82UMA (spirou_offline_udem)

This page was last modified: 2026-02-12 19:23:20.477857 (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=82UMA

Target Information

RA

204.8758943 [deg] (Gaia DR2)

Dec

52.92144831 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

8710.0 [K] (2012A&A…537A.120Z)

Spectral Type

A2Vnp (1995ApJS…99..135A)

Proper Motion (RA)

-136.3774617 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

56.0585155 [mas/yr] (Gaia DR2)

Parallax

19.05762478 [mas/yr] (Gaia DR2)

Radial Velocity

-17.1 [mas/yr] (2006AstL…32..759G)

Aliases

* 82 UMa, 2MASS J13393044+5255164, AG+53 912, BD+53 1640, GC 18473, GCRV 8077, GEN# +1.00119024, GSC 03851-00126, Gaia DR2 1560127186438933760, HD 119024, HIC 66634, HIP 66634, HR 5142, IRAS 13375+5310, PLX 3123, PLX 3123.00, PPM 34131, ROT 1984, SAO 28832, SKY# 25105, TD1 16984, TIC 286945730, TYC 3851-126-1, UBV 12241, UBV M 19616, WEB 11754, WISE J133930.29+525517.0, WISEA J133930.27+525516.9, YZ 53 4333, uvby98 100119024, * 82 UMa, 82UMA, 82UMa, AG+53 912, BD+53 1640, GCRV 8077, HIC 66634, HIP 66634, HR 5142, PPM 34131, ROT 1984, SAO 28832, UBV 12241, UBV M 19616, YZ 53 4333, *82UMa, 2MASSJ13393044+5255164, AG+53912, BD+531640, GC18473, GCRV8077, GEN#+1.00119024, GSC03851-00126, GaiaDR21560127186438933760, HD119024, HIC66634, HIP66634, HR5142, IRAS13375+5310, PLX3123, PLX3123.00, PPM34131, ROT1984, SAO28832, SKY#25105, TD116984, TIC286945730, TYC3851-126-1, UBV12241, UBVM19616, WEB11754, WISEJ133930.29+525517.0, WISEAJ133930.27+525516.9, YZ534333, uvby98100119024, *82UMa, 82UMA, 82UMa, AG+53912, BD+531640, GCRV8077, HIC66634, HIP66634, HR5142, PPM34131, ROT1984, SAO28832, UBV12241, UBVM19616, YZ534333

OBJECT name(s) in headers

82UMa

PI name(s) in headers

QSO Team

Project/Run name(s) in headers

25BQ58, 25AQ58, 20BQ58, 21AQ58, 21BQ58, 22AQ58, 22BQ58, 23AQ58, 23BQ58, 24AQ58, 24BQ58, 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_82UMA_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

298213.22 \(\pm\) 4172.33 m/s

CCF FWHM

4855.40 \(\pm\) 81213.62 m/s

Number of CCF files Total

57

Number of CCF passed QC

57

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-04-16 14:13:52.994

Last ccf file [Mid exposure]

2025-09-08 05:02:35.733

Last processed [ccf]

2025-11-04 18:08:32.162

Version [ccf]

0.7.294,0.7.292,0.7.293

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_82UMA_spirou_offline_udem_file_list.txt

2026-02-12 19:23:37.011

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_82UMA_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_82UMA_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_82UMA_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_82UMA_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_82UMA_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.