Abbott, B. P. et al. 2016, Observation of Gravitational Waves from a Binary Black Hole Merger, Phys. Rev. Let., 116, 061102.Google Scholar

Adams, W. S. 1941, Some Results with the COUDÉ Spectrograph of the Mount Wilson Observatory, ApJ, 93, 11.Google Scholar

Akiyama, K. et al. 2019, First M87 Event Horizon Telescope Results. II. Array and Instrumentation, ApJ, 875, L2.Google Scholar

Akiyama, K. et al. 2022, First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way, ApJ, 930, L12.Google Scholar

Alexander, F. E. S. 1945, Report on the Investigation of the “Norfolk Island Effect,” Radio Development Laboratory, Department of Scientific & Industrial Research.Google Scholar

Alexander, F. E. S. 1946, The Sun’s Radio Energy, Radio Electron., 1(1), 16.Google Scholar

Alfvén, H. and Herlofson, N. 1950, Cosmic Radiation and Radio Stars, Phys. Rev., 78, 616.Google Scholar

Allen, L. R. et al. 1962a, Observations of 384 Radio Sources at a Frequency of 158 Mc/s with a Long Baseline Interferometer, MNRAS, 124, 477.CrossRefGoogle Scholar

Allen, L. R. et al. 1962b, An Analysis of the Angular Sizes of Radio Sources, MNRAS, 125, 57.Google Scholar

Alpher, R. A. and Herman, R. C. 1948, Evolution of the Universe, Nature, 162, 774.Google Scholar

Alpher, R. A. and Herman, R. C. 1949, Remarks on the Evolution of the Expanding Universe, Phys. Rev., 75, 1089.Google Scholar

Alpher, R. A. and Herman, R. C. 1951, Neutron-Capture Theory of Element Formation in an Expanding Universe, Phys. Rev., 84, 60.CrossRefGoogle Scholar

Alpher, R. A. and Herman, R. C. 1988, Reflections on Early Work on “Big Bang” Cosmology, Phys. Today, 41(8), 24.Google Scholar

Alpher, R. A. and Herman, R. C. 1990, Early Work on “Big-Bang” Cosmology and the Cosmic Blackbody Radiation. In Modern Cosmology in Retrospect, ed. Bertotti, B., Balbinot, R., and Bergia, S. (Cambridge: Cambridge University Press), 129.Google Scholar

Alpher, R. A., Bethe, H. A., and Gamow, G. 1948, The Origin of Chemical Elements, Phys. Rev., 73, 803.CrossRefGoogle Scholar

Alpher, R. A., Follin, J. W., and Herman, R. C. 1953, Physical Conditions in the Initial Stages of the Expanding Universe, Phys. Rev., 92, 1347.CrossRefGoogle Scholar

Alpher, V. 2014, Ralph A. Alpher, George Antonovich Gamow, and the Prediction of the Cosmic Microwave Background Radiation, Asian J. Phys., 23, 17.Google Scholar

Alsop, L. E. et al. 1958, Observations Using a Maser Radiometer at 3-cm Wave Length, AJ, 63, 30.CrossRefGoogle Scholar

Altenhoff, W. et al. 1988, First Radio Astronomical Estimate of the Temperature of Pluto, A&A, 190, L15.Google Scholar

Altschuler, D. R. 2002, The National Astronomy and Ionospheric Center’s (NAIC) Arecibo Observatory in Puerto Rico. In ASPC 278, Single–Dish Radio Astronomy: Techniques and Applications, ed. Stanimirovic, S. et al. (San Francisco: Astronomical Society of the Pacific), 1.Google Scholar

Ambartsumian, V. 1958, On the Evolution of Galaxies. In La Structure et l’Evolution de l’Univers, ed. Stoops, R. (Brussels: Coudenberg), 266.Google Scholar

Amiri, M. et al. 2022, An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment, ApJS, 261, 29.Google Scholar

Anderson, B., Palmer, H. P., and Rowson, B. 1962, Brightness Distribution of the Radio Source 14N5A, Nature, 195, 165.Google Scholar

Antoniadis, J. et al. 2013, A Massive Pulsar in a Compact Relativistic Binary, Science, 340, 448.Google Scholar

Antoniadis, J. et al. 2022, The International Pulsar Timing Array Second Data Release: Search for an Isotropic Gravitational Wave Background, MNRAS, 510, 4873.Google Scholar

Appleton, E. 1945, Departure of Long-Wave Solar Radiation from Black-Body Intensity, Nature, 156, 534.Google Scholar

Appleton, E. and Hey, J. S. 1946, Solar Radio Noise, Phil. Mag., 7, 73.CrossRefGoogle Scholar

Arp, H. C. 1987, Quasars, Redshifts, and Controversies (Berkeley: Interstellar Media).Google Scholar

Arp, H. C. 1998, Seeing Red: Redshifts, Cosmology, and Academic Science (Montreal: Apeiron).Google Scholar

Baade, W. and Minkowski, R. 1954, Identification of the Radio Sources in Cassiopeia, Cygnus A, and Puppis A, ApJ, 119, 206.Google Scholar

Baade, W. and Zwicky, F. 1934, Remarks on Super-Novae and Cosmic Rays, Phys. Rev., 46, 76.CrossRefGoogle Scholar

Babcock, H. W. 1939, The Rotation of the Andromeda Nebula, Lick Observatory Bulletin, No. 498.Google Scholar

Backer, D. C. et al. 1983, A Millisecond Pulsar, Nature, 300, 615.Google Scholar

Bagchi, M., Nieves, A. C., and McLaughlin, M. 2012, A Search for Dispersed Radio Bursts in Archival Parkes Multibeam Pulsar Survey Data, MNRAS, 425, 250.Google Scholar

Bailes, M., Lyne, A., and Shemar, S. I. 1991a, A Planet Orbiting the Neutron Star PSR1829–10, Nature, 352, 311.CrossRefGoogle Scholar

Bailes, M., Lyne, A., and Shemar, S. 1991b, Radio Astronomers Claim Discovery of First Planet Outside Solar System, J. Brit. Astron. Assoc., 101, 256.Google Scholar

Balick, B. 2005, The Discovery of Sgr A*. In The New Astronomy: Opening the Electromagnetic Window and Expanding Our View of Planet Earth, ed. Orchiston, W. (Dordrecht: Springer), 183.Google Scholar

Balick, B. and Brown, R. L. 1974, Intense Sub-Arcsecond Structure in the Galactic Center, ApJ, 194, 265.CrossRefGoogle Scholar

Bannister, K. W. et al. 2019, A Single Fast Radio Burst Localized to a Massive Galaxy at Cosmological Distance, Science, 365, 565.Google Scholar

Barnothy, J. M. 1963, Astronomical Consequences of the FIB Theory, PASP, 75, 430.Google Scholar

Barnothy, J. M. 1965, Quasars and the Gravitational Image Intensifier, AJ, 70, 666.Google Scholar

Barnothy, J. M. 1966a, Two Observational Tests: Are Quasars Super-Luminous Objects or Optical Effects?, AJ, 71, 154.Google Scholar

Barnothy, J. M. 1966b, An Observational Test of the Hypothesis that Quasars Are Produced by Gravitational Lenses, Obs., 86, 115.Google Scholar

Barnothy, J. M. and Barnothy, M. F. 1966, Apparent Brightness of the Deflector Galaxy of Quasars Produced through Gravitational Lenses, AJ, 71, 378.Google Scholar

Barnothy, J. M. and Barnothy, M. F. 1967, Observations Supporting the Gravitational Lens Explanation of Quasars, AJ, 72, 291.Google Scholar

Barnothy, J. M. and Barnothy, M. F. 1968, Galaxies as Gravitational Lenses, Science, 162, 348.Google Scholar

Barnothy, J. M. and Barnothy, M. F. 1969a, Anomalous Hubble Plot of Quasi-stellar Objects, Nature, 222, 759.CrossRefGoogle Scholar

Barnothy, J. M. and Barnothy, M. F. 1969b, Concentration of QSO’s around z=2 Redshift, BAAS, 1, 181.Google Scholar

Barnothy, J. M. and Barnothy, M. F. 1971, Rapid Differential Proper Motion in the Radio Fine Structure of 3C 279, BAAS, 3, 472.Google Scholar

Barnothy, J. M. and Barnothy, M. F. 1972, Expected Density of Gravitational-Lens Quasars, ApJ, 174, 477.Google Scholar

Barrett, A. H. 1965, Passive Radio Observations of Mercury, Venus, Mars, Saturn, and Uranus, Radio Science, 69D, 1565.Google Scholar

Barrett, A. H. 1984, The Beginnings of Molecular Radio Astronomy. In Serendipitous Discoveries in Radio Astronomy, ed. Kellermann, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 280.Google Scholar

Barrett, A. H. and Lilley, A. E. 1957, A Search for the 18-cm Line of OH in the Interstellar Medium, AJ, 62, 5.Google Scholar

Barrett, A. H. and Rogers, A. E. E. 1966, Observations of Circularly Polarized OH Emission and Narrow Spectral Features, Nature, 210, 188.Google Scholar

Barrett, A. H., Schwartz, P. R., and Waters, J. W. 1971, Detection of Methyl Alcohol in Orion at a Wavelength of ~1 Centimeter, ApJ, 168, L102.CrossRefGoogle Scholar

Bastian, T. S., Benz, A. O., and Gary, D. E. 1998, Radio Emission from Solar Flares, ARAA, 36, 131.Google Scholar

Bay, Z. 1946, Reflection of Microwaves from the Moon, Hungarian Physics Acta, 1, 1.Google Scholar

Beck, A. 1984, Personal Recollections of Karl Jansky. In Serendipitous Discoveries in Radio Astronomy, ed. Kellermann, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 32.Google Scholar

Bell, S. J. 1968, The Measurement of Radio Source Diameters Using a Diffraction Method, PhD Dissertation, Cambridge University.Google Scholar

Bell, S. J. and Hewish, A. 1967, Angular Size and Flux Density of the Small Source in the Crab Nebula at 81.5 Mc/s, Nature, 213, 1214.Google Scholar

Bell Burnell, S. J. 1977, Petit Four. In Proceedings of the 8th Texas Symposium on Relativistic Astrophysics, ed. M. D. Papagiannis. Annals of the New York Academy of Science, 302, 685, reprinted under the title “Little Green Men, White Dwarfs or Pulsars,” Cosmic Search, 1, 16.Google Scholar

