Skip to main content Accessibility help
×
Home
Hostname: page-component-559fc8cf4f-sbc4w Total loading time: 0.499 Render date: 2021-03-01T04:50:06.245Z Has data issue: true Feature Flags: { "shouldUseShareProductTool": true, "shouldUseHypothesis": true, "isUnsiloEnabled": true, "metricsAbstractViews": false, "figures": false, "newCiteModal": false, "newCitedByModal": true }

ATLAS probe: Breakthrough science of galaxy evolution, cosmology, Milky Way, and the Solar System

Published online by Cambridge University Press:  08 April 2019

Yun Wang
Affiliation:
IPAC, California Institute of Technology, Mail Code 314-6, 1200 East California Blvd., Pasadena, CA 91125, USA
Massimo Robberto
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA Department of Physics & Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA
Mark Dickinson
Affiliation:
NOAO, 950 North Cherry Ave., Tucson, AZ 85719, USA
Lynne A. Hillenbrand
Affiliation:
Department of Astronomy, California Institute of Technology, Mail Code 249-17, 1200 East California Blvd., Pasadena, CA 91125, USA
Wesley Fraser
Affiliation:
School of Mathematics and Physics, Queen’s University Belfast, University Road, BT7 1NN Belfast, UK
Peter Behroozi
Affiliation:
Steward Observatory, University of Arizona, 933 N Cherry Ave., Tucson, AZ 85719, USA
Jarle Brinchmann
Affiliation:
Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA Leiden, The Netherlands Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT-4150-762 Porto, Portugal
Chia-Hsun Chuang
Affiliation:
Department of Physics, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305, USA
Andrea Cimatti
Affiliation:
Department of Physics and Astronomy, Alma Mater Studiorum - University of Bologna, via Gobetti 93/2, I-40129 Bologna, Italy INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy
Robert Content
Affiliation:
Australian Astronomical Optics, Macquarie University, 105 Delhi Road, North Ryde, NSW 2113, Australia
Emanuele Daddi
Affiliation:
CEA, IRFU, DAp, AIM, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, CNRS, F-91191 Gif-sur-Yvette, France
Henry C. Ferguson
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
Christopher Hirata
Affiliation:
Center for Cosmology and Astroparticle Physics, The Ohio State University, 191 West Woodruff Avenue, Columbus, OH 43210
Michael J. Hudson
Affiliation:
Department of Physics & Astronomy, University of Waterloo, 200 University Avenue West, Waterloo, ON, CanadaN2L 3G1
J. Davy Kirkpatrick
Affiliation:
IPAC, California Institute of Technology, Mail Code 314-6, 1200 East California Blvd., Pasadena, CA 91125, USA
Alvaro Orsi
Affiliation:
Centro de Estudios de Física del Cosmos de Aragón, Plaza de San Juan 1, Teruel 44001, Spain
Russell Ryan
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
Alice Shapley
Affiliation:
Department of Physics & Astronomy, UCLA, 430 Portola Plaza, P.O. Box 951547, Los Angeles, CA 90095-1547, USA
Mario Ballardini
Affiliation:
Department of Physics & Astronomy, University of the Western Cape, Cape Town 7535, South Africa INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, via Gobetti 93/3, I-40129 Bologna, Italy
Robert Barkhouser
Affiliation:
Department of Physics & Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA
James Bartlett
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
Robert Benjamin
Affiliation:
Department of Physics, University of Wisconsin - Whitewater, 800 W. Main Street, Whitewater, WI 53190-1790, USA
Ranga Chary
Affiliation:
IPAC, California Institute of Technology, Mail Code 314-6, 1200 East California Blvd., Pasadena, CA 91125, USA
Charlie Conroy
Affiliation:
Harvard Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Megan Donahue
Affiliation:
Physics and Astronomy Department, Michigan State University, 567 Wilson Rd., East Lansing, MI 48824, USA
Olivier Doré
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
Peter Eisenhardt
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
Karl Glazebrook
Affiliation:
Centre for Astrophysics & Supercomputing, Mail number H29, Swinburne University of Technology, P.O. Box 218, Hawthorn, VIC 3122, Australia
George Helou
Affiliation:
IPAC, California Institute of Technology, Mail Code 314-6, 1200 East California Blvd., Pasadena, CA 91125, USA
Sangeeta Malhotra
Affiliation:
Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771, USA
Lauro Moscardini
Affiliation:
Department of Physics and Astronomy, Alma Mater Studiorum - University of Bologna, via Gobetti 93/2, I-40129 Bologna, Italy INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, via Gobetti 93/3, I-40129 Bologna, Italy INFN - Sezione di Bologna, viale Berti Pichat 6/2, I-40127 Bologna, Italy
Jeffrey A. Newman
Affiliation:
University of Pittsburgh and PITT PACC, 3941 O’Hara St., Pittsburgh, PA 15260, USA
Zoran Ninkov
Affiliation:
Center for Imaging Science, Rochester Institute of Technology, 54 Lomb Memorial Drive, Rochester, NY 14623, USA
Michael Ressler
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
James Rhoads
Affiliation:
Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771, USA
Jason Rhodes
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
Daniel Scolnic
Affiliation:
Department of Physics, Duke University, Durham, NC 27708, USA
Stephen Smee
Affiliation:
Department of Physics & Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA
Francesco Valentino
Affiliation:
Cosmic Dawn Center (DAWN), Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen Ø, Denmark DTU-Space, Technical University of Denmark, Elektrovej 327, DK-2800 Kgs. Lyngby, Denmark
Risa H. Wechsler
Affiliation:
Department of Physics, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305, USA Particle Physics & Astrophysics Department, SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
Corresponding
E-mail address:

