HD154363 (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:41:36.820886 (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=HD154363
Target Information |
|
|---|---|
RA |
256.2600549 [deg] (Gaia EDR3) |
Dec |
-5.071571995 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
4440.0 [K] (2021AJ….161..134H) |
Spectral Type |
K4/5V (1986AJ…..92..139S) |
Proper Motion (RA) |
-916.3429266 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
-1138.761891 [mas/yr] (Gaia EDR3) |
Parallax |
95.56697122 [mas/yr] (Gaia EDR3) |
Radial Velocity |
34.035 [mas/yr] (2018A&A…616A…7S) |
Aliases |
LHS 431, ** LDS 585A, AGKR 15220, AKARI-IRC-V1 J1705029-050407, BD-04 4225, CCDM J17051-0504A, Ci 20 1017, CSI-04 4225 1, FK5 5505, GC 23043, GCRV 9850, GEN# +1.00154363A, G 19-13, GJ 653, HD 154363, HIC 83591, HIP 83591, IDS 16597-0456 A, IRAS 17023-0459, JP11 2814, LFT 1316, LPM 625, LTT 6822, 2MASS J17050345-0503584, MCC 787, NLTT 44127, PLX 3878, PM 17025-0459, PPM 200318, SAO 141508, SKY# 30801, SRS 13983, StKM 2-1291, TIC 142456308, TYC 5072-408-1, UBV 14305, UBV 14406, UBV M 21889, UCAC4 425-069303, UGP 424, uvby98 100154363 A, VVO 143, WDS J17050-0504A, WEB 14132, WISEA J170502.78-050410.9, Wolf 635, YZC 17 5817, YZ 94 5817, [B10] 4342, Gaia DR2 4364527594192166400, Gaia EDR3 4364527594192166400, LHS431, **LDS585A, AGKR15220, AKARI-IRC-V1J1705029-050407, BD-044225, CCDMJ17051-0504A, Ci201017, CSI-0442251, FK55505, GC23043, GCRV9850, GEN#+1.00154363A, G19-13, GJ653, HD154363, HIC83591, HIP83591, IDS16597-0456A, IRAS17023-0459, JP112814, LFT1316, LPM625, LTT6822, 2MASSJ17050345-0503584, MCC787, NLTT44127, PLX3878, PM17025-0459, PPM200318, SAO141508, SKY#30801, SRS13983, StKM2-1291, TIC142456308, TYC5072-408-1, UBV14305, UBV14406, UBVM21889, UCAC4425-069303, UGP424, uvby98100154363A, VVO143, WDSJ17050-0504A, WEB14132, WISEAJ170502.78-050410.9, Wolf635, YZC175817, YZ945817, [B10]4342, GaiaDR24364527594192166400, GaiaEDR34364527594192166400, LHS431, LHS431, GJ653, GJ653, GJ653, GL653, GL653, GL653, HD154363, HD154363, HD154363, GL 653 |
OBJECT name(s) in headers |
HD 154363 |
PI name(s) in headers |
Ryan Cloutier |
Project/Run name(s) in headers |
21AC33, 22AC25, 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 |
34542.20 \(\pm\) 10.72 m/s |
CCF FWHM |
7193.46 \(\pm\) 140.36 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] |
2021-05-01 15:05:09.762 |
Last ccf file [Mid exposure] |
2022-03-17 14:59:41.832 |
Last processed [ccf] |
2025-02-23 18:19:07.838 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:41:39.138 |
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.