Bell Burnell, S. J. 1984, The Discovery of Pulsars. In Serendipitous Discoveries in Radio Astronomy, ed. Kellermann, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 160.Google Scholar

Bell Burnell, S. J. 2015, Reflections on the Discovery of Pulsars. Paper presented at IAU General Assembly, Honolulu, HI, available at: https://rahist.nrao.edu/1-Bell_Hawaii_PSR_Refln.pptx (last accessed 23 November 2022).Google Scholar

Bennett, A. S. 1962, The Revised 3C Catalogue of Radio Sources, MNRAS, 68, 162.Google Scholar

Berge, G. L. 1966, An Interferometric Study of Jupiter’s Decimeter Radio Emission, ApJ, 146, 767.CrossRefGoogle Scholar

Berge, G. L. 1968, Recent Observations of Saturn, Uranus, and Neptune at 3.12 cm, Astrophys. Lett., 2, 127.Google Scholar

Berger, E. et al., 2001, Discovery of Radio Emission from the Brown Dwarf LP944–20, Nature, 410, 338.Google Scholar

Bethe, H. 2003, My Life in Astrophysics, ARAA, 41, 1.Google Scholar

Bigg, E. K. 1964, Influence of the Satellite Io on Jupiter’s Decametric Emission, Nature, 203, 1008.Google Scholar

Blaauw, A. et al. 1960, The New I.A.U. System of Galactic Coordinates (1958 Revision), MNRAS, 121, 123.Google Scholar

Blackett, P. M. S. and Lovell, A. C. B. 1941, Radio Echoes and Cosmic Ray Showers, Proc. R. Soc. A, 177, 183.Google Scholar

Blandford, R. D. (ed.) 2010, New Worlds, New Horizons (Washington: NAS Press).Google Scholar

Bochenek, C. D. et al. 2020, A Fast Radio Burst Associated with a Galactic Magnetar, Nature, 587, 59.CrossRefGoogle ScholarPubMed

Boischot, A. 1957, Caractѐres d’un Type d’Émission Herzienne Associé à Certaines Éruptions Chromosphériques, Comptes Rendus, 244, 1326 [Characteristics of a Herzian Emission Type Associated with Certain Chromospheric Eruptions].Google Scholar

Boischot, A. and Denisse, J.-F. 1957, Les Émissions de Type IV et l’Origine des Rayons Cosmiques Associés aux Éruptions Chromosphériques, Comptes Rendus, 245, 2194 [Type IV Emissions and the Origin of Cosmic Rays Associated with Chromospheric Eruptions].Google Scholar

Bolton, J. G. 1948, Discrete Sources of Galactic Radio Frequency Noise, Nature, 162, 141.Google Scholar

Bolton, J. G. 1955, Australian Work on Radio Stars, Vistas Astron., 1, 568.Google Scholar

Bolton, J. G. 1960, The Discrete Sources of Cosmic Radiation, Introductory Talk at the URSI General Assembly, London, reprinted in Observations of the California Institute of Technology Radio Observatory, no. 5.Google Scholar

Bolton, J. G. 1973, Prospects of Astronomy in Australia, Nature, 246, 282.Google Scholar

Bolton, J. G. 1982, Radio Astronomy at Dover Heights, Proc. Astron. Soc. Austrl., 4, 349. Reprinted in Kellermann and Sheets 1984, p. 312.Google Scholar

Bolton, J. G. 1990, The Fortieth Anniversary of Extragalactic Radio Astronomy: Radiophysics in Exile, Pub. Astron. Soc. Austrl., 8, 381.Google Scholar

Bolton, J. G. and Stanley, G. J. 1948a, Variable Source of Radio Frequency Radiation in the Constellation of Cygnus, Nature, 161, 312.Google Scholar

Bolton, J. G. and Stanley, G. J. 1948b, Observations on the Variable Source of Cosmic Radio Frequency Radiation in the Constellation of Cygnus, Austrl. J. Sci. Res. A, 1, 58.Google Scholar

Bolton, J. G. and Stanley, G. J. 1949, The Position and Probable Identification of the Source of Galactic Radio-Frequency Radiation Taurus-A, Austrl. J. Sci. Res. A, 2, 139.Google Scholar

Bolton, J. G. and Westfold, K. C. 1951, Galactic Radiation at Radio Frequencies: IV. The Distribution of Radio Stars in the Galaxy, Austrl. J. Sci. Res., 4, 476.Google Scholar

Bolton, J. G., Clarke, M. E., and Ekers, R. D. 1965, Identification of Extragalactic Radio Sources Between Declinations ‒20° and ‒44°, Austrl. J. Phys., 18, 627.Google Scholar

Bolton, J. G., Gardner, F. F., and Mackey, M. B. 1963, A Radio Source with a Very Unusual Spectrum, Nature, 199, 682.Google Scholar

Bolton, J. G., Gardner, F. F., and Mackey, M. B. 1964, The Parkes Catalogue of Radio Sources, Declination Zone ‒20° to ‒60°, Austrl. J. Phys., 17, 340.Google 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.Google Scholar

Bolton, J. G., Stanley, G. J., and Slee, O. B. 1954, Galactic Radiation at Radio Frequencies. VIII. Discrete Sources at 100 Mc/s between Declinations +50° and ‒50°, Austrl. J. Phys., 7, 110.Google Scholar

Bolton, J. G. et al. 1964a, Observations of OH Absorption Lines in the Radio Spectrum of the Galactic Centre, Nature, 201, 279.Google Scholar

Bolton, J. G. et al. 1964b, Distribution and Motions of OH Near the Galactic Centre, Nature, 204, 30.Google Scholar

Bolton, J. G. et al. 1965, Identifications of Six Faint Radio Sources with Quasi-Stellar Objects, ApJ, 142, 1289.Google Scholar

Bondi, H. and Gold, T. 1948, MNRAS, 108, 252.Google Scholar

Bosma, A. 1978, The Distribution and Kinematics of Neutral Hydrogen in Spiral Galaxies of Various Morphological Types, PhD Thesis, Groningen University.Google Scholar

Bosma, A. and van der Kruit, P. C. 1979, The Local Mass-to-Light Ratio in Spiral Galaxies, A&A, 79, 281.Google Scholar

Bourke, T. et al. (eds.) 2015, Advancing Astrophysics with the Square Kilometre Array, Proceedings of Science (Manchester: SKA Organization), available at: www.skatelescope.org/books/ (last accessed 30 November 2022).Google Scholar

Bowen, E. G. 1987, Radar Days (Bristol: A. Hilger).Google Scholar

Bowles, K. L. 1958, Observation of Vertical-Incidence Scatter from the Ionosphere at 41 Mc/sec., Phys. Rev. Let., 1, 454.Google Scholar

Bowman, J. D. et al. 2018, An Absorption Profile Centred at 78 Megahertz in the Sky-Averaged Spectrum, Nature, 555, 67.Google Scholar

Bown, R. 1927, Transatlantic Radio Telephony, Bell Syst. Tech. J., 6, 248.CrossRefGoogle Scholar

Boynton, P. E. and Partridge, R. B. 1973, Fine-Scale Anisotropy of the Microwave Background: An Upper Limit at λ = 3.5 Millimeters, ApJ, 181, 243.Google Scholar

Bracewell, R. N. 1960, Communication from Superior Galactic Communities, Nature, 186, 670.Google Scholar

Bracewell, R. N. 2000, The Fourier Transform and its Applications, 3rd ed. (New York: McGraw Hill).Google Scholar

Bracewell, R. N. 2002, The Discovery of Strong Extragalactic Polarization Using the Parkes Radio Telescope, J. Astron. Hist. Heritage, 5, 107.Google Scholar

Bracewell, R. N. 2005, Radio Astronomy at Stanford, J. Astron. Hist. Heritage, 8, 75.CrossRefGoogle Scholar

Bracewell, R. N. and Swarup, G. 1961, The Stanford Microwave Spectro Heliograph Antenna, A Microsteradian Pencil Beam Antenna, IRE Tr. Ant. Prop., AP-9, 22.Google Scholar

Bracewell, R. N., Cooper, B. F. C., and Cousins, T. E. 1962, Polarization in the Central Component of Centaurus A, Nature, 195, 1289.Google Scholar

Brans, C. and Dicke, R. H. 1961, Mach’s Principle and a Relativistic Theory of Gravitation, Phys. Rev., 124, 924.CrossRefGoogle Scholar

Briggs, F. H. and Drake, F. D. 1972, Interferometric Observations of Mars at 21-cm Wavelength, Icarus, 17, 543.Google Scholar

Broderick, J. 1984, The Buffalo Syndrome. In Serendipitous Discoveries in Radio Astronomy, ed. Kellermann, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 221.Google Scholar

Broten, N. W. 1988, Early Days of Canadian Long-Baseline Interferometry: Reflections and Reminiscences, JRASC, 82, 233.Google Scholar

Brown, R. L. et al. 1978, Radio Recombination Lines, ARAA, 16, 445.Google Scholar

Buderi, C. 1996, The Invention that Changed the World (New York: Simon & Schuster).Google Scholar

Buhl, D. et al. 1969, An Investigation of the Spectra and Time Variations of Galactic Water-Vapor Sources, ApJ, 158, 97.Google Scholar

Burbidge, G. R. 1959a, The Theoretical Explanation of Radio Emission. In IAU Symposium No. 9, Paris Symposium on Radio Astronomy, ed. Bracewell, R. N. (Stanford: Stanford University Press), 541.Google Scholar

Burbidge, G. R. 1959b, Estimates of the Total Energy in Particles and Magnetic Field in the Non-Thermal Radio Sources, ApJ, 129, 849.Google Scholar

Burbidge, G. R. 1968, The Distribution of Redshifts in Quasi-Stellar Objects, N-Systems and Some Radio and Compact Galaxies, ApJ, 7, 41.Google Scholar

Burbidge, G. R. 1971, Was There Really a Big Bang?, Nature, 233, 36.Google Scholar

Burbidge, G. R. 1975, On the Masses and Relative Motions of Galaxies, ApJ, 196, L7.Google Scholar

Burbidge, G. R. and Burbidge, E. M. 1967, Quasi-stellar Objects (San Francisco: Freeman).Google Scholar

