HR8489 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:48:07.305464 (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=HR8489

Target Information

RA

333.6851299 [deg] (Gaia DR2)

Dec

42.95380836 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

8840.0 [K] (HEADER[CFHT])

Spectral Type

A2Vnn (None)

Proper Motion (RA)

48.4887784 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-20.49452327 [mas/yr] (Gaia DR2)

Parallax

12.22203034 [mas/yr] (Gaia DR2)

Radial Velocity

-30.7 [mas/yr] (2006AstL…32..759G)

Aliases

2MASS J22144436+4257141, AG+42 2150, BD+42 4333, FK5 3778, GC 31127, GCRV 13993, GEN# +1.00211211, GSC 03207-02263, Gaia DR1 1958476259155515008, Gaia DR2 1958476259155515008, HD 211211, HIC 109831, HIP 109831, HR 8489, N30 4903, PMC 90-93 1463, PPM 62681, ROT 3241, SAO 51797, SKY# 42399, TD1 28928, TIC 199128129, TYC 3207-2263-1, WEB 19726, uvby98 100211211, BD+42 4333, HR 8489, HR8489, PMC 90-93 1463, PPM 62681, ROT 3241, SAO 51797, 2MASSJ22144436+4257141, AG+422150, BD+424333, FK53778, GC31127, GCRV13993, GEN#+1.00211211, GSC03207-02263, GaiaDR11958476259155515008, GaiaDR21958476259155515008, HD211211, HIC109831, HIP109831, HR8489, N304903, PMC90-931463, PPM62681, ROT3241, SAO51797, SKY#42399, TD128928, TIC199128129, TYC3207-2263-1, WEB19726, uvby98100211211, BD+424333, HR8489, HR8489, PMC90-931463, PPM62681, ROT3241, SAO51797

OBJECT name(s) in headers

HR8489

PI name(s) in headers

QSO Team, Claire Moutou

Project/Run name(s) in headers

25BQ58, 25AQ58, 24BQ58, 20AQ58, 20BQ58, 21AQ58, 21BQ58, 22AQ58, 22BQ58, 23AQ58, 23BQ58, 24AQ58, 18BE93, 18BE96, 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_HR8489_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

299179.41 \(\pm\) 3142.16 m/s

CCF FWHM

4830.32 \(\pm\) 87290.12 m/s

Number of CCF files Total

62

Number of CCF passed QC

62

Number CCF files failed QC

0

First ccf file [Mid exposure]

2018-09-22 09:28:40.947

Last ccf file [Mid exposure]

2025-12-01 04:37:08.030

Last processed [ccf]

2026-01-07 12:05:42.173

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_HR8489_spirou_offline_udem_file_list.txt

2026-02-12 20:48:18.578

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_HR8489_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_HR8489_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HR8489_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HR8489_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_HR8489_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.