Abstract

Astrophysics Telescope for Large Area Spectroscopy Probe is a concept for a National Aeronautics and Space Administration probe-class space mission that will achieve ground-breaking science in the fields of galaxy evolution, cosmology, Milky Way, and the Solar System. It is the follow-up space mission to Wide Field Infrared Survey Telescope (WFIRST), boosting its scientific return by obtaining deep 1–4 μm slit spectroscopy for ∼70% of all galaxies imaged by the ∼2 000 deg2 WFIRST High Latitude Survey at z > 0.5. Astrophysics Telescope for Large Area Spectroscopy will measure accurate and precise redshifts for ∼200 M galaxies out to z < 7, and deliver spectra that enable a wide range of diagnostic studies of the physical properties of galaxies over most of cosmic history. Astrophysics Telescope for Large Area Spectroscopy Probe and WFIRST together will produce a 3D map of the Universe over 2 000 deg2, the definitive data sets for studying galaxy evolution, probing dark matter, dark energy and modifications of General Relativity, and quantifying the 3D structure and stellar content of the Milky Way. Astrophysics Telescope for Large Area Spectroscopy Probe science spans four broad categories: (1) Revolutionising galaxy evolution studies by tracing the relation between galaxies and dark matter from galaxy groups to cosmic voids and filaments, from the epoch of reionisation through the peak era of galaxy assembly; (2) Opening a new window into the dark Universe by weighing the dark matter filaments using 3D weak lensing with spectroscopic redshifts, and obtaining definitive measurements of dark energy and modification of General Relativity using galaxy clustering; (3) Probing the Milky Way’s dust-enshrouded regions, reaching the far side of our Galaxy; and (4) Exploring the formation history of the outer Solar System by characterising Kuiper Belt Objects. Astrophysics Telescope for Large Area Spectroscopy Probe is a 1.5 m telescope with a field of view of 0.4 deg2, and uses digital micro-mirror devices as slit selectors. It has a spectroscopic resolution of R = 1 000, and a wavelength range of 1–4 μm. The lack of slit spectroscopy from space over a wide field of view is the obvious gap in current and planned future space missions; Astrophysics Telescope for Large Area Spectroscopy fills this big gap with an unprecedented spectroscopic capability based on digital micro-mirror devices (with an estimated spectroscopic multiplex factor greater than 5 000). Astrophysics Telescope for Large Area Spectroscopy is designed to fit within the National Aeronautics and Space Administration probe-class space mission cost envelope; it has a single instrument, a telescope aperture that allows for a lighter launch vehicle, and mature technology (we have identified a path for digital micro-mirror devices to reach Technology Readiness Level 6 within 2 yr). Astrophysics Telescope for Large Area Spectroscopy Probe will lead to transformative science over the entire range of astrophysics: from galaxy evolution to the dark Universe, from Solar System objects to the dusty regions of the Milky Way.

