1 |
ID |
ID (specifically ID_FARMER, as this is the Farmer catalogue) |
INT64 |
1 |
meta.id;meta.main |
|
2 |
ALPHA_J2000 |
Right ascension (J2000) of model, or of SEP when model is not avail. |
DOUBLE |
1 |
pos.eq.ra;meta.main |
deg |
3 |
DELTA_J2000 |
Declination (J2000) of model, or of SEP when model is not available |
DOUBLE |
1 |
pos.eq.dec;meta.main |
deg |
4 |
X_MODEL |
Object model position along X, with the scale being 0.15"/px |
DOUBLE |
1 |
pos.cartesian.x |
pix |
5 |
Y_MODEL |
Object model position along Y, with the scale being 0.15"/px |
DOUBLE |
1 |
pos.cartesian.y |
pix |
6 |
ERRX_MODEL |
Uncertainty on object model position along X |
DOUBLE |
1 |
stat.error;pos.cartesian.x |
pix |
7 |
ERRY_MODEL |
Uncertainty on object model position along Y |
DOUBLE |
1 |
stat.error;pos.cartesian.y |
pix |
8 |
ALPHA_DETECTION |
Right ascension (J2000) of object as determined by SEP at detection |
DOUBLE |
1 |
pos.eq.ra |
deg |
9 |
DELTA_DETECTION |
Declination (J2000) of object as determined by SEP at detection |
DOUBLE |
1 |
pos.eq.dec |
deg |
10 |
FARMER_ID |
Farmer internal source identifier ({brick}_{source}) |
STRING |
8 |
meta.id |
|
11 |
GROUP_ID |
Farmer group identifier; unique within a brick |
INT64 |
1 |
meta.code |
|
12 |
N_GROUP |
Farmer group occupation number |
INT64 |
1 |
meta.number |
|
13 |
MODEL_FLAG |
Flag (0: OK, 1: failed to converge, 2: drifted >0.6" from detection) |
INT16 |
1 |
meta.code |
|
14 |
SOLUTION_MODEL |
The Tractor model type selected by The Farmer |
STRING |
20 |
meta.code |
|
15 |
FLAG_HSC |
Flag indicating quality of HSC imaging (0:clean, 1:masked) |
INT16 |
1 |
meta.code |
|
16 |
FLAG_SUPCAM |
Flag indicating quality of Suprime-Cam imaging (0:clean, 1:masked) |
INT16 |
1 |
meta.code |
|
17 |
FLAG_UDEEP |
Flag for the UltraVISTA ultra-deep regions (0:ultra-deep, 1:deep) |
INT16 |
1 |
meta.code |
|
18 |
FLAG_UVISTA |
Flag for the UltraVISTA region (0:inside, 1:outside) |
INT16 |
1 |
meta.code |
|
19 |
FLAG_COMBINED |
Comb. FLAG_UVISTA, FLAG_HSC, FLAG_SUPCAM (0:clean and inside UVISTA) |
INT64 |
1 |
meta.code |
|
20 |
EBV_MW |
Galactic reddening E(B-V) (Schlegel+1998, Schlafly&Finkbeiner 2011) |
DOUBLE |
1 |
phys.absorption.gal |
|
21 |
CFHT_u_FLUX |
CFHT_u flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.U |
uJy |
22 |
CFHT_u_FLUXERR |
CFHT_u flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.U |
uJy |
23 |
CFHT_u_MAG |
CFHT_u AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.U |
mag |
24 |
CFHT_u_MAGERR |
CFHT_u AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.U |
mag |
25 |
CFHT_u_CHISQ |
CFHT_u reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.U |
|
26 |
CFHT_u_DRIFT |
CFHT_u distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.U |
arcsec |
27 |
CFHT_u_VALID |
CFHT_u flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.U |
|
28 |
CFHT_ustar_FLUX |
CFHT_ustar flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.U |
uJy |
29 |
CFHT_ustar_FLUXERR |
CFHT_ustar flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.U |
uJy |
30 |
CFHT_ustar_MAG |
CFHT_ustar AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.U |
mag |
31 |
CFHT_ustar_MAGERR |
CFHT_ustar AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.U |
mag |
32 |
CFHT_ustar_CHISQ |
CFHT_ustar reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.U |
|
33 |
CFHT_ustar_DRIFT |
CFHT_ustar distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.U |
arcsec |
34 |
CFHT_ustar_VALID |
CFHT_ustar flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.U |
|
35 |
HSC_g_FLUX |
HSC_g flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.B |
uJy |
36 |
HSC_g_FLUXERR |
HSC_g flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.B |
uJy |
37 |
HSC_g_MAG |
HSC_g AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.B |
mag |
38 |
HSC_g_MAGERR |
HSC_g AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.B |
mag |
39 |
HSC_g_CHISQ |
HSC_g reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.B |
|
40 |
HSC_g_DRIFT |
HSC_g distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.B |
arcsec |
41 |
HSC_g_VALID |
HSC_g flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.B |
|
42 |
HSC_r_FLUX |
HSC_r flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.R |
uJy |
43 |
HSC_r_FLUXERR |
HSC_r flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.R |
uJy |
44 |
HSC_r_MAG |
HSC_r AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.R |
mag |
45 |
HSC_r_MAGERR |
HSC_r AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.R |
mag |
46 |
HSC_r_CHISQ |
HSC_r reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.R |
|
47 |
HSC_r_DRIFT |
HSC_r distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.R |
arcsec |
48 |
HSC_r_VALID |
HSC_r flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.R |
|
49 |
HSC_i_FLUX |
HSC_i flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.I |
uJy |
50 |
HSC_i_FLUXERR |
HSC_i flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.I |
uJy |
51 |
HSC_i_MAG |
HSC_i AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.I |
mag |
52 |
HSC_i_MAGERR |
HSC_i AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.I |
mag |
53 |
HSC_i_CHISQ |
HSC_i reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.I |
|
54 |
HSC_i_DRIFT |
HSC_i distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.I |
arcsec |
55 |
HSC_i_VALID |
HSC_i flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.I |
|
56 |
HSC_z_FLUX |
HSC_z flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.I |
uJy |
57 |
HSC_z_FLUXERR |
HSC_z flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.I |
uJy |
58 |
HSC_z_MAG |
HSC_z AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.I |
mag |
59 |
HSC_z_MAGERR |
HSC_z AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.I |
