59PEG (spirou_offline_udem)

This page was last modified: 2026-02-12 19:23:22.350094 (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=59PEG

Target Information

RA

347.9340914 [deg] (Gaia DR2)

Dec

8.72009375 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

8395.0 [K] (2012A&A…537A.120Z)

Spectral Type

A5Vn (None)

Proper Motion (RA)

-7.742445696 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-4.523715991 [mas/yr] (Gaia DR2)

Parallax

13.09191222 [mas/yr] (Gaia DR2)

Radial Velocity

10.6 [mas/yr] (2006AstL…32..759G)

Aliases

* 59 Peg, 2MASS J23114419+0843122, AG+08 3201, BD+07 4991, FK5 1606, GC 32302, GCRV 14557, GEN# +1.00218918, GSC 01161-01795, Gaia DR2 2665976777193321600, HD 218918, HIC 114520, HIP 114520, HR 8826, IRAS 23092+0827, N30 5100, PLX 5612, PLX 5612.00, PMC 90-93 1142, PPM 173843, ROT 3376, SAO 128022, SKY# 43996, TD1 29684, TIC 402934237, TYC 1161-1795-1, UBV 19847, UBV M 26884, WEB 20323, YZ 8 11552, uvby98 100218918, * 59 Peg, 59PEG, 59Peg, BD+07 4991, HR 8826, PMC 90-93 1142, ROT 3376, UBV 19847, UBV M 26884, YZ 8 11552, *59Peg, 2MASSJ23114419+0843122, AG+083201, BD+074991, FK51606, GC32302, GCRV14557, GEN#+1.00218918, GSC01161-01795, GaiaDR22665976777193321600, HD218918, HIC114520, HIP114520, HR8826, IRAS23092+0827, N305100, PLX5612, PLX5612.00, PMC90-931142, PPM173843, ROT3376, SAO128022, SKY#43996, TD129684, TIC402934237, TYC1161-1795-1, UBV19847, UBVM26884, WEB20323, YZ811552, uvby98100218918, *59Peg, 59PEG, 59Peg, BD+074991, HR8826, PMC90-931142, ROT3376, UBV19847, UBVM26884, YZ811552

OBJECT name(s) in headers

59Peg

PI name(s) in headers

QSO Team, Claire Moutou, Matt Wilson

Project/Run name(s) in headers

25BQ58, 25AQ58, 20AQ58, 20BQ58, 21AQ58, 21BQ58, 22AQ58, 22BQ58, 23AQ58, 23BQ58, 24AQ58, 24BQ58, 18BE93, 19AQ58, 19BQ58

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_59PEG_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

299611.41 \(\pm\) 4051.92 m/s

CCF FWHM

7248.08 \(\pm\) 84334.08 m/s

Number of CCF files Total

66

Number of CCF passed QC

66

Number CCF files failed QC

0

First ccf file [Mid exposure]

2018-09-22 12:16:26.271

Last ccf file [Mid exposure]

2025-11-25 04:52:23.216

Last processed [ccf]

2026-01-07 12:10:13.699

Version [ccf]

0.7.294,0.7.292,0.7.295,0.7.293

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_59PEG_spirou_offline_udem_file_list.txt

2026-02-12 19:23:41.992

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_59PEG_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_59PEG_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_59PEG_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_59PEG_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_59PEG_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.