Type
Research Article
Copyright
Copyright © Astronomical Society of Australia 2019 

Access options

Get access to the full version of this content by using one of the access options below.

References

Abell, P. A., et al. 2009, LSST Science Book, arXiv:0912.0201Google Scholar
Abolfathi, B., et al. 2017, arXiv:1707.09322Google Scholar
Aghamousa, A., et al. 2016, The DESI experiment part I: science, targeting, and survey design, arXiv:1611.00036Google Scholar
Alcorn, L. Y., et al. 2018, ApJ, 858, 47CrossRefGoogle Scholar
Alvarez-Candal, A., et al. 2011, A&A, 532, 130Google Scholar
Baldwin, J. A., Phillips, M. M., & Terlevich, R. 1981, PASP, 93, 5CrossRefGoogle Scholar
Baraffe, I., Chabrier, G., Barman, T. S., Allard, F., & Hauschildt, P. H. 2003, 402, 701Google Scholar
Barkume, K. M., Brown, M. E., & Schaller, E. L. 2008, AJ, 135, 55CrossRefGoogle Scholar
Barucci, M. A., et al. 2011, ICARUS, 214, 297CrossRefGoogle Scholar
Bate, M. R. 2014, MNRAS, 442, 285CrossRefGoogle Scholar
Behroozi, P., et al. 2013, ApJ, 770, 57CrossRefGoogle Scholar
Belli, S., et al. 2017, ApJ, 834, 18CrossRefGoogle Scholar
Blake, C., & Glazebrook, K. 2003, ApJ, 594, 665BCrossRefGoogle Scholar
Bruzual, G., & Charlot, S. 2003, MNRAS, 344, 1000CrossRefGoogle Scholar
Bowler, R., et al. 2017, MNRAS, 469, 448CrossRefGoogle Scholar
Brown, M. E., Schaller, E. L., & Fraser, W. C. 2012, AJ, 143, 146CrossRefGoogle Scholar
Burgasser, A. J., Blake, C. H., Gelino, C. R., Sahlmann, J., & Bardalez Gagliuffi, D. 2016, ApJ, 827, 25CrossRefGoogle Scholar
Burgasser, A. J., Sheppard, S. S., & Luhman, K. L. 2013, ApJ, 772, 129CrossRefGoogle Scholar
Burgasser, A. J. 2007, AJ, 134, 1330CrossRefGoogle Scholar
Burrows, A., et al. 1997, ApJ, 491, 856CrossRefGoogle Scholar
Calabrò, A., et al. 2018, ApJ, 862, L22CrossRefGoogle Scholar
Calzetti, D., Armus, L., Bohlin, R. C., Kinney, A. L., Koornneef, J., & Storchi-Bergmann, T. 2000, ApJ, 533, 682CrossRefGoogle Scholar
Carbone, C., Verde, L., Wang, Y., & Cimatti, A. 2011, JCAP 03, 030CrossRefGoogle Scholar
Cardelli, J. A., Clayton, G. C., & Mathis, J. S. 1989, ApJ, 345, 245CrossRefGoogle Scholar
Carey, S., et al. 2008, in Spitzer Proposal ID No. 50398Google Scholar
Castellano, M., et al. 2016, ApJL, 818, L3CrossRefGoogle Scholar
Chabrier, G. 2003, PASP, 115, 763CrossRefGoogle Scholar
Chuang, C. H., Kitaura, F. S., Prada, F., Zhao, C., & Yepes, G. 2015, MNRAS, 446, 2621CrossRefGoogle Scholar
Churchwell, E., et al. 2009, PASP, 121, 213CrossRefGoogle Scholar
Cedeno, F. X. L., Gonzalez-Morales, A. X., & Urena-Lopez, L. A. 2017, PhRvD, 96, 061301Google Scholar
Charlot, S., & Fall, S. M. 2000, ApJ, 539, 718CrossRefGoogle Scholar
Chen, Y.-M., et al. 2010, AJ, 140, 445CrossRefGoogle Scholar
Cimatti, A., et al. (the SPACE Team), 2009, ExA, 23, 39Google Scholar
Connelley, M. S., & Greene, T. P. 2010, AJ, 140, 1214CrossRefGoogle Scholar
Conroy, C., Gunn, J. E., & White, M. 2009, ApJ, 699, 486CrossRefGoogle Scholar
Content, R. 2008, in Proceedings of the SPIE, 701025Google Scholar
