Name |
Intype |
Units |
Description |
unwise_objid |
char |
|
unique object ID |
ra |
double |
deg |
right ascension: W1 position, if available; otherwise W2 position |
dec |
double |
deg |
declination: W1 position, if available; otherwise W2 position |
ra_1 |
double |
deg |
right ascension, band 1 |
dec_1 |
double |
deg |
declination, band 1 |
ra_2 |
double |
deg |
right ascension, band 2 |
dec_2 |
double |
deg |
declination, band 2 |
x_1 |
double |
pix |
x coordinate, band 1 |
dx_1 |
double |
pix |
uncertainty in x_1 |
x_2 |
double |
pix |
x coordinate, band 2 |
dx_2 |
double |
pix |
uncertainty in x_2 |
y_1 |
double |
pix |
y coordinate, band 1 |
dy_1 |
double |
pix |
uncertainty in y_1 |
y_2 |
double |
pix |
y coordinate, band 2 |
dy_2 |
double |
pix |
uncertainty in y_2 |
flux_1 |
double |
'nMgy' (nanomaggies) |
flux, band 1 |
dflux_1 |
double |
'nMgy' (nanomaggies) |
statistical uncertainty in flux_1 |
flux_2 |
double |
'nMgy' (nanomaggies) |
flux, band 2 |
dflux_2 |
double |
'nMgy' (nanomaggies) |
statistical uncertainty in flux_2 |
fluxlbs_1 |
double |
'nMgy' (nanomaggies) |
local-background-subtracted flux, band 1 |
dfluxlbs_1 |
double |
'nMgy' (nanomaggies) |
uncertainty in fluxlbs_1 |
fluxlbs_2 |
double |
'nMgy' (nanomaggies) |
local-background-subtracted flux, band 2 |
dfluxlbs_2 |
double |
'nMgy' (nanomaggies) |
uncertainty in fluxlbs_2 |
qf_1 |
double |
|
quality factor, band 1: PSF-weighted fraction of pixels contributing to this detection |
qf_2 |
double |
|
quality factor, band 2: PSF-weighted fraction of pixels contributing to this detection |
rchi2_1 |
double |
|
average chi^2 per pixel, weighted by PSF, band 1 |
rchi2_2 |
double |
|
average chi^2 per pixel, weighted by PSF, band 2 |
fracflux_1 |
double |
|
fraction of flux in this object's PSF that comes from this object, band 1 |
fracflux_2 |
double |
|
fraction of flux in this object's PSF that comes from this object, band 2 |
spread_model_1 |
double |
|
SExtractor spread_model parameter, band 1 |
dspread_model_1 |
double |
|
uncertainty in spread_model_1 |
spread_model_2 |
double |
|
SExtractor spread_model parameter, band 2 |
dspread_model_2 |
double |
|
uncertainty in spread_model_2 |
fwhm_1 |
double |
pix |
full-width at half-maximum of PSF, band 1 |
fwhm_2 |
double |
pix |
full-width at half-maximum of PSF, band 2 |
sky_1 |
double |
'nMgy' (nanomaggies) |
sky, band 1 |
sky_2 |
double |
'nMgy' (nanomaggies) |
sky, band 2 |
nm_1 |
int |
|
number of single-exposure images of this part of sky in coadd, band 1 |
nm_2 |
int |
|
number of single-exposure images of this part of sky in coadd, band 2 |
primary_1 |
int |
|
primary region of coadd flag, band 1 |
primary_2 |
int |
|
primary region of coadd flag, band 2 |
primary |
int |
|
primary region of coadd flag |
flags_unwise_1 |
int |
|
unWISE Coadd Flags flags at central pixel, band 1
bit | description |
0 | In core or wings |
1 | In diffraction spike |
2 | In ghost |
3 | In first latent |
4 | In second latent |
5 | In circular halo |
6 | Saturated |
7 | In geometric diffraction spike |
|
flags_unwise_2 |
int |
|
unWISE Coadd Flags flags at central pixel, band 2
bit | description |
0 | In core or wings |
1 | In diffraction spike |
2 | In ghost |
3 | In first latent |
4 | In second latent |
5 | In circular halo |
6 | Saturated |
7 | In geometric diffraction spike |
|
flags_info_1 |
int |
|
additional informational flags at central pixel, band 1
bit | description |
0 | In PSF of bright star falling off coadd |
1 | In HyperLeda large galaxy |
2 | In "big object" (e.g., a Magellanic cloud) |
3 | Pixel may contain the centroid of a very bright star |
4 | crowdsource considers this pixel potentially affected by saturation |
5 | Pixel may contain nebulosity |
6 | Sources in this pixel will not be aggressively deblended |
7 | Candidate sources in this pixel must be "sharp" to be optimized |
|
flags_info_2 |
int |
|
additional informational flags at central pixel, band 2
bit | description |
0 | In PSF of bright star falling off coadd |
1 | In HyperLeda large galaxy |
2 | In "big object" (e.g., a Magellanic cloud) |
3 | Pixel may contain the centroid of a very bright star |
4 | crowdsource considers this pixel potentially affected by saturation |
5 | Pixel may contain nebulosity |
6 | Sources in this pixel will not be aggressively deblended |
7 | Candidate sources in this pixel must be "sharp" to be optimized |
|
coadd_id |
char |
|
coadd ID |
unwise_detid_1 |
char |
|
unique detection ID, band 1 |
unwise_detid_2 |
char |
|
unique detection ID, band 2 |