Burbidge, G. R. and Narlikar, J. V. 1976, The Log N-Log S Curve for 3CR Radio Galaxies and the Problem of Identifying Faint Radio Galaxies, ApJ, 205, 329.Google Scholar

Burke, B. F. 2006, Planetary Radio Astronomy, Fifty Years Ago and Fifty Years Hence. In Planetary Radio Emissions VI, Proceedings of the 6th International Workshop, ed. Rucker, H. O., Kurth, W. S., and Mann, G. (Wein: Austrian Academy of Sciences Press), 1.Google Scholar

Burke, B. F. 2009, Radio Astronomy from First Contacts to the CMBR. In Finding the Big Bang, ed. Peebles, J. E., Page, L. A., and Partridge, R. B. (Cambridge: Cambridge University Press), 176.Google Scholar

Burke, B. F. and Franklin, K. L. 1955a, High Resolution Radio Astronomy at 13.5 m Wavelength, AJ, 60, 155.Google Scholar

Burke, B. F. and Franklin, K. L. 1955b, Observations of a Variable Radio Source Associated with the Planet Jupiter, J. Geophys. Res., 60, 213.CrossRefGoogle Scholar

Burke, B. F. et al. 1970, Studies of H₂O Sources by Means of a Very-Long-Baseline Interferometer, ApJ, 160, L63.Google Scholar

Burke, B. F. et al. 1972, Observations of Maser Radio Sources with an Angular Resolution of 0″.0002, Sov. Astron., 16, 379; Russian original, Astron Zh., 49, 465.Google Scholar

Burke-Spolaor, S. et al. 2011, Radio Bursts with Extragalactic Spectral Characteristics Show Terrestrial Origins, AJ, 727, 18.CrossRefGoogle Scholar

Burke-Spolaor, S. et al. 2019, The Astrophysics of Nanohertz Gravitational Waves, A&A Rev., 27, 5.Google Scholar

Butrica, A. J. 1996, To See the Unseen: A History of Planetary Radar Astronomy (Washington: NASA).Google Scholar

Caputo, F., Marconi, M., and Musella, I. 2002, The Cepheid Period-Luminosity Relation and the Maser Distance to NGC 4258, ApJ, 566, 833.Google Scholar

Carilli, C. C. and Rawlings, S. (eds.) 2004, Science with the Square Kilometre Array (Amsterdam: Elsevier).Google Scholar

Carr, T. D. et al. 1958, 18-Megacycle Observations of Jupiter in 1957, ApJ, 127, 274.Google Scholar

Carr, T. D. et al. 1965, Post-Detector Correlation Interferometry of Jupiter at 18 Mc/s, IEEE NEREM Record, 7, 222.Google Scholar

Chae, K.-H. et al. 2002, Constraints on Cosmological Parameters from the Analysis of the Cosmic Lens All Sky Survey, Radio-Selected Gravitational Lens Statistics, Phys. Rev. Let., 89, 151301.Google Scholar

Chatterjee, S. et al. 2017, A Direct Localization of a Fast Radio Burst and Its Host, Nature, 541, 5.CrossRefGoogle ScholarPubMed

Cheung, A. et al. 1968, Detection of NH3 Molecules in the Interstellar Medium by Their Microwave Emission, Phys. Rev. Let., 21, 170.Google Scholar

Cheung, A. et al. 1969, Detection of Water in Interstellar Regions by Its Microwave Radiation, Nature, 221, 626.CrossRefGoogle Scholar

Chiu, H.-Y. 1964, Gravitational Collapse, Phys. Today, 17, 21.Google Scholar

Christiansen, W. N. 1984, The First Decade of Solar Radio Astronomy in Australia. In The Early Years of Radio Astronomy, ed. Sullivan, W. T. III (Cambridge: Cambridge University Press), 113.Google Scholar

Christiansen, W. N. and Hindman, J. V. 1952a, 21 cm Line Radiation from Galactic Hydrogen, Obs., 72, 149.Google Scholar

Christiansen, W. N. and Hindman, J. V. 1952b, A Preliminary Survey of 1420 Mc/s. Line Emission from Galactic Hydrogen, Austrl. J. Sci. Res., A5, 437.Google Scholar

Christiansen, W. N. and Warburton, J. A. 1953, The Distribution of Radio Brightness over the Solar Disk at a Wavelength of 21cm: I. A New Highly-Directional Aerial System, Austrl. J. Phys., 6, 190.Google Scholar

Christiansen, W. N. and Warburton, J. A. 1955, The Distribution of Radio Brightness over the Solar Disk at a Wavelength of 21cm: III. The Quiet Sun: Two Dimensional Observations, Austrl. J. Phys., 8, 474.Google Scholar

Christiansen, W. N., Mathewson, D. S., and Pawsey, J. L. 1957, Radio Pictures of the Sun, Nature, 180, 944.CrossRefGoogle Scholar

Churchill, W. S., 1950, The Second World War, Vol. 4, The Hinge of Fate (Boston: Houghton Mifflin Company).Google Scholar

Churchwell, E. and Mezger, P. G. 1970, On the Determination of Helium Abundance from Radio Recombination Lines, Astrophys. Lett., 5, 227.Google Scholar

Clancy, R. T., Grossman, A. W., and Muhleman, D. O. 1992, Mapping Mars Water Vapor with the Very Large Array, Icarus, 100, 48.CrossRefGoogle Scholar

Clark, D. 1980, How Diana Touched the Moon, IEEE Spectrum, 17, 44.Google Scholar

Clark, D. H. and Murdin, P. 1978, An Unusual Emission-Line Star/X-ray Source Radio Star, Possibly Associated with an SNR, Nature, 276, 44.Google Scholar

Clarke, M. E. 1964a, Two Topics in Radiophysics, PhD Dissertation, Cambridge University.Google Scholar

Clarke, M. E. 1964b, The Determination of the Positions of 88 Radio Sources, MNRAS, 127, 405.Google Scholar

Clarke, M. E. 1964c, Some Radio Source Flux Density Measurements at 178 MHz, Obs., 85, 67.Google Scholar

Clarke, M. E., Bolton, J. G., and Shimmins, A. J. 1966, Identification of Extragalactic Radio Sources between Declinations 0° and +20°, Austrl. J. Phys., 19, 375.Google Scholar

Claussen, M. J. and Lo, K. Y. 1986, Circumnuclear Water Vapor Masers in Active Galaxies, ApJ, 308, 592.Google Scholar

Cocconi, G. and Morrison, P. 1959, Searching for Interstellar Communications, Nature, 184, 844.Google Scholar

Cocke, W. J., Disney, M., and Taylor, D. J. 1969, Discovery of Optical Signals from Pulsar NP 0532, Nature, 221, 525.Google Scholar

Cohen, M. H. 1958a, The Cornell Radio Polarimeter, Proc. IRE, 46, 183.Google Scholar

Cohen, M. H. 1958b, Radio Astronomy Polarization Measurements, Proc. IRE, 46, 172.Google Scholar

Cohen, M. H. 1994, The Owens Valley Radio Observatory: Early Years, Eng. Sci., 57, 8.Google Scholar

Cohen, M. H. 2005, Dark Matter and the Owens Valley Radio Observatory. In The New Astronomy: Opening the Electromagnetic Window and Expanding Our View of the Planet Earth, ed. Orchiston, W. (Dordrecht: Springer), 169.Google Scholar

Cohen, M. H. 2007, A History of OVRO Part II, Eng. Sci., 70, 33.Google Scholar

Cohen, M. H. 2009, Genesis of the 1000-Foot Arecibo Dish, J. Astron. Hist. Heritage, 12, 141.Google Scholar

Cohen, M. H. et al. 1971, The Small-Scale Structure of Radio Galaxies and Quasi-Stellar Sources at 3.8 Centimeters, ApJ, 170, 207.Google Scholar

Cohen, M. H. et al. 1977, Radio Sources with Superluminal Velocities, Nature, 268, 405.Google Scholar

Cohen, M. H. et al. 2007, Relativistic Beaming and the Intrinsic Properties of Extragalactic Radio Jets, ApJ, 658, 232.Google Scholar

Colgate, S. A. 1975, Electromagnetic Pulse from Supernovae, ApJ, 198, 439.Google Scholar

Colombo, G. 1965, Rotational Period of the Planet Mercury, Nature, 208, 575.Google Scholar

Colombo, G. and Shapiro, I. I. 1966, The Rotation of the Planet Mercury, ApJ, 145, 296.Google Scholar

Comella, J. M. et al. 1969, Crab Nebula Pulsar NP 0532, Nature, 221, 453.Google Scholar

Condon, J. J. 2008, ZAPPED! … by Hostile Space Aliens! In ASPC 398, Frontiers of Astrophysics: A Celebration of NRAO 50th Anniversary, ed. Bridle, A. H., Condon, J. J., and Hunt, G. C. (San Francisco: Astronomical Society of the Pacific), 323.Google Scholar

Condon, J. J. and Mitchell, K. J. 1984, A Deeper VLA Survey of the α = 08h 52m 15s, δ = +17° 16’ Field, AJ, 89, 610.Google Scholar

Condon, J. J. et al. 1994, A 4.85 GHz Sky Survey. III. Epoch 1986 and Combined (1986–1987) Maps Covering 0^o<δ<+75 ^o, AJ, 107, 1829.Google Scholar

Condon, J. J. et al. 2012, Resolving the Radio Source Background: Deeper Understanding through Confusion, ApJ, 768, 37.Google Scholar

Conklin, E. K. 1967, Isotropy of the Cosmic Background Radiation at 10 690 MHz, Phys. Rev. Let., 18, 614.Google Scholar

Conklin, E. K. 1969a, Anisotropy and Inhomogeneity in the Cosmic Background Radiation, PhD Dissertation, Stanford University.Google Scholar

Conklin, E. K. 1969b, Velocity of the Earth with Respect to the Cosmic Background Radiation, Nature, 222, 97.Google Scholar

Conklin, E. K. 1972, Observations of Large-Scale Anisotropy in the 3 K Background Radiation. In IAU Symposium no. 44, External Galaxies and Quasi-Stellar Objects, ed. Evans, D. E. (Dordrecht: Reidel), 518.Google Scholar