Content, R., et al. 2008, in Proceedings of the SPIE, 70104SGoogle Scholar
Cooper, H. D. B., et al. 2013, MNRAS, 430, 1125CrossRefGoogle Scholar
Cruikshank, D. P., et al. 1998, ICARUS, 135, 389CrossRefGoogle Scholar
Cushing, M. C., Rayner, J. T., & Vacca, W. D. 2005, ApJ, 623 1115CrossRefGoogle Scholar
Cushing, M. C., et al. 2011, ApJ, 743, 50CrossRefGoogle Scholar
Cushing, M. C., et al. 2014, AJ, 147, 113CrossRefGoogle Scholar
Daddi, E., et al. 2007, ApJ, 670, 156CrossRefGoogle Scholar
Draine, B. T., & Li, A. 2001, ApJ, 551, 807CrossRefGoogle Scholar
Draine, B. T. 2011, in Physics of the Interstellar and Intergalactic Medium, ed. Draine, B. T. (Princeton University Press). ISBN: 978-0-691-12214-4.Google Scholar
Driver, S., et al. 2009, A&G, 50, 5.12Google Scholar
Elbaz, D., et al. 2007, A&A, 468, 33Google Scholar
Epps, S. D., & Hudson, M. J. 2017, MNRAS, 468, 2605CrossRefGoogle Scholar
Feltre, A., Charlot, S., & Gutkin, J. 2016, MNRAS, 456, 3354CrossRefGoogle Scholar
Ferreras, I., et al., Chronos: a NIR spectroscopic galaxy survey. From the formation of galaxies to the peak of activity, arXiv:1306.6333, white paper for the science definition of ESA’s future L2, L3 missionsGoogle Scholar
Finkelstein, S. L. 2016, PASA, 33, 37CrossRefGoogle Scholar
Fourspring, K., et al. 2013, Opt. Eng. 52, 091807CrossRefGoogle Scholar
Fraser, W. C., & Brown, M. E. 2012, ApJ, 749, 33CrossRefGoogle Scholar
Fraser, W. C., Brown, M. E., Morbidelli, A., Parker, A., & Batygin, K. 2014, ApJ, 782, 100CrossRefGoogle Scholar
Fraser, W. C., Brown, M. E., & Glass, F. ApJ, 804, 31CrossRefGoogle Scholar
Fraser, W. C., et al. 2017, NatAs, 1, 88Google Scholar
Fraser, W. C., & Brown, M. E. 2018, AJ, 156, 23FCrossRefGoogle Scholar
Gagrani, P., & Samushia, L. 2017, MNRAS, 467, 928Google Scholar
Gizis, J. E., & Reid, I. N. 1999, AJ, 117, 508CrossRefGoogle Scholar
Gladman, B., Marsden, B. G., & Vanlaerhoven, C. 2008, in The Solar System Beyond Neptune, ed. M. Barucci, A., Boehnhardt, H., Cruikshank, D. P., Morbidelli, A., & Dotson, R. (Tucson: University of Arizona Press), 43Google Scholar
Gobat, R., et al. 2013, ApJ, 776, 9CrossRefGoogle Scholar
Gonzalez, O. A., et al. 2012, A&A 543, A13Google Scholar
Gonzalez-Perez, V., et al. 2018, MNRAS, 474, 4024CrossRefGoogle Scholar
Guo, Y., et al. 2013, ApJS, 207, 24CrossRefGoogle Scholar
Guzzo, L., et al. 2008, Nature, 451, 541CrossRefGoogle ScholarPubMed
Hearin, A. P., Behroozi, P. S., & van den Bosch, F. C. 2016, MNRAS, 461, 2135CrossRefGoogle Scholar
Hlozek, R., Grin, D., Marsh, D. J. E., & Ferreira, P. G. 2015, PhRvD, 91, 103512Google Scholar
Hogg, D. W., Eilers, A.-C., & Rix, H.-W. 2018, Spectrophotometric parallaxes with Linear models: Accurate distances for Luminous red–giant starsGoogle Scholar
Hora, J., et al. 2007, in Spitzer Proposal ID No. 40184Google Scholar
Hounsell, R., et al. 2018, ApJ, 867, 23CrossRefGoogle Scholar
Hudson, M. J., et al. 2015, MNRAS, 447, 298CrossRefGoogle Scholar
