophysics and Space Science Library. Astrophysics and Space Science Library, vol. 457.Google Scholar
Deller, A. T., Tingay, S. J., Bailes, M., and Reynolds, J. E. 2009. Precision southern hemisphere VLBI pulsar astrometry. II. Measurement of seven parallaxes. ApJ, 701, 1243–1257.CrossRefGoogle Scholar
Deller, A. T., Weisberg, J. M., Nice, D. J., and Chatterjee, S. 2018. A VLBI distance and transverse velocity for PSR B1913+16. ApJ, 862(2), 2.Google Scholar
Deller, A. T., Goss, W. M., Brisken, W. F., and 8 others. 2019. Microarcsecond VLBI pulsar astrometry with PSRπ II. Parallax distances for 57 pulsars. ApJ, 875(2), 2.Google Scholar
Demorest, P. B., Pennucci, T., Ransom, S. M., Roberts, M. S. E., and Hessels, J. W. T. 2010. A two-solar-mass neutron star measured using Shapiro delay. Nature, 467(7319), 1081–1083.CrossRefGoogle ScholarPubMed
Deneva, J. S., Cordes, J. M., and Lazio, T. J. W. 2009. Discovery of three pulsars from a Galactic Center pulsar population. ApJ, 702, L177–L181.CrossRefGoogle Scholar
Deneva, J. S., Stovall, K., McLaughlin, M. A., Bates, S. D., Freire, P. C. C., Martinez, J. G., Jenet, F., and Bagchi, M. 2013. Goals, strategies and first discoveries of AO327, the Arecibo all-sky 327 MHz drift pulsar survey. ApJ, 775(1), 1.Google Scholar
Deshpande, A. A., and Rankin, J. M. 1999. Pulsar magnetospheric emission mapping: Images and implications of polar CAP weather. ApJ, 524, 1008–1013.CrossRefGoogle Scholar
Desvignes, G., Kramer, M., Lee, K., van Leeuwen, J., Stairs, I., Jessner, A., Cognard, I., Kasian, L., Lyne, A., and Stappers, B. W. 2019. Radio emission from a pulsar’s magnetic pole revealed by general relativity. Science, 365(6457), 1013–1017.CrossRefGoogle ScholarPubMed
Detweiler, S. 1979. Pulsar timing measurements and the search for gravitational waves. ApJ, 234, 1100.CrossRefGoogle Scholar
Dewey, R. J., Taylor, J. H., Weisberg, J. M., and Stokes, G. H. 1985. A search for low- luminosity pulsars. ApJ, 294, L25–L29.CrossRefGoogle Scholar
Dib, R., Kaspi, V. M., and Gavriil, F. P. 2009. Rossi X-ray timing explorer monitoring of the anomalous X-ray pulsar 1E 1048.1 – 5937: Long-term variability and the 2007 march event. ApJ, 702(1), 614–630.CrossRefGoogle Scholar
Diehl, R., Halloin, H., Kretschmer, K., and 12 others. 2006. 26Al in the inner Galaxy. Large- scale spectral characteristics derived with SPI/INTEGRAL. A&A, 449, 1025–1031.Google Scholar
Dodson, R. G., McCulloch, P. M., and Lewis, D. R. 2002. High time resolution observations of the January 2000 glitch in the Vela Pulsar. ApJ, 564, L85–L88.CrossRefGoogle Scholar
Dombrovsky, V. A. 1954. On the nature of the radiation from the Crab Nebula. Dokl. Akad. Nauk. USSR, 94, 1021.Google Scholar
Driessen, L. N., Janssen, G. H., Bassa, C. G., Stappers, B. W., and Stinebring, D. R. 2019. Scattering features and variability of the Crab Pulsar. MNRAS, 483(1), 1224–1232.CrossRefGoogle Scholar
Dubner, G., and Giacani, E. 2015. Radio emission from supernova remnants. Astron. Astrophys. Rev., 23(Sept.), 3.CrossRefGoogle Scholar
Duffet-Smith, P. J., and Readhead, A. C. S. 1976. The angular broadening of radio sources by scattering in the interstellar medium. MNRAS, 174, 7–17.CrossRefGoogle Scholar
Duncan, J. C. 1939. Second report on the expansion of the Crab Nebula. ApJ, 89, 482.CrossRefGoogle Scholar
Duncan, R. C., and Thompson, C. 1992. Formation of very strongly magnetized neutron stars: Implications for gamma-ray bursts. ApJ, 392, L9–L13.CrossRefGoogle Scholar
Durdin, J. M., Large, M. I., Little, A. G., Manchester, R. N., Lyne, A. G., and Taylor, J. H. 1979. An unusual pulsar – PSR0826-34. MNRAS, 186, 39P-41P.Google Scholar
Duyvendak, J. J. L. 1942. Further data bearing on the identification of the Crab Nebula with the supernova of A.D. 1054, Part I: The ancient Oriental chronicles. PASP, 54, 91–94.CrossRefGoogle Scholar
Dyks, J., and Harding, A. K. 2004. Rotational sweepback of magnetic field lines in geometric models of pulsar radio emission. ApJ, 614(Oct.), 869–880.CrossRefGoogle Scholar
Dyks, J., and Rudak, B. 2003. Two-pole caustic model for high-energy light curves of pulsars. ApJ, 598, 1201–1206.CrossRefGoogle Scholar
Dyks, J., Rudak, B., and Harding, A. K. 2004. On the methods of determining the radio emission geometry in pulsar magnetospheres. ApJ, 607, 939–948.CrossRefGoogle Scholar
Eatough, R. P., Keane, E. F., and Lyne, A. G. 2009. An interference removal technique for radio pulsar searches. MNRAS, 395(1), 410–415.CrossRefGoogle Scholar
Eatough, R. P., Falcke, H., Karuppusamy, R., and 20 others. 2013. A strong magnetic field around the supermassive black hole at the centre of the Galaxy. Nature, 501(7467), 391–394.CrossRefGoogle Scholar
Edwards, R. T., and Stappers, B. W. 2002. Drifting sub-pulse analysis using the twodimensional Fourier transform. A&A, 393(Oct.), 733–748.Google Scholar
Edwards, R. T., Bailes, M., van Straten, W., and Britton, M. C. 2001. The Swinburne intermediate-latitude pulsar survey. MNRAS, 326(Sept.), 358–374.CrossRefGoogle Scholar
Edwards, R. T., Hobbs, G. B., and Manchester, R. N. 2006. TEMPO2, a new pulsar timing package – II. The timing model and precision estimates. MNRAS, 372, 1549–1574.CrossRefGoogle Scholar
Eilek, J. A., Arendt, P. N. Jr., Hankins, T. H., and Weatherall, J. C. 2002. The radio-loud plasma in pulsars. Proceedings of the 270 WE-Heraeus seminar on neutron stars, pulsars, and supernova remnants, MPE Report 278, 249.Google Scholar
Esamdin, A., Lyne, A. G., Kramer, M., Graham-Smith, F., and Manchester, R. N. 2004 (Jan.). Thirteen drift bands in PSR B0826-34. Page 341 of: Camilo, F., and Gaensler, B. M. (eds), Young Neutron Stars and Their Environments. IAU Symposium, vol. 218.Google Scholar
Espinoza, C. M., Lyne, A. G., Kramer, M., Manchester, R. N., and Kaspi, V. M. 2011. The braking index of PSR J1734-333 and the magnetar population. ApJ, 741, 13.CrossRefGoogle Scholar
Espinoza, C. M., Lyne, A. G., and Stappers, B. W. 2017. New long-term braking index measurements for glitching pulsars using a glitch-template method. MNRAS, 466(1), 147–162.CrossRefGoogle Scholar
Esposito-Farèse, G. 1999. Binary-pulsar tests of strong-field gravity. Pulsar Timing, General Relativity and the Internal Structure of Neutron Stars, 13.Google Scholar
Evans, W. D., Klebesadel, R. W., Laros, J. G., and 11 others. 1980. Location of the gammaray transient event of 1979 March 5. ApJ, 237, L7–L9.CrossRefGoogle Scholar
Faber, J. A., and Rasio, F. A. 2002. Post-Newtonian SPH calculations of binary neutron star coalescence. III. Irrotational systems and gravitational wave spectra. Phys. Rev. D, 65(8), 8.CrossRefGoogle Scholar
Fahlman, G. G., and Gregory, P. C. 1981. An X-ray pulsar in SNR G109.1-1.0. Nature, 293, 202–204.CrossRefGoogle Scholar
Fantin, N. J., Côté, P., Hanes, D. A., Gwyn, S. D. J., Bianchi, L., Ferrarese, L., Cuillandre, J.-C., McConnachie, A., and Starkenburg, E. 2017. The next generation Virgo Cluster survey. XXVIII. Characterization of the Galactic white dwarf population. ApJ, 843(1), 1.Google Scholar
Faucher-Giguére, C.-A., and Kaspi, V. M. 2006. Birth and evolution of isolated radio pulsars. ApJ, 643, 332–355.CrossRefGoogle Scholar
Faulkner, A. J., Kramer, M., Lyne, A. G., Manchester, R. N., McLaughlin, M. A., Stairs, I. H., Hobbs, G., Possenti, A., Lorimer, D. R., D’Amico, N., Camilo, F., and Burgay, M. 2005. PSR J1756-2251: A new relativistic double neutron star system. ApJ, 618, L119–L122.CrossRefGoogle Scholar
Ferdman, R. D., Stairs, I. H., Kramer, M., and 14 others. 2010. A precise mass measurement of the intermediate-mass binary pulsar PSR J1802 – 2124. ApJ, 711(2), 764–771.CrossRefGoogle Scholar
Ferdman, R. D., Archibald, R. F., Gourgouliatos, K. N., and Kaspi, V. M. 2018. The glitches and rotational history of the highly energetic young pulsar PSR J0537-6910. ApJ, 852(2), 2.Google Scholar