Conklin, E. K. and Bracewell, R. N. 1967, Limits on Small Scale Variations in the Cosmic Background Radiation, Nature, 216, 777.Google Scholar

Contopoulos, G. and Jappel, A. (eds.) 1974, Transactions of the IAU XV: B (Dordrecht: Reidel).Google Scholar

Conway, R. G., Kellermann, K. I., and Long, R. J. 1963, The Radio Frequency Spectra of Discrete Radio Sources, MNRAS, 125, 261.Google Scholar

Cook, J. J. et al. 1960, Radio Detection of the Planet Saturn, Nature, 188, 393.Google Scholar

Cooper, B. F. C. 1998, Parkes, Centaurus A, and All That, unpublished memo, NAA, Bracewell Papers, Stanford University, Centaurus A Research.Google Scholar

Cooper, B. F. C. and Price, R. M. 1962, Faraday Rotation Effects Associated with the Radio Source Centaurus A, Nature, 195, 1064.Google Scholar

Cotton, W. D. 1979, A Method of Mapping Compact Structure in Radio Sources Using VLBI Observations, AJ, 84, 1122.Google Scholar

Counselman III, C. C. et al. 1974, Solar Gravitational Deflection of Radio Waves Measured by Very-Long-Baseline Interferometry, Phys. Rev. Let., 33, 162.Google Scholar

Covington, A. E. 1947, Micro-Wave Solar Noise Observations during the Partial Eclipse of November 23, 1946, Nature, 159, 404.Google Scholar

Covington, A. E. 1948, Solar Noise Observations at 10.7 Centimeters, Proc. IRE, 36, 454.CrossRefGoogle Scholar

Covington, A. E. 1984a, Early Radar Research and a Beginning in Radio Astronomy. In Serendipitous Discoveries in Radio Astronomy, ed. Kellermann, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 105.Google Scholar

Covington, A. E. 1984b, Beginnings of Solar Radio Astronomy in Canada. In The Early Years of Radio Astronomy, ed. Sullivan, W. T. III (Cambridge: Cambridge University Press), 317.Google Scholar

Covington, A. E. 1988, Origins of Canadian Radio Astronomy, JRASC, 82, 165.Google Scholar

Crawford, A. B., Hogg, D. C., and Hunt, L. E. 1961, Bell Syst. Tech. J., 40, 1095.Google Scholar

Crawford, D. F., Jauncey, D. L., and Murdoch, H. S. 1970, Maximum-Likelihood Estimation of the Slope from Number-Flux Counts of Radio Sources, ApJ, 162, 405.Google Scholar

Cromartie, H. T. et al. 2020, Relativistic Shapiro Delay Measurements of an Extremely Massive Millisecond Pulsar, Nat. Astron., 4, 72.Google Scholar

Cudaback, D. D., Read, R. B., and Rougoor, G. W. 1966, Diameters and Positions of Three Sources of 18-cm OH Emission, Phys. Rev. Let., 17, 452.CrossRefGoogle Scholar

Davies, R. D. and Fennison, R. C. 1964, A Search for Intergalactic Neutral Hydrogen, I. The Observations, MNRAS, 128, 123.Google Scholar

Davies, R. D., De Jager, G., and Verschuur, G. L. 1966, Detection of Circular and Linear Polarization in the OH Emission Sources near W3 and W49, Nature, 209, 974.Google Scholar

Davis, R. J. et al. 1978, Interferometric Observations of Weak Radio Flares from a Red Dwarf Star, Nature, 273, 644.Google Scholar

de Pater, I. 1990, Radio Images of the Planets, ARAA, 28, 347.Google Scholar

de Pater, I., Schultz, M., and Brecht, H. 1997, Synchrotron Evidence for Amalthea’s Influence on Jupiter’s Electron Radiation Belt, J. Geophys. Res., 102, 22043.CrossRefGoogle Scholar

de Pater, I. et al. 2019, First ALMA Millimeter-Wavelength Maps of Jupiter, with a Multiwavelength Study of Convection, AJ, 158, 139.Google Scholar

Débarbat, S., Lequeux, J., and Orchiston, W., 2007, Highlighting the History of French Radio Astronomy. 1. Nordmann’s Attempt to Observe Solar Radio Emission in 1901, J. Astron. Hist. Heritage, 19, 3.CrossRefGoogle Scholar

Demorest, P. B. et al. 2010, A Two-Solar-Mass Neutron Star Measured Using Shapiro Delay, Nature, 467, 1081.Google Scholar

Denisse, J. G. 1984, The Early Years of Radio Astronomy in France. In The Early Years of Radio Astronomy, ed. Sullivan, W. T. III (Cambridge: Cambridge University Press), 303.Google Scholar

Dent, W. A. 1965a, Variation in the Radio Emission of 3C273 and Other Quasi-Stellar Sources, AJ, 70, 672.Google Scholar

Dent, W. A. 1965b, Quasi-Stellar Sources: Variation in the Radio Emission of 3C 273, Science, 148, 1458.Google Scholar

Dent, W. A. 1966, Variation in the Radio Emission from the Seyfert Galaxy NGC 1275, ApJ, 144, 843.Google Scholar

Deslandres, H. and Décombre, L. 1902, On the Search for Hertzian Radiation Emanating from the Sun, Comptes Rendus, 134, 527 (In French). English translation 1982 in Classics in Radio Astronomy, ed. W. T. Sullivan III (Dordrecht: Reidel), 161.Google Scholar

DeSoto, C. B. 1936, 200 Meters and Down (West Hartford: American Radio Relay League).Google Scholar

Dewhurst, D. 1951, 12 October 1951 Meeting of the Royal Astronomical Society, Obs., 71, 209.Google Scholar

DeWitt, J. M. and Stodola, E. K. 1949, Detection of Radio Signals Reflected from the Moon, Proc. IRE, 37, 229.CrossRefGoogle Scholar

Dick, S. J. 1996, The Biological Universe (Cambridge: Cambridge University Press).Google Scholar

Dicke, R. H. 1946, The Measurement of Thermal Radiation at Microwave Frequencies, Rev. Sci. Instr., 17, 7.Google Scholar

Dicke, R. H. 1974, The Oblateness of the Sun and Relativity, Science, 184, 419.Google Scholar

Dicke, R. H. and Beringer, R. 1946, Microwave Radiation from the Sun and Moon, ApJ, 103, 375.Google Scholar

Dicke, R. H. et al. 1946, Atmospheric Absorption Measurements with a Microwave Radiometer, Phys. Rev., 70, 340.CrossRefGoogle Scholar

Dicke, R. H. et al. 1965, Cosmic Black-Body Radiation, ApJ, 142, 414.Google Scholar

Dieter, N. H. 1967, Observations of the Hydrogen Recombination Line 158α in Galactic H II Regions, ApJ, 150, 435.Google Scholar

Dieter, N. H., Weaver, H., and Williams, D. R. W. 1966, Secular Variations in the Radio-Frequency Emission of OH, AJ, 71, 160.Google Scholar

Djorgovski, G. 1982, Optical Identification of the Millisecond Pulsar 1937+214, Nature, 300, 618.Google Scholar

Dogel, B. A. et al. 2012, Radio Astronomy Studies at the Lebedev Physical Institute. In A Brief History of Radio Astronomy in the USSR, ed. Braude, S. and Kellermann, K. I. (Dordrecht: Springer), 1; English translation of 1985 Russian edition.Google Scholar

Dolfuss, A. 1953, Observation Visuelle et Photographique des Planètes Mercure et Vénus a L’observatoire du Pic du Midi, L’Astronomie, 67, 61.Google Scholar

Doroshkevich, A. G. and Novikov, I. D. 1964, Mean Density of Radiation in the Metagalaxy and Certain Problems in Relativistic Cosmology, Sov. Phys. Doklady, 9, 11.Google Scholar

Drake, F. 1962, 10 cm Observations of Venus Near Superior Conjunction, Nature, 195, 894.Google Scholar

Drake, F. 1964, Microwave Observations of Venus, 1962–1963, AJ, 69, 62.CrossRefGoogle Scholar

Drake, F. 1984, Discovery of Jupiter Radiation Belts. In Serendipitous Discoveries in Radio Astronomy, ed. Kellermann, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 258.Google Scholar

Drake, F. 1986, The Search for Extraterrestrial Intelligence. In Proceedings of the NRAO Workshop on the Search for Extraterrestrial Intelligence, ed. Kellermann, K. I. and Seielstad, G. A. (Green Bank: NRAO/AUI), 17.Google Scholar

Drake, F. and Ewen, H. I. 1958, A Broad-Band Microwave Source Comparison Radiometer for Advanced Research in Radio Astronomy, Proc. IRE, 46, 53.CrossRefGoogle Scholar

Drake, F. and Hvatum, H. 1959, Non-thermal Microwave Radiation from Jupiter, AJ, 645, 329.Google Scholar

Drake, F. D. and Sobel, D. 1992, Is Anyone Out There? The Scientific Search for Extraterrestrial Intelligence (New York: Delacorte Press).Google Scholar

Dravskikh, A. F. et al. 1966, Investigation of the Radio Line of Excited Hydrogen at a Wavelength of 5 cm Using a Quantum Paramagnetic Amplifier, Sov. Phys. Dokl., 10, 627; Russian original: Dokl. Akad. Nauk SSSR, 163, 332, 1960.Google Scholar

Dupree, A. K. and Goldberg, L. 1970, Radio Frequency Recombination Lines, ARAA, 8, 231.Google Scholar

Dyson, F. W., Eddington, A. S., and Davidson, C. 1920, A Determination of the Deflection of Light by the Sun’s Gravitational Field, from Observations Made at the Total Eclipse of May 29, 1919, Phil. Trans. Roy. Soc. A, 220, 291.Google Scholar

Dyson, R. 1960, Search for Artificial Stellar Sources of Infrared Radiation, Science, 131, 1667.Google Scholar

Eddington, A. S. 1913, On a Formula for Correcting Statistics for the Effects of a Known Error of Observation, MNRAS, 73, 359.Google Scholar

Edge, D. O. and Mulkay, J. M. 1976, Astronomy Transformed (New York: Wiley)Google Scholar

Edge, D. O., Scheuer, P. A. G., and Shakeshaft, J. R. 1958, Evidence on the Spatial Distribution of Radio Sources Derived from a Survey at a Frequency of 159 Mcs^‒1, MNRAS, 118, 183.Google Scholar

