ID |
|
Unique object identifier for mutli-wavelength catalogue in this field |
ID_OPTICAL |
|
Identifier for the optical-NIR detected chi2 catalogue (internal use only) |
ID_SPITZER |
|
Identifier for the Spitzer detected chi2 catalogue (internal use only) |
RA |
deg |
Right ascension of multi-wavelength counterpart (J2000) |
DEC |
deg |
Declination of multi-wavelength counterpart (J2000) |
help_id |
|
HELP ID of matched far-IR prior list source |
RA_HELP |
deg |
Right ascension of help_id source in HELP catalog |
DEC_HELP |
deg |
Declination of help_id source in HELP catalog |
EBV |
|
E(B-V) galactic extinction for the source based on its position and Schlegel, Finkbeiner & Davis (1998) |
CLASS_STAR |
|
|
FLAG_DEEP |
|
Manual masking and duplicate source flag from Brown et al. I-band catalog (Reliable sources: FLAG_DEEP != 0) |
FLAG_OVERLAP |
|
Bit flag indicating the multi-wavelength coverage region of the optical source position (ALPHAJ2000, DELTAJ2000) (see flag description above) |
FLAG_CLEAN |
|
3-valued flag indicating bright star masking at the optical source position (see flag description above) |
FUV_flux |
microJy |
Recommended GALEX FUV-band flux (aperture and extinction corrected from 3'' aperture) |
FUV_fluxerr |
microJy |
Recommended GALEX FUV-band flux error (aperture and extinction corrected from 3'' aperture) |
NUV_flux |
microJy |
Recommended GALEX NUV-band flux (aperture and extinction corrected from 3'' aperture) |
NUV_fluxerr |
microJy |
Recommended GALEX NUV-band flux error (aperture and extinction corrected from 3'' aperture) |
u_flux |
microJy |
Recommended u-band flux (aperture and extinction corrected from 3'' aperture) |
u_fluxerr |
microJy |
Recommended u-band flux error (aperture and extinction corrected from 3'' aperture) |
Bw_flux |
microJy |
Recommended NDWFS Bw-band flux (aperture and extinction corrected from 3'' aperture) |
Bw_fluxerr |
microJy |
Recommended NDWFS Bw-band flux error (aperture and extinction corrected from 3'' aperture) |
R_flux |
microJy |
Recommended NDWFS R-band flux (aperture and extinction corrected from 3'' aperture) |
R_fluxerr |
microJy |
Recommended NDWFS R-band flux error (aperture and extinction corrected from 3'' aperture) |
I_flux |
microJy |
Recommended NDWFS I-band flux (aperture and extinction corrected from 3'' aperture) |
I_fluxerr |
microJy |
Recommended NDWFS I-band flux error (aperture and extinction corrected from 3'' aperture) |
z_flux |
microJy |
Recommended z-band flux (aperture and extinction corrected from 3'' aperture) |
z_fluxerr |
microJy |
Recommended z-band flux error (aperture and extinction corrected from 3'' aperture) |
z_Subaru_flux |
microJy |
Recommended z_Subaru-band flux (aperture and extinction corrected from 3'' aperture) |
z_Subaru_fluxerr |
microJy |
Recommended z_Subaru-band flux error (aperture and extinction corrected from 3'' aperture) |
y_flux |
microJy |
Recommended y-band flux (aperture and extinction corrected from 3'' aperture) |
y_fluxerr |
microJy |
Recommended y-band flux error (aperture and extinction corrected from 3'' aperture) |
J_flux |
