42_PEG (spirou_offline_udem)¶
This page was last modified: 2026-02-12 19:21:00.160969 (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=42_PEG
Target Information |
|
|---|---|
RA |
340.3658416 [deg] (Gaia DR2) |
Dec |
10.83131282 [deg] (Gaia DR2) |
Finder chart |
|
Teff |
11000.0 [K] (2016A&A…589A..83G) |
Spectral Type |
B8V (None) |
Proper Motion (RA) |
78.28356239 [mas/yr] (Gaia DR2) |
Proper Motion (Dec) |
-10.64426949 [mas/yr] (Gaia DR2) |
Parallax |
14.27774223 [mas/yr] (Gaia DR2) |
Radial Velocity |
6.1 [mas/yr] (2006AstL…32..759G) |
Aliases |
* 42 Peg, * zet Peg, 2MASS J22412773+1049526, ADS 16182 A, AG+10 3107, AKARI-IRC-V1 J2241277+104952, BD+10 4797, CCDM J22415+1050A, CSI+10 4797 1, FK5 855, GC 31664, GCRV 14247, GEN# +1.00214923, GSC 01155-02187, Gaia DR2 2717594072113581696, HD 214923, HIC 112029, HIP 112029, HR 8634, IDS 22365+1019 A, IRAS 22389+1034, JP11 3523, N30 4992, NAME Homam, PLX 5492, PLX 5492.00, PMC 90-93 602, PPM 141743, ROT 3307, SAO 108103, SKY# 43140, SRS 30855, TD1 29271, TIC 322187270, TYC 1155-2187-1, UBV 19416, UBV M 26553, UCAC3 202-315734, WDS J22415+1050A, WEB 19999, YZ 10 9059, uvby98 100214923, (B) HR 8634, * 42 Peg, 42_PEG, BD+10 4797, CSI+10 4797 1, FK5 855, HR 8634, JP11 3523, PMC 90-93 602, ROT 3307, SRS 30855, UBV 19416, UBV M 26553, YZ 10 9059, *42Peg, *zetPeg, 2MASSJ22412773+1049526, ADS16182A, AG+103107, AKARI-IRC-V1J2241277+104952, BD+104797, CCDMJ22415+1050A, CSI+1047971, FK5855, GC31664, GCRV14247, GEN#+1.00214923, GSC01155-02187, GaiaDR22717594072113581696, HD214923, HIC112029, HIP112029, HR8634, IDS22365+1019A, IRAS22389+1034, JP113523, N304992, NAMEHomam, PLX5492, PLX5492.00, PMC90-93602, PPM141743, ROT3307, SAO108103, SKY#43140, SRS30855, TD129271, TIC322187270, TYC1155-2187-1, UBV19416, UBVM26553, UCAC3202-315734, WDSJ22415+1050A, WEB19999, YZ109059, uvby98100214923, (B)HR8634, *42Peg, 42PEG, BD+104797, CSI+1047971, FK5855, HR8634, JP113523, PMC90-93602, ROT3307, SRS30855, UBV19416, UBVM26553, YZ109059 |
OBJECT name(s) in headers |
|
PI name(s) in headers |
Emily Deibert, Romain Allart, QSO Team |
Project/Run name(s) in headers |
20AC01, 21BC16, 24AC16, 20AQ54 |
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 |
300000.00 \(\pm\) 345.42 m/s |
CCF FWHM |
183543.38 \(\pm\) 97974.79 m/s |
Number of CCF files Total |
104 |
Number of CCF passed QC |
104 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2020-06-03 15:07:03.882 |
Last ccf file [Mid exposure] |
2024-06-25 14:50:28.882 |
Last processed [ccf] |
2025-02-23 19:59:45.102 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 19:21:21.765 |
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.