Ibata, R. A., et al. 2017, ApJ, 848, 128CrossRefGoogle Scholar
Izotov, Y. I., et al. 2018, MNRAS, 474, 4514CrossRefGoogle Scholar
Izquierdo-Villalba, D., Orsi, A. A., Bonoli, S., Lacey, C. G., Baugh, C. M., & Griffin, A. J. 2018, MNRAS, 480, 1340CrossRefGoogle Scholar
Kashino, D., et al. 2013, ApJ, 777, L8CrossRefGoogle Scholar
Kennicutt, R. C. Jr 1998, ARA&A, 36, 189CrossRefGoogle Scholar
Khostovan, A. A., et al. 2015, MNRAS, 452, 3948CrossRefGoogle Scholar
Kirkpatrick, J. D., et al. 2016, ApJS, 224, 36CrossRefGoogle Scholar
Kirkpatrick, J. D., et al. 2014, ApJ, 783, 122CrossRefGoogle Scholar
Kirkpatrick, J. D., et al. 2012, ApJ, 753, 156CrossRefGoogle Scholar
Kirkpatrick, J. D., et al. 2010, ApJS, 190, 100CrossRefGoogle Scholar
Kirkpatrick, J. D. 2005, ARA&A, 43, 195CrossRefGoogle Scholar
Kraljic, K., et al. 2018, MNRAS, 474, 547CrossRefGoogle Scholar
Kravtsov, A. V., et al. 2013, ApJ, 764, 31CrossRefGoogle Scholar
Kriek, M., et al. 2009, ApJ, 700, 221CrossRefGoogle Scholar
Lacey, C. G., et al. 2016, MNRAS, 462, 3854CrossRefGoogle Scholar
Lagos, C. d. P., et al. 2014, MNRAS, 443, 1002CrossRefGoogle Scholar
Laureijs, R., et al. 2011, Euclid definition study report, arXiv:1110.3193Google Scholar
Lee, C. T., et al. 2017, MNRAS, 466, 3834CrossRefGoogle Scholar
Lépine, S., & DiStefano, R. 2012, ApJ, 749, L6CrossRefGoogle Scholar
Lesgourgues, J., & Pastor, S. 2006, PhR, 429, 307Google Scholar
Levison, H. F., Morbidelli, A., Van Laerhoven, C., Gomes, R., & Tsiganis, K. 2008, ICARUS, 196, 258CrossRefGoogle Scholar
Long, P., et al. 2017, ApJ, 840, 92CrossRefGoogle Scholar
Lucas, P. W., et al. 2010, MNRAS, 408, L56CrossRefGoogle Scholar
Luhman, K. L. 2013, ApJ, 767, L1CrossRefGoogle Scholar
MacKenty, J., et al. 2006, SPIE, 6269, 15Google Scholar
Majewski, S., et al. 2007, in Spitzer Proposal ID No. 40791Google Scholar
Marchesini, D., et al. 2007, ApJ, 656, 42CrossRefGoogle Scholar
Martin, C. L., et al. 2012, ApJ, 760, 127CrossRefGoogle Scholar
McDonald, P., & Seljak, U. 2009, JCAP, 10, 007CrossRefGoogle Scholar
Meade, M. R., et al. 2014, GLIMPSE360 data description GLIMPSE360: completing the Spitzer galactic plane survey, https://irsa.ipac.caltech.edu/data/SPITZER/GLIMPSE/doc/glimpse360_dataprod_v1.5.pdfGoogle Scholar
Merson, A., et al. 2018, MNRAS, 474, 177CrossRefGoogle Scholar
Meyer, R. D., et al. 2004, SPIE, 5492, 200MGoogle Scholar
Miyatake, H., et al. 2015, ApJ, 806, 1CrossRefGoogle Scholar
More, S., et al. 2016, ApJ, 825, 39CrossRefGoogle Scholar
Mostek, N., et al. (2013), ApJ, 767, 89CrossRefGoogle Scholar
Moster, B. P., Naab, T., & White, S. D. M. 2013, MNRAS 428, 3121CrossRefGoogle Scholar
Nesvorný, D., Vokrouhlický, D., & Morbidelli, A. 2007, AJ, 133, 1962Google Scholar
Newman, J. A. 2008, ApJ, 684, 88CrossRefGoogle Scholar
Newman, J. A., et al. 2015, APh, 63, 81Google Scholar
Noeske, K. G., et al. 2007, ApJ, 660, L43CrossRefGoogle Scholar
Norris, R. P., et al. 2011, PASA, 28, 215CrossRefGoogle Scholar
Orsi, Á., Baugh, C. M., Lacey, C. G., Cimatti, A., Wang, Y., & Zamorani, G. 2010, MNRAS, 405, 1006Google Scholar
