HR875 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:48:07.184284 (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=HR875

Target Information

RA

44.15577748 [deg] (Gaia DR2)

Dec

-3.712512725 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

8770.0 [K] (2012A&A…537A.120Z)

Spectral Type

A1V (1999MSS…C05….0H)

Proper Motion (RA)

-37.17858954 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-44.45703519 [mas/yr] (Gaia DR2)

Parallax

15.64871323 [mas/yr] (Gaia DR2)

Radial Velocity

-10.7 [mas/yr] (2006AstL…32..759G)

Aliases

2MASS J02563742-0342444, BD-04 502, FK5 1080, GC 3541, GCRV 1639, GEN# +1.00018331, GSC 04703-01166, Gaia DR2 5186208817062871168, HD 18331, HIC 13717, HIP 13717, HR 875, IRAS 02541-0354, JP11 721, N30 603, PLX 612, PLX 612.00, PMC 90-93 712, PPM 185207, ROT 394, SAO 130199, SKY# 4420, TD1 1781, TIC 439876264, TYC 4703-1166-1, UBV 2858, UBV M 9239, WEB 2720, YZ 93 704, uvby98 100018331, BD-04 502, GC 3541, GCRV 1639, HD 18331, HIC 13717, HIP 13717, HR 875, HR875, JP11 721, N30 603, PLX 612, PLX 612.00, PMC 90-93 712, ROT 394, SKY# 4420, TD1 1781, UBV 2858, UBV M 9239, WEB 2720, YZ 93 704, 2MASSJ02563742-0342444, BD-04502, FK51080, GC3541, GCRV1639, GEN#+1.00018331, GSC04703-01166, GaiaDR25186208817062871168, HD18331, HIC13717, HIP13717, HR875, IRAS02541-0354, JP11721, N30603, PLX612, PLX612.00, PMC90-93712, PPM185207, ROT394, SAO130199, SKY#4420, TD11781, TIC439876264, TYC4703-1166-1, UBV2858, UBVM9239, WEB2720, YZ93704, uvby98100018331, BD-04502, GC3541, GCRV1639, HD18331, HIC13717, HIP13717, HR875, HR875, JP11721, N30603, PLX612, PLX612.00, PMC90-93712, ROT394, SKY#4420, TD11781, UBV2858, UBVM9239, WEB2720, YZ93704

OBJECT name(s) in headers

HR875

PI name(s) in headers

QSO Team, Claire Moutou, Matt Wilson

Project/Run name(s) in headers

25BQ58, 25AQ58, 20AQ58, 20BQ58, 21AQ58, 21BQ58, 22BQ58, 23BQ58, 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_HR875_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

298361.68 \(\pm\) 4301.05 m/s

CCF FWHM

4236.79 \(\pm\) 83312.68 m/s

Number of CCF files Total

61

Number of CCF passed QC

61

Number CCF files failed QC

0

First ccf file [Mid exposure]

2018-09-25 13:03:32.639

Last ccf file [Mid exposure]

2025-12-02 04:32:09.648

Last processed [ccf]

2026-01-07 12:17:14.083

Version [ccf]

0.7.295,0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HR875_spirou_offline_udem_file_list.txt

2026-02-12 20:48:17.818

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_HR875_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_HR875_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HR875_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HR875_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_HR875_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.