Edge, D. O. et al. 1959, A Survey of Radio Sources at a Frequency of 159 Mc/s, Mem. RAS, 68, 37.Google Scholar

Edlén, B. 1946, Untitled Letter, Nature, 157, 297.Google Scholar

Edmondson, F. 1956, Review of “The Changing Universe. The Story of the New Astronomy,” Science, 124, 541.Google Scholar

Ehman, J. R. 1998, The Big Ear Wow! Signal, available at: www.bigear.org/wow20th.htm (last accessed 1 December 2022).Google Scholar

Ehrenstein, G., Townes, C. H., and Stevenson, M. J. 1959, Ground State Λ-Doubling Transitions of OH Radical, Phys. Rev Let., 3, 40.Google Scholar

Einasto, J., Kaasik, A., and Saar, E. 1974, Dynamic Evidence on Massive Coronas of Galaxies, Nature, 250, 309.Google Scholar

Einasto, J. et al. 1974, Missing Mass around Galaxies: Morphological Evidence, Nature, 252, 111.Google Scholar

Einstein, A. 1911, Über den Einfluß der Schwerkraft auf die Ausbreitung des Lichtes, Annalen der Physik, 35, 898; English translation, On the Influence of Gravitation on the Propagation of Light, in 1952, The Principle of Relativity (New York: Dover) 97.Google Scholar

Einstein, A. 1916, The Foundation of the General Theory of Relativity, Annalen der Physik, 49, 769 (in German).Google Scholar

Einstein, A. 1936, Lens-Like Action of a Star by the Deviation of Light in the Gravitational Field, Science, 84, 506.CrossRefGoogle ScholarPubMed

Ekers, R. D. 2013, The History of the Square Kilometer Array (SKA) Born Global. In Resolving the Sky: Radio Interferometry: Past, Present, and Future, ed. Garrett, M. A. and Greenwood, J. C. (Manchester: SKA Organization), 68.Google Scholar

Ekers, R. D. 2014, Non-Thermal Radio Astronomy, Astropar. Phys., 53, 152.Google Scholar

Elbers, A. 2017, The Rise of Radio Astronomy in the Netherlands (Cham: Switzerland).CrossRefGoogle Scholar

Elder, F. R., Langmuir, R. V. and Pollock, H. C. 1948, Radiation from Electrons Accelerated in a Synchrotron, Phys. Rev., 74, 52.Google Scholar

Elsmore, B., Ryle, M., and Leslie, P. R. R. 1959, The Positions, Flux Densities and Angular Diameters of 64 Radio Sources Observed at a Frequency of 178 Mc/s, Mem. RAS, 68, 61.Google Scholar

Evans, D. S. 1949, Photometry of NGC 5128, MNRAS, 109, 94.Google Scholar

Evans, J. V. and Taylor, G. N. 1959, Radio Echo Observations of Venus, Nature, 184, 1358.Google Scholar

Ewen, H. I. and Purcell, E. M. 1951a, Radiation from Hyperfine Levels of Interstellar Hydrogen, Phys. Rev., 83, 881.Google Scholar

Ewen, H. I. and Purcell, E. M. 1951b, Radiation from Hyperfine Levels of Interstellar Hydrogen, AJ, 56, 125.Google Scholar

Ewen, H. I. and Purcell, E. M. 1951c, Observation of a Line in the Galactic Radio Spectrum, Nature, 168, 356.Google Scholar

Faber, S. M. and Gallagher, J. S. 1979, Masses and Mass-to-Light Ratios of Galaxies, ARAA, 17, 135.Google Scholar

Fabian, A. C. and Rees, M. J. 1979, SS 433: A Double Jet in Action?, MNRAS, 187, 13.Google Scholar

Feain, I. J. et al. 2011, The Radio Continuum Structure of Centaurus A at 1.4 GHz, ApJ, 740, 17.Google Scholar

Field, G. 1962a, Absorption by Intergalactic Hydrogen, ApJ, 135, 684.Google Scholar

Field, G. 1962b, Atmosphere of Mercury, AJ, 67, 575.Google Scholar

Field, G. 2009, Cyanogen and the CMBR. In Finding the Big Bang, ed. Peebles, P. J. E., Page, L. A., and Partridge, R. B. (Cambridge: Cambridge University Press), 75.Google Scholar

Field, G. and Hitchcock, J. L. 1966, Cosmic Black-Body Radiation at λ=2.6 mm, Phys. Rev. Let., 16, 817.Google Scholar

Field, G., Arp, H., and Bahcall, J. N. 1973, The Redshift Controversy (Reading: Benjamin).Google Scholar

Field, G., Herbig, G. H., and Hitchcock, J. 1966, Radiation Temperature of Space at λ2.6 mm, AJ, 71, 161.Google Scholar

Findlay, J. W., Hvatum, H., and Waltman, W. B. 1965, An Absolute Flux-Density Measurement of Cassiopeia A, ApJ, 141, 873.Google Scholar

Fixsen, D. J. et al. 2011, ARCADE 2 Measurement of the Absolute Sky Brightness at 3–90 GHz, ApJ, 734, 5.Google Scholar

Fomalont, E. B. and Sramek, R. A. 1975, A Confirmation of Einstein’s General Theory of Relativity by Measuring the Bending of Microwave Radiation in the Gravitational Field of the Sun, ApJ, 199, 749.Google Scholar

Fomalont, E. B. and Sramek, R. A. 1976, Measurements of the Solar Gravitational Deflection of Radio Waves in Agreement with General Relativity, Phys. Rev. Let., 36, 147.Google Scholar

Fomalont, E. B. et al. 1964, Accurate Right Ascensions for 226 Radio Sources, AJ, 69, 772.Google Scholar

Fomalont, E. B. et al. 2009, Progress in Measurements of the Gravitational Bending of Radio Waves Using the VLBA, ApJ, 699, 1395.Google Scholar

Franklin, K. L. 1959, An Account of the Discovery of Jupiter as a Radio Source, AJ, 64, 37.Google Scholar

Franklin, K. L. 1984, The Discovery of Jupiter Bursts. In Serendipitous Discoveries in Radio Astronomy, ed. Kellermann, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 252.Google Scholar

Franklin, K. L. and Burke, B. F. 1956, Radio Observations of Jupiter, AJ, 61, 177.Google Scholar

Fränz, K. 1942, Measurement of the Sensitivity of Short Wave Receivers, Hochfrequenztechnik. und Elektroakustik, 59, 105 (in German).Google Scholar

Frater, R. H. and Ekers, R. D. 2012, John Paul Wild 1923–2008, Mem. Roy. Soc., 58, 327.Google Scholar

Frater, R. H., Goss, W. M., and Wendt, H. W. 2017, Four Pillars of Radio Astronomy: Mills, Christiansen, Wild, Bracewell (Cham: Springer).Google Scholar

Friis, H. T. 1965, Karl Jansky: His Career at Bell Telephone Laboratories, Science, 149, 841.Google Scholar

Friis, H. T. 1971, Seventy-Five Years in an Exciting World (San Francisco: San Francisco Press).Google Scholar

Friis, H. T. and Feldman, C. B. 1937, A Multiple Unit Steerable Antenna for Short-Wave Radio Reception, Proc. IRE, 25, 841.Google Scholar

Gamow, G. 1948, The Evolution of the Universe, Nature, 162, 680.CrossRefGoogle ScholarPubMed

Gamow, G. 1949, On Relativistic Cosmology, Rev. Mod. Phys., 21, 367.Google Scholar

Gamow, G. 1950, Half an Hour of Creation, Phys. Today, 3, 16.Google Scholar

Gardner, F. F. and McGee, R. X. 1967, Detection of β-Transitions in the Recombination Spectrum of Hydrogen Near 9 cm Wavelength, Nature, 213, 480.Google Scholar

Gardner, F. F. and Whiteoak, J. B. 1962, Polarization of 20-cm Wavelength Radiation from Radio Sources, Phys. Rev. Let., 9, 197.Google Scholar

Gardner, F. F. et al. 1964, Detection of the Interstellar OH Lines at 1612 and 1720 Mc/sec, Phys. Rev. Let., 13, 3.Google Scholar

Garwin, R. L. 1974, Detection of Gravity Waves Challenged, Phys. Today, 27, 9.Google Scholar

Geller, M. J. and Huchra, J. P. 1989, Mapping the Universe, Science, 246, 897.Google Scholar

George, M., Orchiston, W., and Wielebinski, R. 2017, The History of Early Low Frequency Radio Astronomy in Australia. 8: Grote Reber and the ‘Square Kilometre Array’ near Bothwell, Tasmania, in the 1960s and 1970s, J. Astron. Hist. Heritage, 20, 195.Google Scholar

Getmantsev, G. G. 1952, Cosmic Electrons as a Source of Radio Emission from the Galaxy, Dokl. Akad. Nauk SSSR, 83, 557 (in Russian).Google Scholar

Ginzburg, V. L. 1946, On Solar Radiation in the Radio Spectrum, Dokl. Akad. Nauk, SSSR, 52, 487 (in Russian).Google Scholar

Ginzburg, V. L. 1951, Cosmic Rays as a Source of Galactic Radio Emission, Dokl. Akad. Nauk SSSR, 76, 377 (in Russian). English translation in Classics in Radio Astronomy, ed. W. T. Sullivan III (Dordrecht: Reidel), 93.Google Scholar

Ginzburg, V. L. 1961, On the Nature of the Radio Galaxies, Sov. Astron., 5, 282; English translation of Astron. Zh., 38, 380.Google Scholar

Gold, T. 1951, The Origin of Cosmic Radio Noise. In Proceedings of the Conference on Dynamics of Ionized Media, ed. Boyd, R. I. (London: University College London), 105. Reprinted in 1979 in A Source Book in Astronomy and Astrophysics, 1900–1975, ed. K. R. Lang and O. Gingerich (Cambridge, MA: Harvard University Press), 783.Google Scholar

Gold, T. 1968, Rotating Neutron Stars as the Origin of the Pulsating Radio Sources, Nature, 218, 731.Google Scholar

Gold, T. 1984, The Reception of New Ideas by the Scientific Community. Paper Presented at the Third Annual Meeting of the Society for Scientific Exploration, October 1984.Google Scholar

