GL169_1A (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:15:51.178801 (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=GL169_1A
Target Information |
|
|---|---|
RA |
67.80919063 [deg] (Gaia EDR3) |
Dec |
58.96797997 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
3307.0 [K] (2022MNRAS.516.3802C) |
Spectral Type |
M4.0Ve (2013AJ….145..102L) |
Proper Motion (RA) |
1300.364784 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
-2046.105519 [mas/yr] (Gaia EDR3) |
Parallax |
181.243839 [mas/yr] (Gaia EDR3) |
Radial Velocity |
29.05 [mas/yr] (2018MNRAS.475.1960F) |
Aliases |
** STI 2051A, 2MASS J04311147+5858375, 8pc 181.36A, AKARI-IRC-V1 J0431126+585823, ASCC 176742, CCDM J04312+5858A, CSI+58-04268 1, G 175-34, GJ 169.1 A, Gaia DR2 470826482635704064, Gaia EDR3 470826482637310080, HIC 21088, HIP 21088, IDS 04224+5849 A, IRAS 04268+5852, JP11 5943, Karmn J04311+589, LHS 26, LSPM J0431+5858W, NAME Stein 2051, NAME Stein 2051A, NLTT 13373, PM 04268+5854, PM J04311+5858, TIC 356322721, UBV 4295, UCAC4 745-033846, USNO 120, USNO 807, USNO-B1.0 1489-00136092, WDS J04312+5858A, WISE J043113.20+585816.7, WISEA J043113.21+585816.7, Zkh 62, [RHG95] 780, ** STN 2051A, ASCC 176742, CSI+58-04268 1, G 175-34A, GJ 169.1 A, GL169.1A, GL169_1A, Gl169.1A, JP11 5943, LHS 26, NAME Stein 2051 A, UBV 4295, Zkh 62, [RHG95] 780, **STI2051A, 2MASSJ04311147+5858375, 8pc181.36A, AKARI-IRC-V1J0431126+585823, ASCC176742, CCDMJ04312+5858A, CSI+58-042681, G175-34, GJ169.1A, GaiaDR2470826482635704064, GaiaEDR3470826482637310080, HIC21088, HIP21088, IDS04224+5849A, IRAS04268+5852, JP115943, KarmnJ04311+589, LHS26, LSPMJ0431+5858W, NAMEStein2051, NAMEStein2051A, NLTT13373, PM04268+5854, PMJ04311+5858, TIC356322721, UBV4295, UCAC4745-033846, USNO120, USNO807, USNO-B1.01489-00136092, WDSJ04312+5858A, WISEJ043113.20+585816.7, WISEAJ043113.21+585816.7, Zkh62, [RHG95]780, **STN2051A, ASCC176742, CSI+58-042681, G175-34A, GJ169.1A, GL169.1A, GL1691A, Gl169.1A, JP115943, LHS26, NAMEStein2051A, UBV4295, Zkh62, [RHG95]780 |
OBJECT name(s) in headers |
Gl169.1A |
PI name(s) in headers |
Jean-Francois Donati |
Project/Run name(s) in headers |
20BP40, 21AP40, 21BP40, 19BP40, 20AP40 |
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 |
29015.93 \(\pm\) 10.15 m/s |
CCF FWHM |
5315.21 \(\pm\) 50.22 m/s |
Number of CCF files Total |
736 |
Number of CCF passed QC |
736 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2019-09-18 14:26:11.242 |
Last ccf file [Mid exposure] |
2022-01-26 08:14:12.584 |
Last processed [ccf] |
2025-02-23 20:53:51.996 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:17:28.945 |
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.