GJ617B (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:00:24.801675 (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=GJ617B
Target Information |
|
|---|---|
RA |
244.1832577 [deg] (Gaia EDR3) |
Dec |
67.25664063 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
3525.0 [K] (2022MNRAS.516.3802C) |
Spectral Type |
M3.0Ve (2013AJ….145..102L) |
Proper Motion (RA) |
-483.0059406 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
89.04882414 [mas/yr] (Gaia EDR3) |
Parallax |
92.89848935 [mas/yr] (Gaia EDR3) |
Radial Velocity |
-18.36 [mas/yr] (2018MNRAS.475.1960F) |
Aliases |
WDS J16167+6714B, GL617B, HIC79762, GALEX6370950986031173392, UBV13870, LFT1264, AC+675226, HIP 79762, UBV 13870, TIC 230073588, CSI+67 935 2, Gl617B, Gaia EDR3 1642642957122493824, USNO-B1.01572-00194547, Gaia DR3 1642642957122493824, G 225-58, GALEX J161644.8+671522, WDSJ16167+6714B, WEB13499, ** ENG 57B, IDS16165+6729B, GaiaDR11642642952826225024, VVO405, CSI+679352, GEN#+1.20147379, 2MASS J16164537+6715224, GJ617B, TYC 4195-1167-1, WISEAJ161644.44+671523.3, [RHG95]2567, GSC04195-01167, WISEA J161644.44+671523.3, PMJ16167+6715, G 257-33, LTT14864, V* EW Dra, EW_DRA, EW Dra, LHS 3176, GCRV 66176, GJ 617 B, CCDMJ16167+6715B, LSPMJ1616+6715, AC +67 5226-0, PM J16167+6715, GaiaDR31642642957122493824, AC +67 5226, IDS 16166+6729 B, CSI+67 935 2, [RHG95] 2567, AC +67 5226, GCRV66176, Gaia DR2 1642642957122493824, EWDRA, Karmn J16167+672N, LSPM J1616+6715, GaiaDR21642642957122493824, G 240-15, NLTT42489, GJ 617 B, HIP 79762, NLTT 42489, HIC 79762, GALEXJ161644.8+671522, GaiaEDR31642642957122493824, VVO 405, IDS16166+6729B, TIC230073588, ** ENG 57B, ASCC 86598, G240-15, HIC 79762, CCDM J16167+6715B, KarmnJ16167+672N, AC +67 5226-0, GEN# +1.00147379B, GEN#+1.00147379B, LHS3176, UCAC4787-024324, **ENG57B, WEB 13499, [RHG95] 2567, UCAC4 787-024324, ASCC86598, LHS 3176, LFT 1264, G257-33, UBV 13870, GEN# +1.20147379, GALEX 6370950986031173392, Gaia DR1 1642642952826225024, AC+675226-0, USNO-B1.0 1572-00194547, IDS 16165+6729 B, V*EWDra, GSC 04195-01167, LTT 14864, TYC4195-1167-1, G225-58, 2MASSJ16164537+6715224, HIP79762, ASCC 86598 |
OBJECT name(s) in headers |
Gl617B |
PI name(s) in headers |
Andres Carmona, Etienne Artigau, Jean-Francois Donati, |
Project/Run name(s) in headers |
25BF27, 25AF23, 24BC05, 20AP40, 20BP40, 21AP40, 22AP40, 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 |
GL846_neg.fits |
CCF systemic velocity |
-18536.75 \(\pm\) 10.35 m/s |
CCF FWHM |
6802.71 \(\pm\) 84.62 m/s |
Number of CCF files Total |
781 |
Number of CCF passed QC |
781 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2019-09-18 05:48:00.280 |
Last ccf file [Mid exposure] |
2025-10-08 04:42:42.168 |
Last processed [ccf] |
2025-11-04 18:11:23.540 |
Version [ccf] |
0.7.294,0.7.292,0.7.293 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:02:05.639 |
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.