mag |
60 |
HSC_z_CHISQ |
HSC_z reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.I |
|
61 |
HSC_z_DRIFT |
HSC_z distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.I |
arcsec |
62 |
HSC_z_VALID |
HSC_z flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.I |
|
63 |
HSC_y_FLUX |
HSC_y flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.I |
uJy |
64 |
HSC_y_FLUXERR |
HSC_y flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.I |
uJy |
65 |
HSC_y_MAG |
HSC_y AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.I |
mag |
66 |
HSC_y_MAGERR |
HSC_y AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.I |
mag |
67 |
HSC_y_CHISQ |
HSC_y reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.I |
|
68 |
HSC_y_DRIFT |
HSC_y distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.I |
arcsec |
69 |
HSC_y_VALID |
HSC_y flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.I |
|
70 |
UVISTA_Y_FLUX |
UVISTA_Y flux density |
DOUBLE |
1 |
phot.flux.density;em.IR.J |
uJy |
71 |
UVISTA_Y_FLUXERR |
UVISTA_Y flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.IR.J |
uJy |
72 |
UVISTA_Y_MAG |
UVISTA_Y AB magnitude |
DOUBLE |
1 |
phot.mag;em.IR.J |
mag |
73 |
UVISTA_Y_MAGERR |
UVISTA_Y AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.IR.J |
mag |
74 |
UVISTA_Y_CHISQ |
UVISTA_Y reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.IR.J |
|
75 |
UVISTA_Y_DRIFT |
UVISTA_Y distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.IR.J |
arcsec |
76 |
UVISTA_Y_VALID |
UVISTA_Y flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.IR.J |
|
77 |
UVISTA_J_FLUX |
UVISTA_J flux density |
DOUBLE |
1 |
phot.flux.density;em.IR.J |
uJy |
78 |
UVISTA_J_FLUXERR |
UVISTA_J flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.IR.J |
uJy |
79 |
UVISTA_J_MAG |
UVISTA_J AB magnitude |
DOUBLE |
1 |
phot.mag;em.IR.J |
mag |
80 |
UVISTA_J_MAGERR |
UVISTA_J AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.IR.J |
mag |
81 |
UVISTA_J_CHISQ |
UVISTA_J reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.IR.J |
|
82 |
UVISTA_J_DRIFT |
UVISTA_J distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.IR.J |
arcsec |
83 |
UVISTA_J_VALID |
UVISTA_J flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.IR.J |
|
84 |
UVISTA_H_FLUX |
UVISTA_H flux density |
DOUBLE |
1 |
phot.flux.density;em.IR.H |
uJy |
85 |
UVISTA_H_FLUXERR |
UVISTA_H flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.IR.H |
uJy |
86 |
UVISTA_H_MAG |
UVISTA_H AB magnitude |
DOUBLE |
1 |
phot.mag;em.IR.H |
mag |
87 |
UVISTA_H_MAGERR |
UVISTA_H AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.IR.H |
mag |
88 |
UVISTA_H_CHISQ |
UVISTA_H reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.IR.H |
|
89 |
UVISTA_H_DRIFT |
UVISTA_H distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.IR.H |
arcsec |
90 |
UVISTA_H_VALID |
UVISTA_H flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.IR.H |
|
91 |
UVISTA_Ks_FLUX |
UVISTA_Ks flux density |
DOUBLE |
1 |
phot.flux.density;em.IR.K |
uJy |
92 |
UVISTA_Ks_FLUXERR |
UVISTA_Ks flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.IR.K |
uJy |
93 |
UVISTA_Ks_MAG |
UVISTA_Ks AB magnitude |
DOUBLE |
1 |
phot.mag;em.IR.K |
mag |
94 |
UVISTA_Ks_MAGERR |
UVISTA_Ks AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.IR.K |
mag |
95 |
UVISTA_Ks_CHISQ |
UVISTA_Ks reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.IR.K |
|
96 |
UVISTA_Ks_DRIFT |
UVISTA_Ks distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.IR.K |
arcsec |
97 |
UVISTA_Ks_VALID |
UVISTA_Ks flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.IR.K |
|
98 |
UVISTA_NB118_FLUX |
UVISTA_NB118 flux density |
DOUBLE |
1 |
phot.flux.density;em.IR.J |
uJy |
99 |
UVISTA_NB118_FLUXERR |
UVISTA_NB118 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.IR.J |
uJy |
100 |
UVISTA_NB118_MAG |
UVISTA_NB118 AB magnitude |
DOUBLE |
1 |
phot.mag;em.IR.J |
mag |
101 |
UVISTA_NB118_MAGERR |
UVISTA_NB118 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.IR.J |
mag |
102 |
UVISTA_NB118_CHISQ |
UVISTA_NB118 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.IR.J |
|
103 |
UVISTA_NB118_DRIFT |
UVISTA_NB118 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.IR.J |
arcsec |
104 |
UVISTA_NB118_VALID |
UVISTA_NB118 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.IR.J |
|
105 |
SC_IB427_FLUX |
SC_IB427 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.B |
uJy |
106 |
SC_IB427_FLUXERR |
SC_IB427 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.B |
uJy |
107 |
SC_IB427_MAG |
SC_IB427 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.B |
mag |
108 |
SC_IB427_MAGERR |
SC_IB427 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.B |
mag |
109 |
SC_IB427_CHISQ |
SC_IB427 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.B |
|
110 |
SC_IB427_DRIFT |
SC_IB427 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.B |
arcsec |
111 |
SC_IB427_VALID |
SC_IB427 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.B |
|
112 |
SC_IB464_FLUX |
SC_IB464 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.B |
uJy |
113 |
SC_IB464_FLUXERR |
SC_IB464 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.B |
uJy |
114 |
SC_IB464_MAG |
SC_IB464 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.B |
mag |
115 |
SC_IB464_MAGERR |
SC_IB464 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.B |
mag |
116 |
SC_IB464_CHISQ |
SC_IB464 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.B |
|
117 |
SC_IB464_DRIFT |
SC_IB464 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.B |
arcsec |
118 |
SC_IB464_VALID |
SC_IB464 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.B |
|
119 |
SC_IA484_FLUX |
SC_IA484 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.B |