Fichtel, C. E., Hartman, R. C., Kniffen, D. A., Thompson, D. J., Bignami, G. F., Ögelman, H., Özel, M. E., and Tümer, T. 1975. High-energy gamma-ray results from the Second Small Astronomy Satellite. ApJ, 198, 163–182.CrossRefGoogle Scholar
Filippenko, A. V. 1997. Optical spectra of supernovae. Ann. Rev. Astr. Ap., 35, 309–355.CrossRefGoogle Scholar
Filippenko, A. V., and Radhakrishnan, V. 1982. Pulsar nulling and drifting subpulse phase memory. ApJ, 263, 828–834.CrossRefGoogle Scholar
Finger, M. H., Koh, D. T., Nelson, R. W., Prince, T. A., Vaughan, B. A., and Wilson, R. B. 1996. Discovery of hard X-ray pulsations from the transient source GRO J1744-28. Nature, 381, 291–293.CrossRefGoogle Scholar
Fishman, G. J., Harnden, F. R., and Haymes, R. C. 1969. Observation of pulsed hard X-radiation from NP 0532 from 1967 data. ApJ, 156, L107–L110.CrossRefGoogle Scholar
Flanagan, C. S. 1990. Rapid recovery of the Vela Pulsar from a giant glitch. Nature, 345, 416–417.CrossRefGoogle Scholar
Fomalont, E. B., Goss, W. M., Lyne, A. G., and Manchester, R. N. 1984. Astrometry of 59 pulsars: A comparison of interferometric and timing positions. MNRAS, 210, 113–130.CrossRefGoogle Scholar
Fomalont, E. B., Goss, W. M., Lyne, A. G., Manchester, R. N., and Justtanont, K. 1992. Positions and proper motions of pulsars. MNRAS, 258, 497–510.CrossRefGoogle Scholar
Fonseca, E. Stairs, I. H., and Thorsett, S. E. 2014. A comprehensive study of relativistic gravity using PSR B1534+12. ApJ, 787(1), 1.Google Scholar
Fontaine, G., Brassard, P., and Bergeron, P. 2001. The potential of white dwarf cos- mochronology. PASP, 113(782), 409–435.CrossRefGoogle Scholar
Foster, R. S., and Backer, D. C. 1990. Constructing a pulsar timing array. ApJ, 361, 300.CrossRefGoogle Scholar
Foster, R. S., Cadwell, B. J., Wolszczan, A., and Anderson, S. B. 1995. A high Galactic latitude pulsar survey of the Arecibo sky. ApJ, 454, 826–830.CrossRefGoogle Scholar
Frail, D. A., and Kulkarni, S. R. 1991. Unusual interaction of the high-velocity pulsar PSR 1757-24 with the supernova remnant G5.4-1.2. Nature, 352, 785–787.CrossRefGoogle Scholar
Frail, D. A., and Weisberg, J. M. 1990. A critical evaluation of pulsar distance measurements. AJ, 100, 743–757.CrossRefGoogle Scholar
Frail, D. A., Goss, W. M., and Whiteoak, J. B. Z. 1994. The radio lifetime of supernova remnants and the distribution of pulsar velocities at birth. ApJ, 437, 781–793.CrossRefGoogle Scholar
Freire, P., Ransom, S., Begin, S., and Stairs, I. 2008. Eight new millisecond pulsars in NGC 6440 and NGC 6441. ApJ, 675, 670–682.CrossRefGoogle Scholar
Freire, P. C., Kramer, M., Lyne, A. G., Camilo, F., Manchester, R. N., and D’Amico, N. 2001a. Detection of inoized gas in the globular cluster 47 Tucanae. ApJ, 557, L105–L108.CrossRefGoogle Scholar
Freire, P. C., Kramer, M., and Lyne, A. G. 2001b. Determination of the orbital parameters of binary pulsars. MNRAS, 322, 885–890.CrossRefGoogle Scholar
Freire, P. C., Camilo, F., Lorimer, D. R., Lyne, A. G., Manchester, R. N., and D’Amico, N. 2001c. Timing the millisecond pulsars in 47 Tucanae. MNRAS, 326(Sept.), 901–915.CrossRefGoogle Scholar
Freire, P. C., Camilo, F., Kramer, M., Lorimer, D. R., Lyne, A. G., Manchester, R. N., and D’Amico, N. 2003. Further results from the timing of the millisecond pulsars in 47 Tucanae. MNRAS, 340, 1359–1374.CrossRefGoogle Scholar
Freire, P. C. C., and Wex, N. 2010. The orthometric parametrization of the Shapiro delay and an improved test of general relativity with binary pulsars. MNRAS, 409, 199–212.CrossRefGoogle Scholar
Fritz, G., Henry, R. C., Meekins, J. F., Chubb, T. A., and Friedmann, H. 1969. X-ray pulsar in the Crab Nebula. Science, 164, 709–712.CrossRefGoogle ScholarPubMed
Fruchter, A. S., Stinebring, D. R., and Taylor, J. H. 1988a. A millisecond pulsar in an eclipsing binary. Nature, 333, 237–239.CrossRefGoogle Scholar
Fruchter, A. S., Gunn, J. E., Lauer, T. R., and Dressler, A. 1988b. Optical detection and characterization of the eclipsing pulsar’s companion. Nature, 334, 686–689.CrossRefGoogle Scholar
Fuentes, J. R., Espinoza, C. M., Reisenegger, A., Shaw, B., Stappers, B. W., and Lyne, A. G. 2017. The glitch activity of neutron stars. A&A, 608, A131.Google Scholar
Gaensler, B. M., and Slane, P. O. 2006. The evolution and structure of pulsar wind nebulae. Ann. Rev. Astr. Ap., 44(1), 17–47.CrossRefGoogle Scholar
Gaensler, B. M., and Wallace, B. J. 2003. A multi-frequency radio study of supernova remnant G292.0+1.8 and its pulsar wind nebula. ApJ, 594, 326–339.CrossRefGoogle Scholar
Gaensler, B. M., Slane, P. O., Gotthelf, E. V., and Vasisht, G. 2001. Anomalous X-Ray pulsars and soft gamma-ray repeaters in supernova remnants. ApJ, 559, 963–972.CrossRefGoogle Scholar
Gaensler, B. M., Arons, J., Kaspi, V. M., Pivovaroff, M. J., Kawai, N., and Tamura, K. 2002a. High-resolution X-ray imaging of pulsar B1509-58 and its environment. ApJ, 569, 878–893.CrossRefGoogle Scholar
Gaensler, B. M., Jones, D. H., and Stappers, B. W. 2002b. An optical bow shock around the nearby millisecond pulsar J2124-3358. ApJ, 580, L137–L141.CrossRefGoogle Scholar
Gaensler, B. M., Madsen, G. J., Chatterjee, S., and Mao, S. A. 2008. The vertical structure of warm ionised gas in the Milky Way. PASA, 25, 184–200.CrossRefGoogle Scholar
Galloway, D. K., and Keek, L. 2017. Thermonuclear X-ray bursts. arXiv e-prints, Dec., arXiv:1712.06227.Google Scholar
Galt, J. A., and Lyne, A. G. 1972. The interstellar scintillation pattern of PSR 0329+54. MNRAS, 158, 281–290.CrossRefGoogle Scholar
Gandolfi, S., Lippuner, J., Steiner, A. W., Tews, I., Du, X., and Al-Mamun, M. 2019. From the microscopic to the macroscopic world: From nucleons to neutron stars. J. Phys. G Nucl. Phys., 46(10), 10.CrossRefGoogle Scholar
Gardner, F. F., Morris, D., and Whiteoak, J. B. 1969. The linear polarization of radio sources between 11 and 20 cm wavelength. II Influence of the Galaxy on source depolarization and Faraday rotation. Aust. J. Phys., 22, 813–819.CrossRefGoogle Scholar
Gavriil, F. P., Kaspi, V. M., and Woods, P. M. 2002. Magnetar-like X-ray bursts from an anomalous X-ray pulsar. Nature, 419, 142–144.CrossRefGoogle ScholarPubMed
Gavriil, F. P., Gonzalez, M. E., Gotthelf, E. V., Kaspi, V. M., Livingstone, M. A., and Woods, P. M. 2008. Magnetar-like emission from the young pulsar in Kes 75. Science, 319, 1802–1805.CrossRefGoogle Scholar
Gedalin, M., Gruman, E., and Melrose, D. B. 2002. New mechanism of pulsar radio emission. Phys. Rev. Lett., 88, 121101.CrossRefGoogle ScholarPubMed
Gehrels, N., and Chen, W. 1993. The Geminga supernova as a possible cause of the local interstellar bubble. Nature, 361, 706–707.CrossRefGoogle Scholar
Gelfand, J. D., Gaensler, B. M., Slane, P. O., Patnaude, D. J., Hughes, J. P., and Camilo, F. 2007. The radio emission, X-ray emission, and hydrodynamics of G328.4+0.2: A comprehensive analysis of a luminous pulsar wind nebula, its neutron star, and the progenitor supernova explosion. ApJ, 663, 468–486.CrossRefGoogle Scholar
Geppert, U., Page, D., and Zannias, T. 1999. Submergence and re-diffusion of the neutron star magnetic field after the supernova. A&A, 345, 847–854.Google Scholar
Geyer, M., Karastergiou, A., Kondratiev, V. I., and 8 others. 2017. Scattering analysis of LOFAR pulsar observations. MNRAS, 470(3), 2659–2679.CrossRefGoogle Scholar
Giacconi, R. 1974. Page 27 of: Proc. 16th Int. Conf. on Physics. Editions de l’Université de Bruxelles.Google Scholar
Giacconi, R., Gursky, H., Paolini, F. R., and Rossi, B. 1962. Evidence for X-rays from sources outside the solar system. Phys. Rev. Lett., 9, 439–443.CrossRefGoogle Scholar
