HD37394 (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:46:36.514356 (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=HD37394
Target Information |
|
|---|---|
RA |
85.33475294 [deg] (Gaia EDR3) |
Dec |
53.47873144 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
5360.0 [K] (2021AJ….161..134H) |
Spectral Type |
K1 (1985ApJS…59..197B) |
Proper Motion (RA) |
2.803536777 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
-523.4774904 [mas/yr] (Gaia EDR3) |
Parallax |
81.49871331 [mas/yr] (Gaia EDR3) |
Radial Velocity |
0.89 [mas/yr] (2018A&A…616A…7S) |
Aliases |
HD 37394, ** ENG 22A, ** BUP 82A, AG+53 486, ASCC 246596, BD+53 934, CCDM J05413+5329A, Ci 20 341, CSI+53 934 1, GC 7064, GCRV 3500, GEN# +1.00037394, GJ 211, GSC 03749-01334, HIC 26779, HIP 26779, HR 1925, IDS 05332+5326 A, IRAS 05373+5327, JP11 1201, LFT 423, LHS 1774, LSPM J0541+5328, LTT 11694, 2MASS J05412033+5328523, NLTT 15439, NSV 16618, PLX 1289, PMC 90-93 4855, PPM 29972, 2RE J0541+532, 2RE J054119+532931, RE J0541+532, RE J054117+532855, 1RXS J054122.0+532903, SAO 25319, SKY# 9285, SPOCS 276, TIC 311063391, TYC 3749-1334-1, UBV 5672, UBV M 11289, USNO-B1.0 1434-00163923, uvby98 100037394, V* V538 Aur, WDS J05413+5329A, WEB 5281, WISEA J054120.37+532846.5, YZ 53 2262, [GKL99] 145, Gaia DR2 263916708025623680, Gaia EDR3 263916708025623680, HD37394, **ENG22A, **BUP82A, AG+53486, ASCC246596, BD+53934, CCDMJ05413+5329A, Ci20341, CSI+539341, GC7064, GCRV3500, GEN#+1.00037394, GJ211, GSC03749-01334, HIC26779, HIP26779, HR1925, IDS05332+5326A, IRAS05373+5327, JP111201, LFT423, LHS1774, LSPMJ0541+5328, LTT11694, 2MASSJ05412033+5328523, NLTT15439, NSV16618, PLX1289, PMC90-934855, PPM29972, 2REJ0541+532, 2REJ054119+532931, REJ0541+532, REJ054117+532855, 1RXSJ054122.0+532903, SAO25319, SKY#9285, SPOCS276, TIC311063391, TYC3749-1334-1, UBV5672, UBVM11289, USNO-B1.01434-00163923, uvby98100037394, V*V538Aur, WDSJ05413+5329A, WEB5281, WISEAJ054120.37+532846.5, YZ532262, [GKL99]145, GaiaDR2263916708025623680, GaiaEDR3263916708025623680 |
OBJECT name(s) in headers |
HD 37394 |
PI name(s) in headers |
Ryan Cloutier |
Project/Run name(s) in headers |
21AC33, 21BC28 |
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 |
1167370.77 \(\pm\) 3483.68 m/s |
CCF FWHM |
31083.99 \(\pm\) 5977.33 m/s |
Number of CCF files Total |
2 |
Number of CCF passed QC |
2 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2021-03-31 07:18:07.944 |
Last ccf file [Mid exposure] |
2021-10-14 15:46:09.088 |
Last processed [ccf] |
2025-02-23 18:26:00.123 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:46:38.796 |
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.