Goldreich, P. and Lynden-Bell, D. 1969, Io, a Jovian Unipolar Inductor, ApJ, 156, 59.CrossRefGoogle Scholar

Goldstein, R. M. and Carpenter, R. L. 1963, Rotation of Venus: Period Estimated from Radar Measurements, Science, 139, 910.Google Scholar

Goldstein, S. et al. 1964, OH Absorption Spectra in Sagittarius, Nature, 203, 65.Google Scholar

Gordon, M. A. and Sorochenko, R. L. 2002, Radio Recombination Lines (Dordrecht: Kluwer).Google Scholar

Gordon, W. E. 1958, Incoherent Scattering of Radio Waves by Free Electrons with Applications to Space Exploration by Radar, Proc. IRE, 46, 1824.CrossRefGoogle Scholar

Gordon, W. E. and LaLonde, L. 1961, The Design and Capabilities of an Ionospheric Radar Probe, Trans. IRE, AP-9, 17.Google Scholar

Gorenstein, M. V. and Smoot, G. 1981, Large-Angular-Scale Anisotropy in the Cosmic Background Radiation, ApJ, 244, 361.CrossRefGoogle Scholar

Goss, W. M. 2013, Making Waves: The Story of Ruby Payne-Scott: Australian Pioneer Radio Astronomer (Berlin: Springer).Google Scholar

Goss, W. M. and McGee, R. X. 1996, The Discovery of the Radio Source Sagittarius A (Sgr A). In ASPC 102, The Galactic Center, ed. Gredel, R. (San Francisco: Astronomical Society of the Pacific), 369.Google Scholar

Goss, W. M. and McGee, R. X. 2010. Under the Radar: The First Woman in Radio Astronomy: Ruby Payne-Scott (Berlin: Springer).Google Scholar

Goss, W. M., Brown, R. L., and Lo, K. Y. 2003, The Discovery of Sgr A*. In Proceedings of the Galactic Center Workshop 2002: The Central 300 Parsecs of the Milky Way, ed. A. Cotera et al. Astron. Nachtr., 324, 497.Google Scholar

Goss, W. M., Hooker, C., and Ekers, R. D. 2023, Joe Pawsey and the Founding of Australian Radio Astronomy: Early Discoveries, from the Sun to the Cosmos (Cham: Springer).Google Scholar

Gottesman, S. T., Davies, R. D., and Reddish, V. C. 1966, A Neutral Hydrogen Survey of the Southern Regions of the Andromeda Nebula, MNRAS, 133, 359.Google Scholar

Gower, J. F. R. 1966, The Source Counts from the 4C Survey, MNRAS, 133, 151.Google Scholar

Gower, J. F. R., Scott, P. F., and Wills, D. 1967, A Survey of Radio Sources in the Declination Ranges ‒07° to 20° and 40° to 80°, Mem. RAS, 71, 4.Google Scholar

Graham-Smith, F. 1950, Origin of the Fluctuations in the Intensity of Radio Waves from Galactic Sources: Cambridge Observations, Nature, 165, 422.Google Scholar

Graham-Smith, F. 1951, An Accurate Determination of the Positions of Four Radio Stars, Nature, 168, 555.Google Scholar

Graham-Smith, F. 1952, Apparent Angular Sizes of Discrete Radio Sources: Observations at Cambridge, Nature, 170, 1065.Google Scholar

Graham-Smith, F. 1986, Martin Ryle 1918–1984, Mem. Roy. Soc., 32, 495.Google Scholar

Gray, R. H. 2012, The Elusive WOW: Search for Extraterrestrial Intelligence (Chicago: Palmer Square Press).Google Scholar

Gray, R. H. and Marvel, K. B. 2001, A VLA Search for the Ohio State “Wow,” ApJ, 546, 1171.CrossRefGoogle Scholar

Green, P. E. and Pettengill, G. H. 1960, Exploring the Solar System by Radar, Sky Tel., 20, 9.Google Scholar

Greenfield, P. D., Roberts, D. H., and Burke, B. F. 1985, The Gravitationally Lensed Quasar 0957+561: VLA Observations and Mass Models, ApJ, 293, 356.Google Scholar

Greenstein, J. L. 1961, The First True Radio Star. Eng. Sci., 24, 18.Google Scholar

Greenstein, J. L. 1984, Optical and Radio Astronomers in the Early Years. In Serendipitous Discoveries in Radio Astronomy, ed. Kellerman, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 79.Google Scholar

Greenstein, J. L. and Matthews, T. A. 1963, Redshift of the Radio Source 3C 48, Nature, 197, 1041.Google Scholar

Greenstein, J. L. and Schmidt, M. 1963, The Quasi-Stellar Radio Sources 3C 48 and 3C 273, ApJ, 140, 1.Google Scholar

Güdel, M. 2002, Stellar Radio Astronomy: Probing Stellar Atmospheres from Protostars to Giants, ARAA, 40, 217.Google Scholar

Gundermann, E. 1965, Observations of the Interstellar Hydroxyl Radical, PhD Dissertation, Harvard University.Google Scholar

Gurvits, L., Kellermann, K. I., and Frey, L. 1999, The “Angular Size–Redshift Relation” for Compact Radio Structures in Quasars and Radio Galaxies, A&A, 342, 378.Google Scholar

Gush, H. P., Halpern, M., and Wisnow, E. H. 1990, Rocket Measurement of the Cosmic-Background Radiation mm Wave Spectrum, Phys. Rev. Let., 65, 537.Google Scholar

Haddock, F. 1984, U.S. Radio Astronomy Following World War II. In Serendipitous Discoveries in Radio Astronomy, ed. Kellermann, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 115.Google Scholar

Hagen, J. P. 1951, Naval Research Laboratory Eclipse Expedition to Attu, Alaska, September 12, 1950, AJ, 56, 39.Google Scholar

Hagen, J. P., Haddock, F. T., and Reber, G., 1951, NRL Aleutian Radio Eclipse Expedition, Sky Tel., 10, 111.Google Scholar

Hagen, J. P. et al., 1948, Observations on the May 20, 1947, Total Eclipse of the Sun, NRL Report, March 1948.Google Scholar

Hall, P. (ed.) 2005, The SKA; An Engineering Perspective (Dordrecht: Springer).Google Scholar

Ham, R. A. 1975, The Hissing Phenomena, J. Br. Astron. Assoc., 85, 317.Google Scholar

Hanbury Brown, R. 1984, The Development of Michelson and Intensity Long Baseline Interferometry. In Serendipitous Discoveries in Radio Astronomy, ed. Kellermann, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 133.Google Scholar

Hanbury Brown, R. and Hazard, C. 1950, Radio-Frequency Radiation from the Great Nebula in Andromeda (M.31), Nature, 166, 901.Google Scholar

Hanbury Brown, R. and Hazard, C. 1952, Radio-Frequency Radiation from Tycho Brahe’s Supernova (A.D. 1572), Nature, 170, 364.Google Scholar

Hanbury Brown, R. and Hazard, C. 1953a, Radio-Frequency Radiation from the Spiral Nebula Messier 81, Nature, 172, 853.Google Scholar

Hanbury Brown, R. and Hazard, C. 1953b, A Survey of 23 Localized Radio Sources in the Northern Hemisphere, MNRAS, 113, 123.Google Scholar

Hanbury Brown, R. and Twiss, R. Q. 1956, A Test of a New Type of Stellar Interferometer on Sirius, Nature, 178, 1046.CrossRefGoogle Scholar

Hanbury Brown, R., Jennison, R. C., and Das Gupta, M. K. 1952, Apparent Angular Sizes of Discrete Radio Source, Nature, 170, 1061.Google Scholar

Hargrave, P. J. and Ryle, M. 1974, Observations of Cygnus A with the 5-km Radio Telescope, MNRAS, 166, 305.Google Scholar

Harp, G. R. et al. 2020, An ATA Search for a Repetition of the Wow Signal, AJ, 160, 162.Google Scholar

Harris, D. E. and Roberts, J. A. 1960, Radio Source Measurements at 960 Mc/s, PASP, 72, 237.Google Scholar

Harris, M. 2019, Untitled, Radio Science Bulletin, 371, 91.Google Scholar

Harwit, M. 1981, Cosmic Discovery (New York: Basic Books).Google Scholar

Harwit, M. 1984, Observational Discovery vs. Theoretical Discovery. In Serendipitous Discoveries in Radio Astronomy, ed. Kellermann, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 197.Google Scholar

Harwit, M. 2013, In Search of the True Universe (New York: Cambridge University Press).Google Scholar

Harwit, M. 2019, Cosmic Discovery, revised issue (Cambridge: Cambridge University Press).Google Scholar

Harwit, M. 2021, Cosmic Messengers (Cambridge: Cambridge University Press).CrossRefGoogle Scholar

Haynes, M. P. and Giovanelli, R. 1986, The Connection between Pisces–Perseus and the Local Supercluster ApJ, 306, L55.CrossRefGoogle Scholar

Haynes, R. F. and Haynes, D. H. 1993, 3C 273: The Hazards of Publication, PASA, 10 355.Google Scholar

Haynes, R. et al. 1996, Explorers of the Southern Sky: A History of Australian Radio Astronomy (Cambridge: Cambridge University Press).Google Scholar

Hazard, C. 1962, The Method of Lunar Occultations and Its Application to a Survey of Radio Source 3C 212, MNRAS, 124, 343.Google Scholar

Hazard, C. and Walsh, D. 1959, An Experimental Investigation of the Effects of Confusion in a Survey of Localized Radio Sources, MNRAS, 119, 648.Google Scholar

Hazard, C., Mackey, M. B., and Shimmins, A. J. 1963, Investigation of the Radio Source 3C 273 by the Method of Lunar Occultations, Nature, 197, 1037.CrossRefGoogle Scholar

Hazard, C. et al. 2018, The Sequence of Events that Led to the 1963 Publication in Nature of 3C 273, the First Quasar and the First Extragalactic Radio Jet, PASA, 35, 6.Google Scholar

Heightman, D. W. 1946, Signals from the Sun, Wireless World, March, 99.Google Scholar

Helfand, D. J. 1982, A Superfast New Pulsar, Nature, 300, 573.CrossRefGoogle Scholar