uJy |
120 |
SC_IA484_FLUXERR |
SC_IA484 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.B |
uJy |
121 |
SC_IA484_MAG |
SC_IA484 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.B |
mag |
122 |
SC_IA484_MAGERR |
SC_IA484 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.B |
mag |
123 |
SC_IA484_CHISQ |
SC_IA484 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.B |
|
124 |
SC_IA484_DRIFT |
SC_IA484 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.B |
arcsec |
125 |
SC_IA484_VALID |
SC_IA484 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.B |
|
126 |
SC_IB505_FLUX |
SC_IB505 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.V |
uJy |
127 |
SC_IB505_FLUXERR |
SC_IB505 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.V |
uJy |
128 |
SC_IB505_MAG |
SC_IB505 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.V |
mag |
129 |
SC_IB505_MAGERR |
SC_IB505 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.V |
mag |
130 |
SC_IB505_CHISQ |
SC_IB505 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.V |
|
131 |
SC_IB505_DRIFT |
SC_IB505 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.V |
arcsec |
132 |
SC_IB505_VALID |
SC_IB505 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.V |
|
133 |
SC_IA527_FLUX |
SC_IA527 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.V |
uJy |
134 |
SC_IA527_FLUXERR |
SC_IA527 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.V |
uJy |
135 |
SC_IA527_MAG |
SC_IA527 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.V |
mag |
136 |
SC_IA527_MAGERR |
SC_IA527 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.V |
mag |
137 |
SC_IA527_CHISQ |
SC_IA527 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.V |
|
138 |
SC_IA527_DRIFT |
SC_IA527 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.V |
arcsec |
139 |
SC_IA527_VALID |
SC_IA527 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.V |
|
140 |
SC_IB574_FLUX |
SC_IB574 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.V |
uJy |
141 |
SC_IB574_FLUXERR |
SC_IB574 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.V |
uJy |
142 |
SC_IB574_MAG |
SC_IB574 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.V |
mag |
143 |
SC_IB574_MAGERR |
SC_IB574 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.V |
mag |
144 |
SC_IB574_CHISQ |
SC_IB574 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.V |
|
145 |
SC_IB574_DRIFT |
SC_IB574 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.V |
arcsec |
146 |
SC_IB574_VALID |
SC_IB574 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.V |
|
147 |
SC_IA624_FLUX |
SC_IA624 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.R |
uJy |
148 |
SC_IA624_FLUXERR |
SC_IA624 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.R |
uJy |
149 |
SC_IA624_MAG |
SC_IA624 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.R |
mag |
150 |
SC_IA624_MAGERR |
SC_IA624 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.R |
mag |
151 |
SC_IA624_CHISQ |
SC_IA624 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.R |
|
152 |
SC_IA624_DRIFT |
SC_IA624 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.R |
arcsec |
153 |
SC_IA624_VALID |
SC_IA624 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.R |
|
154 |
SC_IA679_FLUX |
SC_IA679 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.R |
uJy |
155 |
SC_IA679_FLUXERR |
SC_IA679 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.R |
uJy |
156 |
SC_IA679_MAG |
SC_IA679 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.R |
mag |
157 |
SC_IA679_MAGERR |
SC_IA679 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.R |
mag |
158 |
SC_IA679_CHISQ |
SC_IA679 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.R |
|
159 |
SC_IA679_DRIFT |
SC_IA679 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.R |
arcsec |
160 |
SC_IA679_VALID |
SC_IA679 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.R |
|
161 |
SC_IB709_FLUX |
SC_IB709 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.R |
uJy |
162 |
SC_IB709_FLUXERR |
SC_IB709 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.R |
uJy |
163 |
SC_IB709_MAG |
SC_IB709 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.R |
mag |
164 |
SC_IB709_MAGERR |
SC_IB709 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.R |
mag |
165 |
SC_IB709_CHISQ |
SC_IB709 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.R |
|
166 |
SC_IB709_DRIFT |
SC_IB709 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.R |
arcsec |
167 |
SC_IB709_VALID |
SC_IB709 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.R |
|
168 |
SC_IA738_FLUX |
SC_IA738 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.R |
uJy |
169 |
SC_IA738_FLUXERR |
SC_IA738 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.R |
uJy |
170 |
SC_IA738_MAG |
SC_IA738 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.R |
mag |
171 |
SC_IA738_MAGERR |
SC_IA738 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.R |
mag |
172 |
SC_IA738_CHISQ |
SC_IA738 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.R |
|
173 |
SC_IA738_DRIFT |
SC_IA738 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.R |
arcsec |
174 |
SC_IA738_VALID |
SC_IA738 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.R |
|
175 |
SC_IA767_FLUX |
SC_IA767 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.I |
uJy |
176 |
SC_IA767_FLUXERR |
SC_IA767 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.I |
uJy |
177 |
SC_IA767_MAG |
SC_IA767 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.I |
mag |
178 |
SC_IA767_MAGERR |
SC_IA767 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.I |
mag |
179 |
SC_IA767_CHISQ |
SC_IA767 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.I |
|
180 |
SC_IA767_DRIFT |
