4PEG (spirou_offline_udem)

This page was last modified: 2026-02-12 19:20:37.472056 (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=4PEG

Target Information

RA

324.633576 [deg] (Gaia DR2)

Dec

5.771869825 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

7379.0 [K] (2012A&A…537A.120Z)

Spectral Type

A9IV-Vn (None)

Proper Motion (RA)

113.8042896 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

29.52553461 [mas/yr] (Gaia DR2)

Parallax

18.88041621 [mas/yr] (Gaia DR2)

Radial Velocity

-18.5 [mas/yr] (1953GCRV..C……0W)

Aliases

* 4 Peg, 2MASS J21383194+0546183, ADS 15157 A, AG+05 3164, BD+05 4834, BD+05 4834A, CCDM J21385+0546A, CSI+05 4834 1, GC 30291, GCRV 13595, GEN# +1.00205924, GSC 00555-01662, Gaia DR2 2698772632069758464, HD 205924, HIC 106856, HIP 106856, HR 8270, IDS 21335+0519 A, PLX 5216, PLX 5216.00, PPM 172049, Renson 57330, SAO 126956, SKY# 41263, TD1 28314, TIC 353103358, TYC 555-1662-1, UBV 18595, UBV M 25834, WDS J21385+0546A, WEB 19314, YZ 0 2250, YZ 5 10855, uvby98 100205924, * 4 Peg, 4PEG, 4Peg, BD+05 4834, BD+05 4834A, CSI+05 4834 1, HR 8270, TYC 555-1662-1, UBV 18595, UBV M 25834, YZ 0 2250, YZ 5 10855, *4Peg, 2MASSJ21383194+0546183, ADS15157A, AG+053164, BD+054834, BD+054834A, CCDMJ21385+0546A, CSI+0548341, GC30291, GCRV13595, GEN#+1.00205924, GSC00555-01662, GaiaDR22698772632069758464, HD205924, HIC106856, HIP106856, HR8270, IDS21335+0519A, PLX5216, PLX5216.00, PPM172049, Renson57330, SAO126956, SKY#41263, TD128314, TIC353103358, TYC555-1662-1, UBV18595, UBVM25834, WDSJ21385+0546A, WEB19314, YZ02250, YZ510855, uvby98100205924, *4Peg, 4PEG, 4Peg, BD+054834, BD+054834A, CSI+0548341, HR8270, TYC555-1662-1, UBV18595, UBVM25834, YZ02250, YZ510855

OBJECT name(s) in headers

4Peg

PI name(s) in headers

Claire Moutou

Project/Run name(s) in headers

18BE96

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.

../../../_images/ccf_plot_4PEG_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

295517.85 \(\pm\) 630.38 m/s

CCF FWHM

6773.91 \(\pm\) 1648.58 m/s

Number of CCF files Total

2

Number of CCF passed QC

2

Number CCF files failed QC

0

First ccf file [Mid exposure]

2018-09-23 08:23:28.133

Last ccf file [Mid exposure]

2018-10-26 05:32:08.035

Last processed [ccf]

2025-02-23 21:24:17.612

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_4PEG_spirou_offline_udem_file_list.txt

2026-02-12 19:20:39.739

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

../../../_images/debug_tcorr_map_plot_4PEG_spirou_offline_udem.png

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

../../../_images/debug_extsmax_plot_4PEG_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_4PEG_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_4PEG_spirou_offline_udem.png

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

../../../_images/debug_mjd_cdt_plot_4PEG_spirou_offline_udem.png

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.