Henyey, L. G. and Keenan, P. C. 1940, Interstellar Radiation from Free Electrons and Hydrogen Atoms, ApJ, 91, 625.CrossRefGoogle Scholar

Hernstein, J. R. et al. 1999, A Geometric Distance to the Galaxy NGC 4258 from Orbital Motions in a Nuclear Gas Disk, Nature, 400, 539.Google Scholar

Hewish, A. 1961, Extrapolation of the Number-Flux Density Relation of Radio Stars by Scheuer’s Statistical Methods, MNRAS, 123, 167.Google Scholar

Hewish, A. 1974, Pulsars and High Density Physics, 1974 Nobel Lecture. In Nobel Lectures, Physics 1971–1980, ed. Lundqvist, S. (Singapore: World Scientific Publishing).Google Scholar

Hewish, A. 2008, Background to Discovery: Some Recollections. In 40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More, ed. Bassa, C. G. et al. (New York: American Institute of Physics), 3.Google Scholar

Hewish, A. and Okoye, S. E. 1965, Evidence for an Unusual Source of High Radio Brightness Temperature in the Crab Nebula, Nature, 207, 59.Google Scholar

Hewish, A. and Wyndham, J. D. 1963, The Solar Corona in Interplanetary Space, MNRAS, 126, 469.CrossRefGoogle Scholar

Hewish, A., Scott, P. F., and Wills, D. 1964, Interplanetary Scintillation of Small Diameter Radio Source, Nature, 203, 1214.Google Scholar

Hewish, A. et al. 1968, Observations of a Rapidly Pulsating Radio Source, Nature, 217, 709.CrossRefGoogle Scholar

Hewitt, J. N. et al. 1988, Unusual Radio Source MG1131+0456: A Possible Einstein Ring, Nature, 333, 537.CrossRefGoogle Scholar

Hey, J. S. 1946, Solar Radiation in the 4–6 Metre Radio Wave-Length Band, Nature, 157, 47.Google Scholar

Hey, J. S. 1973, The Evolution of Radio Astronomy (New York: Science History Publications).Google Scholar

Hey, J. S., Parsons, S. J., and Phillips, J. W. 1946, Fluctuations in Cosmic Radiation at Radio Frequencies, Nature, 158, 234.Google Scholar

Hey, J. S., Phillips, J. W., and Parsons, S. J. 1946, Cosmic Radiations at 5 Metre Wavelength, Nature, 157, 296.Google Scholar

Hills, R. et al. 2018, Concerns about Modelling of the EDGES Data, Nature, 564, 32.CrossRefGoogle ScholarPubMed

Hirabayashi, H., Edwards, P. G., and Murphy, D. W. (eds.) 2000, Astrophysical Phenomena Revealed by Space VLBI (Sagamihara: Institute of Space and Astronautical Science).Google Scholar

Hjellming, R. M. 1988, Radio Stars. In Galactic and Extragalactic Radio Astronomy, ed. Verschuur, G. L. and Kellermann, K. I. (Berlin: Springer), 384.Google Scholar

Hjellming, R. M. and Johnston, K. J. 1981, An Analysis of the Proper Motions of SS 433 Radio Jets, Nature, 290, 100.Google Scholar

Hjellming, R. M. and Wade, C. M. 1970, Radio Novae, ApJ, 162, L1.Google Scholar

Högbom, J. A. and Shakeshaft, J. R. 1961, Secular Variations of the Flux Density of the Radio Source Cassiopeia A, Nature, 189, 561.Google Scholar

Hoglund, B. and Mezger, P. G. 1965a, The Detection of the Hydrogen Emission Line N110–N109 at the Frequency 5009 Mc/Sec in Galactic H II Regions, AJ, 70, 678.Google Scholar

Hoglund, B. and Mezger, P. G. 1965b, Hydrogen Emission Line n₁₁₀→n₁₀₉: Detection at 5009 Megahertz in Galactic H II Regions, Science, 150, 339.Google Scholar

Horowitz, P. and Sagan, C. 1993, Five Years of Project Meta: An All-Sky Narrow-Band Radio Search for Extraterrestrial Signals, ApJ, 415, 218.Google Scholar

Hotan, A. W. 2021, Australian Square Kilometre Array Pathfinder: I. System Description, PASA, 38, 9.CrossRefGoogle Scholar

Howard, W. E., Barrett, A. H., and Haddock, F. T. 1962, Measurement of the Microwave Radiation from the Planet Mercury, ApJ, 136, 995.Google Scholar

Howell, T. F. and Shakeshaft, J. R. 1966, Measurement of the Minimum Cosmic Background Radiation at 20.7-cm Wave-Length, Nature, 210, 1318.Google Scholar

Howell, T. F. and Shakeshaft, J. R. 1967, Spectrum of the 3° K Cosmic Microwave Radiation, Nature, 216, 753.Google Scholar

Hoyle, F. 1948, A New Model for the Expanding Universe, MNRAS, 108, 372.Google Scholar

Hoyle, F. 1959, The Relation of Radio Astronomy to Cosmology. In IAU Symposium no. 9, Paris Symposium on Radio Astronomy, ed. Bracewell, R. N. (Stanford: Stanford University Press), 529.Google Scholar

Hoyle, F. 1968, The Bakerian Lecture: Review of Recent Developments in Cosmology, Proc. Roy. Soc. London, 308, 1.Google Scholar

Hoyle, F. 1981, The Quasar Controversy Resolved (Cardiff: University College Cardiff Press).Google Scholar

Hoyle, F. 1982, The Universe Past and Present, ARAA, 220, 1.Google Scholar

Hoyle, F. and Burbidge, G. 1966, On the Nature of the Quasi-Stellar Objects, ApJ, 144, 534.Google Scholar

Hoyle, F. and Fowler, W. A. 1963, Nature of Strong Radio Sources, Nature, 197, 533.Google Scholar

Hoyle, F. and Narlikar, J. 1961, On the Counting of Radio Sources in the Steady-State Cosmology, MNRAS, 123, 133.CrossRefGoogle Scholar

Hoyle, F. and Narlikar, J. 1962, On the Counting of Radio Sources in the Steady-State Cosmology, II, MNRAS, 125, 13.Google Scholar

Hoyle, F., Burbidge, G., and Narlikar, J. V. 1994, Astrophysical Deductions from the Quasi-Steady-State Cosmology, MNRAS, 267, 1007.Google Scholar

Hubble, E. 1936a, The Realm of the Nebulae (New Haven: Yale University Press), reprinted 1958 by Dover Publications Inc.Google Scholar

Hubble, E. 1936b, Effects of Red Shifts on the Distribution of Nebulae, PNAS, 22, 621.Google Scholar

Hulse, R. A. 1994a, The Discovery of the Binary Pulsar, Rev. Mod. Phys., 66, 699.Google Scholar

Hulse, R. A. 1994b, The Discovery of the Binary Pulsar, BAAS, 26, 971.Google Scholar

Hulse, R. A. and Taylor, J. H. 1974a, A High Sensitivity Pulsar Survey, ApJ, 191, L59.Google Scholar

Hulse, R. A. and Taylor, J. H. 1974b, Discovery of a Pulsar in a Close Binary System, BAAS, 6, 453.Google Scholar

Hulse, R. A. and Taylor, J. H. 1975, Discovery of a Pulsar in a Binary System, ApJ, 195, L51.Google Scholar

Humphreys, E. M. L. et al. 2013, Toward a New Geometric Distance to the Active Galaxy NGC 4258. III. Final Results and the Hubble Constant, ApJ, 775, 13.Google Scholar

Hyman, S. D. et al. 2005, A Powerful Bursting Radio Source toward the Galactic Center, Nature, 434, 50.Google Scholar

Jaffe, A. H. et al. 2001, Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR Cosmic Microwave Background Observations, Phys. Rev. Let., 86, 3475.Google Scholar

Jakes, W. C. 1963, Participation of the Holmdel Station in the Telstar Project, Bell Syst. Tech. J., 42, 1421.Google Scholar

Jansky, C. M, Jr. 1958, The Discovery and Identification by Karl Guthe Jansky of Electromagnetic Radiation of Extraterrestrial Origin in the Radio Spectrum, Proc. IRE, 46, 13.Google Scholar

Jansky, K. G. 1932, Directional Studies of Atmospherics at High Frequencies, Proc. IRE, 20, 1920.Google Scholar

Jansky, K. G. 1933a, Electrical Disturbances Apparently of Extraterrestrial Origin, Proc. IRE, 21, 1387.Google Scholar

Jansky, K. G. 1933b, Radio Waves from Outside the Solar System, Nature, 132, 66.CrossRefGoogle Scholar

Jansky, K. G. 1933c, Electrical Phenomena that Apparently Are of Interstellar Origin, Popular Astronomy, 41, 548.Google Scholar

Jansky, K. G. 1935, A Note on the Source of Interstellar Interference, Proc. IRE, 23, 1158.Google Scholar

Jansky, K. G. 1937, Minimum Noise Levels Obtained on Short Wave Receiving Systems, Proc. IRE, 25, 1517.Google Scholar

Jansky, K. G. 1939, An Experimental Investigation of the Characteristics of Certain Types of Noise, Proc. IRE, 27, 763.Google Scholar

Jarosik, N. et al. 2007, Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles, Data Processing, Radiometer Characterization, and Systematic Error Limits, ApJS, 170, 263.Google Scholar

Jauncey, D. 1967, Re-Examination of the Source Counts for the 3C Revised Catalogue, Nature, 216, 877.Google Scholar

Jauncey, D. J. 1975, Radio surveys and Source Counts, ARAA, 13, 23.Google Scholar

Jeans, J. 1929, Astronomy and Cosmogony (Cambridge: The University Press).Google Scholar

Jeffrey, R. M. et al. 2016, Fast Launch Speeds in Radio Flares, From a New Determination of the Intrinsic Motions of SS 433’s Jet Bolides, MNRAS, 461, 312.Google Scholar

Jennison, R. C. and Das Gupta, M. K. 1953, Fine Structure in the Extraterrestrial Radio Source Cygnus I, Nature, 172, 996.Google Scholar

Jones, D. E. 1961, The Microwave Temperature of Venus, Planet. Space Sci., 5, 166.Google Scholar

