GOODS IRS 16 micron Catalog Definitions
Overview
The Great Observatories Origins Deep Survey (GOODS) aims to unite extremely deep observations from NASA's Great Observatories (Spitzer, Hubble and Chandra), ESA's Herschel and XMM-Newton, and the most powerful ground-based facilities. The aim is to survey the distant universe to the faintest flux limits across the broadest range of wavelengths.
GOODS surveyed 150 square arcminutes in each of the two GOODS fields (North and South), to an average 3 sigma depth of 40 and 65 microJy, respectively.
These sources have been cross-correlated with Spitzer, Chandra, and HST measurements in other bands.
Name |
Intype |
Units |
Description |
ID |
int |
|
Source ID |
ra |
double |
deg |
Right Ascension (J2000) |
dec |
double |
deg |
Declination (J2000) |
Cov |
int |
|
Coverage in number of exposures.
Exposure times were 30s in GOODS-N and 60s in GOODS-S. |
S3_6 |
double |
microjy |
3.6 micron flux density |
e_S3_6 |
double |
microjy |
3.6 micron flux density uncertainty |
S4_5 |
double |
microjy |
4.5 micron flux density |
e_S4_5 |
double |
microjy |
4.5 micron flux density uncertainty |
S5_8 |
double |
microjy |
5.8 micron flux density |
e_S5_8 |
double |
microjy |
5.8 micron flux density uncertainty |
S8 |
double |
microjy |
8 micron flux density |
e_S8 |
double |
microjy |
8 micron flux density uncertainty |
S16 |
double |
microjy |
16 micron flux density |
e_S16 |
double |
microjy |
16 micron flux density uncertainty |
S24 |
double |
microjy |
24 micron flux density |
e_S24 |
double |
microjy |
24 micron flux density uncertainty |
zspec |
double |
|
Spectroscopic redshift |
r_zspec |
int |
|
Reference for the spectroscopic redshift:
1 = Le Fevre et al. 2004
2 = Szokoly et al. 2004
3 = Croom et al. 2001
9 = K20 Survey, Mignoli et al. 2005
11 = Strolger et al. 2004
30 = Vanzella et al. 2005
41 = Popesso et al. 2009
42 = Balestra et al. 2010
62 = Doherty et al. 2005
70 = Ravikumar et al. 2007
72 = Stern et al. 2011
81 = Kriek et al. 2008 |
Xdet |
int |
|
X-ray detection flag |
SBF |
double |
1e-15 mW m^-2 |
Soft X-ray flux |
HBF |
double |
1e-15 mW m^-2 |
Hard X-ray flux |
Star |
int |
|
Star flag |
Ratio |
double |
|
16 micron concentration index:
ratio of aperture flux in 6" and 2" radii. |
Ncf |
int |
|
Number of 8 micron sources within 4 arcsec |
Ncf16 |
int |
|
Number of 16 micron sources within 5.4 arcsec |
Q |
int |
|
Quality flag:
bit 0 = included in the catalog
bit 1 = more than one 16 micron source within 5.4 arcsec; possible confusion
bit 2 = source concentration differs from that expected for point source
bit 3 = S/N < 5, but coverage indicates it should be higher
bit 4 = source with coverage of two exposures instead of three |
E |
int |
|
Extended source flag |
Bmag |
double |
mag |
HST B magnitude |
Vmag |
double |
mag |
HST V magnitude |
Imag |
double |
mag |
HST I magnitude |
zmag |
double |
mag |
HST z magnitude |
eBmag |
double |
mag |
HST B magnitude uncertainty |
eVmag |
double |
mag |
HST V magnitude uncertainty |
eImag |
double |
mag |
HST I magnitude uncertainty |
ezmag |
double |
mag |
HST z magnitude uncertainty |
Icls |
int |
|
Number of I-band sources within 1 arcsec |