Gil, J. A., and Han, J. L. 1996. Geometry of pulsar emission and pulse width distribution. ApJ, 458, 265.CrossRefGoogle Scholar
Gil, J. A., and Kijak, K. 1993. Period dependence of radio emission altitudes in the pulsar magnetosphere. A&A, 273, 563–569.Google Scholar
Gil, J. A., Kijak, J., and Seiradakis, J. H. 1993. On the Two-dimensional structure of pulsar beams. A&A, 272, 268.Google Scholar
Glendenning, N. K. 2000. Compact Stars: Nuclear Physics, Particle Physics, and General Relativity. New York: Springer.CrossRefGoogle Scholar
Gold, T. 1968. Rotating neutron stars as the origin of the pulsating radio sources. Nature, 218, 731–732.CrossRefGoogle Scholar
Gold, T. 1969. Rotating neutron stars and the nature of pulsars. Nature, 221, 25–27.CrossRefGoogle Scholar
Goldreich, P., and Julian, W. H. 1969. Pulsar electrodynamics. ApJ, 157, 869–880.CrossRefGoogle Scholar
Golenetskii, S. V., Ilyinskii, V. N., and Mazets, E. P. 1984. Recurrent bursts in GBS 0526-66, the source of the 5 March 1979 gamma-ray burst. Nature, 307, 41–43.CrossRefGoogle Scholar
Gómez, G. C., Benjamin, R. A., and Cox, D. P. 2001. A reexamination of the distribution of Galactic free electrons. AJ, 122, 908–920.Google Scholar
Gonthier, P. L., Ouellette, M. S., Berrier, J., O’Brien, S., and Harding, A. K. 2002. Galactic populations of radio and gamma-ray pulsars in the polar cap model. ApJ, 565, 482–499.CrossRefGoogle Scholar
Gotthelf, E. V., Vasisht, G., Boylan-Kolchin, M., and Torii, K. 2000. A 700 year-old pulsar in the supernova remnant Kesteven 75. ApJ, 542(Oct.), L37–L40.CrossRefGoogle Scholar
Gould, D. M., and Lyne, A. G. 1998. Multifrequency polarimetry of 300 radio pulsars. MNRAS, 301, 235–260.CrossRefGoogle Scholar
Graham, D. A., Mebold, U., Hesse, K. H., Hills, D. L., and Wielebinski, R. 1974. HI absorbtion of nine pulsars. A&A, 37, 405–410.Google Scholar
Graham-Smith, F., Dolan, J. F., Boyd, P. T., Biggs, J. D., Lyne, A. G., and Percival, J. 1996. The ultraviolet polarization of the Crab Pulsar. MNRAS, 282, 1354–1358.CrossRefGoogle Scholar
Grenier, I. A., and Harding, A. K. 2015. Gamma-ray pulsars: A gold mine. Comptes Rendus Physique, 16(6-7), 641–660.CrossRefGoogle Scholar
Grewing, M., and Warmsley, M. 1971. On the interpretation of the pulsar dispersion measure. A&A, 11, 65–69.Google Scholar
Grindlay, J., Gursky, H., Schnopper, H., Parsignault, D. R., Heise, J., Brinkman, A. C., and Shriver, J. 1976. Discovery of intense X-ray bursts from the globular cluster NGC 6624. ApJ, 205, L127–L130.CrossRefGoogle Scholar
Gunn, J. E., and Ostriker, J. P. 1970. On the nature of pulsars. III. Analysis of observations. ApJ, 160, 979–1002.CrossRefGoogle Scholar
Gupta, Y., and Gangadhara, R. T. 2003. Understanding the radio emission geometry of multiple-component radio pulsars from retardation and aberration effects. ApJ, 584, 418–426.CrossRefGoogle Scholar
Gupta, Y., Rickett, B. J., and Lyne, A. G. 1994. Refractive interstellar scintillation in pulsar dynamic spectra. MNRAS, 269, 1035–1068.CrossRefGoogle Scholar
Haberl, F. 2007. The magnificent seven: Magnetic fields and surface temperature distributions. ApJS, 73.CrossRefGoogle Scholar
Haensel, P., Salgado, M., and Bonazzola, S. 1995. Equation of state of dense matter and maximum rotation frequency of neutron stars. A&A, 296, 745.Google Scholar
Hall, J. S., and Mikesell, A. H. 1950. Polarization of light in the Galaxy as determined from observations of 557 early-type stars. Pub. of US Naval Obs Second Ser., 17, 1–62.Google Scholar
Hamilton, T. T., Helfand, D. J., and Becker, R. H. 1985. A search for millisecond pulsars in globular clusters. AJ, 90, 606–608.CrossRefGoogle Scholar
Han, J. L. 2017. Observing interstellar and intergalactic magnetic fields. Ann. Rev. Astr. Ap., 55(1), 111–157.CrossRefGoogle Scholar
Han, J. L., and Manchester, R. N. 2001. The shape of pulsar radio beams. MNRAS, 320, L35–L39.CrossRefGoogle Scholar
Han, J. L., Manchester, R. N., and Qiao, G. J. 1999. Pulsar rotation measures and the magnetic structure of our Galaxy. MNRAS, 306, 371–380.CrossRefGoogle Scholar
Han, J. L., Demorest, P. B., van Straten, W., and Lyne, A. G. 2009. Polarization observations of 100 pulsars at 774 MHz by the Green Bank Telescope. ApJS, 181, 557–571.CrossRefGoogle Scholar
Han, J. L., Manchester, R. N., van Straten, W., and Demorest, P. 2018. Pulsar rotation measures and large-scale magnetic field reversals in the galactic disk. ApJS, 234(1), 1.CrossRefGoogle Scholar
Hankins, T. H. 1971. Microsecond intensity variation in the radio emission from CP 0950. ApJ, 169, 487–494.CrossRefGoogle Scholar
Hankins, T. H., and Cordes, J. M. 1981. Interpulse emission from pulsar 0950+08: How many poles? ApJ, 249, 241–253.CrossRefGoogle Scholar
Hankins, T. H., and Eilek, J. A. 2007. Radio emission signatures in the Crab Pulsar. ApJ, 670(1), 693–701.CrossRefGoogle Scholar
Hankins, T. H., and Rickett, B. J. 1975. Pulsar signal processing. Pages 55–129 of: Methods in Computational Physics Volume 14 – Radio Astronomy. New York: Academic Press.Google Scholar
Hankins, T. H., Eilek, J. A., and Jones, G. 2016. The Crab Pulsar at centimeter wavelengths. II. Single pulses. ApJ, 833(1), 1.Google Scholar
Harding, A. K., Contopoulos, I., and Kazanas, D. 1999. Magnetar spin-down. ApJ, 525, L125–L128.CrossRefGoogle ScholarPubMed
Harding, A. K., Stern, J. V., Dyks, J., and Frackowiak, M. 2008. High-altitude emission from pulsar slot gaps: The Crab Pulsar. ApJ, 680, 1378–1393.CrossRefGoogle Scholar
Harding, A. K., Kalapotharakos, C., Barnard, M., and Venter, C. 2018. Multi-TeV emission from the Vela Pulsar. ApJ, 869(1), L18.CrossRefGoogle ScholarPubMed
Harrison, E. R., and Tademaru, E. 1975. Acceleration of pulsars by asymmetric radiation. ApJ, 201, 447–461.CrossRefGoogle Scholar
Harrison, P. A., and Lyne, A. G. 1993. Pulsar velocities and the scale height of scattering in the Galaxy. MNRAS, 265, 778–780.CrossRefGoogle Scholar
Harrison, P. A., Lyne, A. G., and Anderson, B. 1993. New determinations of the proper motions of 44 pulsars. MNRAS, 261, 113–124.CrossRefGoogle Scholar
Hartman, J. W., Bhattacharya, D., Wijers, R., and Verbunt, F. 1997. A study of the evolution of radio pulsars through improved population synthesis. A&A, 322, 477–488.Google Scholar
Hartnett, J. G., and Luiten, A. 2010. Comparison of astrophysical and terrestrial frequency standards. arXiv:1004.0115.Google Scholar
Hartnett, J. G., and Luiten, A. N. 2011. Colloquium: Comparison of astrophysical and terrestrial frequency standards. Rev. Mod. Phys., 83(1), 1–9.CrossRefGoogle Scholar
Haskell, B., and Melatos, A. 2015. Models of pulsar glitches. Int. J Modern Phys. D, 24(3), 3.CrossRefGoogle Scholar
Hayakawa, S., and Matsouka, M. 1964. Origin of Cosmic X-rays. Prog. Theor. Phys. Suppl., 30, 204.CrossRefGoogle Scholar
Heinke, C. O., and Ho, W. C. G. 2010. Direct observation of the cooling of the Cassiopeia A neutron star. ApJ, 719, L167–L171.CrossRefGoogle Scholar
Helfand, D. J., Fowler, L. A., and Kuhlman, J. V. 1977a. Pulsar flux observations: Longterm intensity and spectral variations. AJ, 82, 701–705.CrossRefGoogle Scholar
Helfand, D. J., Taylor, J. H., and Manchester, R. N. 1977b. Pulsar proper motions. ApJ, 213, L1–L4.CrossRefGoogle Scholar
Helfand, D. J., Gotthelf, E. V., and Halpern, J. P. 2001. The Vela Pulsar and its synchrotron nebula: Aftermath of a glitch. ApJ, 556(July), 380–391.CrossRefGoogle Scholar
Hellings, R. W. 1986. Relativistic effects in astronomical timing measurements. AJ, 91, 650.CrossRefGoogle Scholar
Hellings, R. W., and Downs, G. S. 1983. Upper limits on the isotropic gravitational radiation background from pulsar timing analysis. ApJ, 265, L39.CrossRefGoogle Scholar
Hessels, J. W. T., Ransom, S. M., Stairs, I. H., Freire, P. C. C., Kaspi, V. M., and Camilo, F. 2006. A radio pulsar spinning at 716 Hz. Science, 311(Mar.), 1901–1904.CrossRefGoogle ScholarPubMed