Kaidanovsky, N. I. 2012, The Department of Radio Astronomy of the Main Astrophysical Observatory. In A Brief History of Radio Astronomy in the USSR (English ed.), ed. Kellermann, K. I. (Dordrecht: Springer), 127.Google Scholar

Kapahi, V. K. 1987, The Angular Size-Redshift Relation as a Cosmological Tool. In IAU Symposium no. 124, Observational Cosmology, ed. Hewitt, A., Burbidge, G., and Fang, L. Z. (Dordrecht: Reidel), 251.Google Scholar

Kardashev, N. 1959, On the Possibility of Detection of Allowed Lines of Atomic Hydrogen in the Radio Frequency Spectrum, Sov. Astron., 3, 813; Russian original, Astron. Zh., 36, 838.Google Scholar

Kardashev, N. 1962, Nonstationarity of Spectra of Young Sources of Nonthermal Radio Emission, Sov. Astron., 6, 317; Russian original: Astron. Zh., 39, 393.Google Scholar

Kardashev, N. et al. 2013, RadioAstron-A Telescope with a Size of 300 000 km: Main Parameters and First Observational Results, Astron. Rpts., 57, 153. Russian original, Astron. Zh. 2013, 90, 179.Google Scholar

Kaspi, V. M. and Beloborodov, A. M. 2017, Magnetars, ARAA, 55, 261.Google Scholar

Kauffman, H. 1946, A DX Record: To the Moon and Back, QST, 30, 65.Google Scholar

Kaufman, M. 1965, Limits on the Density of Intergalactic Ionized Hydrogen, Nature, 207, 736.Google Scholar

Kellermann, K. I. 1964, The Spectra of Non-Thermal Radio Sources, ApJ, 140, 969.Google Scholar

Kellermann, K. I. 1965a, 11 cm Observations of the Temperature of Mercury, Nature, 205, 1091.Google Scholar

Kellermann, K. I. 1965b, Radio Observations of Mars, Nature, 206, 1034.Google Scholar

Kellermann, K. I. 1966, The Thermal Radio Emission from Mercury, Venus, Mars, Saturn, and Uranus, Icarus, 5, 478.Google Scholar

Kellermann, K. I. 1972, Radio Galaxies, Quasars, and Cosmology, AJ, 77, 531.Google Scholar

Kellermann, K. I. 1993, The Cosmological Deceleration Parameter Estimated from the Angular-Size/Redshift Relation for Compact Radio Sources, Nature, 361, 134.Google Scholar

Kellermann, K. I. 1996, John Gatenby Bolton (1922–1993), PASP, 108, 729.Google Scholar

Kellermann, K. I. 1999, Grote Reber’s Observations on Cosmic Static, ApJ, 525, 37.Google Scholar

Kellermann, K. I. 2003, Grote Reber (1911–2002), Nature, 421, 596.CrossRefGoogle ScholarPubMed

Kellermann, K. I. 2004, Grote Reber (1911–2002), PASP, 116, 703.Google Scholar

Kellermann, K. I. 2014, The Discovery of Quasars and Its Aftermath, J. Astron. Hist. Heritage, 17, 267.Google Scholar

Kellermann, K. I., and Cohen, M. H. 1988, The Origin and Evolution of the NRAO-Cornell VLBI System, JRASC, 82, 248.Google Scholar

Kellermann, K. I. and Moran, J. M. 2001, The Development of High-Resolution Imaging in Radio Astronomy, ARAA, 29, 457.Google Scholar

Kellermann, K. I. and Pauliny-Toth, I. I. K. 1966a, Observations of the Radio Emission from Uranus, Neptune, and Other Planets at 1.9 cm, ApJ, 145, L954.Google Scholar

Kellermann, K. I. and Pauliny-Toth, I. I. K. 1966b, A Search for Radio Emission from the Star Alpha Orionis, ApJ, 145, 953.Google Scholar

Kellermann, K. I. and Pauliny-Toth, I. I. K. 1968, Variable Radio Sources, ARAA, 6, 417.CrossRefGoogle Scholar

Kellermann, K. I. and Pauliny-Toth, I. I. K. 1969, The Spectra of Opaque Radio Sources, ApJ, 155, 71.CrossRefGoogle Scholar

Kellermann, K. I. and Sheets, B. 1984, Serendipitous Discoveries in Radio Astronomy (Green Bank: NRAO).Google Scholar

Kellermann, K. I. and Wall, J. V. 1987, Radio Source Counts and Their Interpretation. In IAU Symposium 124, Observational Cosmology, ed. Hewett, A. et al. (Dordrecht: Reidel), 545.Google Scholar

Kellermann, K. I., Bouton, E. N., and Brandt, S. S. 2020, Open Skies: The National Radio Astronomy Observatory and Its Impact on US Radio Astronomy (Cham: Springer).Google Scholar

Kellermann, K. I., Davis, M. M., and Pauliny-Toth, I. I. K. 1971, Counts of Radio Sources at 6-Centimeter Wavelength, ApJ, 170, L1.CrossRefGoogle Scholar

Kellermann, K. I., Orchiston, W., and Slee, B. 2005, Gordon James Stanley and the Early Development of Radio Astronomy in Australia and the United States, PASA, 22, 13.Google Scholar

Kellermann, K. I., Pauliny-Toth, I. I. K., and Williams, P. J. 1969, The Spectra of Radio Sources in the Revised 3C Catalogue, ApJ, 157, 1.Google Scholar

Kellermann, K. I. et al. 1962, A Correlation between the Spectra of Non-thermal Radio Sources and Their Brightness Temperatures, Nature, 195, 692.Google Scholar

Kellermann, K. I. et al. 1977, The Small Radio Source at the Galactic Center, ApJ, 214, L61.Google Scholar

Kellermann, K. I. et al. 1989, VLA Observations of Objects in the Palomar Bright Quasar Survey, AJ, 96, 1195.Google Scholar

Kellermann, K. I. et al. 2004, Sub-Milliarcsecond Imaging of Quasars and Active Galactic Nuclei. III. Kinematics of Parsec-scale Radio Jets, ApJ, 609, 539.Google Scholar

Kellermann, K. I. et al. 2016, Radio-Loud and Radio-Quiet QSOs, ApJ, 831, 168.Google Scholar

Kennefick, D. 2009, Testing Relativity from the 1919 Eclipse: A Question of Bias, Phys. Today, 62, 37.Google Scholar

Khaikin, S. E. and Chikhachev, B. M. 1948, Investigation of Radio Emission from the Sun during the Total Solar Eclipse of May 20, 1947, Izvestiya Akad. Nauk SSSR, 12, 38 (in Russian).Google Scholar

Kiepenheuer, K. O. 1950, Cosmic Rays As the Source of General Galactic Radio Emission, Phys. Rev., 79, 738.CrossRefGoogle Scholar

Kinman, T. D. 1965, The Nature of the Fainter Haro-Luyten Objects, ApJ, 142, 1241.Google Scholar

Klein, M. J. and Seling, T. V. 1966, Radio Emission from Uranus at 8 Gc/s, ApJ, 146, 599.Google Scholar

Kleppner, D. and Horowitz, P. 2016, A Perfect Proposal, Phys. Today, 69, 48.Google Scholar

Knight, C. A. et al. 1971, Quasars: Millisecond-of-Arc Structure Revealed by Very-Long-Baseline Interferometry, Science, 172, 52.Google Scholar

Knowles, S. G. et al. 1969a, Spectra, Variability, Size, Polarization of H₂O Microwave Emission in the Galaxy, Science, 163, 1055.Google Scholar

Knowles, S. G. et al. 1969b, Galactic Water Vapor Emission: Further Observations of Variability, Science, 166, 221.Google Scholar

Kotelnikov, V. 1961, Radar Contact with Venus, J. Br. Inst. Radio Eng., 22, 293.Google Scholar

Kotelnikov, V. 1963, Radar Observations of the Planet Venus in the Soviet Union in April, 1963, Science Report of the Institute of Radio Engineering and Electronics, Moscow. English translation by the Defense Documentation Center.Google Scholar

Kozyrev, N. A. 1964, The Atmosphere of Mercury, Sky Tel., 27, 339.Google Scholar

Kragh, H. 1996, Cosmology and Controversy (Princeton: Princeton University Press).Google Scholar

Kragh, H. 2017, The Nobel Prize System and the Astronomical Sciences, J. Hist. Astron., 48, 257.CrossRefGoogle Scholar

Kramer, M. et al. 2021, Strong-Field Gravity Tests with the Double Pulsar, Phys. Rev. X, 11, 041050.Google Scholar

Kraus, J. D. 1956, Impulsive Radio Signals from the Planet Venus, Nature, 178, 33; Radio Observations of the Planet Venus at a Wave-length of 11 m., Nature, 178, 103; Class II Radio Signals from Venus at a Wave-length of 11 Metres, Nature, 178, 159.CrossRefGoogle Scholar

Kraus, J. 1984, Karl Guthe Jansky’s Serendipity, Its Impact on Astronomy and Its Lessons for the Future. In Serendipitous Discoveries in Radio Astronomy, ed. Kellermann, K. I. and Sheets, B. (Green Bank: NRAO/AUI), 57.Google Scholar

Kraus, J. 1995, Big Ear Two Listening for Other Worlds (Powell: Cygnus-Quasar Books).Google Scholar

Kuiper, G. P. 1952, The Atmospheres of the Earth and Planets (Chicago: University of Chicago Press).Google Scholar

Kulkarni, S. R. et al. 2014, Giant Sparks at Cosmological Distances?, ApJ, 797, 70.Google Scholar

Kusch, P. and Prodell, A. G. 1950, On the Hyperfine Structure of Hydrogen and Deuterium, Phys. Rev., 79, 1009.Google Scholar

Langer, R. M. 1936, Radio Noise from the Galaxy, Phys. Rev., 49, 209.Google Scholar

Lebach, D. E. et al. 1995, Measurement of the Solar Gravitational Deflection of Radio Waves Using Very-Long-Baseline Interferometry, Phys. Rev. Let., 75, 1439.CrossRefGoogle ScholarPubMed

Legg, T. H. 1970, Redshift and the Size of Double Radio Sources, Nature, 226, 64.CrossRefGoogle ScholarPubMed

Lequeux, J. 1962, Mesures Interférométriques a Haute Résolution du Diamétre et de la Structure des Principales Radiosources, Ann. Astrophys., 25, 221.Google Scholar