HD89269 (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:47:11.930237 (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=HD89269
Target Information |
|
|---|---|
RA |
154.716831 [deg] (Gaia EDR3) |
Dec |
44.04698609 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
5590.0 [K] (2021AJ….161..134H) |
Spectral Type |
G4V (2003AJ….126.2048G) |
Proper Motion (RA) |
61.77181875 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
-300.2678167 [mas/yr] (Gaia EDR3) |
Parallax |
49.54145913 [mas/yr] (Gaia EDR3) |
Radial Velocity |
-7.518 [mas/yr] (2018A&A…616A…7S) |
Aliases |
** ENG 43A, 2MASS J10185193+4402544, AG+44 939, AGKR 9271, ASCC 406501, BD+44 1973, CCDM J10189+4403A, FK5 2826, GC 14143, GCRV 6490, GEN# +1.00089269, GJ 3593, Gaia DR1 806000812673038208, Gaia DR2 806000816970521728, Gaia EDR3 806000816970521728, HD 89269, HIC 50505, HIP 50505, IDS 10127+4433 A, IRAS 10158+4418, LSPM J1018+4402, LTT 12759, N30 2449, NLTT 23953, PLX 2416, PPM 51812, SAO 43279, SKY# 19811, SPOCS 449, TIC 39777146, TYC 3007-67-1, UBV 9542, UBV M 16108, USNO-B1.0 1340-00214023, WDS J10189+4403A, WEB 9264, WISEA J101852.01+440250.7, uvby98 100089269, ** ENG 43A, AG+44 939, AGKR 9271, ASCC 406501, BD+44 1973, GCRV 6490, GJ 3593, HD 89269, HD89269, HD_89269, HIC 50505, HIP 50505, PPM 51812, SAO 43279, SPOCS 449, UBV 9542, UBV M 16108, WEB 9264, **ENG43A, 2MASSJ10185193+4402544, AG+44939, AGKR9271, ASCC406501, BD+441973, CCDMJ10189+4403A, FK52826, GC14143, GCRV6490, GEN#+1.00089269, GJ3593, GaiaDR1806000812673038208, GaiaDR2806000816970521728, GaiaEDR3806000816970521728, HD89269, HIC50505, HIP50505, IDS10127+4433A, IRAS10158+4418, LSPMJ1018+4402, LTT12759, N302449, NLTT23953, PLX2416, PPM51812, SAO43279, SKY#19811, SPOCS449, TIC39777146, TYC3007-67-1, UBV9542, UBVM16108, USNO-B1.01340-00214023, WDSJ10189+4403A, WEB9264, WISEAJ101852.01+440250.7, uvby98100089269, **ENG43A, AG+44939, AGKR9271, ASCC406501, BD+441973, GCRV6490, GJ3593, HD89269, HD89269, HD89269, HIC50505, HIP50505, PPM51812, SAO43279, SPOCS449, UBV9542, UBVM16108, WEB9264 |
OBJECT name(s) in headers |
HD89269 |
PI name(s) in headers |
Lauren Weiss |
Project/Run name(s) in headers |
19AH28 |
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 |
-6864.41 \(\pm\) 19.36 m/s |
CCF FWHM |
8347.74 \(\pm\) 118.57 m/s |
Number of CCF files Total |
6 |
Number of CCF passed QC |
6 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2019-02-16 11:21:31.090 |
Last ccf file [Mid exposure] |
2019-02-16 15:22:28.575 |
Last processed [ccf] |
2025-02-23 21:16:14.284 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:47:15.060 |
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.