This is the calibrated FoV transit photometry from CU5. All instrumental effects should have
been calibrated out and all transits should be on the same photometric system.
This table is complemented by the FinalCalPhotFovTransit table which extends this, including
additional CCD-level epoch photometry for all FoV transits whose sources show a high noise
level. Transits that are selected to appear in the FinalCalPhotFovTransit table will not appear in
the CalPhotFovTransit table.
G Transit Time Serie
Field-of-view transit averaged observation time in units of Barycentric JD (in TCB) in days - 2 455 197.5, computed as follows. First the observation time is converted from On-board Mission Time (OBMT) into Julian date in TCB (Temps Coordonnee Barycentrique). Next a correction´ is applied for the light-travel time to the Solar system barycentre, resulting in Barycentric Julian Date (BJD). Finally, an offset of 2 455 197.5 days is applied (corresponding to a reference time T0 at 2010-01-01T00:00:00) to have a conveniently small numerical value. Although the centroiding time accuracy of the individual CCD observations is (much) below 1 ms, this per-FoV observation time is averaged over typically 9 CCD observations taken in a time range of about 44 sec.
The average G flux value for the FoV transit. The calculation only uses accepted transits. This could include SM and AF fluxes.
The error on the mean G Flux.
G-band mean magnitude for the field-of-view transit, computed from the fluxGFov field using magnitude zero-point defined in ExtPhotZeroPoint.
| 1755.32954 |
22667.037 |
0.001087 |
14.79380 |
| 1755.403519 |
22633.008 |
0.00113 |
14.795432 |
| 1758.32954 |
22603.0083 |
0.001087 |
14.79380 |
BP Time Serie
Observation time of the BP CCD transit in units of Barycentric JD (in TCB) in days -2 455 197.5, computed as follows. First the observation time is converted from On-board Mission Time (OBMT) into Julian date in TCB (Temps Coordonnee Barycentrique). Next a correction is applied for the light-travel time to the Solar system barycentre, resulting in Barycentric Julian Date (BJD). Finally, an offset of 2 455 197.5 days is applied (corresponding to a reference time T0 at 2010-01-01T00:00:00) to have a conveniently small numerical value.
The integrated BP flux value of the transit. If the BP flux has been rejected or is unavailable, the flux will be set to NaN
The error on the BP Flux. If the BP flux has been rejected or is unavailable, this error will be set
to NaN.
Magnitude of the object
| 1755.32986 |
12450.138 |
0.009554 |
15.13604 |
| 1755.403862 |
12333.2679 |
0.00953579 |
15.1462839 |
| 1785.311637 |
12164.75277 |
0.01032739 |
15.1612211 |
RP Time Serie
Observation time of the RP CCD transit in units of Barycentric JD (in TCB) in days -2 455 197.5, computed as follows. First the observation time is converted from On-board Mission Time (OBMT) into Julian date in TCB (Temps Coordonnee Barycentrique). Next a correction is applied for the light-travel time to the Solar system barycentre, resulting in Barycentric Julian Date (BJD). Finally, an offset of 2 455 197.5 days is applied (corresponding to a reference time T0 at 2010-01-01T00:00:00) to have a conveniently small numerical value.
The integrated RP flux value of the transit. If the RP flux has been rejected or is unavailable, the flux will be set to NaN.
The error on the RP Flux. If the RP flux has been rejected or is unavailable, this error will be set to NaN.
G-band mean magnitude for the field-of-view transit, computed from the fluxGFov field using magnitude zero-point defined in ExtPhotZeroPoint
| 1755.329995 |
12450.138 |
0.00844822 |
14.296258875 |
| 1755.4039501 |
12333.2679 |
0.0085103 |
14.250145 |
| 1785.31172437 |
12164.75277 |
0.008866162 |
14.30223461 |