microJy |
Recommended NEWFIRM J-band flux (aperture and extinction corrected from 3'' aperture) |
J_fluxerr |
microJy |
Recommended NEWFIRM J-band flux error (aperture and extinction corrected from 3'' aperture) |
H_flux |
microJy |
Recommended NEWFIRM H-band flux (aperture and extinction corrected from 3'' aperture) |
H_fluxerr |
microJy |
Recommended NEWFIRM H-band flux error (aperture and extinction corrected from 3'' aperture) |
K_flux |
microJy |
Recommended K-band flux (aperture and extinction corrected from 3'' aperture) |
K_fluxerr |
microJy |
Recommended K-band flux error (aperture and extinction corrected from 3'' aperture) |
Ks_flux |
microJy |
Recommended NEWFIRM Ks-band flux (aperture and extinction corrected from 3'' aperture) |
Ks_fluxerr |
microJy |
Recommended NEWFIRM Ks-band flux error (aperture and extinction corrected from 3'' aperture) |
ch1_flux |
microJy |
Recommended SDWFS Spitzer ch1 flux (aperture and extinction corrected from 4'' aperture) |
ch1_fluxerr |
microJy |
Recommended SDWFS Spitzer ch1 flux error (aperture and extinction corrected from 4'' aperture) |
ch2_flux |
microJy |
Recommended SDWFS Spitzer ch2 flux (aperture and extinction corrected from 4'' aperture) |
ch2_fluxerr |
microJy |
Recommended SDWFS Spitzer ch2 flux error (aperture and extinction corrected from 4'' aperture) |
ch3_flux |
microJy |
Recommended SDWFS Spitzer ch3 flux (aperture and extinction corrected from 4'' aperture) |
ch3_fluxerr |
microJy |
Recommended SDWFS Spitzer ch3 flux error (aperture and extinction corrected from 4'' aperture) |
ch4_flux |
microJy |
Recommended SDWFS Spitzer ch4 flux (aperture and extinction corrected from 4'' aperture) |
ch4_fluxerr |
microJy |
Recommended SDWFS Spitzer ch4 flux error (aperture and extinction corrected from 4'' aperture) |
F_MIPS_24 |
microJy |
Flux density at 24 micron (Median) |
FErr_MIPS_24_u |
microJy |
Flux density at 24 micron (84th Percentile) |
FErr_MIPS_24_l |
microJy |
Flux density at 250 micron (16th Percentile) |
Bkg_MIPS_24 |
MJy/Sr |
Fitted Background of 23 micron map (Median) |
Sig_conf_MIPS_24 |
MJy/Sr |
fixed at 0 |
Rhat_MIPS_24 |
|
Convergence Statistic (ideally <1.2) |
n_eff_MIPS_24 |
|
Number of effective samples (ideally >40) |
Pval_res_24 |
|
Local Goodness of fit measure: 0=good, 1=bad |
flag_mips_24 |
|
combined flag, 0=good, 1=bad |
F_PACS_100 |
mJy |
Flux density at 100 micron (Median) |
FErr_PACS_100_u |
mJy |
Flux density at 100 micron (84th Percentile) |
FErr_PACS_100_l |
mJy |
Flux density at 100 micron (16th Percentile) |
F_PACS_160 |
mJy |
Flux density at 160 micron (Median) |
FErr_PACS_160_u |
mJy |
Flux density at 160 micron (84th Percentile) |
FErr_PACS_160_l |
mJy |
Flux density at 160 micron (16th Percentile) |
Bkg_PACS_100 |
mJy/Beam |
Fitted Background of 100 micron map (Median) |
Bkg_PACS_160 |
mJy/Beam |
Fitted Background of 160 micron map (Median) |
Sig_conf_PACS_100 |
mJy/Beam |
Fitted residual noise component due to confusion (Median) |
Sig_conf_PACS_160 |
mJy/Beam |
Fitted residual noise component due to confusion (Median) |
Rhat_PACS_100 |
|
