Abstract
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 deg 2 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 deg 2 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.
Original language | English (US) |
---|---|
Article number | 111 |
Journal | Astrophysical Journal |
Volume | 873 |
Issue number | 2 |
DOIs | |
State | Published - Mar 10 2019 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
Fingerprint
Dive into the research topics of 'LSST: From Science Drivers to Reference Design and Anticipated Data Products'. Together they form a unique fingerprint.Cite this
- APA
- Standard
- Harvard
- Vancouver
- Author
- BIBTEX
- RIS
In: Astrophysical Journal, Vol. 873, No. 2, 111, 10.03.2019.
Research output: Contribution to journal › Article › peer-review
}
TY - JOUR
T1 - LSST
T2 - From Science Drivers to Reference Design and Anticipated Data Products
AU - Ivezić, Željko
AU - Kahn, Steven M.
AU - Tyson, J. Anthony
AU - Abel, Bob
AU - Acosta, Emily
AU - Allsman, Robyn
AU - Alonso, David
AU - Alsayyad, Yusra
AU - Anderson, Scott F.
AU - Andrew, John
AU - Angel, James Roger P.
AU - Angeli, George Z.
AU - Ansari, Reza
AU - Antilogus, Pierre
AU - Araujo, Constanza
AU - Armstrong, Robert
AU - Arndt, Kirk T.
AU - Astier, Pierre
AU - Aubourg, Eric
AU - Auza, Nicole
AU - Axelrod, Tim S.
AU - Bard, Deborah J.
AU - Barr, Jeff D.
AU - Barrau, Aurelian
AU - Bartlett, James G.
AU - Bauer, Amanda E.
AU - Bauman, Brian J.
AU - Baumont, Sylvain
AU - Bechtol, Ellen
AU - Bechtol, Keith
AU - Becker, Andrew C.
AU - Becla, Jacek
AU - Beldica, Cristina
AU - Bellavia, Steve
AU - Bianco, Federica B.
AU - Biswas, Rahul
AU - Blanc, Guillaume
AU - Blazek, Jonathan
AU - Blandford, Roger D.
AU - Bloom, Josh S.
AU - Bogart, Joanne
AU - Bond, Tim W.
AU - Booth, Michael T.
AU - Borgland, Anders W.
AU - Borne, Kirk
AU - Bosch, James F.
AU - Boutigny, Dominique
AU - Brackett, Craig A.
AU - Bradshaw, Andrew
AU - Brandt, William Nielsen
AU - Brown, Michael E.
AU - Bullock, James S.
AU - Burchat, Patricia
AU - Burke, David L.
AU - Cagnoli, Gianpietro
AU - Calabrese, Daniel
AU - Callahan, Shawn
AU - Callen, Alice L.
AU - Carlin, Jeffrey L.
AU - Carlson, Erin L.
AU - Chandrasekharan, Srinivasan
AU - Charles-Emerson, Glenaver
AU - Chesley, Steve
AU - Cheu, Elliott C.
AU - Chiang, Hsin Fang
AU - Chiang, James
AU - Chirino, Carol
AU - Chow, Derek
AU - Ciardi, David R.
AU - Claver, Charles F.
AU - Cohen-Tanugi, Johann
AU - Cockrum, Joseph J.
AU - Coles, Rebecca
AU - Connolly, Andrew J.
AU - Cook, Kem H.
AU - Cooray, Asantha
AU - Covey, Kevin R.
AU - Cribbs, Chris
AU - Cui, Wei
AU - Cutri, Roc
AU - Daly, Philip N.
AU - Daniel, Scott F.
AU - Daruich, Felipe
AU - Daubard, Guillaume
AU - Daues, Greg
AU - Dawson, William
AU - Delgado, Francisco
AU - Dellapenna, Alfred
AU - Peyster, Robert De
AU - Val-Borro, Miguel De
AU - Digel, Seth W.
AU - Doherty, Peter
AU - Dubois, Richard
AU - Dubois-Felsmann, Gregory P.
AU - Durech, Josef
AU - Economou, Frossie
AU - Eifler, Tim
AU - Eracleous, Michael
AU - Emmons, Benjamin L.