Hessels, J. W. T., Ransom, S. M., Stairs, I. H., Kaspi, V. M., and Freire, P. C. C. 2007. A 1.4-GHz Arecibo survey for pulsars in globular clusters. ApJ, 670, 363–378.CrossRefGoogle Scholar
Hessels, J. W. T., Nice, D. J., Gaensler, B. M., and 21 others. 2008a. PSR J1856+0245: Arecibo discovery of a young, energetic pulsar coincident with the TeV gamma-ray source HESS J1857+026. ApJ, 682, L41–L44.CrossRefGoogle Scholar
Hessels, J. W. T., Ransom, S. M., Kaspi, V. M., Roberts, M. S. E., Champion, D. J., and Stappers, B. W. 2008b (Feb.). The GBT350 survey of the northern Galactic plane for radio pulsars and transients. Pages 613–615 of: Bassa, C., Wang, Z., Cumming, A., and Kaspi, V. M. (eds), 40 Years of Pulsars: Millisecond Pulsars, Magnetars and More. American Institute of Physics Conference Series, vol. 983.Google Scholar
Hessels, J. W. T., Spitler, L. G., Seymour, A. D., and 23 others. 2019. FRB 121102 bursts show complex time-frequency structure. ApJ, 876(2), L23.CrossRefGoogle Scholar
Hewish, A. 1980. Frequency-time structure of pulsar scintillation. MNRAS, 192, 799–804.Google Scholar
Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., and Collins, R. A. 1968. Observation of a rapidly pulsating radio source. Nature, 217, 709–713.CrossRefGoogle Scholar
Hibschman, J. A., and Arons, J. 2001. Polarization sweeps in rotation-powered pulsars. ApJ, 546, 382–393.CrossRefGoogle Scholar
Hill, A. S., Stinebring, D. R., Barnor, H. A., Berwick, D. E., and Webber, A. B. 2003. Pulsar scintillation arcs. I. Frequency dependence. ApJ, 599, 457–464.CrossRefGoogle Scholar
Hillebrandt, W., and Niemeyer, J. C. 2000. Type IA supernova explosion models. Ann. Rev. Astr. Ap., 38, 191–230.CrossRefGoogle Scholar
Hiltner, W. A. 1949. Polarization of stellar radiation III. The polarisation of 841 stars. ApJ, 114, 241–271.CrossRefGoogle Scholar
Ho, P.-Y. 1962. Ancient and mediaeval observations of comets and novae in Chinese sources. Vistas Astron., 5, 127–225.Google Scholar
Ho, W. C. G., Ng, C. Y., Lyne, A. G., Stappers, B. W., Coe, M. J., Halpern, J. P., Johnson, T. J., and Steele, I. A. 2017. Multiwavelength monitoring and X-ray brightening of Be X-ray binary PSR J2032+4127/MT91 213 on its approach to periastron. MNRAS, 464(1), 1211–1219.CrossRefGoogle Scholar
Hobbs, G., Lyne, A. G., and Kramer, M. 2003. Jodrell Bank timing astrometry. Pages 215–218 of: Bailes, M., Nice, D. J., and Thorsett, S. E. (eds), Radio Pulsars. San Francisco: Astronomical Society of the Pacific.Google Scholar
Hobbs, G., Lyne, A. G., Kramer, M., Martin, C. E., and Jordan, C. 2004. Long-term timing observations of 374 pulsars. MNRAS, 353, 1311–1344.CrossRefGoogle Scholar
Hobbs, G., Lorimer, D. R., Lyne, A. G., and Kramer, M. 2005. A statistical study of 233 pulsar proper motions. MNRAS, 360, 974–992.CrossRefGoogle Scholar
Hobbs, G., Lyne, A. G., and Kramer, M. 2010. An analysis of the timing irregularities for 366 pulsars. MNRAS, 402, 1027–1048.CrossRefGoogle Scholar
Hobbs, G., Archibald, A., Arzoumanian, Z., and 55 others. 2010. The International Pulsar Timing Array project: Using pulsars as a gravitational wave detector. Classical and Quantum Gravity, 27, 084013.CrossRefGoogle Scholar
Hobbs, G., Guo, L., Caballero, R. N., and 57 others. 2020. A pulsar-based time-scale from the International Pulsar Timing Array. MNRAS, 491(4), 5951–5965.CrossRefGoogle Scholar
Hoyle, F., Narlikar, J., and Wheeler, J. A. 1964. Electromagnetic waves from very dense stars. Nature, 203, 914–916.CrossRefGoogle Scholar
Hui, C. Y., and Becker, W. 2008. Resolving the bow-shock nebula around the old pulsar PSR B1929+10 with multi-epoch Chandra observations. A&A, 486, 485–491.Google Scholar
Hulse, R. A., and Taylor, J. H. 1974. A high sensitivity pulsar survey. ApJ, 191, L59–L61.Google Scholar
Hurley, K. 2000. The 4.5 +/- 0.5 soft gamma repeaters in review. Page 515 of: McConnell, M. L., and Ryan, J. M. (eds), The Fifth Compton Symposium; AIP Conference Proceedings No. 510. New York: AIP Press.Google Scholar
Hurley, K., Cline, T., Mazets, E., and 11 others. 1999. A giant periodic flare from the soft gamma-ray repeater SGR1900+14. Nature, 397, 41–43.CrossRefGoogle Scholar
Hurley-Walker, N., Gaensler, B. M., Leahy, D. A., and 18 others. 2019a. Candidate radio supernova remnants observed by the GLEAM survey. PASA, 36(Nov.), e048.CrossRefGoogle Scholar
Hurley-Walker, N., Filipović, M. D., Gaensler, B. M., and 18 others. 2019b. New candidate radio supernova remnants detected in the GLEAM survey. PASA, 36(Jan.), e045.CrossRefGoogle Scholar
Ibrahim, A. I., Safi-Harb, S., Swank, J. H., Parke, W., Zane, S., and Turolla, R. 2002. Discovery of cyclotron resonance features in the soft gamma repeater SGR 1806-20. ApJ, 574, L51–L55.CrossRefGoogle Scholar
Ibrahim, A. I., Swank, J. H., and Parke, W. 2003. New evidence of proton-cyclotron resonance in a magnetar strength field from SGR 1806-20. ApJ, 584, L17–L21.CrossRefGoogle Scholar
Ibrahim, A. I., Markwardt, C. B., Swank, J. H., and 10 others. 2004. Discovery of a transient magnetar: XTE J1810-197. ApJ, 609, L21–L24.CrossRefGoogle Scholar
Ilie, C. D., Weltevrede, P., Johnston, S., and Chen, T. 2020. The drifting sub-pulses of PSR B0031-07 and its synchronously modulated radio polarization. MNRAS, 491(3), 3385–3394.Google Scholar
Ilovaisky, S. A., and Lequeux, J. 1972. A study of galactic supernova remnants I. Distances, radio luminosity function and galactic distribution. A&A, 18, 169–185.Google Scholar
Israel, G., Covino, S., Mignani, R., and 9 others. 2005. Discovery and monitoring of the likely IR counterpart of SGR 1806-20 during the 2004 gamma-ray burst-active state. A&A, 438, L1–L4.Google Scholar
Jackson, M. S., Halpern, J. P., Gotthelf, E. V., and Mattox, J. R. 2002. A high-energy study of the Geminga Pulsar. ApJ, 578(2), 935–942.CrossRefGoogle Scholar
Jacoby, B. A., Bailes, M., van Kerkwijk, M. H., Ord, S., Hotan, A., Kulkarni, S. R., and Anderson, S. B. 2003. PSR J1909-3744: A binary millisecond pulsar with a very small duty cycle. ApJ, 599(2), L99–L102.CrossRefGoogle Scholar
Jacoby, B. A., Cameron, P. B., Jenet, F. A., Anderson, S. B., Murty, R. N., and Kulkarni, S. R. 2006. Measurement of orbital decay in the double neutron star binary PSR B2127+11C. ApJ, 644, L113–L116.CrossRefGoogle Scholar
Jacoby, B. A., Bailes, M., Ord, S. M., Edwards, R. T., and Kulkarni, S. R. 2009. A large-area survey for radio pulsars at high Galactic latitudes. ApJ, 699(2), 2009–2016.CrossRefGoogle Scholar
Jaffe, T. R., Leahy, J. P., Banday, A. J., Leach, S. M., Lowe, S. R., and Wilkinson, A. 2010. Modelling the Galactic magnetic field on the plane in two dimensions. MNRAS, 401, 1013–1028.CrossRefGoogle Scholar
Jahan-Miri, M. 2010. Rotational coupling of the pinned core superfluid. ApJ, 725, 29–35.CrossRefGoogle Scholar
Janka, Hans-Thomas. 2012. Explosion mechanisms of core-collapse supernovae. Annual Review of Nuclear and Particle Science, 62(1), 407–451.CrossRefGoogle Scholar
Janssen, G. H., and van Leeuwen, J. 2004. Intermittent nulls in PSR B0818-13, and the subpulse-drift alias mode. A&A, 425(Oct.), 255–261.Google Scholar
Janssen, G. H., Stappers, B. W., Kramer, M., Purver, M., Jessner, A., and Cognard, I. 2008a. European Pulsar Timing Array. 40 Years of Pulsars: Millisecond Pulsars, Magnetars and More. AIP Conference Proceedings, Volume 983, 633–635.Google Scholar
Janssen, G. H., Stappers, B. W., Kramer, M., Nice, D. J., Jessner, A., Cognard, I., and Purver, M. B. 2008b. Multi-telescope timing of PSR J1518+4904. A&A, 490, 753–761.Google Scholar
Jansson, R., and Farrar, G. R. 2012. The Galactic magnetic field. ApJ, 761(1), L11.CrossRefGoogle Scholar
