The LSST DESC DC2 Simulated Sky Survey
Abstract
Here, we describe the simulated sky survey underlying the second data challenge (DC2) carried out in preparation for analysis of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) by the LSST Dark Energy Science Collaboration (LSST DESC). Significant connections across multiple science domains will be a hallmark of LSST; the DC2 program represents a unique modeling effort that stresses this interconnectivity in a way that has not been attempted before. This effort encompasses a full end-to-end approach: starting from a large N-body simulation, through setting up LSST-like observations including realistic cadences, through image simulations, and finally processing with Rubin's LSST Science Pipelines. This last step ensures that we generate data products resembling those to be delivered by the Rubin Observatory as closely as is currently possible. The simulated DC2 sky survey covers six optical bands in a wide-fast-deep area of approximately 300 deg2, as well as a deep drilling field of approximately 1 deg2. We simulate 5 yr of the planned 10 yr survey. The DC2 sky survey has multiple purposes. First, the LSST DESC working groups can use the data set to develop a range of DESC analysis pipelines to prepare for the advent ofmore »
- Authors:
- more »
- Publication Date:
- Research Org.:
- SLAC National Accelerator Lab., Menlo Park, CA (United States); Brookhaven National Lab. (BNL), Upton, NY (United States); Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Argonne National Lab. (ANL), Argonne, IL (United States); Carnegie Mellon Univ., Pittsburgh, PA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Basic Energy Sciences (BES); USDOE Office of Science (SC), High Energy Physics (HEP)
- Contributing Org.:
- The LSST Dark Energy Science Collaboration (LSST DESC); Institut National de Physique Nucleaire et de Physique des Particules (France), Science & Technology Facilities Council (UK)
- OSTI Identifier:
- 1781655
- Alternate Identifier(s):
- OSTI ID: 1693446; OSTI ID: 1770988; OSTI ID: 1823245; OSTI ID: 1826084; OSTI ID: 1827160; OSTI ID: 1837682
- Report Number(s):
- FERMILAB-PUB-20-574-AE; arXiv:2010.05926; BNL-222275-2021-JAAM
Journal ID: ISSN 0067-0049; TRN: US2209942
- Grant/Contract Number:
- AC02-76SF00515; AC02-06CH11357; SC0011636; SC0010118; SC0010007; SC0009999; SC0011635; SC0010008; SC009193; SC0019206; HST-HF2-51441.001; 2015-106; ICN12\_009; Basal AFB-170002; 1190818; 1200495; N56981C; AC02-07CH11359; SC0012704
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal. Supplement Series
- Additional Journal Information:
- Journal Volume: 253; Journal Issue: 1; Journal ID: ISSN 0067-0049
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Cosmology; N-body simulations; Sky surveys; Numerical methods; Large scale structure of universe; Large-scale structure of the universe; Methods: numerical
Citation Formats
Abolfathi, Bela, Alonso, David, Armstrong, Robert, Aubourg, Éric, Awan, Humna, Babuji, Yadu N., Bauer, Franz Erik, Bean, Rachel, Beckett, George, Biswas, Rahul, Bogart, Joanne R., Boutigny, Dominique, Chard, Kyle, Chiang, James, Claver, Chuck F., Cohen-Tanugi, Johann, Combet, Céline, Connolly, Andrew J., Daniel, Scott F., Digel, Seth W., Drlica-Wagner, Alex, Dubois, Richard, Gangler, Emmanuel, Gawiser, Eric, Glanzman, Thomas, Gris, Phillipe, Habib, Salman, Hearin, Andrew P., Heitmann, Katrin, Hernandez, Fabio, Hložek, Renée, Hollowed, Joseph, Ishak, Mustapha, Ivezić, Željko, Jarvis, Mike, Jha, Saurabh W., Kahn, Steven M., Kalmbach, J. Bryce, Kelly, Heather M., Kovacs, Eve, Korytov, Danila, Krughoff, K. Simon, Lage, Craig S., Lanusse, François, Larsen, Patricia, Le Guillou, Laurent, Li, Nan, Longley, Emily Phillips, Lupton, Robert H., Mandelbaum, Rachel, Mao, Yao-Yuan, Marshall, Phil, Meyers, Joshua E., Moniez, Marc, Morrison, Christopher B., Nomerotski, Andrei, O’Connor, Paul, Park, HyeYun, Park, Ji Won, Peloton, Julien, Perrefort, Daniel, Perry, James, Plaszczynski, Stéphane, Pope, Adrian, Rasmussen, Andrew, Reil, Kevin, Roodman, Aaron J., Rykoff, Eli S., Sánchez, F. Javier, Schmidt, Samuel J., Scolnic, Daniel, Stubbs, Christopher W., Tyson, J. Anthony, Uram, Thomas D., Villarreal, Antonio, Walter, Christopher W., Wiesner, Matthew P., Wood-Vasey, W. Michael, and Zuntz, Joe. The LSST DESC DC2 Simulated Sky Survey. United States: N. p., 2021.
