33LYN (spirou_offline_udem)

This page was last modified: 2026-02-12 19:20:58.995253 (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=33LYN

Target Information

RA

128.6827139 [deg] (Gaia DR2)

Dec

36.41944482 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

8840.0 [K] (HEADER[CFHT])

Spectral Type

A2Vnn (None)

Proper Motion (RA)

-26.11661601 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-40.89996874 [mas/yr] (Gaia DR2)

Parallax

9.995273104 [mas/yr] (Gaia DR2)

Radial Velocity

24.9 [mas/yr] (1953GCRV..C……0W)

Aliases

* 33 Lyn, 2MASS J08344388+3625107, AG+36 857, BD+36 1840, GC 11744, GCRV 5634, GEN# +1.00072524, GSC 02489-02141, Gaia DR2 909820931110880640, HD 72524, HIC 42090, HIP 42090, HR 3377, PPM 73821, Renson 20100, SAO 60907, SKY# 16381, TD1 12658, TIC 468449171, TYC 2489-2141-1, UBV 8134, UBV M 14440, WEB 8092, uvby98 100072524, * 33 Lyn, 33LYN, 33Lyn, AG+36 857, BD+36 1840, GCRV 5634, HD 72524, HIC 42090, HIP 42090, HR 3377, PPM 73821, SAO 60907, UBV 8134, UBV M 14440, WEB 8092, *33Lyn, 2MASSJ08344388+3625107, AG+36857, BD+361840, GC11744, GCRV5634, GEN#+1.00072524, GSC02489-02141, GaiaDR2909820931110880640, HD72524, HIC42090, HIP42090, HR3377, PPM73821, Renson20100, SAO60907, SKY#16381, TD112658, TIC468449171, TYC2489-2141-1, UBV8134, UBVM14440, WEB8092, uvby98100072524, *33Lyn, 33LYN, 33Lyn, AG+36857, BD+361840, GCRV5634, HD72524, HIC42090, HIP42090, HR3377, PPM73821, SAO60907, UBV8134, UBVM14440, WEB8092

OBJECT name(s) in headers

33Lyn

PI name(s) in headers

QSO Team, Matt Wilson

Project/Run name(s) in headers

25BQ58, 25AQ58, 20BQ58, 21BQ58, 22AQ58, 22BQ58, 23AQ58, 23BQ58, 24AQ58, 24BQ58, 18BE93, 19AQ58, 19BQ58, 20AQ58

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_33LYN_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

300000.00 \(\pm\) 5995.77 m/s

CCF FWHM

37856.35 \(\pm\) 97172.58 m/s

Number of CCF files Total

71

Number of CCF passed QC

71

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-01-18 08:04:37.197

Last ccf file [Mid exposure]

2025-11-03 15:53:54.112

Last processed [ccf]

2026-01-07 12:17:27.437

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_33LYN_spirou_offline_udem_file_list.txt

2026-02-12 19:21:14.462

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_33LYN_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_33LYN_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_33LYN_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_33LYN_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_33LYN_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.