The Dark Energy Camera Plane Survey 2 (DECaPS2): More Sky, Less Bias, and Better Uncertainties
Abstract
Abstract Deep optical and near-infrared imaging of the entire Galactic plane is essential for understanding our Galaxy’s stars, gas, and dust. The second data release of the Dark Energy Camera (DECam) Plane Survey extends the five-band optical and near-infrared survey of the southern Galactic plane to cover 6.5% of the sky, ∣ b ∣ ≤ 10°, and 6° > ℓ > −124°, complementary to coverage by Pan-STARRS1. Typical single-exposure effective depths, including crowding effects and other complications, are 23.5, 22.6, 22.1, 21.6, and 20.8 mag in g , r , i , z , and Y bands, respectively, with around 1″ seeing. The survey comprises 3.32 billion objects built from 34 billion detections in 21,400 exposures, totaling 260 hr open shutter time on the DECam at Cerro Tololo. The data reduction pipeline features several improvements, including the addition of synthetic source injection tests to validate photometric solutions across the entire survey footprint. A convenient functional form for the detection bias in the faint limit was derived and leveraged to characterize the photometric pipeline performance. A new postprocessing technique was applied to every detection to debias and improve uncertainty estimates of the flux in the presence of structured backgrounds, specifically targetingmore »
- Authors:
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); National Aeronautics and Space Administration (NASA)
- OSTI Identifier:
- 1909744
- Alternate Identifier(s):
- OSTI ID: 2323907
- Grant/Contract Number:
- AC02-05CH11231; AST-1614941; 80NSSC21K0634; NNX08AR22G; AST-1238877
- Resource Type:
- Published Article
- Journal Name:
- The Astrophysical Journal. Supplement Series
- Additional Journal Information:
- Journal Name: The Astrophysical Journal. Supplement Series Journal Volume: 264 Journal Issue: 2; Journal ID: ISSN 0067-0049
- Publisher:
- American Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Saydjari, Andrew K., Schlafly, Edward F., Lang, Dustin, Meisner, Aaron M., Green, Gregory M., Zucker, Catherine, Zelko, Ioana, Speagle 沈, Joshua S. 佳士, Daylan, Tansu, Lee, Albert, Valdes, Francisco, Schlegel, David, and Finkbeiner, Douglas P. The Dark Energy Camera Plane Survey 2 (DECaPS2): More Sky, Less Bias, and Better Uncertainties. United States: N. p., 2023.
Web. doi:10.3847/1538-4365/aca594.
Saydjari, Andrew K., Schlafly, Edward F., Lang, Dustin, Meisner, Aaron M., Green, Gregory M., Zucker, Catherine, Zelko, Ioana, Speagle 沈, Joshua S. 佳士, Daylan, Tansu, Lee, Albert, Valdes, Francisco, Schlegel, David, & Finkbeiner, Douglas P. The Dark Energy Camera Plane Survey 2 (DECaPS2): More Sky, Less Bias, and Better Uncertainties. United States. https://doi.org/10.3847/1538-4365/aca594
Saydjari, Andrew K., Schlafly, Edward F., Lang, Dustin, Meisner, Aaron M., Green, Gregory M., Zucker, Catherine, Zelko, Ioana, Speagle 沈, Joshua S. 佳士, Daylan, Tansu, Lee, Albert, Valdes, Francisco, Schlegel, David, and Finkbeiner, Douglas P. Wed .
"The Dark Energy Camera Plane Survey 2 (DECaPS2): More Sky, Less Bias, and Better Uncertainties". United States. https://doi.org/10.3847/1538-4365/aca594.
@article{osti_1909744,
title = {The Dark Energy Camera Plane Survey 2 (DECaPS2): More Sky, Less Bias, and Better Uncertainties},
author = {Saydjari, Andrew K. and Schlafly, Edward F. and Lang, Dustin and Meisner, Aaron M. and Green, Gregory M. and Zucker, Catherine and Zelko, Ioana and Speagle 沈, Joshua S. 佳士 and Daylan, Tansu and Lee, Albert and Valdes, Francisco and Schlegel, David and Finkbeiner, Douglas P.},
abstractNote = {Abstract Deep optical and near-infrared imaging of the entire Galactic plane is essential for understanding our Galaxy’s stars, gas, and dust. The second data release of the Dark Energy Camera (DECam) Plane Survey extends the five-band optical and near-infrared survey of the southern Galactic plane to cover 6.5% of the sky, ∣ b ∣ ≤ 10°, and 6° > ℓ > −124°, complementary to coverage by Pan-STARRS1. Typical single-exposure effective depths, including crowding effects and other complications, are 23.5, 22.6, 22.1, 21.6, and 20.8 mag in g , r , i , z , and Y bands, respectively, with around 1″ seeing. The survey comprises 3.32 billion objects built from 34 billion detections in 21,400 exposures, totaling 260 hr open shutter time on the DECam at Cerro Tololo. The data reduction pipeline features several improvements, including the addition of synthetic source injection tests to validate photometric solutions across the entire survey footprint. A convenient functional form for the detection bias in the faint limit was derived and leveraged to characterize the photometric pipeline performance. A new postprocessing technique was applied to every detection to debias and improve uncertainty estimates of the flux in the presence of structured backgrounds, specifically targeting nebulosity. The images and source catalogs are publicly available at http://decaps.skymaps.info/ .},
doi = {10.3847/1538-4365/aca594},
journal = {The Astrophysical Journal. Supplement Series},
number = 2,
volume = 264,
place = {United States},
year = {Wed Jan 18 00:00:00 EST 2023},
month = {Wed Jan 18 00:00:00 EST 2023}
}
https://doi.org/10.3847/1538-4365/aca594
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