SC_IA767 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.I |
arcsec |
181 |
SC_IA767_VALID |
SC_IA767 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.I |
|
182 |
SC_IB827_FLUX |
SC_IB827 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.I |
uJy |
183 |
SC_IB827_FLUXERR |
SC_IB827 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.I |
uJy |
184 |
SC_IB827_MAG |
SC_IB827 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.I |
mag |
185 |
SC_IB827_MAGERR |
SC_IB827 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.I |
mag |
186 |
SC_IB827_CHISQ |
SC_IB827 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.I |
|
187 |
SC_IB827_DRIFT |
SC_IB827 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.I |
arcsec |
188 |
SC_IB827_VALID |
SC_IB827 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.I |
|
189 |
SC_NB711_FLUX |
SC_NB711 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.R |
uJy |
190 |
SC_NB711_FLUXERR |
SC_NB711 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.R |
uJy |
191 |
SC_NB711_MAG |
SC_NB711 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.R |
mag |
192 |
SC_NB711_MAGERR |
SC_NB711 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.R |
mag |
193 |
SC_NB711_CHISQ |
SC_NB711 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.R |
|
194 |
SC_NB711_DRIFT |
SC_NB711 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.R |
arcsec |
195 |
SC_NB711_VALID |
SC_NB711 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.R |
|
196 |
SC_NB816_FLUX |
SC_NB816 flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.I |
uJy |
197 |
SC_NB816_FLUXERR |
SC_NB816 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.I |
uJy |
198 |
SC_NB816_MAG |
SC_NB816 AB magnitude |
DOUBLE |
1 |
phot.mag;em.opt.I |
mag |
199 |
SC_NB816_MAGERR |
SC_NB816 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.opt.I |
mag |
200 |
SC_NB816_CHISQ |
SC_NB816 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.opt.I |
|
201 |
SC_NB816_DRIFT |
SC_NB816 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.opt.I |
arcsec |
202 |
SC_NB816_VALID |
SC_NB816 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.opt.I |
|
203 |
IRAC_CH1_FLUX |
IRAC_CH1 flux density |
DOUBLE |
1 |
phot.flux.density;em.IR.3-4um |
uJy |
204 |
IRAC_CH1_FLUXERR |
IRAC_CH1 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.IR.3-4um |
uJy |
205 |
IRAC_CH1_MAG |
IRAC_CH1 AB magnitude |
DOUBLE |
1 |
phot.mag;em.IR.3-4um |
mag |
206 |
IRAC_CH1_MAGERR |
IRAC_CH1 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.IR.3-4um |
mag |
207 |
IRAC_CH1_CHISQ |
IRAC_CH1 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.IR.3-4um |
|
208 |
IRAC_CH1_DRIFT |
IRAC_CH1 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.IR.3-4um |
arcsec |
209 |
IRAC_CH1_VALID |
IRAC_CH1 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.IR.3-4um |
|
210 |
IRAC_CH2_FLUX |
IRAC_CH2 flux density |
DOUBLE |
1 |
phot.flux.density;em.IR.4-8um |
uJy |
211 |
IRAC_CH2_FLUXERR |
IRAC_CH2 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.IR.4-8um |
uJy |
212 |
IRAC_CH2_MAG |
IRAC_CH2 AB magnitude |
DOUBLE |
1 |
phot.mag;em.IR.4-8um |
mag |
213 |
IRAC_CH2_MAGERR |
IRAC_CH2 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.IR.4-8um |
mag |
214 |
IRAC_CH2_CHISQ |
IRAC_CH2 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.IR.4-8um |
|
215 |
IRAC_CH2_DRIFT |
IRAC_CH2 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.IR.4-8um |
arcsec |
216 |
IRAC_CH2_VALID |
IRAC_CH2 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.IR.4-8um |
|
217 |
IRAC_CH3_FLUX |
IRAC_CH3 flux density |
DOUBLE |
1 |
phot.flux.density;em.IR.4-8um |
uJy |
218 |
IRAC_CH3_FLUXERR |
IRAC_CH3 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.IR.4-8um |
uJy |
219 |
IRAC_CH3_MAG |
IRAC_CH3 AB magnitude |
DOUBLE |
1 |
phot.mag;em.IR.4-8um |
mag |
220 |
IRAC_CH3_MAGERR |
IRAC_CH3 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.IR.4-8um |
mag |
221 |
IRAC_CH3_CHISQ |
IRAC_CH3 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.IR.4-8um |
|
222 |
IRAC_CH3_DRIFT |
IRAC_CH3 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.IR.4-8um |
arcsec |
223 |
IRAC_CH3_VALID |
IRAC_CH3 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.IR.4-8um |
|
224 |
IRAC_CH4_FLUX |
IRAC_CH4 flux density |
DOUBLE |
1 |
phot.flux.density;em.IR.4-8um |
uJy |
225 |
IRAC_CH4_FLUXERR |
IRAC_CH4 flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.IR.4-8um |
uJy |
226 |
IRAC_CH4_MAG |
IRAC_CH4 AB magnitude |
DOUBLE |
1 |
phot.mag;em.IR.4-8um |
mag |
227 |
IRAC_CH4_MAGERR |
IRAC_CH4 AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.IR.4-8um |
mag |
228 |
IRAC_CH4_CHISQ |
IRAC_CH4 reduced Chi2 goodness of fit stat for source prof model |
DOUBLE |
1 |
stat.fit.goodness;phot;em.IR.4-8um |
|
229 |
IRAC_CH4_DRIFT |
IRAC_CH4 distance travelled from RA,Dec model centroid |
DOUBLE |
1 |
pos.angDistance;phot;em.IR.4-8um |
arcsec |
230 |
IRAC_CH4_VALID |
IRAC_CH4 flag=False if FLUX/MAG or its error is not trustworthy |
LOGICAL |
1 |
meta.code;phot;em.IR.4-8um |
|
231 |
ID_GALEX |
ID in GALEX cat. (Zamojski+2007, Capak+2007), crossm. with 0.6" rad. |
INT64 |
1 |
meta.id |
|
232 |
GALEX_NUV_FLUX |
GALEX_NUV flux density |
DOUBLE |
1 |
phot.flux.density;em.UV.200-300nm |
uJy |
233 |
GALEX_NUV_FLUXERR |
GALEX_NUV flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.UV.200-300nm |
uJy |
234 |
GALEX_NUV_MAG |
GALEX_NUV AB magnitude |
DOUBLE |
1 |
phot.mag;em.UV.200-300nm |
mag |
235 |
GALEX_NUV_MAGERR |
GALEX_NUV AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.UV.200-300nm |
mag |
236 |
GALEX_FUV_FLUX |
GALEX_FUV flux density |
DOUBLE |
1 |
phot.flux.density;em.UV.100-200nm |
uJy |
237 |
GALEX_FUV_FLUXERR |
GALEX_FUV flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.UV.100-200nm |