AU - Neto, Angelo Fausti
AU - Ferguson, Henry
AU - Figueroa, Enrique
AU - Fisher-Levine, Merlin
AU - Focke, Warren
AU - Foss, Michael D.
AU - Frank, James
AU - Freemon, Michael D.
AU - Gangler, Emmanuel
AU - Gawiser, Eric
AU - Geary, John C.
AU - Gee, Perry
AU - Geha, Marla
AU - Gessner, Charles J.B.
AU - Gibson, Robert R.
AU - Gilmore, D. Kirk
AU - Glanzman, Thomas
AU - Glick, William
AU - Goldina, Tatiana
AU - Goldstein, Daniel A.
AU - Goodenow, Iain
AU - Graham, Melissa L.
AU - Gressler, William J.
AU - Gris, Philippe
AU - Guy, Leanne P.
AU - Guyonnet, Augustin
AU - Haller, Gunther
AU - Harris, Ron
AU - Hascall, Patrick A.
AU - Haupt, Justine
AU - Hernandez, Fabio
AU - Herrmann, Sven
AU - Hileman, Edward
AU - Hoblitt, Joshua
AU - Hodgson, John A.
AU - Hogan, Craig
AU - Howard, James D.
AU - Huang, Dajun
AU - Huffer, Michael E.
AU - Ingraham, Patrick
AU - Innes, Walter R.
AU - Jacoby, Suzanne H.
AU - Jain, Bhuvnesh
AU - Jammes, Fabrice
AU - Jee, M. James
AU - Jenness, Tim
AU - Jernigan, Garrett
AU - Jevremović, Darko
AU - Johns, Kenneth
AU - Johnson, Anthony S.
AU - Johnson, Margaret W.G.
AU - Jones, R. Lynne
AU - Juramy-Gilles, Claire
AU - Jurić, Mario
AU - Kalirai, Jason S.
AU - Kallivayalil, Nitya J.
AU - Kalmbach, Bryce
AU - Kantor, Jeffrey P.
AU - Karst, Pierre
AU - Kasliwal, Mansi M.
AU - Kelly, Heather
AU - Kessler, Richard
AU - Kinnison, Veronica
AU - Kirkby, David
AU - Knox, Lloyd
AU - Kotov, Ivan V.
AU - Krabbendam, Victor L.
AU - Krughoff, K. Simon
AU - Kubánek, Petr
AU - Kuczewski, John
AU - Kulkarni, Shri
AU - Ku, John
AU - Kurita, Nadine R.
AU - Lage, Craig S.
AU - Lambert, Ron
AU - Lange, Travis
AU - Langton, J. Brian
AU - Guillou, Laurent Le
AU - Levine, Deborah
AU - Liang, Ming
AU - Lim, Kian Tat
AU - Lintott, Chris J.
AU - Long, Kevin E.
AU - Lopez, Margaux
AU - Lotz, Paul J.
AU - Lupton, Robert H.
AU - Lust, Nate B.
AU - Macarthur, Lauren A.
AU - Mahabal, Ashish
AU - Mandelbaum, Rachel
AU - Markiewicz, Thomas W.
AU - Marsh, Darren S.
AU - Marshall, Philip J.
AU - Marshall, Stuart
AU - May, Morgan
AU - McKercher, Robert
AU - McQueen, Michelle
AU - Meyers, Joshua
AU - Migliore, Myriam
AU - Miller, Michelle
AU - Mills, David J.
AU - Miraval, Connor
AU - Moeyens, Joachim
AU - Moolekamp, Fred E.
AU - Monet, David G.
AU - Moniez, Marc
AU - Monkewitz, Serge
AU - Montgomery, Christopher
AU - Morrison, Christopher B.
AU - Mueller, Fritz
AU - Muller, Gary P.
AU - Arancibia, Freddy Munoz
AU - Neill, Douglas R.
AU - Newbry, Scott P.
AU - Nief, Jean Yves
AU - Nomerotski, Andrei
AU - Nordby, Martin
AU - O'Connor, Paul
AU - Oliver, John
AU - Olivier, Scot S.
