GL445 (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:15:27.717158 (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=GL445
Target Information |
|
|---|---|
RA |
176.939408 [deg] (Gaia EDR3) |
Dec |
78.69329745 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
3356.0 [K] (2022MNRAS.516.3802C) |
Spectral Type |
M4.0Ve (2013AJ….145..102L) |
Proper Motion (RA) |
748.4182886 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
480.8043 [mas/yr] (Gaia EDR3) |
Parallax |
190.3251427 [mas/yr] (Gaia EDR3) |
Radial Velocity |
-111.51 [mas/yr] (2018MNRAS.475.1960F) |
Aliases |
2MASS J11474143+7841283, 8pc 185.48, AC +79 3883-0, AC +79 3888, AC +79 3888-0, ASCC 34165, CSI+78-11446, G 254-29, GCRV 7135, GEN# +6.10010445, GEN# +9.80254029, GJ 445, Gaia DR1 1129149719617136384, Gaia DR2 1129149723913123456, Gaia EDR3 1129149723913123456, HIC 57544, HIP 57544, JP11 5142, LFT 849, LHS 2459, LSPM J1147+7841, LTT 13235, NLTT 28539, PLX 2722, PLX 2722.00, PM J11476+7841, TIC 358615829, TYC 4553-192-1, UCAC4 844-010540, USNO-B1.0 1686-00047479, WEB 10334, Zkh 168, [RHG95] 1845, AC +79 3883-0, AC +79 3888, AC +79 3888-0, ASCC 34165, GCRV 7135, GJ 445, GL445, Gl445, HIC 57544, HIP 57544, JP11 5142, LFT 849, LHS 2459, [RHG95] 1845, 2MASSJ11474143+7841283, 8pc185.48, AC+793883-0, AC+793888, AC+793888-0, ASCC34165, CSI+78-11446, G254-29, GCRV7135, GEN#+6.10010445, GEN#+9.80254029, GJ445, GaiaDR11129149719617136384, GaiaDR21129149723913123456, GaiaEDR31129149723913123456, HIC57544, HIP57544, JP115142, LFT849, LHS2459, LSPMJ1147+7841, LTT13235, NLTT28539, PLX2722, PLX2722.00, PMJ11476+7841, TIC358615829, TYC4553-192-1, UCAC4844-010540, USNO-B1.01686-00047479, WEB10334, Zkh168, [RHG95]1845, AC+793883-0, AC+793888, AC+793888-0, ASCC34165, GCRV7135, GJ445, GL445, Gl445, HIC57544, HIP57544, JP115142, LFT849, LHS2459, [RHG95]1845 |
OBJECT name(s) in headers |
Gl445 |
PI name(s) in headers |
Andres Carmona, Jean-Francois Donati, Etienne Artigau |
Project/Run name(s) in headers |
25BF27, 25AF23, 24BF13, 20AP40, 20BP40, 21AP40, 21BP40, 22AP40, 22BF10, 23AF13, 23AD98, 24AC25, 24AF17, 19BP40 |
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 |
-111343.56 \(\pm\) 11.04 m/s |
CCF FWHM |
5250.11 \(\pm\) 40.79 m/s |
Number of CCF files Total |
571 |
Number of CCF passed QC |
571 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2019-12-07 16:05:15.668 |
Last ccf file [Mid exposure] |
2025-11-28 16:02:36.648 |
Last processed [ccf] |
2026-01-07 12:07:17.926 |
Version [ccf] |
0.7.292,0.7.295,0.7.293 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:16:30.250 |
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.