Orsi, Á.,, et al. 2014, MNRAS, 443, 799CrossRefGoogle Scholar
Orsi, Á.,Fanidakis, N., Lacey, C. G., & Baugh, C. M. 2016, MNRAS, 456, 3827CrossRefGoogle Scholar
Pannella, M., et al. 2015, ApJ, 807, 141CrossRefGoogle Scholar
Parker, A., et al. 2016, PASP, 128, 8010CrossRefGoogle Scholar
Parker, A., et al. 2015, Arxiv: 1511.01112Google Scholar
Peixinho, N., Delsanti, A., Guilbert-Lepoutre, A., Gafeira, R., & Lacerda, P. 2012, A&A, 546A, 86Google Scholar
Peixinho, N., Delsanti, A., & Doressoundiram, A. 2015, A&A, 577, 35Google Scholar
Perlmutter, S., et al. 1999, ApJ, 517, 565CrossRefGoogle Scholar
Petit, J.-M., et al. 2011, AJ, 142, 131CrossRefGoogle Scholar
Pike, R. E., et al. 2017, AJ, 154, 101CrossRefGoogle Scholar
Pinfield, D. J., et al. 2014, MNRAS, 437, 1009CrossRefGoogle Scholar
Price, S. H., et al. 2016, ApJ, 819, 80CrossRefGoogle Scholar
Pozzetti, L., et al. 2016, A&A, 590A, 3Google Scholar
Puglisi, A., et al. 2016, A&A, 586, A83Google Scholar
Quijada, M., et al. 2016, SPIE, 9912, 99125V-1Google Scholar
Rayner, J. T., Cushing, M. C., & Vacca, W. D. 2009, ApJS, 185, 289CrossRefGoogle Scholar
Riess, A., et al. 1998, AJ, 116, 1009CrossRefGoogle Scholar
Robberto, M., et al. 2016, in Proceedings of the SPIE, Vol. 9908, 99088Google Scholar
Rodighiero, G., et al. 2011, ApJ, 739, L40CrossRefGoogle Scholar
Rodighiero, G., et al. 2014, MNRAS, 443, 19CrossRefGoogle Scholar
Rubin, K. H. R., et al. 2012, ApJL, 747, L26Google Scholar
Ryan, R. E. Jr, & Reid, I. N. 2016, AJ, 151, 92CrossRefGoogle Scholar
Salpeter, E. E. 1955, ApJ, 121, 161CrossRefGoogle Scholar
Sargent, M. T., et al. 2014, ApJ, 793, 19CrossRefGoogle Scholar
Schreiber, C., et al. 2015, A&A, 575, A74Google ScholarPubMed
Senchyna, P., et al. 2017, MNRAS, 472, 2608CrossRefGoogle Scholar
Seo, H., & Eisenstein, D. 2003, ApJ, 598, 720CrossRefGoogle Scholar
Shapley, A. E., et al. 2003, ApJ, 588, 65CrossRefGoogle Scholar
Sheppard, S. S. 2010, AJ, 139, 1394CrossRefGoogle Scholar
Silverman, J. D., et al. 2015, ApJS, 220, 12CrossRefGoogle Scholar
Sobral, D., et al. 2013, MNRAS, 428, 1128CrossRefGoogle Scholar
Sobral, D., et al. 2015, ApJ, 808, 139CrossRefGoogle Scholar
Sobral, D., et al. 2019, MNRAS, 482, 2422CrossRefGoogle Scholar
Spanò, P., et al. 2009, SPIE 7436, 74360O-1Google Scholar
Spergel, D.N., et al. 2015, WFIRST SDT final report, arXiv:1503.03757Google Scholar
Stansberry, J., et al. 2008, The Solar System Beyond Neptune, ed. Barucci, M. A., Boehnhardt, H., Cruikshank, D. P., Morbidelli, A., & Dotson, R. (Tucson, University of Arizona Press) 161Google Scholar
Stark, D. P., et al. 2015, MNRAS, 450, 1846Google Scholar
Steidel, C. C., et al. 2010, ApJ, 717, 289CrossRefGoogle Scholar
Steidel, C. C., et al. 2014, ApJ, 795, 165CrossRefGoogle Scholar
Sullivan, M., et al. 2010, MNRAS, 406, 782Google Scholar
Tiley, A.L., et al. 2019, MNRAS, tmp 432TGoogle Scholar
Tilvi, V., et al. 2014, ApJ, 794, 5CrossRefGoogle Scholar
