PEP PACS and MIPS Cross-IDs Catalog Definitions

Overview

The PACS Evolutionary Probe (PEP, Lutz et al. 2011) is a Herschel guaranteed time deep extragalactic survey (KPGT_dlutz_1) targeting six among the most popular "blank fields", ten lensing clusters of galaxies, and two z ~1 clusters at wavelengths of 100, and 160 microns. PEP includes SPIRE observations of the two z ~1 clusters at wavelengths of 250, 350, and 500 microns. SPIRE coverage of all other fields is available from the HerMES survey (Oliver et al. 2010). In addition, deep SPIRE GOODS-N data are provided by the GOODS-Herschel program (Elbaz et al. 2011).

The PACS blind catalogs extracted using Starfinder have been matched to the available 24 micron source lists by means of a maximum likelihood analysis (Ciliegi et al. 2001; Sutherland & Saunders 1992), taking advantage of the available 24 micron fluxes. See the documentation for details.

Name Intype Units Description
ra double deg Right Ascension (J2000)
dec double deg Declination (J2000)
idp160 int PACS 160 micron ID number
flux_160 double jy PACS 160 micron flux density
err_160 double jy Uncertainty in flux_160
ra_160 double deg RA of PACS 160 micron detection
dec_160 double deg Dec of PACS 160 micron detection
idp100 int PACS 100 micron ID number
flux_100 double jy PACS 100 micron flux density
err_100 double jy Uncertainty in flux_100
ra_100 double deg RA of PACS 100 micron detection
dec_100 double deg Dec of PACS 100 micron detection
idm24 int MIPS 24 micron ID number
flux_24 double mjy MIPS 24 micron flux density
err_24 double mjy Uncertainty in flux_24
ra_24 double deg RA of MIPS 24 micron detection
dec_24 double deg Dec of MIPS 24 micron detection
acf c Area Coverage Flag:
N = PACS source lies outside the MIPS 24 micron map
A = PACS source lies inside the MIPS 24 micron map
cln int Clean Index: 24 micron neighbors + 10*(100 micron neighbors) + 100*(160 micron neighbors); see documentation.