22_LYN (spirou_offline_udem)¶
This page was last modified: 2026-02-12 19:19:30.396039 (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=22_LYN
Target Information |
|
|---|---|
RA |
112.4838937 [deg] (Gaia DR2) |
Dec |
49.67210255 [deg] (Gaia DR2) |
Finder chart |
|
Teff |
6395.0 [K] (2017AJ….153…21L) |
Spectral Type |
F6V (2001AJ….121.2148G) |
Proper Motion (RA) |
111.2693196 [mas/yr] (Gaia DR2) |
Proper Motion (Dec) |
-83.38069729 [mas/yr] (Gaia DR2) |
Parallax |
49.0287311 [mas/yr] (Gaia DR2) |
Radial Velocity |
-27.389 [mas/yr] (2018A&A…616A…7S) |
Aliases |
* 22 Lyn, ** ENG 31A, 2MASS J07295595+4940207, AG+49 752, AKARI-IRC-V1 J0729560+494020, BD+49 1630, CCDM J07299+4941A, CSI+49 1630 1, GC 9992, GCRV 4976, GEN# +1.00058855, GJ 9234, GSC 03401-01647, Gaia DR2 976893923544104576, HD 58855, HIC 36439, HIP 36439, HR 2849, IDS 07223+4952 A, IRAS 07262+4946, PLX 1757, PLX 1757.00, PPM 49904, ROT 1204, SAO 41808, SKY# 13715, TD1 10148, TIC 328324648, TYC 3401-1647-1, UBV 7210, UBV M 13284, WDS J07299+4940A, WEB 7251, YPAC 448, YZ 49 2861, uvby98 100058855, (F) 22 Lyn, * 22 Lyn, ** ENG 31A, 22 Lyn, 22_LYN, AG+49 752, BD+49 1630, CSI+49 1630 1, GC 9992, GCRV 4976, GJ 9234, HD 58855, HIC 36439, HIP 36439, HR 2849, PPM 49904, ROT 1204, SAO 41808, UBV 7210, UBV M 13284, WEB 7251, YZ 49 2861, *22Lyn, **ENG31A, 2MASSJ07295595+4940207, AG+49752, AKARI-IRC-V1J0729560+494020, BD+491630, CCDMJ07299+4941A, CSI+4916301, GC9992, GCRV4976, GEN#+1.00058855, GJ9234, GSC03401-01647, GaiaDR2976893923544104576, HD58855, HIC36439, HIP36439, HR2849, IDS07223+4952A, IRAS07262+4946, PLX1757, PLX1757.00, PPM49904, ROT1204, SAO41808, SKY#13715, TD110148, TIC328324648, TYC3401-1647-1, UBV7210, UBVM13284, WDSJ07299+4940A, WEB7251, YPAC448, YZ492861, uvby98100058855, (F)22Lyn, *22Lyn, **ENG31A, 22Lyn, 22LYN, AG+49752, BD+491630, CSI+4916301, GC9992, GCRV4976, GJ9234, HD58855, HIC36439, HIP36439, HR2849, PPM49904, ROT1204, SAO41808, UBV7210, UBVM13284, WEB7251, YZ492861 |
OBJECT name(s) in headers |
|
PI name(s) in headers |
QSO Team |
Project/Run name(s) in headers |
19BQ54 |
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 |
-26591.34 \(\pm\) 81.89 m/s |
CCF FWHM |
13682.66 \(\pm\) 54.94 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] |
2020-01-28 10:56:48.124 |
Last ccf file [Mid exposure] |
2020-01-28 11:00:20.322 |
Last processed [ccf] |
2025-02-23 20:16:30.054 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 19:19:32.993 |
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.