AU - Olsen, Knut
AU - O'Mullane, William
AU - Ortiz, Sandra
AU - Osier, Shawn
AU - Owen, Russell E.
AU - Pain, Reynald
AU - Palecek, Paul E.
AU - Parejko, John K.
AU - Parsons, James B.
AU - Pease, Nathan M.
AU - Peterson, J. Matt
AU - Peterson, John R.
AU - Petravick, Donald L.
AU - Petrick, M. E.Libby
AU - Petry, Cathy E.
AU - Pierfederici, Francesco
AU - Pietrowicz, Stephen
AU - Pike, Rob
AU - Pinto, Philip A.
AU - Plante, Raymond
AU - Plate, Stephen
AU - Plutchak, Joel P.
AU - Price, Paul A.
AU - Prouza, Michael
AU - Radeka, Veljko
AU - Rajagopal, Jayadev
AU - Rasmussen, Andrew P.
AU - Regnault, Nicolas
AU - Reil, Kevin A.
AU - Reiss, David J.
AU - Reuter, Michael A.
AU - Ridgway, Stephen T.
AU - Riot, Vincent J.
AU - Ritz, Steve
AU - Robinson, Sean
AU - Roby, William
AU - Roodman, Aaron
AU - Rosing, Wayne
AU - Roucelle, Cecille
AU - Rumore, Matthew R.
AU - Russo, Stefano
AU - Saha, Abhijit
AU - Sassolas, Benoit
AU - Schalk, Terry L.
AU - Schellart, Pim
AU - Schindler, Rafe H.
AU - Schmidt, Samuel
AU - Schneider, Donald P.
AU - Schneider, Michael D.
AU - Schoening, William
AU - Schumacher, German
AU - Schwamb, Megan E.
AU - Sebag, Jacques
AU - Selvy, Brian
AU - Sembroski, Glenn H.
AU - Seppala, Lynn G.
AU - Serio, Andrew
AU - Serrano, Eduardo
AU - Shaw, Richard A.
AU - Shipsey, Ian
AU - Sick, Jonathan
AU - Silvestri, Nicole
AU - Slater, Colin T.
AU - Smith, J. Allyn
AU - Smith, R. Chris
AU - Sobhani, Shahram
AU - Soldahl, Christine
AU - Storrie-Lombardi, Lisa
AU - Stover, Edward
AU - Strauss, Michael A.
AU - Street, Rachel A.
AU - Stubbs, Christopher W.
AU - Sullivan, Ian S.
AU - Sweeney, Donald
AU - Swinbank, John D.
AU - Szalay, Alexander
AU - Takacs, Peter
AU - Tether, Stephen A.
AU - Thaler, Jon J.
AU - Thayer, John Gregg
AU - Thomas, Sandrine
AU - Thornton, Adam J.
AU - Thukral, Vaikunth
AU - Tice, Jeffrey
AU - Trilling, David E.
AU - Turri, Max
AU - Berg, Richard Van
AU - Berk, Daniel Vanden
AU - Vetter, Kurt
AU - Virieux, Francoise
AU - Vucina, Tomislav
AU - Wahl, William
AU - Walkowicz, Lucianne
AU - Walsh, Brian
AU - Walter, Christopher W.
AU - Wang, Daniel L.
AU - Wang, Shin Yawn
AU - Warner, Michael
AU - Wiecha, Oliver
AU - Willman, Beth
AU - Winters, Scott E.
AU - Wittman, David
AU - Wolff, Sidney C.
AU - Wood-Vasey, W. Michael
AU - Wu, Xiuqin
AU - Xin, Bo
AU - Yoachim, Peter
AU - Zhan, Hu
N1 - Publisher Copyright: © 2019. The American Astronomical Society. All rights reserved..
PY - 2019/3/10
Y1 - 2019/3/10
N2 - 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 deg 2 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 deg 2 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.
AB - 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 deg 2 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 deg 2 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.
UR - http://www.scopus.com/inward/record.url?scp=85064450156&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85064450156&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ab042c
DO - 10.3847/1538-4357/ab042c
M3 - Article
AN - SCOPUS:85064450156
SN - 0004-637X
VL - 873
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 111
ER -