uJy |
238 |
GALEX_FUV_MAG |
GALEX_FUV AB magnitude |
DOUBLE |
1 |
phot.mag;em.UV.100-200nm |
mag |
239 |
GALEX_FUV_MAGERR |
GALEX_FUV AB magnitude error |
DOUBLE |
1 |
stat.error;phot.mag;em.UV.100-200nm |
mag |
240 |
ID_COSMOS2015 |
ID in COSMOS2015 cat. (Laigle+2016), crossmatched with 0.6" radius |
INT64 |
1 |
meta.id |
|
241 |
SPLASH_CH1_FLUX |
SPLASH_CH1 flux density |
FLOAT |
1 |
phot.flux.density;em.IR.3-4um |
uJy |
242 |
SPLASH_CH1_FLUXERR |
SPLASH_CH1 flux density error |
FLOAT |
1 |
stat.error;phot.flux.density;em.IR.3-4um |
uJy |
243 |
SPLASH_CH1_MAG |
SPLASH_CH1 AB magnitude |
FLOAT |
1 |
phot.mag;em.IR.3-4um |
mag |
244 |
SPLASH_CH1_MAGERR |
SPLASH_CH1 AB magnitude error |
FLOAT |
1 |
stat.error;phot.mag;em.IR.3-4um |
mag |
245 |
SPLASH_CH2_FLUX |
SPLASH_CH2 flux density |
FLOAT |
1 |
phot.flux.density;em.IR.4-8um |
uJy |
246 |
SPLASH_CH2_FLUXERR |
SPLASH_CH2 flux density error |
FLOAT |
1 |
stat.error;phot.flux.density;em.IR.4-8um |
uJy |
247 |
SPLASH_CH2_MAG |
SPLASH_CH2 AB magnitude |
FLOAT |
1 |
phot.mag;em.IR.4-8um |
mag |
248 |
SPLASH_CH2_MAGERR |
SPLASH_CH2 AB magnitude error |
FLOAT |
1 |
stat.error;phot.mag;em.IR.4-8um |
mag |
249 |
SPLASH_CH3_FLUX |
SPLASH_CH3 flux density |
FLOAT |
1 |
phot.flux.density;em.IR.4-8um |
uJy |
250 |
SPLASH_CH3_FLUXERR |
SPLASH_CH3 flux density error |
FLOAT |
1 |
stat.error;phot.flux.density;em.IR.4-8um |
uJy |
251 |
SPLASH_CH3_MAG |
SPLASH_CH3 AB magnitude |
FLOAT |
1 |
phot.mag;em.IR.4-8um |
mag |
252 |
SPLASH_CH3_MAGERR |
SPLASH_CH3 AB magnitude error |
FLOAT |
1 |
stat.error;phot.mag;em.IR.4-8um |
mag |
253 |
SPLASH_CH4_FLUX |
SPLASH_CH4 flux density |
FLOAT |
1 |
phot.flux.density;em.IR.4-8um |
uJy |
254 |
SPLASH_CH4_FLUXERR |
SPLASH_CH4 flux density error |
FLOAT |
1 |
stat.error;phot.flux.density;em.IR.4-8um |
uJy |
255 |
SPLASH_CH4_MAG |
SPLASH_CH4 AB magnitude |
FLOAT |
1 |
phot.mag;em.IR.4-8um |
mag |
256 |
SPLASH_CH4_MAGERR |
SPLASH_CH4 AB magnitude error |
FLOAT |
1 |
stat.error;phot.mag;em.IR.4-8um |
mag |
257 |
ID_ACS |
ID in HST ACS F814W cat. (Leauthaud+2007), crossm. with 0.6" radius |
INT64 |
1 |
meta.id |
|
258 |
ACS_F814W_MAG |
ACS_F814W AB magnitude |
FLOAT |
1 |
phot.mag;em.opt.I |
mag |
259 |
ACS_F814W_MAGERR |
ACS_F814W AB magnitude error |
FLOAT |
1 |
stat.error;phot.mag;em.opt.I |
mag |
260 |
ACS_F814W_FLUX |
ACS_F814W flux density |
DOUBLE |
1 |
phot.flux.density;em.opt.I |
uJy |
261 |
ACS_F814W_FLUXERR |
ACS_F814W flux density error |
DOUBLE |
1 |
stat.error;phot.flux.density;em.opt.I |
uJy |
262 |
ACS_A_WORLD |
ACS F814W semi-major axis length |
FLOAT |
1 |
phys.angSize.smajAxis;em.opt.I |
deg |
263 |
ACS_B_WORLD |
ACS F814W semi-minor axis length |
FLOAT |
1 |
phys.angSize.sminAxis;em.opt.I |
deg |
264 |
ACS_THETA_WORLD |
ACS F814W angle; to get PA measured from N through E, add/subtr. 90 |
FLOAT |
1 |
pos.posAng;em.opt.I |
deg |
265 |
ACS_FWHM_WORLD |
ACS F814W FWHM assuming a gaussian core |
FLOAT |
1 |
phys.angSize;stat.fwhm;em.opt.I |
deg |
266 |
ACS_MU_MAX |
ACS F814W peak surface brightness above background |
FLOAT |
1 |
phot.mag.sb;em.opt.I;stat.max |
|
267 |
ACS_MU_CLASS |
ACS F814W star/galaxy classifier: 1=galaxy, 2=star, 3=fake detection |
INT16 |
1 |
src.class.starGalaxy;em.opt.I |
|
268 |
ID_CHANDRA |
ID in Chandra cat. (Civano+2016, Marchesi+2016), crossm. w. 0.6" rad |
STRING |
9 |
meta.id |
|
269 |
ID_CLASSIC |
ID in the Classic catalogue, crossmatched with 0.6" radius |
INT64 |
1 |
meta.id |
|
270 |
lp_zBEST |
LePhare photo-z (=lp_zPDF if galaxy, NaN if X-ray source or masked) |
DOUBLE |
1 |
src.redshift.phot;meta.main |
|
271 |
lp_type |
LePhare type (0: galaxy, 1: star, 2: Xray sour., -9: failure in fit) |
INT64 |
1 |
src.class.starGalaxy |
|
272 |
lp_zPDF |
LePhare photo-z using the galaxy templ., median of likelihood distr. |
DOUBLE |
1 |
src.redshift.phot |
|
273 |
lp_zPDF_l68 |
LePhare photo-z lower limit, 68% confidence level (galaxy templates) |
DOUBLE |
1 |
src.redshift.phot;stat.min |
|
274 |
lp_zPDF_u68 |
LePhare photo-z upper limit, 68% confidence level (galaxy templates) |
DOUBLE |
1 |
src.redshift.phot;stat.max |
|
275 |
lp_zMinChi2 |
LePhare photo-z using the galaxy templates, minimum chi2 |
DOUBLE |
1 |
src.redshift.phot |
|
276 |
lp_chi2_best |
LePhare reduced chi2 for lp_zMinChi2 (NaN if less than 3 filters) |
DOUBLE |
1 |
stat.fit.chi2 |
|
277 |
lp_zp_2 |
LePhare 2nd photo-z solution if a 2nd peak detected w. P>5% in PDF |
DOUBLE |
1 |
src.redshift.phot |
|
278 |
lp_chi2_2 |
LePhare reduced chi2 for the second photo-z solution |
DOUBLE |
1 |
stat.fit.chi2 |
|
279 |
lp_NbFilt |
LePhare number of filters used in the fit |
INT64 |
1 |
meta.number;instr.filter |
|
280 |
lp_zq |
LePhare photo-z for the AGN library |
DOUBLE |
1 |
src.redshift.phot |
|
281 |
lp_chiq |
LePhare reduced chi2 for photo-z for the AGN library |
DOUBLE |
1 |
stat.fit.chi2 |
|
282 |
lp_modq |
LePhare best fit template number in the AGN library |
DOUBLE |
1 |
meta.code |
|
283 |
lp_mods |
LePhare best fit template number in the star library |
DOUBLE |
1 |
meta.code |
|
284 |
lp_chis |
LePhare reduced chi2 for the best fit with the star library |
DOUBLE |
1 |
stat.fit.chi2 |
|
285 |
lp_mask |
LePhare mask flag (0: in UVISTA and in clean part of HSC and SUPCAM) |
DOUBLE |
1 |
meta.code |
|
286 |
lp_model |
LePhare BC03 best fit template number |
INT64 |
1 |
meta.code |
|
287 |
lp_age |
LePhare BC03 age of best fit template at zPDF |
DOUBLE |
1 |
time.age |
yr |
288 |
lp_dust |
LePhare BC03 colour excess E(B-V) of best fit template at zPDF |
DOUBLE |
1 |
phot.color.excess |
|
289 |
lp_Attenuation |
LePhare BC03 best-fit dust law number at zPDF |
INT64 |
1 |
meta.code |
|
290 |
lp_MFUV |
LePhare BC03 absolute rest-frame AB mag in GALEX FUV band at zPDF |
DOUBLE |
1 |
