HR4687 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:47:24.514959 (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=HR4687

Target Information

RA

184.7076767 [deg] (Gaia DR2)

Dec

75.16057808 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

8954.0 [K] (2012A&A…537A.120Z)

Spectral Type

A1V (None)

Proper Motion (RA)

-35.4143085 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

4.102765895 [mas/yr] (Gaia DR2)

Parallax

10.14064122 [mas/yr] (Gaia DR2)

Radial Velocity

-3.3 [mas/yr] (2006AstL…32..759G)

Aliases

2MASS J12184995+7509379, AG+75 540, BD+75 470, EXO 1216.6+7526, FK5 2986, GC 16797, GCRV 7379, GEN# +1.00107193, GSC 04550-02114, Gaia DR2 1692365552989740928, HD 107193, HIC 60044, HIP 60044, HR 4687, IRAS 12165+7526, PLX 2837, PLX 2837.00, PMC 90-93 1312, PPM 8128, Pul -3 930127, ROT 1805, SAO 7540, SKY# 23071, TD1 16203, TIC 154475006, TYC 4550-2114-1, UBV 11066, WEB 10672, uvby98 100107193, AG+75 540, BD+75 470, GCRV 7379, HIC 60044, HIP 60044, HR 4687, HR4687, PMC 90-93 1312, PPM 8128, Pul -3 930127, ROT 1805, SAO 7540, UBV 11066, 2MASSJ12184995+7509379, AG+75540, BD+75470, EXO1216.6+7526, FK52986, GC16797, GCRV7379, GEN#+1.00107193, GSC04550-02114, GaiaDR21692365552989740928, HD107193, HIC60044, HIP60044, HR4687, IRAS12165+7526, PLX2837, PLX2837.00, PMC90-931312, PPM8128, Pul-3930127, ROT1805, SAO7540, SKY#23071, TD116203, TIC154475006, TYC4550-2114-1, UBV11066, WEB10672, uvby98100107193, AG+75540, BD+75470, GCRV7379, HIC60044, HIP60044, HR4687, HR4687, PMC90-931312, PPM8128, Pul-3930127, ROT1805, SAO7540, UBV11066

OBJECT name(s) in headers

HR4687

PI name(s) in headers

QSO Team

Project/Run name(s) in headers

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

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_HR4687_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

297571.41 \(\pm\) 299925.67 m/s

CCF FWHM

8697.54 \(\pm\) 87763.11 m/s

Number of CCF files Total

65

Number of CCF passed QC

65

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-04-22 10:36:35.744

Last ccf file [Mid exposure]

2025-07-16 05:49:17.225

Last processed [ccf]

2025-07-27 10:52:03.682

Version [ccf]

0.7.292,0.7.293

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HR4687_spirou_offline_udem_file_list.txt

2026-02-12 20:47:37.905

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_HR4687_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_HR4687_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HR4687_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HR4687_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_HR4687_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.