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LSST: from Science Drivers to Reference Design and Anticipated Data Products

Title: LSST: from Science Drivers to Reference Design and Anticipated Data Products
Authors: Ivezić, Željko; Kahn, Steven M.; Tyson, J.Anthony; Abel, Bob; Acosta, Emily; Allsman, Robyn; Alonso, David; Alsayyad, Yusra; Anderson, Scott F.; Andrew, John; Angel, James Roger P.; Angeli, George Z.; Ansari, Reza; Antilogus, Pierre; Araujo, Constanza; Armstrong, Robert; Arndt, Kirk T.; Astier, Pierre; Aubourg, Éric; Auza, Nicole; Axelrod, Tim S.; Bard, Deborah J.; Barr, Jeff D.; Barrau, Aurelien; Bartlett, James G.; Bauer, Amanda E.; Bauman, Brian J.; Baumont, Sylvain; Bechtol, Ellen; Bechtol, Keith; Becker, Andrew C.; Becla, Jacek; Beldica, Cristina; Bellavia, Steve; Bianco, Federica B.; Biswas, Rahul; Blanc, Guillaume; Blazek, Jonathan; Blandford, Roger D.; Bloom, Josh S.; Bogart, Joanne; Bond, Tim W.; Booth, Michael T.; Borgland, Anders W.; Borne, Kirk; Bosch, James F.; Boutigny, Dominique; Brackett, Craig A.; Bradshaw, Andrew; Brandt, William Nielsen; Brown, Michael E.; Bullock, James S.; Burchat, Patricia; Burke, David L.; Cagnoli, Gianpietro; Calabrese, Daniel; Callahan, Shawn; Callen, Alice L.; Carlin, Jeffrey L.; Carlson, Erin L.; Chandrasekharan, Srinivasan; Charles-Emerson, Glenaver; Chesley, Steve; Cheu, Elliott C.; Chiang, Hsin-Fang; Chiang, James; Chirino, Carol; Chow, Derek; Ciardi, David R.; Claver, Charles F.; Cohen-Tanugi, Johann; Cockrum, Joseph J.; Coles, Rebecca; Connolly, Andrew J.; Cook, Kem H.; Cooray, Asantha; Covey, Kevin R.; Cribbs, Chris; Cui, Wei; Cutri, Roc; Daly, Philip N.; Daniel, Scott F.; Daruich, Felipe; Daubard, Guillaume; Daues, Greg; Dawson, William; Delgado, Francisco; Dellapenna, Alfred; Peyster, Robert De; de Val-Borro, Miguel; Digel, Seth W.; Doherty, Peter; Dubois, Richard; Dubois-Felsmann, Gregory P.; Durech, Josef; Economou, Frossie; Eifler, Tim; Eracleous, Michael; Emmons, Benjamin L.; Fausti Neto, Angelo; Ferguson, Henry; Figueroa, Enrique; Fisher-Levine, Merlin; Focke, Warren; Foss, Michael D.; Frank, James; Freemon, Michael D.; Gangler, Emmanuel; Gawiser, Eric; Geary, John C.; Gee, Perry; Geha, Marla; Gessner, Charles J.B.; Gibson, Robert R.; Gilmore, D.Kirk; Glanzman, Thomas; Glick, William; Goldina, Tatiana; Goldstein, Daniel A.; Goodenow, Iain; Graham, Melissa L.; Gressler, William J.; Gris, Philippe; Guy, Leanne P.; Guyonnet, Augustin; Haller, Gunther; Harris, Ron; Hascall, Patrick A.; Haupt, Justine; Hernandez, Fabio; Herrmann, Sven; Hileman, Edward; Hoblitt, Joshua; Hodgson, John A.; Hogan, Craig; Howard, James D.; Huang, Dajun; Huffer, Michael E.; Ingraham, Patrick; Innes, Walter R.; Jacoby, Suzanne H.; Jain, Bhuvnesh; Jammes, Fabrice; Jee, James; Jenness, Tim; Jernigan, Garrett; Jevremović, Darko; Johns, Kenneth; Johnson, Anthony S.; Johnson, Margaret W.G.; Jones, R.Lynne; Juramy-Gilles, Claire; Jurić, Mario; Kalirai, Jason S.; Kallivayalil, Nitya J.; Kalmbach, Bryce; Kantor, Jeffrey P.; Karst, Pierre; Kasliwal, Mansi M.; Kelly, Heather; Kessler, Richard; Kinnison, Veronica; Kirkby, David; Knox, Lloyd; Kotov, Ivan V.; Krabbendam, Victor L.; Krughoff, K.Simon; Kubánek, Petr; Kuczewski, John; Kulkarni, Shri; Ku, John; Kurita, Nadine R.; Lage, Craig S.; Lambert, Ron; Lange, Travis; Langton, J.Brian; Le Guillou, Laurent; Levine, Deborah; Liang, Ming; Lim, Kian-Tat; Lintott, Chris J.; Long, Kevin E.; Lopez, Margaux; Lotz, Paul J.; Lupton, Robert H.; Lust, Nate B.; Macarthur, Lauren A.; Mahabal, Ashish; Mandelbaum, Rachel; Markiewicz, Thomas