AN_SEX (spirou_offline_udem)¶
This page was last modified: 2026-02-12 19:26:10.841899 (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=AN_SEX
Target Information |
|
|---|---|
RA |
153.0729586 [deg] (Gaia DR2) |
Dec |
-3.746713797 [deg] (Gaia DR2) |
Finder chart |
|
Teff |
3644.0 [K] (2022MNRAS.516.3802C) |
Spectral Type |
M2V (1991ApJS…77..417K) |
Proper Motion (RA) |
-152.9309691 [mas/yr] (Gaia DR2) |
Proper Motion (Dec) |
-243.5980101 [mas/yr] (Gaia DR2) |
Parallax |
129.7887262 [mas/yr] (Gaia DR2) |
Radial Velocity |
7.87 [mas/yr] (2018MNRAS.475.1960F) |
Aliases |
BD-03 2870, AP J10121768-0344441, ASAS J101218-0344.8, ASAS J101217-0344.6, GALEX J101217.6-034445, GCRV 61131, GEN# -0.00302870, G 162-25, G 53-29, GJ 382, HIC 49986, HIP 49986, IRAS 10097-0329, JP11 247, Karmn J10122-037, LTT 3734, 2MASS J10121768-0344441, MCC 569, NLTT 23680, 8pc 127.99, PLX 2395.11, PM J10122-0344, PPM 193190, 1RXS J101217.2-034442, SAO 137411, StKM 2-618, TIC 77612635, TYC 4907-704-1, UBV M 5136, UCAC4 432-051854, V* AN Sex, VVO 13, WEB 9193, WISEA J101217.55-034447.1, YZC 17 3945, YZ 93 3945, Zkh 139, [RHG95] 1595, Gaia DR3 3828238392559860992, Gaia DR2 3828238392559860992, BD-032870, APJ10121768-0344441, ASASJ101218-0344.8, ASASJ101217-0344.6, GALEXJ101217.6-034445, GCRV61131, GEN#-0.00302870, G162-25, G53-29, GJ382, HIC49986, HIP49986, IRAS10097-0329, JP11247, KarmnJ10122-037, LTT3734, 2MASSJ10121768-0344441, MCC569, NLTT23680, 8pc127.99, PLX2395.11, PMJ10122-0344, PPM193190, 1RXSJ101217.2-034442, SAO137411, StKM2-618, TIC77612635, TYC4907-704-1, UBVM5136, UCAC4432-051854, V*ANSex, VVO13, WEB9193, WISEAJ101217.55-034447.1, YZC173945, YZ933945, Zkh139, [RHG95]1595, GaiaDR33828238392559860992, GaiaDR23828238392559860992, GL382, Gl382 |
OBJECT name(s) in headers |
Gl382 |
PI name(s) in headers |
Etienne Artigau, Andres Carmona, QSO Team |
Project/Run name(s) in headers |
25BC08, 25AF23, 24BC05, 24BF13, 20BQ57, 21AQ57, 21BQ57, 22AQ57, 22BF10, 23AF13, 23AD98, 24AC25, 24AF17, 19AQ57 |
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 |
GL846_neg.fits |
CCF systemic velocity |
7921.15 \(\pm\) 13.43 m/s |
CCF FWHM |
7153.73 \(\pm\) 93.67 m/s |
Number of CCF files Total |
721 |
Number of CCF passed QC |
721 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2019-02-14 12:22:01.672 |
Last ccf file [Mid exposure] |
2025-11-02 15:55:17.867 |
Last processed [ccf] |
2026-01-07 12:18:25.739 |
Version [ccf] |
0.7.294,0.7.292,0.7.295,0.7.293 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 19:27:37.584 |
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.