J20412815P5725473 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:48:09.811461 (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=J20412815P5725473

Target Information

RA

310.3681187 [deg] (Gaia DR2)

Dec

57.43068272 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

3950.0 [K] (2014MNRAS.443.2561G)

Spectral Type

M1V (1986AJ…..92..139S)

Proper Motion (RA)

97.73999574 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

205.7094339 [mas/yr] (Gaia DR2)

Parallax

40.30385735 [mas/yr] (Gaia DR2)

Radial Velocity

-24.14 [mas/yr] (2018yCat.1345….0G)

Aliases

1RXS J204127.8+572545, 2MASS J20412815+5725473, ASAS J204128+5725.8, ASCC 209401, BD+56 2471, GCRV 12976, GEN# +0.05602471, GJ 4156, Gaia DR1 2187263154059233152, Gaia DR2 2187263158355763072, HIC 102101, HIP 102101, LSPM J2041+5725, LTT 16050, MCC 68, NLTT 49738, PLX 4940, PLX 4940.00, PM J20414+5725, StKM 2-1466, TIC 277317887, TYC 3959-428-1, UCAC4 738-070357, USNO-B1.0 1474-00394961, VVO 294, WEB 18468, Wolf 1080, [FS2003] 1086, [RHG95] 3236, ASCC 209401, BD+56 2471, GJ 4156, J20412815+5725473, J20412815P5725473, [RHG95] 3236, Gaia EDR3 2187263158355763072, 1RXSJ204127.8+572545, 2MASSJ20412815+5725473, ASASJ204128+5725.8, ASCC209401, BD+562471, GCRV12976, GEN#+0.05602471, GJ4156, GaiaDR12187263154059233152, GaiaDR22187263158355763072, HIC102101, HIP102101, LSPMJ2041+5725, LTT16050, MCC68, NLTT49738, PLX4940, PLX4940.00, PMJ20414+5725, StKM2-1466, TIC277317887, TYC3959-428-1, UCAC4738-070357, USNO-B1.01474-00394961, VVO294, WEB18468, Wolf1080, [FS2003]1086, [RHG95]3236, ASCC209401, BD+562471, GJ4156, J20412815+5725473, J20412815P5725473, [RHG95]3236, GaiaEDR3 2187263158355763072

OBJECT name(s) in headers

J20412815+5725473

PI name(s) in headers

Ryan Cloutier

Project/Run name(s) in headers

19BC25

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_J20412815P5725473_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-23545.00 \(\pm\) 16.57 m/s

CCF FWHM

7732.12 \(\pm\) 126.97 m/s

Number of CCF files Total

88

Number of CCF passed QC

88

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-09-18 08:17:02.816

Last ccf file [Mid exposure]

2019-11-09 05:51:25.167

Last processed [ccf]

2025-02-23 20:53:32.622

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_J20412815P5725473_spirou_offline_udem_file_list.txt

2026-02-12 20:48:24.360

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_J20412815P5725473_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_J20412815P5725473_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_J20412815P5725473_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_J20412815P5725473_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_J20412815P5725473_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.