Jauncey, D., Bignall, H., Kedziora-Chudczer, L., Koay, J., Lovell, J., Macquart, J.-P., Ojha, R., Pursimo, T., Reynolds, C., and Rickett, B. 2016. Interstellar scintillation and scattering of micro-arc-second AGN. Galaxies, 4(4), 4.CrossRefGoogle Scholar
Jensen, H. J. 1998. Self-organised Critical Systems. Cambridge University Press.Google Scholar
Jennings, R. J., Kaplan, D. L., Chatterjee, S., Cordes, J. M., and Deller, A. T. 2018. Binary pulsar distances and velocities from Gaia Data Release 2. ApJ, 864(1), 26–34.CrossRefGoogle Scholar
Jha, S. W., Maguire, K., and Sullivan, M. 2019. Observational properties of thermonuclear supernovae. Nat. Astron., 3(Aug.), 706–716.CrossRefGoogle Scholar
Johnston, H. M., and Kulkarni, S. R. 1991. On the detectability of pulsars in close binary systems. ApJ, 368, 504–514.CrossRefGoogle Scholar
Johnston, S., and Karastergiou, A. 2019. The period-width relationship for radio pulsars revisited. MNRAS, 485(1), 640–647.CrossRefGoogle Scholar
Johnston, S., Lyne, A. G., Manchester, R. N., Kniffen, D. A., D’Amico, N., Lim, J., and Ashworth, M. 1992. A high frequency survey of the southern Galactic plane for pulsars. MNRAS, 255, 401–411.CrossRefGoogle Scholar
Johnston, S., Koribalski, B. S., Weisberg, J., and Wilson, W. 1996. HI line measurements of pulsars towards the Gum Nebula and Carina Arm. MNRAS, 279, 661–668.CrossRefGoogle Scholar
Johnston, S., Koribalski, B., Weisberg, J. M., and Wilson, W. 2001. HI line measurements of pulsars towards the Galactic Center and the electron density in the inner Galaxy. MNRAS, 322, 715–722.CrossRefGoogle Scholar
Johnston, S., Kramer, M., Lorimer, D. R., Lyne, A. G., McLaughlin, M., Klein, B., and Manchester, R. N. 2006. Discovery of two pulsars towards the Galactic centre. MNRAS, Oct., L96+.CrossRefGoogle Scholar
Johnston, S., Smith, D. A., Karastergiou, A., and Kramer, M. 2020. The Galactic population and properties of young, highly energetic pulsars. MNRAS, 497(2), 1957–1965.CrossRefGoogle Scholar
Jones, D. I., and Anderson, N. 2001. Freely precessing neutron stars: Model and observations. MNRAS, 324, 811–824.CrossRefGoogle Scholar
Jones, P. B. 2002. Post-glitch relaxation in pulsars. MNRAS, 335, 733–740.CrossRefGoogle Scholar
Joss, P. C., and Rappaport, S. A. 1984. Neutron stars in interacting binary systems. Ann. Rev. Astr. Ap., 22, 537–592.CrossRefGoogle Scholar
Kalapotharakos, C., Brambilla, G., Timokhin, A., Harding, A., and Kazanas, D. 2018. Three-dimensional kinetic pulsar magnetosphere models: Connecting to gamma-ray observations. ApJ, 857(1), 1.Google Scholar
Kaplan, D. L., Escoffier, R. P., Lacasse, R. J., O’Neil, K., Ford, J. M., Ransom, S. M., Anderson, S. B., Cordes, J. M., Lazio, T. J. W., and Kulkarni, S. R. 2005. The Green Bank Telescope pulsar spigot. PASP, 117(June), 643–653.CrossRefGoogle Scholar
Kaplan, G. H. 2005. The IAU resolutions on astronomical reference systems, time scales, and earth rotation models: Explanation and implementation. U.S. Naval Observatory Circular, 179.Google Scholar
Karuppusamy, R., Stappers, B. W., and van Straten, W. 2010. Giant pulses from the Crab Pulsar. A wide-band study. A&A, 515(June), A36.Google Scholar
Kaspi, V. M. 1995. Millisecond pulsar timing: Recent advances. Pages 345–356 of: Fruchter, A. S., Tavani, M., and Backer, D. C. (eds), Millisecond Pulsars–A Decade of Surprise, vol. 72. Astronomical Society of the Pacific.Google Scholar
Kaspi, V. M., and Beloborodov, A. M. 2017. Magnetars. Ann. Rev. Astr. Ap., 55(1), 261–301.CrossRefGoogle Scholar
Kaspi, V. M., and Helfand, D. J. 2002. Constraining the birth events of neutron stars. ASP Conf. Ser., 271, 3.Google Scholar
Kaspi, V. M., Lackey, J. R., Mattox, J., Manchester, R. N., Bailes, M., and Pace, R. 2000. High-energy gamma-ray observations of two young, energetic radio pulsars. ApJ, 528, 445–453.CrossRefGoogle Scholar
Katgert, P., and Oort, J. H. 1967. On the frequency of supernova outbursts in galaxies. Bull. Astr. Inst. Netherlands, 19, 239–245.Google Scholar
Keane, E. F., and Kramer, M. 2008. On the birthrates of Galactic neutron stars. MNRAS, 391, 2009–2016.CrossRefGoogle Scholar
Keane, E. F., Ludovici, D. A., Eatough, R. P., Kramer, M., Lyne, A. G., McLaughlin, M. A., and Stappers, B. W. 2010. Further searches for rotating radio transients in the Parkes Multi-beam pulsar survey. MNRAS, 401, 1057–1068.CrossRefGoogle Scholar
Keith, M. J., Kramer, M., Lyne, A. G., Eatough, R. P., Stairs, I. H., Possenti, A., Camilo, F., and Manchester, R. N. 2009. PSR J1753-2240: A mildly recycled pulsar in an eccentric binary system. MNRAS, 393(2), 623–627.CrossRefGoogle Scholar
Keith, M. J., Jameson, A., van Straten, W., and 14 others. 2010. The High Time Resolution Universe pulsar survey – I. System configuration and initial discoveries. MNRAS, 409, 619–627.CrossRefGoogle Scholar
Keith, M. J., Coles, W., Shannon, R. M., and 16 others. 2013. Measurement and correction of variations in interstellar dispersion in high-precision pulsar timing. MNRAS, 429(3), 2161–2174.CrossRefGoogle Scholar
Kemp, J. C. 1970. Circular polarization of thermal radiation in a magnetic field. ApJ, 162(Oct.), 169.CrossRefGoogle Scholar
Kerr, F. J. 1969. The large scale distribution of hydrogen in the Galaxy. Ann. Rev. Astr. Ap., 7, 39–66.CrossRefGoogle Scholar
Kerr, M., Hobbs, G., Johnston, S., and Shannon, R. M. 2016. Periodic modulation in pulse arrival times from young pulsars: a renewed case for neutron star precession. MNRAS, 455(2), 1845–1854.CrossRefGoogle Scholar
Kiel, P. D., and Hurley, J. R. 2009. Populating the Galaxy with pulsars – II. Galactic dynamics. MNRAS, 395, 2326–2346.CrossRefGoogle Scholar
Kijak, J., and Gil, J. 1997. Radio emission altitudes in pulsar magnetospheres. MNRAS, 288, 631–637.CrossRefGoogle Scholar
Klose, S., Henden, A. A., Geppert, U., Greiner, J., Guetter, H. H., Hartmann, D. H., Kouveliotou, C., Luginbuhl, C. B., Stecklum, B., and Vrba, F. J. 2004. A near-infrared survey of the N49 region around the soft gamma repeater SGR 0526-66. ApJ, 609, L13–L16.CrossRefGoogle Scholar
Koester, D. 2002. White dwarfs: Recent developments. Astron. Astrophys. Rev., 11(1), 33–66.CrossRefGoogle Scholar
Kolonko, M., Gil, J., and Maciesiak, K. 2004. On the pulse-width statistics in radio pulsars. A&A, 428(Dec.), 943–951.Google Scholar
Komesaroff, M. M. 1970. Possible mechanism for the pulsar radio emission. Nature, 225, 612–614.CrossRefGoogle ScholarPubMed
Komesaroff, M. M., Morris, D., and Cooke, D. J. 1970. Linear polarization and pulse shape measurements of nine pulsars. Astrophys. Lett., 5, 37–41.Google Scholar
Komissarov, S., and Lyubarsky, Y. 2004. MHD simulations of Crab’s jet and torus. Ap&SS, 293, 107–113.Google Scholar
Konacki, M., and Wolszczan, A. 2003. Masses and orbital inclinations of planets in the PSR B1257+12 system. ApJ, 591, L147–L150.CrossRefGoogle Scholar
Kondratiev, V. I., Verbiest, J. P. W., Hessels, J. W. T., and 29 others. 2016. A LOFAR census of millisecond pulsars. A&A, 585(Jan.), A128.Google Scholar
Kopeikin, S. M. 1995. On possible implications of orbital parallaxes of wide orbit binary pulsars and their measurability. ApJ, 439, L5–L8.CrossRefGoogle Scholar
Koribalski, B. S., Johnston, S., Weisberg, J., and Wilson, W. 1995. HI line measurements of eight southern pulsars. ApJ, 441, 756.CrossRefGoogle Scholar
Kostyuk, S. V., Kondratiev, V. I., Kuzmin, A. D., Popov, M. V., and Soglasnov, V. A. 2003. Peculiarities of giant pulses from the Crab Pulsar at frequencies of 594 and 2228 MHz. Astronomy Letters, 29(June), 387–393.CrossRefGoogle Scholar
Kosugi, G., Ogasawara, R., and Terada, H. 2005. A variable infrared counterpart to the soft gamma-ray repeater SGR 1806-20. ApJ, 623, L125–L128.CrossRefGoogle Scholar
