51_PEG (spirou_offline_udem)¶
This page was last modified: 2026-02-12 19:21:39.082546 (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=51_PEG
Target Information |
|
|---|---|
RA |
344.3675399 [deg] (Gaia DR2) |
Dec |
20.76909575 [deg] (Gaia DR2) |
Finder chart |
|
Teff |
5780.0 [K] (2021AJ….161..134H) |
Spectral Type |
G2IV (1989ApJS…71..245K) |
Proper Motion (RA) |
207.3633663 [mas/yr] (Gaia DR2) |
Proper Motion (Dec) |
62.09404537 [mas/yr] (Gaia DR2) |
Parallax |
64.648808 [mas/yr] (Gaia DR2) |
Radial Velocity |
-33.165 [mas/yr] (2018A&A…616A…7S) |
Aliases |
* 51 Peg, ** RBR 21A, 2MASS J22572795+2046077, AG+20 2595, AKARI-IRC-V1 J2257280+204608, ASCC 826013, BD+19 5036, CSV 102222, GC 32003, GCRV 14411, GEN# +1.00217014, GJ 882, Gaia DR2 2835207319109249920, HD 217014, HIC 113357, HIP 113357, HR 8729, IRAS 22550+2030, JP11 3558, LSPM J2257+2046, LTT 16750, N30 5052, NAME Helvetios, NLTT 55385, NSV 14374, PLX 5568, PLX 5568.00, PPM 114985, ROT 3341, SAO 90896, SKY# 43603, SPOCS 990, TD1 29480, TIC 139298196, TYC 1717-2193-1, UBV 19678, UBV M 26734, USNO-B1.0 1107-00589893, WDS J22575+2046A, WEB 20165, YPAC 218, YZ 0 1227, YZ 20 9382, uvby98 100217014, * 51 Peg, ** RBR 21A, 51_PEG, ASCC 826013, BD+19 5036, GJ 882, HR 8729, JP11 3558, ROT 3341, SAO 90896, SPOCS 990, UBV 19678, UBV M 26734, YZ 0 1227, YZ 20 9382, *51Peg, **RBR21A, 2MASSJ22572795+2046077, AG+202595, AKARI-IRC-V1J2257280+204608, ASCC826013, BD+195036, CSV102222, GC32003, GCRV14411, GEN#+1.00217014, GJ882, GaiaDR22835207319109249920, HD217014, HIC113357, HIP113357, HR8729, IRAS22550+2030, JP113558, LSPMJ2257+2046, LTT16750, N305052, NAMEHelvetios, NLTT55385, NSV14374, PLX5568, PLX5568.00, PPM114985, ROT3341, SAO90896, SKY#43603, SPOCS990, TD129480, TIC139298196, TYC1717-2193-1, UBV19678, UBVM26734, USNO-B1.01107-00589893, WDSJ22575+2046A, WEB20165, YPAC218, YZ01227, YZ209382, uvby98100217014, *51Peg, **RBR21A, 51PEG, ASCC826013, BD+195036, GJ882, HR8729, JP113558, ROT3341, SAO90896, SPOCS990, UBV19678, UBVM26734, YZ01227, YZ209382 |
OBJECT name(s) in headers |
|
PI name(s) in headers |
Stefan Pelletier |
Project/Run name(s) in headers |
20BC35 |
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 |
-32485.67 \(\pm\) 31.07 m/s |
CCF FWHM |
8709.41 \(\pm\) 55.68 m/s |
Number of CCF files Total |
220 |
Number of CCF passed QC |
220 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2020-09-03 05:50:48.510 |
Last ccf file [Mid exposure] |
2020-10-03 12:40:54.625 |
Last processed [ccf] |
2025-02-23 19:20:56.309 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 19:22:03.234 |
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.