COSMOS Photometry Catalog Definitions
COSMOS Overview
The COSMOS Archive serves data taken for the Cosmic Evolution Survey (COSMOS) project. COSMOS is an astronomical survey designed to probe the formation and evolution of galaxies as a function of cosmic time (redshift) and large scale structural environment. The survey covers a 2 square degree equatorial field with imaging by most of the major space-based telescopes (Hubble, Spitzer, GALEX, XMM, Chandra) and a number of large ground based telescopes (Subaru, VLA, ESO-VLT, UKIRT, NOAO, CFHT, and others).
IRSA serves the COSMOS archive using the following search methods:
- Spatial search on all images and small catalogs, using Atlas
- Advanced search on only the larger catalogs, using Gator
COSMOS I band catalog
This is an I band selected multi-color catalog for 2 square degrees centered on the COSMOS field at 10:00:28.6, +02:12:21. A detailed description of the catalog is given in Capak et. al. (2007) and it is recomended that you read this paper before using the catalog.
The total magnitude (SExtractor mag_auto) for a source must have an AB magnitude of less than i+<25 to appear in the archival catalog. All photometry is in the AB magnitude system and measured in a 3 arc second aperture on PSF-matched images unless otherwise noted. A magnitude of -99 indicates a photometric measurement was not possible due to lack of data, a large number of bad pixels, or saturation. A magnitude of 99.0 indicates no detection. In the case of no detection the error given for the object is the 1 sigma limiting magnitude at the position of the souce.
The photometry is as measured on the images with no corrections applied. We recommend applying the magnitude offsets in Capak et. al. (2007) to obtain the best possible photometry. More details on the photometry are available in Capak et. al. (2007). The Photometric Redshifts included in this catalog are described in Mobasher et al. (2007) and have an accuracy of dz/(1+z)<0.031 at z<1.2 and I<24.
It is important to pay attention to the flag columns at the end of the catalog. The cleanest catalog will have all flags set to 0. The photometry flags indicate the area of the photometry aperture, in square arc seconds, which is in a masked region. A flag of 1 indicates 14 percent of the aperture is masked, so any flagged object should be carefully checked. Objects with a de-blending flag set to 1 are potentially spurious and should not be used for statistical studies. However, the photometry for real sources with a de-blending flag set to 1 is good if they fall outside of masked region.
COSMOS Photometry Catalog Column Definitions
Gator serves the COSMOS January 2006 Photometry Catalog (68 columns [63 delivered + 5 IRSA-created], 438,226 data rows). The column descriptions can be found below.
Column Name | Data Type | Units | Description |
ID | int | number | Unique identification number of each source in the catalog. |
image_tile | int | number | Which of the 144 sub-image tiles contains this object. [Tile diagram] |
RA | double | deg | Right Ascension (J2000.0). |
DEC | double | deg | Declination (J2000.0). |
x_pix | double | number | x pixel position on the sub-image tile. |
y_pix | double | number | y pixel position on the sub-image tile. |
i_fwhm | double | pixel | FWHM in pixels measured on the detection image indicated by auto_flag. |
i_max | double | uJy | Peak flux in nJy measured on the detection image indicated by auto_flag. |
i_star | double | number | Sextractor stellarity parameter measured on the detection image indicated by auto_flag. See Bertin and Arnouts (1996) for a detailed description of this parameter. |
i_mag_auto | double | mag | Total i-band magnitude measured on the detection image indicated by auto_flag. The total magnitude given is the mag_auto parameter from SExtractor. See Bertin and Arnouts (1996) for a detailed description of this parameter. |
auto_offset | double | mag | Offset between 3" aperture magnitudes and the total magnitude. This is the apperture correction for the multi-color photometry. |
auto_flag | double | number | Flag indicating which image the total magnitude (i_mag_auto) was measured from. 1=Subaru i+, 2=CFHT i*, -1=No valid total magnitude |
u_mag | double | mag | CFHT u* AB magnitude. |
