ACMC Catalog Definitions
Overview
The Auriga-California molecular cloud is a large region of relatively modest star formation
that is part of the Gould Belt. The "Auriga-California Molecular Cloud" (ACMC) Herschel program
observed a 14.5 square degree area in five far-infrared bands.
The ACMC catalog provides photometry for the 60 point-like and very compact sources in each
band: PACS 70 and 160 microns, SPIRE 250, 350, and 500 microns.
If you use this catalog, please cite Harvey et al. (2013).
| Name |
Intype |
Units |
Description |
| SRC |
char |
|
Source number |
| YSO |
char |
|
YSO candidate |
| SIMBAD |
char |
|
SIMBAD type |
| ra |
double |
|
Right Ascension (J2000) |
| dec |
double |
|
Declination (J2000) |
| MIR |
char |
|
first mid-IR detection:
WISE or Spitzer Gould Belt (SpGB) |
| ALPHA |
float |
|
spectral slope |
| CLASS |
char |
|
YSO class |
| L_BOL |
float |
L_sun |
Bolometric luminosity |
| T_BOL |
long |
K |
Bolometric temperature |
| F_NU1 |
float |
mJy |
Flux density at 22 or 24 microns |
| F_NU1ERROR |
float |
mJy |
Uncertainty in F_NU1 |
| F_NU70PSF |
float |
mJy |
Flux density at 70 microns, PSF fitting photometry |
| F_NU70PSFERROR |
float |
mJy |
Uncertainty in F_NU70PSF |
| F_NU70APER |
float |
mJy |
Flux density at 70 microns, aperture photometry |
| F_NU70APERERROR |
float |
mJy |
Uncertainty in F_NU70APER |
| F_NU160PSF |
float |
mJy |
Flux density at 160 microns, PSF fitting photometry |
| F_NU160PSFERROR |
float |
mJy |
Uncertainty in F_NU160PSF |
| F_NU160APER |
float |
mJy |
Flux density at 160 microns, aperture photometry |
| F_NU160MUMAPERERROR |
float |
mJy |
Uncertainty in F_NU160APER |