GJ876A (spirou_offline_udem)¶
This page was last modified: 2026-02-12 19:58:59.571969 (UTC)
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Contents¶
Target info¶
This section gives some details of the APERO astrometric database used when processing this target (e.g. for BERV calculation). Any observation with a object name in the alias list will be associated with this “APERO target” i.e. DRSOBJN=GJ876A
Target Information |
|
|---|---|
RA |
343.324111 [deg] (Gaia EDR3) |
Dec |
-14.26668939 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
3366.0 [K] (2022MNRAS.516.3802C) |
Spectral Type |
M3.5V (1983SAAOC…7..106W) |
Proper Motion (RA) |
957.7147313 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
-673.6012365 [mas/yr] (Gaia EDR3) |
Parallax |
214.0379889 [mas/yr] (Gaia EDR3) |
Radial Velocity |
-1.47 [mas/yr] (2018MNRAS.475.1960F) |
Aliases |
GSC 05819-00957, GaiaDR22603090003484152064, Zkh 338, EPIC206019392, NC59, HIC 113020, LPM841, UBV 19610, UBV 19209, GEN# -0.01506290, LHS 530, NC 59, PM J22532-1415, ILAQR, BD-156290, GEN#-0.01506290, Karmn J22532-142, BD-15 6290, EPIC206019387, NLTT55130, Ci201387, UCAC2 26801725, Gl876, GCRV 14365, LFT 1745, [RHG95] 3604, NLTT 55130, Ross 780, PLX5546, UCAC2 26801725, KarmnJ22532-142, Gaia DR2 2603090003484152064, UCAC4 379-165686, MCC 337, EPIC 206019392, G156-57, LHS530, 8pc 212.69A, LFT1745, PMJ22532-1415, UBV 19209, GJ 876 A, [RHG95]3604, TIC 188580272, UBV19610, GaiaEDR32603090003484152064, IL_AQR, [RHG95] 3604, JP11 295, WEB 20121, UBV M 5470, NAMENC59, GaiaDR32603090003484152064, GJ876, EPIC 206019387, UBV 19610, Ross780, Gaia DR3 2603090003484152064, GJ 876, G 156-57A, GJ 876 A, UBV M 5470, PLX 5546, UBVM5470, JP11 295, HIC113020, TIC188580272, TYC 5819-1255-1, JP11295, HIP113020, 8pc212.69A, TYC5819-1255-1, V* IL Aqr, WISEA J225317.42-141556.1, LTT 9244, GCRV14365, Ross 780, WISEAJ225317.42-141556.1, UCAC226801725, GSC05819-00957, LHS 530, WEB20121, UCAC4379-165686, GJ876A, Ci 20 1387, IL Aqr, Gaia EDR3 2603090003484152064, LTT9244, PLX5546.00, Zkh338, BD-15 6290, 2MASSJ22531672-1415489, G156-57A, LTT 9244, MCC337, GL876, LPM 841, HIP 113020, G 156-57, UBV19209, NAME NC 59, 2MASS J22531672-1415489, PLX 5546.00, GJ 876, V*ILAqr |
OBJECT name(s) in headers |
Gl876 |
PI name(s) in headers |
QSO Team |
Project/Run name(s) in headers |
20AQ57, 20BQ57, 21AQ57, 21BQ57, 19AQ57, 19BQ57 |
Spectrum¶
This section presents the observation after extraction,with and without telluric correction.
LBL¶
No LBL reduction found
CCF¶
This section presents the APERO CCF results for this object.
CCF stats |
|
|---|---|
Mask used |
GL699_neg.fits |
CCF systemic velocity |
-1141.85 \(\pm\) 178.17 m/s |
CCF FWHM |
5289.53 \(\pm\) 43.14 m/s |
Number of CCF files Total |
368 |
Number of CCF passed QC |
368 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2019-06-14 12:18:11.295 |
Last ccf file [Mid exposure] |
2021-10-27 08:37:07.337 |
Last processed [ccf] |
2025-02-23 21:00:33.701 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 19:59:40.835 |
Time series¶
This section deals with providing the time series information for this object
Debug¶
This section has various debug plots from APERO products
Telluric map¶
Telluric map of e2dsff_tcorr_A files.Files are low-passed and corrected for the stars motion. The QC is displayed to the right of the image - in purple are the files that passed, in orange the files that failed.
Maximum Saturation level plot¶
Maximum saturation level measured at time of extraction
Measured effective readout noise before extraction¶
Measured effective readout noise before extraction
APERO Processing Debug Plot¶
Plotting the version and processed date from the header from APERO. Note that offline reductions should lead to a straight line, while online reductions should be roughly a one-to-one with the Date axis.
APERO Calibration times plot¶
Computed time between observation and calibration used. Some calibrations arereference calibrations (in purple) and thus diverge from the reference night, others should always be from the same night (orange) unless no calibration was taken that night in which case the closest calirbation in time should have been used.