S4G Catalog Definitions
Overview
The Spitzer Survey of Stellar Structure in Galaxies (S4G) is a volume-, magnitude-, and size-limited survey of over 2300 nearby galaxies at 3.6 and 4.5 microns. This is an extremely deep survey reaching an unprecedented 1 sigma surface brightness limit of μ3.6(AB) = 27 mag arcsec-2. This translates to a stellar surface density of << 1 Msun pc-2.
The S4G Catalog provides photometry and model parameters derived from the IRAC images, as well as a link to the summary and data access page for each galaxy and a variety of quantities taken from previously published work.
S4G Images
S4G Home Page
Sheth et al. (2010)
| Name | Intype | Units | Description |
|---|---|---|---|
| object | char | Galaxy name | |
| ra | double | deg | Right ascension (J2000) Measured at centroid of the peak emission at 3.6 microns |
| dec | double | deg | Declination (J2000) Measured at centroid of the peak emission at 3.6 microns |
| sma1_25p5 | double | arcsec | Semi-major axis at mu_3.6 = 25.5 AB mag/arcsec2 |
| PA1_25p5 | double | deg | Position angle at mu_3.6 = 25.5 AB mag/arcsec2 |
| ellip1_25p5 | double | Ellipticity (1-b/a) at mu_3.6 = 25.5 AB mag/arcsec2 | |
| sma1_26p5 | double | arcsec | Semi-major axis at mu_3.6 = 26.5 AB mag/arcsec2 |
| PA1_26p5 | double | deg | Position angle at mu_3.6 = 26.5 AB mag/arcsec2 |
| ellip1_26p5 | double | Ellipticity (1-b/a) at mu_3.6 = 26.5 AB mag/arcsec2 | |
| sma2_25p5 | double | arcsec | Semi-major axis at mu_4.5 = 25.5 AB mag/arcsec2 |
| PA2_25p5 | double | deg | Position angle at mu_4.5 = 25.5 AB mag/arcsec2 |
| ellip2_25p5 | double | Ellipticity (1-b/a) at mu_4.5 = 25.5 AB mag/arcsec2 | |
| sma2_26p5 | double | arcsec | Semi-major axis at mu_4.5 = 26.5 AB mag/arcsec2 |
| PA2_26p5 | double | deg | Position angle at mu_4.5 = 26.5 AB mag/arcsec2 |
| ellip2_26p5 | double | Ellipticity (1-b/a) at mu_4.5 = 26.5 AB mag/arcsec2 | |
| mag1 | double | AB | Asymptotic magnitude at 3.6 microns Growth curve using concentric ellipses with e=ellip1_25p5 and PA=PA1_25p5 |
| emag1 | double | AB | Growth-curve fitting error in mag1 |
| mag2 | double | AB | Asymptotic magnitude at 4.5 microns Growth curve using concentric ellipses with e=ellip2_25p5 and PA=PA2_25p5 |
| emag2 | double | AB | Growth-curve fitting error in mag2 |
| sky1 | double | MJy/sr | Sky level at 3.6 microns Sky measured in ~90 boxes of 1000 pixels each |
| ssky1 | double | MJy/sr | Local, pixel-to-pixel noise at 3.6 microns |
| esky1 | double | MJy/sr | Large scale sky noise at 3.6 microns RMS of the mean sky values among the different boxes |
| sky2 | double | MJy/sr | Sky level at 4.5 microns Sky measured in ~90 boxes of 1000 pixels each |
| ssky2 | double | MJy/sr | Local, pixel-to-pixel noise at 4.5 microns |
| esky2 | double | MJy/sr | Large scale sky noise at 4.5 microns RMS of the mean sky values among the different boxes |
| c31_1 | double | r75/r25 concentration index at 3.6 microns Measured from growth curve with e=ellip1_25p5 and PA=PA1_25p5 |
|
| c42_1 | double | 5*log10(r80/r20) concentration index at 3.6 microns Measured from growth curve with e=ellip1_25p5 and PA=PA1_25p5 |
|
| c31_2 | double | r75/r25 concentration index at 4.5 microns Measured from growth curve with e=ellip2_25p5 and PA=PA2_25p5 |
|
| c42_2 | double | 5*log10(r80/r20) concentration index at 4.5 microns Measured from growth curve with e=ellip2_25p5 and PA=PA2_25p5 |
|
| Mabs1 | double | AB | Absolute magnitude at 3.6 microns From mag1, using dmean when available, vvir & H0=71 otherwise |
| Mabs2 | double | AB | Absolute magnitude at 4.5 microns From mag2, using dmean when available, vvir & H0=71 otherwise |
| Mstar | double | Msun | log10(stellar mass) Using Mabs1 and Mabs2 in the calibration of Eskew et al. (2012) |
| dmean | double | Mpc | Mean redshift-independent distance From NED |
| dstd | double | Mpc | Standard deviation of all redshift-indenpendent distances From NED |
| dmin | double | Mpc | Minimum redshift-independent distance From NED |
| dmax | double | Mpc | Maximum redshift-independent distance From NED |