W.; Marsh, Darren S.; Marshall, Philip J.; Marshall, Stuart; May, Morgan; Mckercher, Robert; Mcqueen, Michelle; Meyers, Joshua; Migliore, Myriam; Miller, Michelle; Mills, David J.; Miraval, Connor; Moeyens, Joachim; Moolekamp, Fred E.; Monet, David G.; Moniez, Marc; Monkewitz, Serge; Montgomery, Christopher; Morrison, Christopher B.; Mueller, Fritz; Muller, Gary P.; Arancibia, Freddy Muñoz; Neill, Douglas R.; Newbry, Scott P.; Nief, Jean-Yves; Nomerotski, Andrei; Nordby, Martin; O'Connor, Paul; Oliver, John; Olivier, Scot S.; Olsen, Knut; O'Mullane, William; Ortiz, Sandra; Osier, Shawn; Owen, Russell E.; Pain, Reynald; Palecek, Paul E.; Parejko, John K.; Parsons, James B.; Pease, Nathan M.; Peterson, J.Matt; Peterson, John R.; Petravick, Donald L.; Petrick, M.E. Libby; Petry, Cathy E.; Pierfederici, Francesco; Pietrowicz, Stephen; Pike, Rob; Pinto, Philip A.; Plante, Raymond; Plate, Stephen; Plutchak, Joel P.; Price, Paul A.; Prouza, Michael; Radeka, Veljko; Rajagopal, Jayadev; Rasmussen, Andrew P.; Regnault, Nicolas; Reil, Kevin A.; Reiss, David J.; Reuter, Michael A.; Ridgway, Stephen T.; Riot, Vincent J.; Ritz, Steve; Robinson, Sean; Roby, William; Roodman, Aaron; Rosing, Wayne; Roucelle, Cecille; Rumore, Matthew R.; Russo, Stefano; Saha, Abhijit; Sassolas, Benoit; Schalk, Terry L.; Schellart, Pim; Schindler, Rafe H.; Schmidt, Samuel; Schneider, Donald P.; Schneider, Michael D.; Schoening, William; Schumacher, German; Schwamb, Megan E.; Sebag, Jacques; Selvy, Brian; Sembroski, Glenn H.; Seppala, Lynn G.; Serio, Andrew; Serrano, Eduardo; Shaw, Richard A.; Shipsey, Ian; Sick, Jonathan; Silvestri, Nicole; Slater, Colin T.; Smith, J.Allyn; Smith, R.Chris; Sobhani, Shahram; Soldahl, Christine; Storrie-Lombardi, Lisa; Stover, Edward; Strauss, Michael A.; Street, Rachel A.; Stubbs, Christopher W.; Sullivan, Ian S.; Sweeney, Donald; Swinbank, John D.; Szalay, Alexander; Takacs, Peter; Tether, Stephen A.; Thaler, Jon J.; Thayer, John Gregg; Thomas, Sandrine; Thornton, Adam J.; Thukral, Vaikunth; Tice, Jeffrey; Trilling, David E.; Turri, Max; van Berg, Richard; Vanden Berk, Daniel; Vetter, Kurt; Virieux, Francoise; Vucina, Tomislav; Wahl, William; Walkowicz, Lucianne; Walsh, Brian; Walter, Christopher W.; Wang, Daniel L.; Wang, Shin-Yawn; Warner, Michael; Wiecha, Oliver; Willman, Beth; Winters, Scott E.; Wittman, David; Wolff, Sidney C.; Wood-Vasey, W.Michael; Wu, Xiuqin; Xin, Bo; Yoachim, Peter; Zhan, Hu
Contributors: University of Washington Seattle; Laboratoire de l'Accélérateur Linéaire (LAL); Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS); Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)); Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS); Large Synoptic Survey Telescope (LSST); AstroParticule et Cosmologie (APC (UMR_7164)); Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris; Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité); Laboratoire de Physique Subatomique et de Cosmologie (LPSC); Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes 2016-2019 (UGA 2016-2019 ); Université Paris Diderot - Paris 7 (UPD7); Laboratoire d'Annecy de Physique des Particules (LAPP); Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS); Kavli Institute for Particle Astrophysics and Cosmology (KIPAC); Stanford University; Laboratoire des matériaux avancés (LMA); Université Claude Bernard Lyon 1 (UCBL); Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS); Laboratoire Univers et Particules de Montpellier (LUPM); Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS); SLAC National