phys.magAbs;em.UV.100-200nm |
mag |
291 |
lp_MNUV |
LePhare BC03 absolute rest-frame AB mag in GALEX NUV band at zPDF |
DOUBLE |
1 |
phys.magAbs;em.UV.200-300nm |
mag |
292 |
lp_MU |
LePhare BC03 absolute rest-frame AB mag in CFHT u* band at zPDF |
DOUBLE |
1 |
phys.magAbs;em.opt.U |
mag |
293 |
lp_MG |
LePhare BC03 absolute rest-frame AB mag in Subaru/HSC g band at zPDF |
DOUBLE |
1 |
phys.magAbs;em.opt.B |
mag |
294 |
lp_MR |
LePhare BC03 absolute rest-frame AB mag in Subaru/HSC r band at zPDF |
DOUBLE |
1 |
phys.magAbs;em.opt.R |
mag |
295 |
lp_MI |
LePhare BC03 absolute rest-frame AB mag in Subaru/HSC i band at zPDF |
DOUBLE |
1 |
phys.magAbs;em.opt.I |
mag |
296 |
lp_MZ |
LePhare BC03 absolute rest-frame AB mag in Subaru/HSC z band at zPDF |
DOUBLE |
1 |
phys.magAbs;em.opt.I |
mag |
297 |
lp_MY |
LePhare BC03 absolute rest-frame AB mag in VISTA Y band at zPDF |
DOUBLE |
1 |
phys.magAbs;em.IR.J |
mag |
298 |
lp_MJ |
LePhare BC03 absolute rest-frame AB mag in VISTA J band at zPDF |
DOUBLE |
1 |
phys.magAbs;em.IR.J |
mag |
299 |
lp_MH |
LePhare BC03 absolute rest-frame AB mag in VISTA H band at zPDF |
DOUBLE |
1 |
phys.magAbs;em.IR.H |
mag |
300 |
lp_MK |
LePhare BC03 absolute rest-frame AB mag in VISTA Ks band at zPDF |
DOUBLE |
1 |
phys.magAbs;em.IR.K |
mag |
301 |
lp_mass_med |
LePhare BC03 log stellar mass at zPDF |
DOUBLE |
1 |
phys.mass |
log(solMass) |
302 |
lp_mass_med_min68 |
LePhare BC03 log stellar mass at zPDF, lower limit, 68% conf. level |
DOUBLE |
1 |
phys.mass;stat.min |
log(solMass) |
303 |
lp_mass_med_max68 |
LePhare BC03 log stellar mass at zPDF, upper limit, 68% conf. level |
DOUBLE |
1 |
phys.mass;stat.max |
log(solMass) |
304 |
lp_mass_best |
LePhare BC03 log stellar mass at zMinChi2 |
DOUBLE |
1 |
phys.mass |
log(solMass) |
305 |
lp_SFR_med |
LePhare BC03 log SFR at zPDF |
DOUBLE |
1 |
phys.SFR |
log(solMass/yr) |
306 |
lp_SFR_med_min68 |
LePhare BC03 log SFR at zPDF, lower limit, 68% confidence level |
DOUBLE |
1 |
phys.SFR;stat.min |
log(solMass/yr) |
307 |
lp_SFR_med_max68 |
LePhare BC03 log SFR at zPDF, upper limit, 68% confidence level |
DOUBLE |
1 |
phys.SFR;stat.max |
log(solMass/yr) |
308 |
lp_SFR_best |
LePhare BC03 log SFR at zMinChi2 |
DOUBLE |
1 |
phys.SFR |
log(solMass/yr) |
309 |
lp_sSFR_med |
LePhare BC03 log sSFR at zPDF |
DOUBLE |
1 |
phys.SFR |
log(yr**(-1)) |
310 |
lp_sSFR_med_min68 |
LePhare BC03 log sSFR at zPDF, lower limit, 68% confidence level |
DOUBLE |
1 |
phys.SFR;stat.min |
log(yr**(-1)) |
311 |
lp_sSFR_med_max68 |
LePhare BC03 log sSFR at zPDF, upper limit, 68% confidence level |
DOUBLE |
1 |
phys.SFR;stat.max |
log(yr**(-1)) |
312 |
lp_sSFR_best |
LePhare BC03 log sSFR at zMinChi2 |
DOUBLE |
1 |
phys.SFR |
log(yr**(-1)) |
313 |
ez_z_phot |
EAZY maximum a-posteriori photo-z |
FLOAT |
1 |
src.redshift.phot;meta.main |
|
314 |
ez_z_phot_chi2 |
EAZY chi2 at ez_z_phot, with z-prior |
FLOAT |
1 |
stat.fit.chi2 |
|
315 |
ez_z_phot_risk |
EAZY risk parameter (Tanaka+2018) at ez_z_phot, R(ez_z_phot) |
FLOAT |
1 |
stat.param |
|
316 |
ez_z_min_risk |
EAZY photo-z where risk parameter R(z) is minimised |
FLOAT |
1 |
src.redshift.phot |
|
317 |
ez_min_risk |
EAZY risk parameter at ez_z_min_risk, R(ez_z_min_risk) |
FLOAT |
1 |
stat.param;stat.min |
|
318 |
ez_z_raw_chi2 |
EAZY photo-z where chi2 is minimised, without priors |
FLOAT |
1 |
src.redshift.phot |
|
319 |
ez_raw_chi2 |
EAZY chi2 at ez_z_raw_chi2 |
FLOAT |
1 |
stat.fit.chi2 |
|
320 |
ez_z025 |
EAZY 2.5% percentile of photo-z |
FLOAT |
1 |
src.redshift.phot;stat.min |
|
321 |
ez_z160 |
EAZY 16.0% percentile of photo-z |
FLOAT |
1 |
src.redshift.phot;stat.min |
|
322 |
ez_z500 |
EAZY 50.0% percentile of photo-z |
FLOAT |
1 |
src.redshift.phot;stat.median |
|
323 |
ez_z840 |
EAZY 84.0% percentile of photo-z |
FLOAT |
1 |
src.redshift.phot;stat.max |
|
324 |
ez_z975 |
EAZY 97.5% percentile of photo-z |
FLOAT |
1 |
src.redshift.phot;stat.max |
|
325 |
ez_nusefilt |
EAZY no. of filters used for photo-z (only filters w/o missing data) |
INT64 |
1 |
meta.number;instr.filter |
|
326 |
ez_lc_min |
EAZY minimum effective wavelength of valid filters |
DOUBLE |
1 |
em.wl.effective;stat.min |
Angstrom |
327 |
ez_lc_max |
EAZY minimum effective wavelength of valid filters |
DOUBLE |
1 |
em.wl.effective;stat.max |
Angstrom |
328 |
ez_star_min_chi2 |
EAZY chi2 best stellar template fit (BT-SETTL models) as, 8% sys unc |
FLOAT |
1 |
stat.fit.chi2 |
|
329 |
ez_star_teff |
EAZY effective temperature of the stellar template |
INT64 |
1 |
phys.temperature.effective |
K |
330 |
ez_restU |
EAZY rest-frame U-band flux density |
FLOAT |
1 |
phot.flux.density;em.opt.U |
uJy |
331 |
ez_restU_err |
EAZY rest-frame U-band flux density uncertainty |
FLOAT |
1 |
stat.error;phot.flux.density;em.opt.U |
uJy |
332 |
ez_restB |
EAZY rest-frame B-band flux density |
FLOAT |
1 |
phot.flux.density;em.opt.B |
uJy |
333 |
ez_restB_err |
EAZY rest-frame B-band flux density uncertainty |
FLOAT |
1 |
stat.error;phot.flux.density;em.opt.B |
uJy |
334 |
ez_restV |
EAZY rest-frame V-band flux density |
FLOAT |
1 |
phot.flux.density;em.opt.V |
uJy |
335 |
ez_restV_err |
EAZY rest-frame V-band flux density uncertainty |
FLOAT |
1 |
stat.error;phot.flux.density;em.opt.V |
uJy |
336 |
ez_restJ |
EAZY rest-frame J-band flux density |
FLOAT |
1 |
phot.flux.density;em.IR.J |
uJy |
337 |
ez_restJ_err |
EAZY rest-frame J-band flux density uncertainty |
FLOAT |
1 |
stat.error;phot.flux.density;em.IR.J |
uJy |
338 |
ez_dL |
EAZY luminosity distance at ez_z_phot |
DOUBLE |
1 |
pos.distance |
Mpc |
339 |
ez_mass |
EAZY log stellar mass |
DOUBLE |
1 |
phys.mass |
log(solMass) |
340 |
ez_sfr |
EAZY log SFR |
DOUBLE |
1 |
phys.SFR |
log(solMass/yr) |
341 |
ez_ssfr |
EAZY log sSFR |
DOUBLE |
1 |
phys.SFR |
log(yr**(-1)) |
342 |
ez_Lv |
