SSO quantities for ops-rehearsals 3 and 4
Data are partitioned by (nside=32, ring ordering) healpixel. For each pixel there is a so-called “main file” and a flux file. The latter contains for each object only fluxes for lsst bands, the object id and the time (mjd) of the observation. The latter two fields may be used to join with the main file.
SSO main file
Name |
Datatype |
Units |
Description |
---|---|---|---|
id |
string |
N/A |
Unique object identifier |
mjd |
double |
days |
Time of observation |
ra |
double |
degrees |
Object right ascension |
dec |
double |
degrees |
Object declination |
trailed_source_mag |
double |
N/A |
Mag. normalization for SED |
ra_rate |
double |
deg/day |
RA rate of change * cos(dec) |
dec_rate |
double |
deg/day |
Declination rate of change |
SSO flux file
Name |
Datatype |
Units |
Description |
---|---|---|---|
id |
string |
N/A |
Unique object identifier |
mjd |
double |
days |
Time of observation (Julian date) |
lsst_flux_u |
float |
photons/sec/cm^2 |
Flux integrated over lsst u-band |
lsst_flux_g |
float |
photons/sec/cm^2 |
Flux integrated over lsst g-band |
lsst_flux_r |
float |
photons/sec/cm^2 |
Flux integrated over lsst r-band |
lsst_flux_i |
float |
photons/sec/cm^2 |
Flux integrated over lsst i-band |
lsst_flux_z |
float |
photons/sec/cm^2 |
Flux integrated over lsst z-band |
lsst_flux_y |
float |
photons/sec/cm^2 |
Flux integrated over lsst y-band |