Convergence Statistic (ideally <1.2) |
Rhat_PACS_160 |
|
Convergence Statistic (ideally <1.2) |
n_eff_PACS_100 |
|
Number of effective samples (ideally >40) |
n_eff_PACS_160 |
|
Number of effective samples (ideally >40) |
Pval_res_100 |
|
Local Goodness of fit measure: 0=good, 1=bad |
Pval_res_160 |
|
Local Goodness of fit measure: 0=good, 1=bad |
flag_PACS_100 |
|
combined flag, 0=good, 1=bad |
flag_PACS_160 |
|
combined flag, 0=good, 1=bad |
F_SPIRE_250 |
mJy |
Flux density at 250 micron (Median) |
FErr_SPIRE_250_u |
mJy |
Flux density at 250 micron (84th Percentile) |
FErr_SPIRE_250_l |
mJy |
Flux density at 250 micron (16th Percentile) |
F_SPIRE_350 |
mJy |
Flux density at 350 micron (Median) |
FErr_SPIRE_350_u |
mJy |
Flux density at 350 micron (84th Percentile) |
FErr_SPIRE_350_l |
mJy |
Flux density at 350 micron (16th Percentile) |
F_SPIRE_500 |
mJy |
Flux density at 500 micron (Median) |
FErr_SPIRE_500_u |
mJy |
Flux density at 500 micron (84th Percentile) |
FErr_SPIRE_500_l |
mJy |
Flux density at 500 micron (16th Percentile) |
Bkg_SPIRE_250 |
mJy/Beam |
Fitted Background of 250 micron map (Median) |
Bkg_SPIRE_350 |
mJy/Beam |
Fitted Background of 350 micron map (Median) |
Bkg_SPIRE_500 |
mJy/Beam |
Fitted Background of 500 micron map (Median) |
Sig_conf_SPIRE_250 |
mJy/Beam |
Fitted residual noise component due to confusion (Median) |
Sig_conf_SPIRE_350 |
mJy/Beam |
Fitted residual noise component due to confusion (Median) |
Sig_conf_SPIRE_500 |
mJy/Beam |
Fitted residual noise component due to confusion (Median) |
Rhat_SPIRE_250 |
|
Convergence Statistic (ideally <1.2) |
Rhat_SPIRE_350 |
|
Convergence Statistic (ideally <1.2) |
Rhat_SPIRE_500 |
|
Convergence Statistic (ideally <1.2) |
n_eff_SPIRE_250 |
|
Number of effective samples (ideally >40) |
n_eff_SPIRE_350 |
|
Number of effective samples (ideally >40) |
n_eff_SPIRE_500 |
|
Number of effective samples (ideally >40) |
Pval_res_250 |
|
Local Goodness of fit measure: 0=good, 1=bad |
Pval_res_350 |
|
Local Goodness of fit measure: 0=good, 1=bad |
Pval_res_500 |
|
Local Goodness of fit measure: 0=good, 1=bad |
flag_spire_250 |
|
combined flag, 0=good, 1=bad |
flag_spire_350 |
|
combined flag, 0=good, 1=bad |
flag_spire_500 |
|
combined flag, 0=good, 1=bad |
Z_BEST |
|
Best available redshift estimate |
Z_BEST_SOURCE |
|
Source of z_best, 0 = photometric, 1 = spectroscopic |
Z_SPEC |
|
Literature Spectroscopic Redshift |
Z_SOURCE |
|
Source of the spectroscopic redshift |
Z_QUAL |
|
Spectroscopic redshift quality: flag Q = 3 means probable, Q >= 4 means reliable |
RA_ZSPEC |
deg |
Right ascension of spectroscopic redshift match (J2000) |
DEC_ZSPEC |
deg |
Declination of spectroscopic redshift match (J2000) |
REL |
|
Expected reliability of the spectroscopic redshift (where available) |
OBJID |
|
Spectroscopic match Object ID (where name depends on Z_SOURCE) |
AGN_ZSPEC |
|
Spectroscopic AGN/QSO flag where provided |
z1_median |
|
Median of the primary redshift peak above 80% HPD CI |
z1_min |
|
Lower bound of the primary 80% HPD CI peak |
z1_max |
|
Upper bound of the primary 80% HPD CI peak |
z1_area |
|