Web. doi:10.3847/1538-4365/abd62c.
Abolfathi, Bela, Alonso, David, Armstrong, Robert, Aubourg, Éric, Awan, Humna, Babuji, Yadu N., Bauer, Franz Erik, Bean, Rachel, Beckett, George, Biswas, Rahul, Bogart, Joanne R., Boutigny, Dominique, Chard, Kyle, Chiang, James, Claver, Chuck F., Cohen-Tanugi, Johann, Combet, Céline, Connolly, Andrew J., Daniel, Scott F., Digel, Seth W., Drlica-Wagner, Alex, Dubois, Richard, Gangler, Emmanuel, Gawiser, Eric, Glanzman, Thomas, Gris, Phillipe, Habib, Salman, Hearin, Andrew P., Heitmann, Katrin, Hernandez, Fabio, Hložek, Renée, Hollowed, Joseph, Ishak, Mustapha, Ivezić, Željko, Jarvis, Mike, Jha, Saurabh W., Kahn, Steven M., Kalmbach, J. Bryce, Kelly, Heather M., Kovacs, Eve, Korytov, Danila, Krughoff, K. Simon, Lage, Craig S., Lanusse, François, Larsen, Patricia, Le Guillou, Laurent, Li, Nan, Longley, Emily Phillips, Lupton, Robert H., Mandelbaum, Rachel, Mao, Yao-Yuan, Marshall, Phil, Meyers, Joshua E., Moniez, Marc, Morrison, Christopher B., Nomerotski, Andrei, O’Connor, Paul, Park, HyeYun, Park, Ji Won, Peloton, Julien, Perrefort, Daniel, Perry, James, Plaszczynski, Stéphane, Pope, Adrian, Rasmussen, Andrew, Reil, Kevin, Roodman, Aaron J., Rykoff, Eli S., Sánchez, F. Javier, Schmidt, Samuel J., Scolnic, Daniel, Stubbs, Christopher W., Tyson, J. Anthony, Uram, Thomas D., Villarreal, Antonio, Walter, Christopher W., Wiesner, Matthew P., Wood-Vasey, W. Michael, & Zuntz, Joe. The LSST DESC DC2 Simulated Sky Survey. United States. https://doi.org/10.3847/1538-4365/abd62c
Abolfathi, Bela, Alonso, David, Armstrong, Robert, Aubourg, Éric, Awan, Humna, Babuji, Yadu N., Bauer, Franz Erik, Bean, Rachel, Beckett, George, Biswas, Rahul, Bogart, Joanne R., Boutigny, Dominique, Chard, Kyle, Chiang, James, Claver, Chuck F., Cohen-Tanugi, Johann, Combet, Céline, Connolly, Andrew J., Daniel, Scott F., Digel, Seth W., Drlica-Wagner, Alex, Dubois, Richard, Gangler, Emmanuel, Gawiser, Eric, Glanzman, Thomas, Gris, Phillipe, Habib, Salman, Hearin, Andrew P., Heitmann, Katrin, Hernandez, Fabio, Hložek, Renée, Hollowed, Joseph, Ishak, Mustapha, Ivezić, Željko, Jarvis, Mike, Jha, Saurabh W., Kahn, Steven M., Kalmbach, J. Bryce, Kelly, Heather M., Kovacs, Eve, Korytov, Danila, Krughoff, K. Simon, Lage, Craig S., Lanusse, François, Larsen, Patricia, Le Guillou, Laurent, Li, Nan, Longley, Emily Phillips, Lupton, Robert H., Mandelbaum, Rachel, Mao, Yao-Yuan, Marshall, Phil, Meyers, Joshua E., Moniez, Marc, Morrison, Christopher B., Nomerotski, Andrei, O’Connor, Paul, Park, HyeYun, Park, Ji Won, Peloton, Julien, Perrefort, Daniel, Perry, James, Plaszczynski, Stéphane, Pope, Adrian, Rasmussen, Andrew, Reil, Kevin, Roodman, Aaron J., Rykoff, Eli S., Sánchez, F. Javier, Schmidt, Samuel J., Scolnic, Daniel, Stubbs, Christopher W., Tyson, J. Anthony, Uram, Thomas D., Villarreal, Antonio, Walter, Christopher W., Wiesner, Matthew P., Wood-Vasey, W. Michael, and Zuntz, Joe. Fri .
