The Dark Energy Camera Plane Survey 2 (DECaPS2): More Sky, Less Bias, and Better Uncertainties
A. K. Saydjari, E. F. Schlafly, D. Lang, A. M. Meisner, G. M. Green,, C. Zucker, I. Zelko, J. S. Speagle, T. Daylan, A. Lee, F. Valdes, D., Schlegel, D. P. Finkbeiner

TL;DR
DECaPS2 provides an extensive, improved optical and near-infrared survey of the southern Galactic plane, with enhanced data reduction techniques, better bias correction, and publicly available catalogs, aiding Galactic structure studies.
Contribution
The paper introduces new data reduction and bias correction methods for the DECaPS2 survey, improving photometric accuracy and uncertainty estimates over previous releases.
Findings
Survey covers 6.5% of the sky with 3.32 billion objects.
Implemented synthetic source injection tests for validation.
Applied new de-biasing techniques to improve flux uncertainties.
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 DECam Plane Survey (DECaPS2) extends the five-band optical and near-infrared survey of the southern Galactic plane to cover of the sky, |b| < 10{\deg} and 6{\deg} > l > -124{\deg}, 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 , , , , and bands, respectively, with around 1 arcsecond seeing. The survey comprises 3.32 billion objects built from 34 billion detections in 21.4 thousand exposures, totaling 260 hours open shutter time on the Dark Energy Camera (DECam) at Cerro Tololo. The data reduction pipeline features several improvements, including the addition of…
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Taxonomy
TopicsCalibration and Measurement Techniques · Infrared Target Detection Methodologies · CCD and CMOS Imaging Sensors