Travinsky, A., et al. 2017, J. Astron. Telesc. Instrum. Syst., 3, 035003CrossRefGoogle Scholar
Travinsky, A., et al. 2016, Opt. Eng. 55, 094107CrossRefGoogle Scholar
Valentino, F., et al. 2015, ApJ, 801, 132CrossRefGoogle Scholar
Valentino, F., et al. 2016, ApJ, 829, 53CrossRefGoogle Scholar
Valentino, F., et al. 2017, MNRAS, 472, 4878CrossRefGoogle Scholar
Van Dokkum, P. G., Kriek, M., & Franx, M. 2009, Nature, 460, 717CrossRefGoogle Scholar
Vavrek, R. D., et al. (2016), in Proceedings of the SPIE, Vol. 9911, 991105Google Scholar
Verhamme, A., et al. 2017, A&A, 597, 13Google Scholar
Verhamme, A., Schaerer, D., & Maselli, A. 2006, A&A, 460, 397Google Scholar
Vorobiev, D., et al. 2016, SPIE, 9912, 99125M-1Google Scholar
Wang, S., Li, A., & Jiang, B. W. 2015, ApJ, 811, 38CrossRefGoogle Scholar
Wang, Y. 2008, JCAP, 05, 021CrossRefGoogle Scholar
Wang, Y., Spergel, D. N., & Strauss, M. 1999, ApJ, 510, 20CrossRefGoogle Scholar
Wang, Y., Chuang, C.-H., & Hirata, C. M. 2013, MNRAS, 430, 2446CrossRefGoogle Scholar
Wang, T., et al. 2016, ApJ, 828, 56CrossRefGoogle Scholar
Weiner, B. J., et al., 2009, ApJ, 692, 187CrossRefGoogle Scholar
Whitney, B., et al. 2008, in Spitzer Proposal ID No. 60020Google Scholar
Williams, R. J., Quadri, R. F., Franx, M., van Dokkum, P., & Labbé, I. 2009, ApJ, 691, 1879Google Scholar
Zamkotsian, F., et al. 2011, in Proceedings of the SPIE, Vol. 7932, 79320AGoogle Scholar
Zamkotsian, F., et al. 2017, in Proceedings of the SPIE, Vol. 10565, 1056521Google Scholar
Zhai, Z., et al. 2017, ApJ, 848, 76CrossRefGoogle Scholar

Altmetric attention score

Full text views

Full text views reflects PDF downloads, PDFs sent to Google Drive, Dropbox and Kindle and HTML full text views.

Total number of HTML views: 20
Total number of PDF views: 65 *
View data table for this chart

* Views captured on Cambridge Core between 08th April 2019 - 1st March 2021. This data will be updated every 24 hours.

Send article to Kindle

To send this article to your Kindle, first ensure no-reply@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about sending to your Kindle. Find out more about sending to your Kindle.

Note you can select to send to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be sent to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

ATLAS probe: Breakthrough science of galaxy evolution, cosmology, Milky Way, and the Solar System
Available formats
×

Send article to Dropbox

To send this article to your Dropbox account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Dropbox.

ATLAS probe: Breakthrough science of galaxy evolution, cosmology, Milky Way, and the Solar System
Available formats
×

Send article to Google Drive

To send this article to your Google Drive account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Google Drive.

ATLAS probe: Breakthrough science of galaxy evolution, cosmology, Milky Way, and the Solar System
Available formats
×
×

Reply to: Submit a response


Your details


Conflicting interests

Do you have any conflicting interests? *