Kouveliotou, C., Dieters, S., Strohmayer, T., van Paradijs, J., Fishman, G. J., Meegan, C. A., Hurley, K., Kommers, J., Smith, I., Frail, D., and Murakami, T. 1998. An X-ray pulsar with a superstrong magnetic field in the soft γ -ray repeater SGR 1806-20. Nature, 393, 235–237.CrossRefGoogle Scholar
Kouveliotou, C., Strohmayer, T., Hurley, K., Van Paradijs, J., Finger, M. H., Dieters, S., Woods, P., Thompson, C., and Duncan, R. C. 1999. Discovery of a magnetar associated with the soft gamma repeater SGR 1900+14. ApJ, 510, L115–L118.CrossRefGoogle Scholar
Kramer, M. 1998. Determination of the geometry of the PSR B1913+16 system by geodetic precession. ApJ, 509, 856–860.CrossRefGoogle Scholar
Kramer, M., and Stairs, I. H. 2008. The double pulsar. Ann. Rev. Astr. Ap., 46, 541–572.CrossRefGoogle Scholar
Kramer, M., Lange, C., Lorimer, D. R., Backer, D. C., Xilouris, K. M., Jessner, A., and Wielebinski, R. 1999. The characteristics of millisecond pulsar emission: III. From low to high frequencies. ApJ, 526, 957–975.CrossRefGoogle Scholar
Kramer, M., Johnston, S., and van Straten, W. 2002. High-resolution single-pulse studies of the Vela Pulsar. MNRAS, 334, 523–532.CrossRefGoogle Scholar
Kramer, M., Lyne, A. G., O’Brien, J. T., Jordan, C. A., and Lorimer, D. R. 2006a. A periodically active pulsar giving insight into magnetospheric physics. Science, 312, 549–551.CrossRefGoogle ScholarPubMed
Kramer, M., Stairs, I. H., Manchester, R. N., and 12 others. 2006b. Tests of general relativity from timing the Double Pulsar. Science, 314, 97–102.CrossRefGoogle ScholarPubMed
Krishnakumar, M. A., Maan, Yogesh, Joshi, B. C., and Manoharan, P. K. 2019. Multifrequency scatter-broadening evolution of pulsars. II. Scatter-broadening of nearby pulsars. ApJ, 878(2), 2.Google Scholar
Krishnamohan, S., and Downs, G. S. 1983. Intensity dependence of the pulse profile and polarization of the Vela pulsar. ApJ, 265, 372.CrossRefGoogle Scholar
Kronberg, P. P., and Newton-McGee, K. J. 2009. Remarkable symmetries in the Milky Way disk’s magnetic field. arXiv:0909.4753.Google Scholar
Kuiper, L., and Hermsen, W. 2009. High-energy characteristics of the schizophrenic pulsar PSR J1846-0258 in Kes 75. Multi-year RXTE and INTEGRAL observations crossing the magnetar-like outburst. A&A, 501(3), 1031–1046.Google Scholar
Kulkarni, S. R. 1986. Optical identification of binary pulsars: Implications for magnetic field decay in neutron stars. ApJ, 306, L85–L89.CrossRefGoogle Scholar
Kumar, H. S., and Safi-Harb, S. 2008. Variability of the high magnetic field X-ray pulsar PSR J1846-0258 associated with the supernova remnant Kes 75 as revealed by the Chandra X-ray observatory. ApJ, 678, L43–L46.CrossRefGoogle Scholar
Kuzmin, A. 2001. Scattering of the low frequency pulsar radiation. Astrophys. Space Sci., 278, 53–56.CrossRefGoogle Scholar
Kuzmin, A. D., Hamilton, P. A., Shitov, Y. P., McCulloch, P. M., McConnell, D., and Pugatchev, V. D. 2003. High temporal resolution observations of the pulsar microstructure at 102 MHz. MNRAS, 344, 1187–1192.CrossRefGoogle Scholar
Lai, D. 2001. Matter in strong magnetic fields. Rev. Modern Phys., 73(July), 629.CrossRefGoogle Scholar
Lam, M. T., Cordes, J. M., Chattergee, S., and 22 others. 2017. The NANOGrav nine-year data set: Excess noise in millisecond pulsar arrival times. ApJ, 834(1), 1.Google Scholar
Lampland, C. O. 1921. Observed changes in the structure of the Crab Nebula (NGC 1952). PASP, 33, 79–84.CrossRefGoogle Scholar
Lang, K. R. 1971. Interstellar scintillation of pulsar radiation. ApJ, 164, 249–264.CrossRefGoogle Scholar
Lange, C., Camilo, F., Wex, N., Kramer, M., Backer, D. C., Lyne, A. G., and Doroshenko, O. 2001. Precision timing measurements of PSR J1012+5307. MNRAS, 326, 274–282.CrossRefGoogle Scholar
Large, M. I., and Vaughan, A. E. 1971. A search of the Galactic plane for high dispersion pulsars. MNRAS, 151, 277–287.CrossRefGoogle Scholar
Large, M. I., Vaughan, A. E., and Wielebinski, R. 1968a. Pulsar searches at the Molonglo radio observatory. Nature, 220, 753–756.CrossRefGoogle Scholar
Large, M. I., Vaughan, A. E., and Mills, B. Y. 1968b. A pulsar supernova association. Nature, 220, 340–341.CrossRefGoogle Scholar
Laros, J. G., Fenimore, E. E., Klebesadel, R. W., and 14 others. 1987. A new type of repetitive behavior in a high-energy transient. ApJ, 320, L111–L115.CrossRefGoogle Scholar
Lattimer, J. M., and Prakash, M. 2001. Neutron star structure and the equation of state. ApJ, 550, 426–442.CrossRefGoogle Scholar
Lattimer, J. M. 2012. The nuclear equation of state and neutron star masses. ARNPS, 62(1), 485–515.Google Scholar
Lazaridis, K., Wex, N., Jessner, A., and 10 others. 2009. Generic tests of the existence of the gravitational dipole radiation and the variation of the gravitational constant. MNRAS, 400, 805–814.CrossRefGoogle Scholar
Lazio, T. J. W., and Cordes, J. M. 1998. Hyperstrong radio-wave scattering in the Galactic center. II. A likelihood analysis of free electrons in the Galactic Center. ApJ, 505, 715–731.CrossRefGoogle Scholar
Lazio, T. J. W., Bhaskaran, S., Cutler, C., Folkner, W. M., Park, R. S., Ellis, J. A., Ely, T., Taylor, S. R., and Vallisneri, M. 2018 (Aug.). Solar system ephemerides, pulsar timing, gravitational waves, & navigation. Pages 150–153 of: Weltevrede, P., Perera, B. B. P., Preston, L. L., and Sanidas, S. (eds), Pulsar Astrophysics the Next Fifty Years, vol. 337.Google Scholar
Lee, L. C. 1976. Strong scintillations in astrophysics. ApJ, 206, 744–752.CrossRefGoogle Scholar
Lee, L. C., and Jokipii, J. R. 1976. The irregularity spectrum in interstellar space. ApJ, 206, 735–743.CrossRefGoogle Scholar
Lentati, L., Shannon, R. M., Coles, W. A., and 80 others. 2016. From spin noise to systematics: Stochastic processes in the first International Pulsar Timing Array data release. MNRAS, 458(2), 2161–2187.CrossRefGoogle Scholar
Lesch, H., Jessner, A., Kramer, M., and Kunzl, T. 1998. On the possibility of curvature radiation from radio pulsars. A&A, 332, L21–L24.Google Scholar
Levin, L., Bailes, M., Bates, S., and 12 others. 2010. A radio-loud magnetar in X-ray quiescence. ApJ, 721, L33–L37.CrossRefGoogle Scholar
Lewandowski, W., Rozko, K., Kijak, J., Bhattacharyya, B., and Roy, J. 2015. The study of multi-frequency scattering of 10 radio pulsars. MNRAS, 454(3), 2517–2528.CrossRefGoogle Scholar
Lewin, W. H. G., and Joss, P. C. 1981. X-ray bursters and the X-ray sources of the galactic bulge. Space Sci. Rev., 28, 3–87.CrossRefGoogle Scholar
Lewin, W. H. G., and van Paradijs, J. 1986. Quasi-periodic oscillations, the ‘latest’ in X-ray astronomy. Comm. Astrophys., 11, 127–134.Google Scholar
Lewin, W. H. G., Doty, J., Clark, G. W., and 11 others. 1976. The discovery of a rapidly repetitive X-ray burst from a new source in Scorpius. ApJ, 207, L95–L99.CrossRefGoogle Scholar
Li, J., Torres, D. F., Lin, T. T., Grondin, M.-H., Kerr, M., Lemoine-Goumard, M., and de Ona Wilhelmi, E. 2018. Observing and modeling the gamma-ray emission from pulsar/pulsar wind nebula complex PSR J0205+6449/3C 58. ApJ, 858(2), 2.Google Scholar
Li, X. H., and Han, J. L. 2003. The effect of scattering on pulsar polarization angle. A&A, 410, 253–256.Google Scholar
Linares, M.. 2019. Super-massive neutron stars and compact binary millisecond pulsars. arXiv e-prints, Oct., arXiv:1910.09572.Google Scholar
Link, B. 2006. Incompatibility of long-period neutron star precession with creeping neutron vortices. A&A, 458, 881–884.Google Scholar
Link, B., and Epstein, R. I. 2001. Precession interpretation of the isolated pulsar PSR 182811. ApJ, 556, 392–398.CrossRefGoogle Scholar
Link, B., Epstein, R. I., and Baym, G. 1992. Postglitch behaviour of the Crab Pulsar: Evidence for external torque variations. ApJ, 390, L21–L22.CrossRefGoogle Scholar
Liu, K., Young, A., Wharton, R., and 20 others. 2019. Detection of pulses from the Vela pulsar at millimeter wavelengths with Phased ALMA. ApJ, 885(1), L10.CrossRefGoogle Scholar
