BDP31_3330 (spirou_offline_udem)

This page was last modified: 2026-02-12 19:23:01.822944 (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=BDP31_3330

Target Information

RA

280.2291167 [deg] (Gaia EDR3)

Dec

31.52936146 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

4860.0 [K] (2021AJ….161..134H)

Spectral Type

K2.5V (2003AJ….126.2048G)

Proper Motion (RA)

84.60750164 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-836.9079322 [mas/yr] (Gaia EDR3)

Parallax

41.74509729 [mas/yr] (Gaia EDR3)

Radial Velocity

28.5 [mas/yr] (2018yCat.1345….0G)

Aliases

LHS 3401, ** HJ 1337A, ADS 11576 A, AG+31 1670, ASCC 604683, BD+31 3330, CCDM J18409+3132A, Ci 18 2450, Ci 20 1103, CSI+31 3330 3, CSI+31 3330 1, GCRV 11135, GEN# +0.03103330A, G 206-38, HIC 91605, HIP 91605, IDS 18371+3128 A, LFT 1425, LSPM J1840+3131N, LTT 15508, 2MASS J18405487+3132004, NLTT 46857, PLX 4314, PPM 81646, SPOCS 2979, TIC 68340481, TYC 2637-1534-1, UBV 15893, UBV 15895, UBV M 2228, USNO-B1.0 1215-00298048, uvby98 003103330, WDS J18409+3132A, WEB 15753, Gaia DR2 2090051761936884864, Gaia EDR3 2090051761936884864, LHS3401, **HJ1337A, ADS11576A, AG+311670, ASCC604683, BD+313330, CCDMJ18409+3132A, Ci182450, Ci201103, CSI+3133303, CSI+3133301, GCRV11135, GEN#+0.03103330A, G206-38, HIC91605, HIP91605, IDS18371+3128A, LFT1425, LSPMJ1840+3131N, LTT15508, 2MASSJ18405487+3132004, NLTT46857, PLX4314, PPM81646, SPOCS2979, TIC68340481, TYC2637-1534-1, UBV15893, UBV15895, UBVM2228, USNO-B1.01215-00298048, uvby98003103330, WDSJ18409+3132A, WEB15753, GaiaDR22090051761936884864, GaiaEDR32090051761936884864

OBJECT name(s) in headers

BD+31 3330, BD+31 3330

PI name(s) in headers

Ryan Cloutier

Project/Run name(s) in headers

21AC33, 22AC25, 22BC27

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_BDP31_3330_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

28965.08 \(\pm\) 20.03 m/s

CCF FWHM

7713.35 \(\pm\) 296.08 m/s

Number of CCF files Total

5

Number of CCF passed QC

5

Number CCF files failed QC

0

First ccf file [Mid exposure]

2021-03-04 15:27:16.456

Last ccf file [Mid exposure]

2022-11-09 04:16:54.721

Last processed [ccf]

2025-02-23 18:31:29.053

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_BDP31_3330_spirou_offline_udem_file_list.txt

2026-02-12 19:23:05.102

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_BDP31_3330_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_BDP31_3330_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_BDP31_3330_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_BDP31_3330_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_BDP31_3330_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.