u_mag_err | double | mag | 1 Sigma error on CFHT u* AB magnitude. |
B_mag | double | mag | Subaru Bj AB magnitude. |
B_mag_err | double | mag | 1 Sigma error on Subaru Bj AB magnitude. |
V_mag | double | mag | Subaru Vj AB magnitude. |
V_mag_err | double | mag | 1 Sigma error on Subaru Vj AB magnitude. |
g_mag | double | mag | Subaru g+ AB magnitude. |
g_mag_err | double | mag | 1 Sigma error on Subaru g+ AB magnitude. |
r_mag | double | mag | Subaru r+ AB magnitude. |
r_mag_err | double | mag | 1 Sigma error on Subaru r+ AB magnitude. |
i_mag | double | mag | Subaru i+ AB magnitude. |
i_mag_err | double | mag | 1 Sigma error on Subaru i+ AB magnitude. |
z_mag | double | mag | Subaru z+ AB magnitude. |
z_mag_err | double | mag | 1 Sigma error on Subaru z+ AB magnitude. |
K_mag | double | mag | CTIO/KPNO Ks AB magnitude. |
K_mag_err | double | mag | 1 Sigma error on CTIO/KPNO Ks AB magnitude. |
i_cfht_mag | double | mag | CFHT i* AB magnitude. |
i_cfht_mag_err | double | mag | 1 Sigma error on CFHT i* AB magnitude. |
u_sdss_mag | double | mag | SDSS u AB magnitude. |
u_sdss_mag_err | double | mag | 1 Sigma error on SDSS u AB magnitude. |
g_sdss_mag | double | mag | SDSS g AB magnitude. |
g_sdss_err | double | mag | 1 Sigma error on SDSS g AB magnitude. |
r_sdss_mag | double | mag | SDSS r AB magnitude. |
r_sdss_mag_err | double | mag | 1 Sigma error on SDSS r AB magnitude. |
i_sdss_mag | double | mag | SDSS i AB magnitude. |
i_sdss_mag_err | double | mag | 1 Sigma error on SDSS i AB magnitude. |
z_sdss_mag | double | mag | SDSS z AB magnitude. |
z_sdss_mag_err | double | mag | 1 Sigma error on SDSS z AB magnitude. |
F814W_mag | double | mag | HST F814W magnitude. |
F814W_mag_err | double | mag | 1 Sigma error on HST F814W magnitude. |
NB816_mag | double | mag | Subaru NB816 magnitude. |
NB816_mag_err | double | mag | 1 Sigma error on Subaru NB816 magnitude. |
Ebv | double | number | e(B-V) for this object position from Schlegel et al. (1998). |
Zphot | double | number | Photometric Redshift from Mobasher et al. (2007). |
Zerr_68_min | double | number | Minimum photometric redshift at 68% probability. |
Zerr_68_max | double | number | Maximum photometric redshift at 68% probability. |
Zerr_95_min | double | number | Minimum photometric redshift at 95% probability. |
Zerr_95_max | double | number | Maximum photometric redshift at 95% probability. |
Tphot | double | number | Photometric type of the object as described in Mobasher et al. (2007). 1=El, 2=Sbc, 3=Scd, 4=Irr, 5=SB3, 6=SB2 Non integer values indicate a type between the integer types. |
Rphot | double | number | Intrinsic e(B-V) of the object estimated by the photometric redshift code. See Mobasher et al. (2007) for details. |
Chisq | double | number | Chi-sq of best fit redshift and photometric type. |
Nbands | double | number | Number of filters used for in the photometric redshift estimation. |
Mv | double | mag | Absolute V band AB magnitude. |
D95 | double | number | D95 parameter from Mobasher et al. (2007) Defined as the ratio of the 95% confidence interval to the best fit redshift. |
logMass | double | number | Log base 10 of the stellar mass in units of solar mass. See Mobasher et al. (2007) for more details. |
star | double | number | Star flag based on color and morphology from Capak et al. (2007). 0=Non-Star, 1=Star |
B_mask | double | number | The area of the photometry aperture in square arc seconds which falls into a masked area on the Bj image. Please refer to the text above for more information on masks and flags. |
V_mask | double | number | The area of the photometry aperture in square arc seconds which falls into a masked area on the Vj image. Please refer to the text above for more information on masks and flags. |
i_mask | double | number | The area of the photometry aperture in square arc seconds which falls into a masked area on the i+ image. Please refer to the text above for more information on masks and flags. |
z_mask | double | number | The area of the photometry aperture in square arc seconds which falls into a masked area on the z+ image. Please refer to the text above for more information on masks and flags. |
blend_mask | double | number | Object may be over de-blended or a false detection, see Capak et al. (2007) for details. 0=Good Detection, 1=Problematic Detection. |