Liu, Q. Z., van Paradijs, J., and van den Heuvel, E. P. J. 2005. High-mass X-ray binaries in the Magellanic Clouds. A&A, 442, 1135–1138.Google Scholar
Liu, Q. Z., van Paradijs, J., and van den Heuvel, E. P. J. 2006. Catalogue of high-mass X-ray binaries in the Galaxy (4th edition). A&A, 455, 1165–1168.Google Scholar
Liu, Q. Z., van Paradijs, J., and van den Heuvel, E. P. J. 2007. A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition). A&A, 469, 807–810.Google Scholar
Livingstone, M. A., Kaspi, V. M., Gavriil, F. P., Manchester, R. N., Gotthelf, E. V. G., and Kuiper, L. 2007. New phase-coherent measurements of pulsar braking indices. Astrophys. Space Sci., 308(Apr.), 317–323.CrossRefGoogle Scholar
Livingstone, M. A., Kaspi, V. M., and Gavriil, F. P. 2010. Timing behavior of the magnetically active rotation-powered pulsar in the supernova remnant Kesteven 75. ApJ, 710(2), 1710–1717.CrossRefGoogle Scholar
Lockhart, W., Gralla, S. E., Özel, F., and Psaltis, D. 2019. X-ray light curves from realistic polar cap models: Inclined pulsar magnetospheres and multipole fields. MNRAS, 490(2), 1774–1783.CrossRefGoogle Scholar
Löhmer, O., Kramer, M., Driebe, T., Jessner, A., Mitra, D., and Lyne, A. G. 2004a. The parallax, mass and age of the PSR J2145-0750 binary system. A&A, 426, 631–640.Google Scholar
Löhmer, O., Mitra, D., Gupta, Y., Kramer, M., and Ahuja, A. 2004b. The frequency evolution of interstellar pulse broadening from radio pulsars. A&A, 425, 569–575.Google Scholar
Löhmer, O., Jessner, A., Kramer, M., Wielebinski, R., and Maron, O. 2008. Observations of pulsars at 9 millimetres. A&A, 480, 623–628.Google Scholar
Lorimer, D. R. 2008. Binary and millisecond pulsars. Living Rev. Rel., 11.CrossRefGoogle ScholarPubMed
Lorimer, D. R. 2010. The Galactic pulsar population. Highlights of Astronomy, 15(Nov.), 807–807.Google Scholar
Lorimer, D. R. 2013. The galactic millisecond pulsar population. Pages 237–242 of: van Leeuwen, Joeri (ed), Neutron Stars and Pulsars: Challenges and Opportunities after 80 Years, vol. 291.Google Scholar
Lorimer, D. R., Bailes, M., Dewey, R. J., and Harrison, P. A. 1993. Pulsar statistics: The birthrate and initial spin periods of radio pulsars. MNRAS, 263, 403–415.CrossRefGoogle Scholar
Lorimer, D. R., Festin, L., Lyne, A. G., and Nicastro, L. 1995. Birth rate of millisecond pulsars. Nature, 376, 393.CrossRefGoogle Scholar
Lorimer, D. R., Bailes, M., and Harrison, P. A. 1997. Pulsar statistics IV: Pulsar velocities. MNRAS, 289, 592–604.CrossRefGoogle Scholar
Lorimer, D. R., Lyne, A. G., and Camilo, F. 1998. A search for pulsars in supernova remnants. A&A, 331, 1002–1010.Google Scholar
Lorimer, D. R., McLaughlin, M. A., Arzoumanian, Z., Xilouris, K. M., Cordes, J. M., Lommen, A. N., Fruchter, A. S., Chandler, A. M., and Backer, D. C. 2004. PSR J0609+2130: A disrupted binary pulsar? MNRAS, 347, L21–L25.CrossRefGoogle Scholar
Lorimer, D. R., Stairs, I. H., Freire, P. C., and 33 others. 2006a. Arecibo pulsar survey using ALFA. II. The young, highly relativistic binary pulsar J1906+0746. ApJ, 640, 428–434.CrossRefGoogle Scholar
Lorimer, D. R., Faulkner, A. J., Lyne, A. G, and 11 others. 2006b. The Parkes Multibeam pulsar survey – VI. Discovery and timing of 142 pulsars and a Galactic population analysis. MNRAS, 372, 777–800.CrossRefGoogle Scholar
Lorimer, D. R., Bailes, M., McLaughlin, M. A., Narkevic, D. J., and Crawford, F. 2007. A bright millisecond radio burst of extragalactic origin. Science, 318, 777.CrossRefGoogle ScholarPubMed
Lu, F. J., Wang, Q. D., Aschenbach, B., Durouchoux, P., and Song, L. M. 2002. Chandra observation of supernova remnant G54.1+0.3: A close cousin of the Crab Nebula. ApJ, 568, L49–L52.CrossRefGoogle Scholar
Luken, K. J., Filipovic, M. D., and 18 others. 2020. Radio observations of supernova remnant G1.9+0.3. MNRAS, 492(2), 2606–2621.CrossRefGoogle Scholar
Lundgren, S. C., Cordes, J. M., Ulmer, M., Matz, S. M., Lomatch, S., Foster, R. S., and Hankins, T. 1995. Giant pulses from the Crab Pulsar: A joint radio and gamma-ray study. ApJ, 453(Nov.), 433.CrossRefGoogle Scholar
Lundmark, K. 1921. Suspected new stars recorded in old chronicles and among recent meridian observations. PASP, 33, 225–238.CrossRefGoogle Scholar
Lynch, R. S. 2018 (Aug.). The Green Bank North Celestial Cap pulsar survey: Status and future. Pages 13–16 of: Weltevrede, P., Perera, B. B. P., Preston, L. L., and Sanidas, S. (eds), Pulsar Astrophysics the Next Fifty Years, vol. 337.Google Scholar
Lynch, R. S., Ransom, S. M., Freire, P. C. C., and Stairs, I. H. 2011. Six new recycled globular cluster pulsars discovered with the Green Bank Telescope. arXiv:1101.1467.CrossRefGoogle Scholar
Lynch, R. S., Swiggum, J. K., Kondratiev, V. I., and 37 others. 2018. The Green Bank North Celestial Cap pulsar survey. III. 45 new pulsar timing solutions. ApJ, 859(2), 2.Google Scholar
Lynden-Bell, D. 1969. Galactic nuclei as collapsed old quasars. Nature, 223(5207), 690–694.CrossRefGoogle Scholar
Lyne, A. G. 1971. The comparative properties of the pulsars. Pages 182–194 of: Davies, R. D., and Smith, F. G. (eds), IAU Symp. 46. Reidel.Google Scholar
Lyne, A. G. 1984. Orbital inclination and mass of the binary pulsar PSR 0655+64. Nature, 310, 300–302.CrossRefGoogle Scholar
Lyne, A. G. 1987. A massive glitch in an old pulsar. Nature, 326, 569–571.CrossRefGoogle Scholar
Lyne, A. G., and Ashworth, M. 1983. The effect of nulls upon subpulse drift in PSRs 0809+74 and 0818-13. MNRAS, 204, 519–536.CrossRefGoogle Scholar
Lyne, A. G., and Lorimer, D. R. 1994. High birth velocities of radio pulsars. Nature, 369, 127–129.CrossRefGoogle Scholar
Lyne, A. G., and Manchester, R. N. 1988. The shape of pulsar radio beams. MNRAS, 234, 477–508.CrossRefGoogle Scholar
Lyne, A. G., and Rickett, B. J. 1968. Measurements of the pulse shape and spectra of the pulsating radio sources. Nature, 218, 326–330.CrossRefGoogle Scholar
Lyne, A. G., and Smith, F. G. 1968. Linear polarization in pulsating radio sources. Nature, 218, 124–126.CrossRefGoogle Scholar
Lyne, A. G., and Smith, F. G. 1982. Interstellar scintillation and pulsar velocities. Nature, 298, 825–827.CrossRefGoogle Scholar
Lyne, A. G., and Thorne, D. J. 1975. Anomalous scattering in the Crab Nebula. MNRAS, 172, 97–108.CrossRefGoogle Scholar
Lyne, A. G., Smith, F. G., and Graham, D. A. 1971. Characteristics of the radio pulses from the pulsars. MNRAS, 153, 337–382.CrossRefGoogle Scholar
Lyne, A. G., Anderson, B., and Salter, M. J. 1982. The proper motions of 26 pulsars. MNRAS, 201, 503–520.CrossRefGoogle Scholar
Lyne, A. G., Manchester, R. N., and Taylor, J. H. 1985. The Galactic population of pulsars. MNRAS, 213, 613–639.CrossRefGoogle Scholar
Lyne, A. G., Brinklow, A., Middleditch, J., Kulkarni, S. R., Backer, D. C., and Clifton, T. R. 1987. The discovery of a millisecond pulsar in the globular cluster M28. Nature, 328, 399–401.CrossRefGoogle Scholar
Lyne, A. G., Pritchard, R. S., and Smith, F G. 1988a. Crab Pulsar timing 1982-1987. MNRAS, 233, 667–676.CrossRefGoogle Scholar
Lyne, A. G., Biggs, J. D., Brinklow, A., Ashworth, M., and McKenna, J. 1988b. Discovery of a binary millisecond pulsar in the globular cluster M4. Nature, 332, 45–47.CrossRefGoogle Scholar
Lyne, A. G., Manchester, R. N., D’Amico, N., Staveley-Smith, L., Johnston, S., Lim, J., Fruchter, A. S., Goss, W. M., and Frail, D. 1990. An eclipsing millisecond pulsar in the globular cluster Terzan 5. Nature, 347, 650–652.CrossRefGoogle Scholar
Lyne, A. G., Pritchard, R. S., and Smith, F. G. 1993. 23 years of Crab Pulsar rotational history. MNRAS, 265, 1003–1012.CrossRefGoogle Scholar
Lyne, A. G., Pritchard, R. S., Graham-Smith, F., and Camilo, F. 1996. Very low braking index for the Vela Pulsar. Nature, 381, 497–498.CrossRefGoogle Scholar
