GL48 (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:16:46.746814 (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=GL48
Target Information |
|
|---|---|
RA |
15.65901188 [deg] (Gaia EDR3) |
Dec |
71.67812049 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
3529.0 [K] (2022MNRAS.516.3802C) |
Spectral Type |
M3.0Ve (2013AJ….145..102L) |
Proper Motion (RA) |
1746.701013 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
-381.7623697 [mas/yr] (Gaia EDR3) |
Parallax |
121.4598287 [mas/yr] (Gaia EDR3) |
Radial Velocity |
1.56 [mas/yr] (2018MNRAS.475.1960F) |
Aliases |
1RXS J010232.2+714110, 2MASS J01023213+7140475, AC +71 532, ASCC 3719, BD+70 68b, CSI+71-00588, Ci 20 66, G 242-76, G 243-51, G 245-15, GCRV 577, GEN# +0.07000068, GEN# +9.80242076, GJ 48, Gaia DR1 533621855139954816, Gaia DR2 533621859441169920, Gaia EDR3 533621859441169920, HIC 4856, HIP 4856, IRAS 00589+7124, Karmn J01025+716, LFT 93, LHS 131, LSPM J0102+7140, LTT 10362, MCC 364, NLTT 3359, NSV 365, PLX 202, PLX 202.00, PM 00589+7125, PM J01025+7140, Ross 318, TIC 379084450, TYC 4304-700-1, UBV 937, UCAC4 809-003873, USNO-B1.0 1616-00016948, VVO 273, WEB 928, WISEA J010235.99+714043.2, Zkh 19, [GKL99] 32, [HFE83] 46, [KW97] 4-36, [RHG95] 195, AC +71 532, ASCC 3719, BD+70 68b, Ci 20 66, GCRV 577, GJ 48, GL48, Gl48, HIC 4856, HIP 4856, LFT 93, LHS 131, NLTT 3359, NSV 365, PLX 202, PLX 202.00, Ross 318, UBV 937, WEB 928, Zkh 19, [HFE83] 46, [KW97] 4-36, [RHG95] 195, 1RXSJ010232.2+714110, 2MASSJ01023213+7140475, AC+71532, ASCC3719, BD+7068b, CSI+71-00588, Ci2066, G242-76, G243-51, G245-15, GCRV577, GEN#+0.07000068, GEN#+9.80242076, GJ48, GaiaDR1533621855139954816, GaiaDR2533621859441169920, GaiaEDR3533621859441169920, HIC4856, HIP4856, IRAS00589+7124, KarmnJ01025+716, LFT93, LHS131, LSPMJ0102+7140, LTT10362, MCC364, NLTT3359, NSV365, PLX202, PLX202.00, PM00589+7125, PMJ01025+7140, Ross318, TIC379084450, TYC4304-700-1, UBV937, UCAC4809-003873, USNO-B1.01616-00016948, VVO273, WEB928, WISEAJ010235.99+714043.2, Zkh19, [GKL99]32, [HFE83]46, [KW97]4-36, [RHG95]195, AC+71532, ASCC3719, BD+7068b, Ci2066, GCRV577, GJ48, GL48, Gl48, HIC4856, HIP4856, LFT93, LHS131, NLTT3359, NSV365, PLX202, PLX202.00, Ross318, UBV937, WEB928, Zkh19, [HFE83]46, [KW97]4-36, [RHG95]195 |
OBJECT name(s) in headers |
Gl48 |
PI name(s) in headers |
Etienne Artigau, Andres Carmona, Jean-Francois Donati |
Project/Run name(s) in headers |
25BC08, 24BC05, 24BF13, 20AP40, 20BP40, 21AP40, 21BP40, 23AD98, 23BF12, 23BC10, 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 |
1485.01 \(\pm\) 20.40 m/s |
CCF FWHM |
6852.18 \(\pm\) 91.58 m/s |
Number of CCF files Total |
989 |
Number of CCF passed QC |
989 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2019-09-11 14:50:39.930 |
Last ccf file [Mid exposure] |
2025-10-13 08:03:47.791 |
Last processed [ccf] |
2025-11-04 17:45:17.393 |
Version [ccf] |
0.7.294,0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:19:14.540 |
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.