| dmed | double | Mpc | Median redshift-independent distance From NED |
| type | char | t | Optical Hubble type From Leda |
| bar | char | Bar presence ("B"). NULL does not necessarily mean unbarred! From Leda |
|
| ring | char | Ring presence ("R"). NULL does not necessarily mean no ring! From Leda |
|
| multiple | char | Multiple system ("M") From Leda |
|
| compactness | char | C=Compact. D=Difusse. NULL just means not classified! From Leda |
|
| t | double | Morphological type code From Leda |
|
| e_t | double | Error on t From Leda |
|
| lc | double | Luminosity class From Leda |
|
| e_lc | double | Error on lc From Leda |
|
| logd25 | double | 0.1arcmin | log10 of apparent diameter (d25 in 0.1') From Leda |
| e_logd25 | double | Error on logd25 From Leda |
|
| logr25 | double | log10 of axis ratio (major axis/minor axis) From Leda |
|
| e_logr25 | double | Error on logr25 From Leda |
|
| pa | double | deg | Major axis position angle at mu_B = 25 mag/arcsec2 From Leda |
| brief | double | mag/arcsec2 | Mean effective surface brightness in the B band From Leda |
| e_brief | double | mag/arcsec2 | Error on brief From Leda |
| bt | double | mag | Total B-magnitude From Leda |
| e_bt | double | mag | Error on bt From Leda |
| it | double | mag | Total I-magnitude From Leda |
| e_it | double | mag | Error on it From Leda |
| ubt | double | mag | Total U-B color From Leda |
| bvt | double | mag | Total B-V color From Leda |
| ube | double | mag | Effective U-B color From Leda |
| bve | double | mag | Effective B-V color From Leda |
| vmaxg | double | km/s | Apparent maximum rotation velocity of gas From Leda |
| e_vmaxg | double | km/s | Error on vmaxg From Leda |
| vdis | double | km/s | Central velocity dispersion From Leda |
| e_vdis | double | km/s | Error on vdis From Leda |
| mg2 | double | mag | Central Mg2 Lick index From Leda |
| e_mg2 | double | mag | Error on mg2 From Leda |
| m21 | double | mag | 21-cm line flux in magnitude (see definition in text) From Leda |
| e_m21 | double | mag | Error on m21 From Leda |
| mfir | double | mag | Far infrared magnitude (see definition in text) From Leda |
| vrad | double | km/s | Heliocentric radial velocity from radio measurement From Leda |
| e_vrad | double | km/s | Error on vrad From Leda |
| vopt | double | km/s | Heliocentric radial velocity from optical measurement From Leda |
| e_vopt | double | km/s | Error on vopt From Leda |
| v | double | km/s | Mean heliocentric radial velocity From Leda |
| e_v | double | km/s | Error on v From Leda |
| ag | double | mag | Galactic extinction in B magnitude From Leda |
| ai | double | mag | Extinction due to inclination in B magnitude From Leda |
| incl | double | deg | Inclination between line of sight and polar axis From Leda |
| a21 | double | mag | 21-cm self absorption in magnitude From Leda |
| lambda | double | Luminosity index From Leda |
|
| logdc | double | 0.1arcmin | log10 of apparent corrected diameter (dc in 0.1') From Leda |
| btc | double | mag | Total apparent corrected B-magnitude From Leda |
| ubtc | double | mag | Total apparent corrected U-B color From Leda |
| bvtc | double | mag | Total apparent corrected B-V color From Leda |
| bri25 | double | mag/arcsec2 | Mean surface brightness within isophote 25 From Leda |
| vrot | double | km/s | Maximum velocity rotation From Leda |
| e_vrot | double | km/s | Error on vrot From Leda |
| m21c | double | mag | Corrected 21-cm line flux in magnitude (see text) From Leda |
| hic | double | mag | 21-cm index bt-m21c in magnitude From Leda |
| vlg | double | km/s | Radial velocity with respect to the Local Group From Leda |
| vgsr | double | km/s | Radial velocity with respect to the GSR From Leda |
| vvir | double | km/s | Radial velocity corrected for Virgocentric infall From Leda |
| v3k | double | km/s | Radial velocity with respect to the CMB radiation From Leda |
| modz | double | mag | Redshift distance modulus From Leda |
| mod0 | double | mag | True distance modulus (from parameters) From Leda |
| mabs | double | mag | Absolute B-magnitude From Leda |
| summary | char | Summary and data access |