Lyne, A. G., Manchester, R. N., Lorimer, D. R., Bailes, M., D’Amico, N., Tauris, T. M., Johnston, S., Bell, J. F., and Nicastro, L. 1998. The Parkes Southern pulsar survey – II. Final results and population analysis. MNRAS, 295, 743–755.CrossRefGoogle Scholar
Lyne, A. G., Camilo, F., Manchester, R. N., and 8 others. 2000. The Parkes Multibeam pulsar survey: PSR J1811-1736 – A pulsar in a highly eccentric binary system. MNRAS, 312, 698–702.CrossRefGoogle Scholar
Lyne, A. G., Pritchard, R. S., and Graham-Smith, F. 2001. Pulsar reflections in the Crab Nebula. MNRAS, 321, 67–70.CrossRefGoogle Scholar
Lyne, A. G., Burgay, M., Kramer, M., and 9 others. 2004. A double-pulsar system: A rare laboratory for relativistic gravity and plasma physics. Science, 303, 1153–1157.CrossRefGoogle ScholarPubMed
Lyne, A. G., Hobbs, G., Kramer, M., Stairs, I., and Stappers, B. 2010. Switched magnetospheric regulation of pulsar spin-down. Science, 329, 408.CrossRefGoogle ScholarPubMed
Lyne, A. G., Jordan, C. A., Graham-Smith, F., Espinoza, C. M., Stappers, B. W., and Weltevrede, P. 2015. 45 years of rotation of the Crab Pulsar. MNRAS, 446(Jan.), 857–864.CrossRefGoogle Scholar
Lyne, A. G., Stappers, B. W., Freire, P. C. C., and 31 others. 2017. Two long-term intermittent pulsars discovered in the PALFA survey. ApJ, 834(1), 1.Google Scholar
Lyne, A., Levin, L., Stappers, B., Mickaliger, M., Desvignes, G., and Kramer, M. 2018. Intense radio flare from the magnetar XTE J1810-197. The Astronomer’s Telegram, 12284(Dec.), 1.Google Scholar
Ma, C., Arias, E. F., Bianco, G., and 30 others. 2009. The second realization of the international celestial reference frame by very long baseline interferometry. IERS Technical Note, 35(Jan.), 1.Google Scholar
Maciesiak, K., Gil, J., and Ribeiro, V. A. R. M. 2011. On the pulse-width statistics in radio pulsars – I. Importance of the interpulse emission. MNRAS, 414(2), 1314–1328.CrossRefGoogle Scholar
Macquart, J. P., Prochaska, J. X., McQuinn, M., and 13 others. 2020. A census of baryons in the Universe from localized fast radio bursts. Nature, 581(7809), 391–395.CrossRefGoogle ScholarPubMed
Malov, I. F., and Timirkeeva, M. A. 2019. On X-ray emission of radio pulsars. MNRAS, 485(4), 5319–5328.CrossRefGoogle Scholar
Manchester, R. N., and Lyne, A. G. 1977. Pulsar interpulses – Two poles or one? MNRAS, 181, 761–767.CrossRefGoogle Scholar
Manchester, R. N., and Peterson, B. A. 1996. A search for optical pulsations in SN 1987A. ApJ, 456, L107–L109.Google Scholar
Manchester, R. N., and Taylor, J. H. 1981. Observed and derived parameters for 330 pulsars. AJ, 86, 1953–1973.CrossRefGoogle Scholar
Manchester, R. N., Taylor, J. H., and Van, Y.-Y. 1974. Detection of pulsar proper motion. ApJ, 189, L119–L122.CrossRefGoogle Scholar
Manchester, R. N., Taylor, J. H., and Huguenin, G. R. 1975. Observations of pulsar radio emission II. Polarisation of individual radio pulses. ApJ, 196, 83–102.CrossRefGoogle Scholar
Manchester, R. N., Lyne, A. G., Taylor, J. H., Durdin, J. M., Large, M. I., and Little, A. G. 1978. The second Molonglo pulsar survey – Discovery of 155 pulsars. MNRAS, 185, 409–421.CrossRefGoogle Scholar
Manchester, R. N., Lyne, A. G., Robinson, C., D’Amico, N., Bailes, M., and Lim, J. 1991. Discovery of ten millisecond pulsars in the globular cluster 47 Tucanae. Nature, 352, 219–221.CrossRefGoogle Scholar
Manchester, R. N., Lyne, A. G., D’Amico, N., Bailes, M., Johnston, S., Lorimer, D. R., Harrison, P. A., Nicastro, L., and Bell, J. F. 1996. The Parkes southern pulsar survey I. Observing and data analysis systems and initial results. MNRAS, 279, 1235–1250.CrossRefGoogle Scholar
Manchester, R. N., Lyne, A. G., Camilo, F., and 9 others. 2001. The Parkes multi-beam pulsar survey – I. Observing and data analysis systems, discovery and timing of 100 pulsars. MNRAS, 328, 17–35.CrossRefGoogle Scholar
Manchester, R. N., Bell, J. F., Camilo, F., and 9 others. 2002. Young pulsars from the Parkes multibeam pulsar survey and their associations. ASP Conf. Ser., 271, 31.Google Scholar
Manchester, R. N., Fan, G., Lyne, A. G., Kaspi, V. M., and Crawford, F. 2006. Discovery of 14 radio pulsars in a survey of the Magellanic Clouds. ApJ, 649, 235–242.CrossRefGoogle Scholar
Mao, S. A., Gaensler, B. M., Haverkorn, M., Zweibel, E. G., Madsen, G. J., McClure-Griffiths, N. M., Shukurov, A., and Kronberg, P. P. 2010. A survey of extragalactic Faraday rotation at high Galactic latitude: The vertical magnetic field of the Milky Way toward the Galactic poles. ApJ, 714, 1170–1186.CrossRefGoogle Scholar
Maoz, D., Mannucci, F., Li, W., Filippenko, A. V., Della Valle, M., and Panagia, N. 2011. Nearby supernova rates from the Lick observatory supernova search – IV. A recovery method for the delay-time distribution. MNRAS, 412(3), 1508–1521.CrossRefGoogle Scholar
Markwardt, C. B., Swank, J. H., Strohmayer, T. E., Zand, J. J., and Marshall, F. E. 2002. Discovery ofa second millisecond accreting pulsar: XTE J1751-305. ApJ, 575, L21–L24.CrossRefGoogle Scholar
Marsh, T. R., Gänsicke, B. T., Hümmerich, S., and 23 others. 2016. A radio-pulsing white dwarf binary star. Nature, 537(7620), 374–377.CrossRefGoogle ScholarPubMed
Martinez, J. G., Stovall, K., Freire, P. C. C., Deneva, J. S., Jenet, F. A., McLaughlin, M. A., Bagchi, M., Bates, S. D., and Ridolfi, A. 2015. Pulsar J0453+1559: A double neutron star system with a large mass asymmetry. ApJ, 812(2), 2.Google Scholar
Martinez, J. G., Gentile, P., Freire, P. C. C., Stovall, K., Deneva, J. S., Desvignes, G., Jenet, F. A., McLaughlin, M. A., Bagchi, M., and Devine, T. 2019. The discovery of six recycled pulsars from the Arecibo 327 MHz drift-scan pulsar survey. ApJ, 881(2), 2.Google Scholar
Matheson, H., and Safi-Harb, S. 2010. The Plerionic supernova remnant G21.5-0.9 powered by PSR J1833-1034: New spectroscopic and imaging results revealed with the Chandra X-ray observatory. ApJ, 724, 572–587.CrossRefGoogle Scholar
Matsakis, D. N., Taylor, J. H., Eubanks, T. M., and Marshall, T. 1997. A statistic for describing pulsar and clock stabilities. A&A, 326, 924–928.Google Scholar
Mayer-Hasselwander, H. A., Bennett, K., Bignami, G. F., and 13 others. 1982. Large-scale distribution of galactic gamma radiation observed by COS-B. A&A, 105(1), 164–175.Google Scholar
Maza, J., and van den Bergh, S. 1976. Statistics of extragalactic supernovae. ApJ, 204, 519–529.CrossRefGoogle Scholar
Mazets, E. P., Golenetskii, S. V., and Gur’yan, Yu. A. 1979. Soft gamma-ray bursts from the source B1900+14. Sov. Astron. Lett., 5, 343–344.Google Scholar
Mazets, E. P., Golenskii, S. V., Aptekar, R. L., Guryan, Y. A., and Ilyinskii, V. N. 1981. Cyclotron and annihilation lines in gamma-ray bursts. Nature, 290, 378–382.CrossRefGoogle Scholar
McCarthy, D. D., and Petit, G (eds). 2004. IERS Conventions 2003, IERS Technical Note 32. Frankfurt am Main: Verlag des Bundesamts für Kartographie und Geodäsie.Google Scholar
McConnell, D., McCulloch, P. M., Hamilton, P. A., Ables, J. G., Hall, P. J., Jacka, C. E., and Hunt, A. J. 1991. Radio pulsars in the Magellanic Clouds. MNRAS, 249, 654–657.CrossRefGoogle Scholar
McCulloch, P. M., Hamilton, P. A., Royle, G. W. R., and Manchester, R. N. 1983. Daily observations of a large period jump of the Vela Pulsar. Nature, 302, 319–321.CrossRefGoogle Scholar
McKee, J. W., Janssen, G. H., Stappers, B. W., and 17 others. 2016. A glitch in the millisecond pulsar J0613-0200. MNRAS, 461(3), 2809–2817.CrossRefGoogle Scholar
McKee, J. W., Lyne, A. G., Stappers, B. W., Bassa, C. G., and Jordan, C. A. 2018. Temporal variations in scattering and dispersion measure in the Crab Pulsar and their effect on timing precision. MNRAS, 479(3), 4216–4224.CrossRef