GL408 (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:15:41.788398 (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=GL408
Target Information |
|
|---|---|
RA |
165.0156786 [deg] (Gaia EDR3) |
Dec |
22.8317023 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
3487.0 [K] (2022MNRAS.516.3802C) |
Spectral Type |
M4V (1986AJ…..92..139S) |
Proper Motion (RA) |
-426.9577222 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
-282.2984032 [mas/yr] (Gaia EDR3) |
Parallax |
148.1985503 [mas/yr] (Gaia EDR3) |
Radial Velocity |
3.29 [mas/yr] (2018MNRAS.475.1960F) |
Aliases |
2MASS J11000432+2249592, 8pc 150.96, AC +23 468-46, ASCC 776322, CSI+23-10574, Ci 20 601, G 58-32, G 119-49, G 120-9, GALEX 6387874711957667994, GCRV 6797, GEN# +9.80058032, GJ 408, Gaia DR2 3988987164339438208, Gaia EDR3 3988987164339438208, HIC 53767, HIP 53767, Karmn J11000+228, LHS 6193, LSPM J1100+2249, LTT 12942, MCC 128, NLTT 25946, PLX 2561, PLX 2561.00, PM J11000+2249, Ross 104, StKM 2-688, TIC 97472519, TYC 1978-1286-1, UBV 10057, UCAC2 39850706, UCAC4 565-047644, USNO-B1.0 1128-00230478, WEB 9740, WISEA J110003.93+224955.7, Zkh 148, [HFE83] 768, [RHG95] 1709, AC +23 468-46, ASCC 776322, Ci 20 601, G 58-32, GCRV 6797, GJ 408, GL408, Gl408, HIC 53767, HIP 53767, LHS 6193, Ross 104, UBV 10057, UCAC2 39850706, WEB 9740, [HFE83] 768, [RHG95] 1709, 2MASSJ11000432+2249592, 8pc150.96, AC+23468-46, ASCC776322, CSI+23-10574, Ci20601, G58-32, G119-49, G120-9, GALEX6387874711957667994, GCRV6797, GEN#+9.80058032, GJ408, GaiaDR23988987164339438208, GaiaEDR33988987164339438208, HIC53767, HIP53767, KarmnJ11000+228, LHS6193, LSPMJ1100+2249, LTT12942, MCC128, NLTT25946, PLX2561, PLX2561.00, PMJ11000+2249, Ross104, StKM2-688, TIC97472519, TYC1978-1286-1, UBV10057, UCAC239850706, UCAC4565-047644, USNO-B1.01128-00230478, WEB9740, WISEAJ110003.93+224955.7, Zkh148, [HFE83]768, [RHG95]1709, AC+23468-46, ASCC776322, Ci20601, G58-32, GCRV6797, GJ408, GL408, Gl408, HIC53767, HIP53767, LHS6193, Ross104, UBV10057, UCAC239850706, WEB9740, [HFE83]768, [RHG95]1709 |
OBJECT name(s) in headers |
Gl408 |
PI name(s) in headers |
Jean-Francois Donati |
Project/Run name(s) in headers |
20BP40, 21AP40, 21BP40, 22AP40, 19AP40, 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 |
3464.76 \(\pm\) 10.33 m/s |
CCF FWHM |
5404.47 \(\pm\) 59.53 m/s |
Number of CCF files Total |
701 |
Number of CCF passed QC |
701 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2019-02-14 14:32:12.779 |
Last ccf file [Mid exposure] |
2022-06-11 06:15:24.244 |
Last processed [ccf] |
2025-02-23 21:17:00.203 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:17:14.186 |
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.