SR13 (spirou_offline_udem)¶
This page was last modified: 2026-02-12 21:01:46.420066 (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=SR13
Target Information |
|
|---|---|
RA |
247.1886026 [deg] (Gaia EDR3) |
Dec |
-24.47204989 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
3474.0 [K] (2020AJ….160..120J) |
Spectral Type |
M2e (1980AJ…..85..438R) |
Proper Motion (RA) |
-10.409004 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
-29.62725996 [mas/yr] (Gaia EDR3) |
Parallax |
8.660277422 [mas/yr] (Gaia EDR3) |
Radial Velocity |
nan [mas/yr] (None) |
Aliases |
** GHE 25, BKLT J162845-242819, DoAr 40, EM* StHA 130, EM* SR 13, EPIC 203905625, HBC 266, HGBS J162845.5-242819, IRAS 16257-2421, ISO-Oph 199, JCMTLSG J162845.1-242815, JP11 5453, 2MASS J16284527-2428190, ROXR2 36, ROX 34, ROXs 34, 1RXS J162845.5-242813, SPM2.0 57603136, SSTc2d J162845.3-242819, SSTc2d J162845.2-242818, TIC 175860953, V* V853 Oph, WDS J16288-2428AB, WRAY 15-1494, WSB 62, [EDJ2009] 958, [HL2013] 247.18859-24.47189, [WMR2005] 1-15, [WMR2005] J162845.3-242819.0, Gaia EDR3 6049102961266075392, Gaia DR2 6049102961266075392, EM_SR_13, **GHE25, BKLTJ162845-242819, DoAr40, EM*StHA130, EM*SR13, EPIC203905625, HBC266, HGBSJ162845.5-242819, IRAS16257-2421, ISO-Oph199, JCMTLSGJ162845.1-242815, JP115453, 2MASSJ16284527-2428190, ROXR236, ROX34, ROXs34, 1RXSJ162845.5-242813, SPM2.057603136, SSTc2dJ162845.3-242819, SSTc2dJ162845.2-242818, TIC175860953, V*V853Oph, WDSJ16288-2428AB, WRAY15-1494, WSB62, [EDJ2009]958, [HL2013]247.18859-24.47189, [WMR2005]1-15, [WMR2005]J162845.3-242819.0, GaiaEDR36049102961266075392, GaiaDR26049102961266075392, EMSR13, SR13, SR 13, SR_13 |
OBJECT name(s) in headers |
SR 13, SR13 |
PI name(s) in headers |
Jean-Francois Donati, |
Project/Run name(s) in headers |
25AP45, 22AP40, 23AP45, 23BP45 |
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 |
-5968.96 \(\pm\) 43.46 m/s |
CCF FWHM |
6414.47 \(\pm\) 149.87 m/s |
Number of CCF files Total |
271 |
Number of CCF passed QC |
271 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2022-05-11 12:17:02.746 |
Last ccf file [Mid exposure] |
2025-05-13 10:09:37.193 |
Last processed [ccf] |
2025-07-27 10:52:30.853 |
Version [ccf] |
0.7.292,0.7.293 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 21:02:10.885 |
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.