EAZY log V-band luminosity |
DOUBLE |
1 |
phys.luminosity;em.opt.V |
log(solLum) |
343 |
ez_LIR |
EAZY total 8-1000 um luminosity |
DOUBLE |
1 |
phys.luminosity;em.IR |
solLum |
344 |
ez_energy_abs |
EAZY implied absorbed energy associated with Av |
DOUBLE |
1 |
phys.energy |
solLum |
345 |
ez_Lu |
EAZY luminosity in rest-frame U band |
DOUBLE |
1 |
phys.luminosity;em.opt.U |
solLum |
346 |
ez_Lj |
EAZY luminosity in rest-frame J band |
DOUBLE |
1 |
phys.luminosity;em.IR.J |
solLum |
347 |
ez_L1400 |
EAZY luminosity in tophat filter at 1400 A (200 A wide) rest-frame |
DOUBLE |
1 |
phys.luminosity;em.UV.100-200nm |
solLum |
348 |
ez_L2800 |
EAZY luminosity in tophat filter at 2800 A (200 A wide) rest-frame |
DOUBLE |
1 |
phys.luminosity;em.UV.200-300nm |
solLum |
349 |
ez_LHa |
EAZY Halpha line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;em.line.Halpha |
solLum |
350 |
ez_LOIII |
EAZY [OIII] 4959+5007 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;em.line.OIII |
solLum |
351 |
ez_LHb |
EAZY Hbeta line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;em.line.Hbeta |
solLum |
352 |
ez_LOII |
EAZY [OII] 3726+3729 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;em.line |
solLum |
353 |
ez_MLv |
EAZY mass-to-light ratio in V band |
DOUBLE |
1 |
phys.composition.massLightRatio;em.opt.V |
solMass/solLum |
354 |
ez_Av |
EAZY extinction in V band |
DOUBLE |
1 |
phys.absorption;em.opt.V |
mag |
355 |
ez_lwAgeV |
EAZY light-weighted age in the V band |
DOUBLE |
1 |
time.age;em.opt.V |
Gyr |
356 |
ez_mass_p025 |
EAZY 2.5% percentile of log stellar mass |
DOUBLE |
1 |
phys.mass;stat.min |
log(solMass) |
357 |
ez_mass_p160 |
EAZY 16.0% percentile of log stellar mass |
DOUBLE |
1 |
phys.mass;stat.min |
log(solMass) |
358 |
ez_mass_p500 |
EAZY 50.0% percentile of log stellar mass |
DOUBLE |
1 |
phys.mass;stat.median |
log(solMass) |
359 |
ez_mass_p840 |
EAZY 84.0% percentile of log stellar mass |
DOUBLE |
1 |
phys.mass;stat.max |
log(solMass) |
360 |
ez_mass_p975 |
EAZY 97.5% percentile of log stellar mass |
DOUBLE |
1 |
phys.mass;stat.max |
log(solMass) |
361 |
ez_sfr_p025 |
EAZY 2.5% percentile of log SFR |
DOUBLE |
1 |
phys.SFR;stat.min |
log(solMass/yr) |
362 |
ez_sfr_p160 |
EAZY 16.0% percentile of log SFR |
DOUBLE |
1 |
phys.SFR;stat.min |
log(solMass/yr) |
363 |
ez_sfr_p500 |
EAZY 50.0% percentile of log SFR |
DOUBLE |
1 |
phys.SFR;stat.median |
log(solMass/yr) |
364 |
ez_sfr_p840 |
EAZY 84.0% percentile of log SFR |
DOUBLE |
1 |
phys.SFR;stat.max |
log(solMass/yr) |
365 |
ez_sfr_p975 |
EAZY 97.5% percentile of log SFR |
DOUBLE |
1 |
phys.SFR;stat.max |
log(solMass/yr) |
366 |
ez_Lv_p025 |
EAZY 2.5% percentile of log V-band luminosity |
DOUBLE |
1 |
phys.luminosity;stat.min;em.opt.V |
log(solLum) |
367 |
ez_Lv_p160 |
EAZY 16.0% percentile of log V-band luminosity |
DOUBLE |
1 |
phys.luminosity;stat.min;em.opt.V |
log(solLum) |
368 |
ez_Lv_p500 |
EAZY 50.0% percentile of log V-band luminosity |
DOUBLE |
1 |
phys.luminosity;stat.median;em.opt.V |
log(solLum) |
369 |
ez_Lv_p840 |
EAZY 84.0% percentile of log V-band luminosity |
DOUBLE |
1 |
phys.luminosity;stat.max;em.opt.V |
log(solLum) |
370 |
ez_Lv_p975 |
EAZY 97.5% percentile of log V-band luminosity |
DOUBLE |
1 |
phys.luminosity;stat.max;em.opt.V |
log(solLum) |
371 |
ez_LIR_p025 |
EAZY 2.5% percentile of total 8-1000 um luminosity |
DOUBLE |
1 |
phys.luminosity;stat.min;em.IR |
solLum |
372 |
ez_LIR_p160 |
EAZY 16.0% percentile of total 8-1000 um luminosity |
DOUBLE |
1 |
phys.luminosity;stat.min;em.IR |
solLum |
373 |
ez_LIR_p500 |
EAZY 50.0% percentile of total 8-1000 um luminosity |
DOUBLE |
1 |
phys.luminosity;stat.median;em.IR |
solLum |
374 |
ez_LIR_p840 |
EAZY 84.0% percentile of total 8-1000 um luminosity |
DOUBLE |
1 |
phys.luminosity;stat.max;em.IR |
solLum |
375 |
ez_LIR_p975 |
EAZY 97.5% percentile of total 8-1000 um luminosity |
DOUBLE |
1 |
phys.luminosity;stat.max;em.IR |
solLum |
376 |
ez_energy_abs_p025 |
EAZY 2.5% percentile of implied absorbed energy associated with Av |
DOUBLE |
1 |
phys.energy;stat.min |
solLum |
377 |
ez_energy_abs_p160 |
EAZY 16.0% percentile of implied absorbed energy associated with Av |
DOUBLE |
1 |
phys.energy;stat.min |
solLum |
378 |
ez_energy_abs_p500 |
EAZY 50.0% percentile of implied absorbed energy associated with Av |
DOUBLE |
1 |
phys.energy;stat.median |
solLum |
379 |
ez_energy_abs_p840 |
EAZY 84.0% percentile of implied absorbed energy associated with Av |
DOUBLE |
1 |
phys.energy;stat.max |
solLum |
380 |
ez_energy_abs_p975 |
EAZY 97.5% percentile of implied absorbed energy associated with Av |
DOUBLE |
1 |
phys.energy;stat.max |
solLum |
381 |
ez_Lu_p025 |
EAZY 2.5% percentile of luminosity in rest-frame U band |
DOUBLE |
1 |
phys.luminosity;stat.min;em.opt.U |
solLum |
382 |
ez_Lu_p160 |
EAZY 16.0% percentile of luminosity in rest-frame U band |
DOUBLE |
1 |
phys.luminosity;stat.min;em.opt.U |
solLum |
383 |
ez_Lu_p500 |
EAZY 50.0% percentile of luminosity in rest-frame U band |
DOUBLE |
1 |
phys.luminosity;stat.median;em.opt.U |
solLum |
384 |
ez_Lu_p840 |
EAZY 84.0% percentile of luminosity in rest-frame U band |
DOUBLE |
1 |
phys.luminosity;stat.max;em.opt.U |
solLum |
385 |
ez_Lu_p975 |
EAZY 97.5% percentile of luminosity in rest-frame U band |
DOUBLE |
1 |
phys.luminosity;stat.max;em.opt.U |
solLum |
386 |
ez_Lj_p025 |
EAZY 2.5% percentile of luminosity in rest-frame J band |
DOUBLE |
1 |
phys.luminosity;stat.min;em.IR.J |
solLum |
387 |
ez_Lj_p160 |
EAZY 16.0% percentile of luminosity in rest-frame J band |
DOUBLE |
1 |
phys.luminosity;stat.min;em.IR.J |
solLum |
388 |
ez_Lj_p500 |
EAZY 50.0% percentile of luminosity in rest-frame J band |
DOUBLE |
1 |
phys.luminosity;stat.median;em.IR.J |
solLum |
389 |
ez_Lj_p840 |
EAZY 84.0% percentile of luminosity in rest-frame J band |
