HD37479 (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:46:36.739201 (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=HD37479
Target Information |
|
|---|---|
RA |
84.69669302 [deg] (Gaia DR2) |
Dec |
-2.594590152 [deg] (Gaia DR2) |
Finder chart |
|
Teff |
12000.0 [K] (HEADER[CFHT]) |
Spectral Type |
B2IV-Vp_He (1977PASP…89..797A) |
Proper Motion (RA) |
1.280955545 [mas/yr] (Gaia DR2) |
Proper Motion (Dec) |
-0.6218041258 [mas/yr] (Gaia DR2) |
Parallax |
2.280145387 [mas/yr] (Gaia DR2) |
Radial Velocity |
32.66 [mas/yr] (2019AJ….157..196K) |
Aliases |
* sig Ori E, ** RAS 22, ** STF 762E, 1E 0536.2-0237, 2MASS J05384719-0235405, ADS 4241 E, ALS 8475, BD-02 1327, CCDM J05387-0236E, GBS-VLA J053847.19-023540.3, GC 7034, GCRV 3489, GEN# +1.00037479A, GSC 04771-01194, Gaia DR2 3216486478101981056, HD 37479, HR 1932, LS VI -02 3, Mayrit 41062, Mayrit 42062, PMSC 05337-0239E, PPM 188304, Renson 10080, SAO 132408, SKY# 9180, TIC 11286209, TYC 4771-1194-1, UBV 5703, UBV M 11312, V* V1030 Ori, WDS J05387-0236E, WDS J05387-0236Ea,Eb, WEB 5234, WH 414, YZ 92 1712, [FPS2006] NX 84, [HHM2007] 724, [SSC2008] 23, [W96] rJ053847-0235, ** RAS 22, ** STF 762E, ADS 4241 E, ALS 8475, BD-02 1327, GC 7034, GCRV 3489, HD 37479, HD37479, HD_37479, HR 1932, LS VI -02 3, SKY# 9180, UBV 5703, UBV M 11312, WEB 5234, YZ 92 1712, [FPS2006] NX 84, *sigOriE, **RAS22, **STF762E, 1E0536.2-0237, 2MASSJ05384719-0235405, ADS4241E, ALS8475, BD-021327, CCDMJ05387-0236E, GBS-VLAJ053847.19-023540.3, GC7034, GCRV3489, GEN#+1.00037479A, GSC04771-01194, GaiaDR23216486478101981056, HD37479, HR1932, LSVI-023, Mayrit41062, Mayrit42062, PMSC05337-0239E, PPM188304, Renson10080, SAO132408, SKY#9180, TIC11286209, TYC4771-1194-1, UBV5703, UBVM11312, V*V1030Ori, WDSJ05387-0236E, WDSJ05387-0236Ea,Eb, WEB5234, WH414, YZ921712, [FPS2006]NX84, [HHM2007]724, [SSC2008]23, [W96]rJ053847-0235, **RAS22, **STF762E, ADS4241E, ALS8475, BD-021327, GC7034, GCRV3489, HD37479, HD37479, HD37479, HR1932, LSVI-023, SKY#9180, UBV5703, UBVM11312, WEB5234, YZ921712, [FPS2006]NX84 |
OBJECT name(s) in headers |
HD37479 |
PI name(s) in headers |
Claire Moutou |
Project/Run name(s) in headers |
18BE99 |
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 |
297640.68 \(\pm\) 3427.74 m/s |
CCF FWHM |
40983.89 \(\pm\) 44657.67 m/s |
Number of CCF files Total |
4 |
Number of CCF passed QC |
4 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2018-09-26 14:13:03.937 |
Last ccf file [Mid exposure] |
2018-09-26 14:29:52.544 |
Last processed [ccf] |
2025-02-23 21:22:23.299 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:46:39.268 |
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.