HD286955 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:46:36.115863 (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=HD286955

Target Information

RA

69.92746823 [deg] (Gaia EDR3)

Dec

9.870399108 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

4850.0 [K] (2018MNRAS.479.1332M)

Spectral Type

K3 (1985ApJS…59..197B)

Proper Motion (RA)

-14.95725304 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-375.9123752 [mas/yr] (Gaia EDR3)

Parallax

32.99860209 [mas/yr] (Gaia EDR3)

Radial Velocity

-27.57 [mas/yr] (2018A&A…619A..81H)

Aliases

HD 286955, ** GIC 51A, ** HDS 601, AG+09 434, ASCC 2498588, BD+09 621A, CCDM J04397+0952AC, Ci 18 601, GCRV 55300, G 83-28, GJ 9162 A, GJ 173.1 A, HIC 21710, HIP 21710, IDS 04343+0941 A, LSPM J0439+0952, LTT 11478, 2MASS J04394259+0952194, MCC 451, NLTT 13705, PLX 1030, PPM 147791, SAO 111962, SBC9 3620, TIC 373209819, Tou 668, TYC 686-1084-1, UBV M 28949, UCAC2 35148703, UGP 86, USNO-B1.0 0998-00055510, WDS J04397+0952A, WDS J04397+0952Aa,Ab, WEB 4173, WISEA J043942.59+095215.6, YZC 22 1724, YZ 9 1724, Gaia EDR3 3293515101648626816, Gaia DR2 3293515101646468352, HD286955, **GIC51A, **HDS601, AG+09434, ASCC2498588, BD+09621A, CCDMJ04397+0952AC, Ci18601, GCRV55300, G83-28, GJ9162A, GJ173.1A, HIC21710, HIP21710, IDS04343+0941A, LSPMJ0439+0952, LTT11478, 2MASSJ04394259+0952194, MCC451, NLTT13705, PLX1030, PPM147791, SAO111962, SBC93620, TIC373209819, Tou668, TYC686-1084-1, UBVM28949, UCAC235148703, UGP86, USNO-B1.00998-00055510, WDSJ04397+0952A, WDSJ04397+0952Aa,Ab, WEB4173, WISEAJ043942.59+095215.6, YZC221724, YZ91724, GaiaEDR33293515101648626816, GaiaDR23293515101646468352

OBJECT name(s) in headers

HD 286955

PI name(s) in headers

Ryan Cloutier

Project/Run name(s) in headers

21BC28

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_HD286955_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-27621.59 \(\pm\) 0.00 m/s

CCF FWHM

7561.75 \(\pm\) 0.00 m/s

Number of CCF files Total

1

Number of CCF passed QC

1

Number CCF files failed QC

0

First ccf file [Mid exposure]

2021-10-18 15:40:11.792

Last ccf file [Mid exposure]

2021-10-18 15:40:11.792

Last processed [ccf]

2025-02-23 17:23:52.281

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HD286955_spirou_offline_udem_file_list.txt

2026-02-12 20:46:37.878

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_HD286955_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_HD286955_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD286955_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD286955_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_HD286955_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.