DOUBLE |
1 |
phys.luminosity;stat.max;em.IR.J |
solLum |
390 |
ez_Lj_p975 |
EAZY 97.5% percentile of luminosity in rest-frame J band |
DOUBLE |
1 |
phys.luminosity;stat.max;em.IR.J |
solLum |
391 |
ez_L1400_p025 |
EAZY 2.5% percentile of lum tophat filter at 1400 A (200 A wide) rf |
DOUBLE |
1 |
phys.luminosity;stat.min;em.UV.100-200nm |
solLum |
392 |
ez_L1400_p160 |
EAZY 16.0% percentile of lum tophat filter at 1400 A (200 A wide) rf |
DOUBLE |
1 |
phys.luminosity;stat.min;em.UV.100-200nm |
solLum |
393 |
ez_L1400_p500 |
EAZY 50.0% percentile of lum tophat filter at 1400 A (200 A wide) rf |
DOUBLE |
1 |
phys.luminosity;stat.median;em.UV.100-200nm |
solLum |
394 |
ez_L1400_p840 |
EAZY 84.0% percentile of lum tophat filter at 1400 A (200 A wide) rf |
DOUBLE |
1 |
phys.luminosity;stat.max;em.UV.100-200nm |
solLum |
395 |
ez_L1400_p975 |
EAZY 97.5% percentile of lum tophat filter at 1400 A (200 A wide) rf |
DOUBLE |
1 |
phys.luminosity;stat.max;em.UV.100-200nm |
solLum |
396 |
ez_L2800_p025 |
EAZY 2.5% percentile of lum tophat filter at 2800 A (200 A wide) rf |
DOUBLE |
1 |
phys.luminosity;stat.min;em.UV.200-300nm |
solLum |
397 |
ez_L2800_p160 |
EAZY 16.0% percentile of lum tophat filter at 2800 A (200 A wide) rf |
DOUBLE |
1 |
phys.luminosity;stat.min;em.UV.200-300nm |
solLum |
398 |
ez_L2800_p500 |
EAZY 50.0% percentile of lum tophat filter at 2800 A (200 A wide) rf |
DOUBLE |
1 |
phys.luminosity;stat.median;em.UV.200-300nm |
solLum |
399 |
ez_L2800_p840 |
EAZY 84.0% percentile of lum tophat filter at 2800 A (200 A wide) rf |
DOUBLE |
1 |
phys.luminosity;stat.max;em.UV.200-300nm |
solLum |
400 |
ez_L2800_p975 |
EAZY 97.5% percentile of lum tophat filter at 2800 A (200 A wide) rf |
DOUBLE |
1 |
phys.luminosity;stat.max;em.UV.200-300nm |
solLum |
401 |
ez_LHa_p025 |
EAZY 2.5% percentile of Halpha line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.min;em.line.Halpha |
solLum |
402 |
ez_LHa_p160 |
EAZY 16.0% percentile of Halpha line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.min;em.line.Halpha |
solLum |
403 |
ez_LHa_p500 |
EAZY 50.0% percentile of Halpha line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.median;em.line.Halpha |
solLum |
404 |
ez_LHa_p840 |
EAZY 84.0% percentile of Halpha line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.max;em.line.Halpha |
solLum |
405 |
ez_LHa_p975 |
EAZY 97.5% percentile of Halpha line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.max;em.line.Halpha |
solLum |
406 |
ez_LOIII_p025 |
EAZY 2.5% percentile of [OIII] 4959+5007 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.min;em.line.OIII |
solLum |
407 |
ez_LOIII_p160 |
EAZY 16.0% percentile of [OIII] 4959+5007 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.min;em.line.OIII |
solLum |
408 |
ez_LOIII_p500 |
EAZY 50.0% percentile of [OIII] 4959+5007 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.median;em.line.OIII |
solLum |
409 |
ez_LOIII_p840 |
EAZY 84.0% percentile of [OIII] 4959+5007 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.max;em.line.OIII |
solLum |
410 |
ez_LOIII_p975 |
EAZY 97.5% percentile of [OIII] 4959+5007 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.max;em.line.OIII |
solLum |
411 |
ez_LHb_p025 |
EAZY 2.5% percentile of Hbeta line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.min;em.line.Hbeta |
solLum |
412 |
ez_LHb_p160 |
EAZY 16.0% percentile of Hbeta line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.min;em.line.Hbeta |
solLum |
413 |
ez_LHb_p500 |
EAZY 50.0% percentile of Hbeta line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.median;em.line.Hbeta |
solLum |
414 |
ez_LHb_p840 |
EAZY 84.0% percentile of Hbeta line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.max;em.line.Hbeta |
solLum |
415 |
ez_LHb_p975 |
EAZY 97.5% percentile of Hbeta line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.max;em.line.Hbeta |
solLum |
416 |
ez_LOII_p025 |
EAZY 2.5% percentile of [OII] 3726+3729 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.min;em.line |
solLum |
417 |
ez_LOII_p160 |
EAZY 16.0% percentile of [OII] 3726+3729 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.min;em.line |
solLum |
418 |
ez_LOII_p500 |
EAZY 50.0% percentile of [OII] 3726+3729 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.median;em.line |
solLum |
419 |
ez_LOII_p840 |
EAZY 84.0% percentile of [OII] 3726+3729 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.max;em.line |
solLum |
420 |
ez_LOII_p975 |
EAZY 97.5% percentile of [OII] 3726+3729 line luminosity (reddened) |
DOUBLE |
1 |
phys.luminosity;stat.max;em.line |
solLum |
421 |
ez_ssfr_p025 |
EAZY 2.5% percentile of log sSFR |
DOUBLE |
1 |
phys.SFR;stat.min |
log(yr**(-1)) |
422 |
ez_ssfr_p160 |
EAZY 16.0% percentile of log sSFR |
DOUBLE |
1 |
phys.SFR;stat.min |
log(yr**(-1)) |
423 |
ez_ssfr_p500 |
EAZY 50.0% percentile of log sSFR |
DOUBLE |
1 |
phys.SFR;stat.median |
log(yr**(-1)) |
424 |
ez_ssfr_p840 |
EAZY 84.0% percentile of log sSFR |
DOUBLE |
1 |
phys.SFR;stat.max |
log(yr**(-1)) |
425 |
ez_ssfr_p975 |
EAZY 97.5% percentile of log sSFR |
DOUBLE |
1 |
phys.SFR;stat.max |
log(yr**(-1)) |
426 |
ez_Av_p025 |
EAZY 2.5% percentile of extinction in V band |
DOUBLE |
1 |
phys.absorption;stat.min;em.opt.V |
mag |
427 |
ez_Av_p160 |
EAZY 16.0% percentile of extinction in V band |
DOUBLE |
1 |
phys.absorption;stat.min;em.opt.V |
mag |
428 |
ez_Av_p500 |
EAZY 50.0% percentile of extinction in V band |
DOUBLE |
1 |
phys.absorption;stat.median;em.opt.V |
mag |
429 |
ez_Av_p840 |
EAZY 84.0% percentile of extinction in V band |
DOUBLE |
1 |
phys.absorption;stat.max;em.opt.V |
mag |
430 |
ez_Av_p975 |
EAZY 97.5% percentile of extinction in V band |
DOUBLE |
1 |
phys.absorption;stat.max;em.opt.V |
mag |