C2D Overview
c2d has delivered 867 catalogs. IRSA has merged these delivered catalogs into four groups - Clouds, Off-Cloud, Cores, Stars - and serves them through the general catalog search engine Gator. Many of the delivered catalogs, images and spectra are accessible through IRSA's general search service, Atlas. A summary of the catalogs types and how to access them is as follows:
Catalog Name | Content | Gator Access (merged) | Atlas Access (as delivered) |
FULL | Complete source lists (Section 3.2 of c2d data delivery document [ps | pdf]) | Y | Y |
HREL | Derived from the full catalogs are high reliability catalogs (Section 3.2.1 [ps | pdf]) | Y | Y |
YSOc | Derived from the full catalogs are young stellar object candidates (Section 3.2.2 [ps | pdf]) | Y | Y |
MM | Millimeter wavelength source lists (Section 3.2.3 [ps | pdf]) | Y | Y |
Transients | Catalogs of transients in two epochs (Section 3.2.4 [ps | pdf]) | Y | N |
resampled-SWIRE | Resampled sources in the ELAIS N1 field measured by the SWIRE Legacy Project, that have been used to study c2d background contamination (Section 3.8 [ps | pdf]) | N (see footnote 1 for download information) 1 |
N (see footnote 1 for download information) 1 |
1 resampled-SWIRE catalogs can be downloaded in their entirety per cloud (CHA_II, LUP, OPH, PER, and SER).
The data are also available for direct download as follows: images and associated catalogs are organized according to object type - CORES or STARS - or the names of 5 major CLOUDS - ChamaeleonII (CHA_II), Lupus (LUP), Ophiuchus (OPH), Perseus (PER) and Serpens (SER); IRS spectra and MIPS SED's are organized by object name.
C2D Millimeter Source Catalog Definitions
Please refer to the data delivery documentation for further information. The column descriptions can be found below.
name | intype | units | description |
region | char | Region or cloud from which this catalog was drawn. Please see section above for the derivation of region column values. All possible region string values in the merged MM catalog are "OPH", "PER" and "SER". | |
Bolo_ID | char | Bolocam source name | |
RA | float | degree | Right Ascension [J2000] |
Dec | float | degree | Declination [J2000] |
Peak_flux | float | Jy_per_beam | Peak flux density per beam |
D_Peak_flux | float | Jy_per_beam | Uncertainty in Peak_flux |
S_N | float | Signal-to-noise ratio of Peak_flux | |
Flux_40asec | float | Jy | Integrated flux density in 40-arcsec diameter aperture |
D_Flux_40asec | float | Jy | Uncertainty in Flux_40asec |
Flux_80asec | float | Jy | Integrated flux density in 80-arcsec diameter aperture |
D_Flux_80asec | float | Jy | Uncertainty in Flux_80asec |
Flux_120asec | float | Jy | Integrated flux density in 120-arcsec diameter aperture |
D_Flux_120asec | float | Jy | Uncertainty in Flux_120asec |
Total_flux | float | Jy | Total integrated flux |
D_Total_flux | float | Jy | Uncertainty in Total_flux |
FWHM_minor | float | arcsec | FWHM along source minor axis |
D_FWHM_minor | float | arcsec | Uncertainty in FWHM_minor |
FWHM_major | float | arcsec | FWHM along source major axis |
D_FWHM_major | float | arcsec | Uncertainty in FWHM_major |
PA | int | degree | Position angle |
D_PA | int | degree | Uncertainty in PA |
Mass_10K | float | M_sun | Total isothermal mass for T=10K |
D_Mass_10K | float | M_sun | Uncertainty in Mass_10K |
Peak_Av | int | magnitudes | Visual extinction calculated from Peak_flux |
mean_density | char | per_cubic_cm | Mean particle density (assuming spherical source) |
Morphology | char | Description of source shape and environment | |
Spitzer_YSO | char | Association with one (yes) or more (multiple) c2d YSO(s) | |
SSTc2d_ID | char | c2d source name of nearest YSO |