Integrated area of the primary 80% HPD CI peak |
z2_median |
|
Median of the secondary redshift peak (if present) above 80% HPD CI |
z2_min |
|
Lower bound of the secondary 80% HPD CI peak |
z2_max |
|
Upper bound of the secondary 80% HPD CI peak |
z2_area |
|
Integrated area of the secondary 80% HPD CI peak |
nfilt_eazy |
|
Number of filters included in EAZY template fit |
nfilt_atlas |
|
Number of filters included in Atlas+AGN template fit |
nfilt_ananna |
|
Number of filters included in Ananna et al. template fit |
chi_r_best |
|
Chi^2 / nfilt for best-fit galaxy/AGN template (any library) |
chi_r_stellar |
|
Chi^2 / nfilt for best-fit stellar template |
stellar_type |
|
Stellar type of best-fit stellar template |
AGN |
|
Sources flagged by any one of optAGN/IRAGN/XrayAGN |
optAGN |
|
Source is included in Million Quasar Catalog compilation or spectroscopically identified AGN |
IRAGN |
|
Source satisfies Donley et al. (2012) IR AGN criteria |
XrayAGN |
|
Source has X-ray counterpart |
XrayFlux_0.5-2 |
1e-14 ergs/cm**2/s |
XBootes Soft X-ray Flux |
XrayHardness |
|
XBootes X-ray Hardness Ratio |
ap_to_model_z_Subaru |
|
Estimated z-band total flux correction from Legacy Surveys model flux (z_Subaru) |
ap_to_model_err_z_Subaru |
|
Statistical uncertainty on tot_z_Subaru |
ap_to_model_z |
|
Estimated z-band total flux correction from Legacy Surveys model flux (z) |
ap_to_model_err_z |
|
Statistical uncertainty on tot_z |
zmodel |
|
Model grid redshift used in stellar mass fit |
chi_best |
|
Minimum Chi^2 in stellar mass fit (for Z_BEST) |
Mass_median |
log10(M_sol) |
50th percentile of the marginalised stellar mass posterior (for Z_BEST) |
Mass_l68 |
log10(M_sol) |
16th percentile of the marginalised stellar mass posterior (for Z_BEST) |
Mass_u68 |
log10(M_sol) |
84th percentile of the marginalised stellar mass posterior (for Z_BEST) |
Nfilts |
|
Number of bands included in stellar mass fit |
u_rest |
mag |
Rest-frame u-band magnitude for best-fit SED (for Z_BEST) |
Bw_rest |
mag |
Rest-frame Bw-band magnitude for best-fit SED (for Z_BEST) |
R_rest |
mag |
Rest-frame R-band magnitude for best-fit SED (for Z_BEST) |
I_rest |
mag |
Rest-frame I-band magnitude for best-fit SED (for Z_BEST) |
z_rest |
mag |
Rest-frame z-band magnitude for best-fit SED (for Z_BEST) |
z_Subaru_rest |
mag |
Rest-frame zSubaru-band magnitude for best-fit SED (for ZBEST) |
y_rest |
mag |
Rest-frame y-band magnitude for best-fit SED (for Z_BEST) |
J_rest |
mag |
Rest-frame J-band magnitude for best-fit SED (for Z_BEST) |
H_rest |
mag |
Rest-frame H-band magnitude for best-fit SED (for Z_BEST) |
K_rest |
mag |
Rest-frame K-band magnitude for best-fit SED (for Z_BEST) |
Ks_rest |
mag |
Rest-frame Ks-band magnitude for best-fit SED (for Z_BEST) |
ch1_rest |
mag |
Rest-frame IRAC 3.6micron magnitude for best-fit SED (for Z_BEST) |
ch2_rest |
mag |
Rest-frame IRAC 4.5micron magnitude for best-fit SED (for Z_BEST) |
ch3_rest |
mag |
Rest-frame IRAC 5.8micron magnitude for best-fit SED (for Z_BEST) |
ch4_rest |
mag |
Rest-frame IRAC 8.0micron magnitude for best-fit SED (for Z_BEST) |