"The LSST DESC DC2 Simulated Sky Survey". United States. https://doi.org/10.3847/1538-4365/abd62c. https://www.osti.gov/servlets/purl/1781655.
@article{osti_1781655,
title = {The LSST DESC DC2 Simulated Sky Survey},
author = {Abolfathi, Bela and Alonso, David and Armstrong, Robert and Aubourg, Éric and Awan, Humna and Babuji, Yadu N. and Bauer, Franz Erik and Bean, Rachel and Beckett, George and Biswas, Rahul and Bogart, Joanne R. and Boutigny, Dominique and Chard, Kyle and Chiang, James and Claver, Chuck F. and Cohen-Tanugi, Johann and Combet, Céline and Connolly, Andrew J. and Daniel, Scott F. and Digel, Seth W. and Drlica-Wagner, Alex and Dubois, Richard and Gangler, Emmanuel and Gawiser, Eric and Glanzman, Thomas and Gris, Phillipe and Habib, Salman and Hearin, Andrew P. and Heitmann, Katrin and Hernandez, Fabio and Hložek, Renée and Hollowed, Joseph and Ishak, Mustapha and Ivezić, Željko and Jarvis, Mike and Jha, Saurabh W. and Kahn, Steven M. and Kalmbach, J. Bryce and Kelly, Heather M. and Kovacs, Eve and Korytov, Danila and Krughoff, K. Simon and Lage, Craig S. and Lanusse, François and Larsen, Patricia and Le Guillou, Laurent and Li, Nan and Longley, Emily Phillips and Lupton, Robert H. and Mandelbaum, Rachel and Mao, Yao-Yuan and Marshall, Phil and Meyers, Joshua E. and Moniez, Marc and Morrison, Christopher B. and Nomerotski, Andrei and O’Connor, Paul and Park, HyeYun and Park, Ji Won and Peloton, Julien and Perrefort, Daniel and Perry, James and Plaszczynski, Stéphane and Pope, Adrian and Rasmussen, Andrew and Reil, Kevin and Roodman, Aaron J. and Rykoff, Eli S. and Sánchez, F. Javier and Schmidt, Samuel J. and Scolnic, Daniel and Stubbs, Christopher W. and Tyson, J. Anthony and Uram, Thomas D. and Villarreal, Antonio and Walter, Christopher W. and Wiesner, Matthew P. and Wood-Vasey, W. Michael and Zuntz, Joe},
abstractNote = {Here, we describe the simulated sky survey underlying the second data challenge (DC2) carried out in preparation for analysis of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) by the LSST Dark Energy Science Collaboration (LSST DESC). Significant connections across multiple science domains will be a hallmark of LSST; the DC2 program represents a unique modeling effort that stresses this interconnectivity in a way that has not been attempted before. This effort encompasses a full end-to-end approach: starting from a large N-body simulation, through setting up LSST-like observations including realistic cadences, through image simulations, and finally processing with Rubin's LSST Science Pipelines. This last step ensures that we generate data products resembling those to be delivered by the Rubin Observatory as closely as is currently possible. The simulated DC2 sky survey covers six optical bands in a wide-fast-deep area of approximately 300 deg2, as well as a deep drilling field of approximately 1 deg2. We simulate 5 yr of the planned 10 yr survey. The DC2 sky survey has multiple purposes. First, the LSST DESC working groups can use the data set to develop a range of DESC analysis pipelines to prepare for the advent of actual data. Second, it serves as a realistic test bed for the image processing software under development for LSST by the Rubin Observatory. In particular, simulated data provide a controlled way to investigate certain image-level systematic effects. Finally, the DC2 sky survey enables the exploration of new scientific ideas in both static and time domain cosmology.},
doi = {10.3847/1538-4365/abd62c},
journal = {The Astrophysical Journal. Supplement Series},
number = 1,
volume = 253,
place = {United States},
year = {Fri Mar 12 00:00:00 EST 2021},
month = {Fri Mar 12 00:00:00 EST 2021}
}
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