Accelerator Laboratory (SLAC); Infrared Processing and Analysis Center (IPAC); California Institute of Technology (CALTECH); Laboratoire de Physique de Clermont (LPC); Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne 2017-2020 (UCA 2017-2020 )-Centre National de la Recherche Scientifique (CNRS); Department of Physics Harvard University; Harvard University; Brookhaven National Laboratory Upton, NY (BNL); UT-Battelle, LLC-Stony Brook University SUNY (SBU); State University of New York (SUNY)-State University of New York (SUNY)-U.S. Department of Energy Washington (DOE); Centre de Calcul de l'IN2P3 (CC-IN2P3); Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS); Centre de Physique des Particules de Marseille (CPPM); Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS); Bruce and Astrid McWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University; U.S. Naval Observatory; Instituto de RadioAstronomía Milimétrica (IRAM); Centre National de la Recherche Scientifique (CNRS); National Center for Supercomputing Applications (NCSA); University of Illinois System; Lawrence Livermore National Laboratory (LLNL); LSST
Source: ISSN: 0004-637X.
Publisher Information: CCSD; American Astronomical Society
Publication Year: 2019
Collection: Université Savoie Mont Blanc: HAL
Subject Terms: Galaxy: general; Methods: observational; Stars: general; Surveys; Cosmology: observations; Astrometry; [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Description: International audience ; We describe here the most ambitious survey currently planned in the optical, the Large Synoptic Survey Telescope (LSST). The LSST design is driven by four main science themes: probing dark energy and dark matter, taking an inventory of the solar system, exploring the transient optical sky, and mapping the Milky Way. LSST will be a large, wide-field ground-based system designed to obtain repeated images covering the sky visible from Cerro Pachón in northern Chile. The telescope will have an 8.4 m (6.5 m effective) primary mirror, a 9.6 deg2 field of view, a 3.2-gigapixel camera, and six filters (ugrizy) covering the wavelength range 320–1050 nm. The project is in the construction phase and will begin regular survey operations by 2022. About 90% of the observing time will be devoted to a deep-wide-fast survey mode that will uniformly observe a 18,000 deg2 region about 800 times (summed over all six bands) during the anticipated 10 yr of operations and will yield a co-added map to r ~ 27.5. These data will result in databases including about 32 trillion observations of 20 billion galaxies and a similar number of stars, and they will serve the majority of the primary science programs. The remaining 10% of the observing time will be allocated to special projects such as Very Deep and Very Fast time domain surveys, whose details are currently under discussion. We illustrate how the LSST science drivers led to these choices of system parameters, and we describe the expected data products and their characteristics.
Document Type: article in journal/newspaper
Language: English
Relation: info:eu-repo/semantics/altIdentifier/arxiv/0805.2366; ARXIV: 0805.2366; INSPIRE: 785865
DOI: 10.3847/1538-4357/ab042c
Availability: https://hal.science/hal-02080729; https://hal.science/hal-02080729v1/document; https://hal.science/hal-02080729v1/file/Ivezi%C4%87_2019_ApJ_873_111.pdf; https://doi.org/10.3847/1538-4357/ab042c
Rights: https://creativecommons.org/licenses/by/4.0/ ; info:eu-repo/semantics/OpenAccess
Accession Number: edsbas.EE164ACA
Database: BASE