DeepDrill Single Band Catalog Definitions

Overview

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will observe several Deep Drilling Fields (DDFs) to a greater depth and with a more rapid cadence than the main survey. The "DeepDrill" survey used the Spitzer Space Telescope Infrared Array Camera (IRAC) to observe three of the four currently defined DDFs in two bands, centered on 3.6 um and 4.5 um. These observations expand the area which was covered by an earlier set of observations in these three fields by the Spitzer Extragalactic Representative Volume Survey (SERVS). The combined DeepDrill and SERVS data cover the footprints of the LSST DDFs in the Extended Chandra Deep Field-South field (ECDFS), the ELAIS-S1 field (ES1), and the XMM-Large-Scale Structure Survey field (XMM-LSS).

If you use DeepDrill data, please cite Lacy et al. (2020).

Name Intype Units Description
Name char Name
ra double deg Right Ascension (J2000)
dec double deg Declination (J2000)
FluxAper1_ch float uJy Aperture corrected flux density, aperture 1 (1.4")
FluxAper2_ch float uJy Aperture corrected flux density, aperture 2 (1.9")
FluxAper3_ch float uJy Aperture corrected flux density, aperture 3 (2.9")
FluxAper4_ch float uJy Aperture corrected flux density, aperture 4 (4.1")
FluxAper5_ch float uJy Aperture corrected flux density, aperture 5 (5.8")
FluxIso_ch float uJy Isophotal flux density
FluxAuto_ch float uJy SExtractor Auto flux density
FluxErrAper1_ch float uJy Aperture corrected flux density uncertainty, aperture 1 (1.4")
FluxErrAper2_ch float uJy Aperture corrected flux density uncertainty, aperture 2 (1.9")
FluxErrAper3_ch float uJy Aperture corrected flux density uncertainty, aperture 3 (2.9")
FluxErrAper4_ch float uJy Aperture corrected flux density uncertainty, aperture 4 (4.1")
FluxErrAper5_ch float uJy Aperture corrected flux density uncertainty, aperture 5 (5.8")
FluxErrIso_ch float uJy Isophotal flux density uncertainty
FluxErrAuto_ch float uJy SExtractor Auto flux density uncertainty
KronRadius_ch float pixel Kron radius
SNR double Signal-to-noise ratio
RMS double uJy Local RMS noise
Coverage double 100s Coverage
Flag double Flag: bit 1 = photometry may be affected by neighbors or bad pixels
bit 2 = the source was blended with a nearby object
bit 3 = the source is either a bright (K<12) star, or within the halo of a bright star