GL581 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:25:11.077333 (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=GL581

Target Information

RA

229.8564725 [deg] (Gaia DR2)

Dec

-7.722693495 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

3470.0 [K] (via spdrs@apikipiha)

Spectral Type

M3V (1986AJ…..92..139S)

Proper Motion (RA)

-1221.466595 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-97.12948413 [mas/yr] (Gaia DR2)

Parallax

158.7491998 [mas/yr] (Gaia DR2)

Radial Velocity

-9.24 [mas/yr] (2018MNRAS.475.1960F)

Aliases

BD-07 4003, Ci 20 923, DENIS J151926.8-074319, GCRV 8863, GEN# -0.00704003, GES J15192557-0743217, G 151-46, G 152-9, GJ 581, GSC 05594-00593, HIC 74995, HIP 74995, JP11 273, Karmn J15194-077, LFT 1195, LHS 394, LPM 564, LTT 6112, 2MASS J15192689-0743200, MCC 159, NLTT 39886, NSV 7023, 8pc 159.52, PLX 3458, PLX 3458.00, PM J15194-0743E, StKM 2-1135, TIC 36853511, TYC 5594-1093-1, UBV 13194, UBV M 5243, UCAC2 29110263, UCAC3 165-136246, UCAC4 412-059591, V* HO Lib, WEB 12795, WISEA J151925.96-074321.2, Wolf 562, Zkh 217, [RHG95] 2420, Gaia DR3 6322070093095493504, Gaia DR2 6322070093095493504, Gaia DR1 6322069882641960448, BD-074003, Ci20923, DENISJ151926.8-074319, GCRV8863, GEN#-0.00704003, GESJ15192557-0743217, G151-46, G152-9, GJ581, GSC05594-00593, HIC74995, HIP74995, JP11273, KarmnJ15194-077, LFT1195, LHS394, LPM564, LTT6112, 2MASSJ15192689-0743200, MCC159, NLTT39886, NSV7023, 8pc159.52, PLX3458, PLX3458.00, PMJ15194-0743E, StKM2-1135, TIC36853511, TYC5594-1093-1, UBV13194, UBVM5243, UCAC229110263, UCAC3165-136246, UCAC4412-059591, V*HOLib, WEB12795, WISEAJ151925.96-074321.2, Wolf562, Zkh217, [RHG95]2420, GaiaDR36322070093095493504, GaiaDR26322070093095493504, GaiaDR16322069882641960448

OBJECT name(s) in headers

Gl581

PI name(s) in headers

Jean-Francois Donati

Project/Run name(s) in headers

19AP40, 19BP40

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_GL581_spirou_offline_udem.png

CCF stats

Mask used

GL699_neg.fits

CCF systemic velocity

-9080.41 \(\pm\) 15.04 m/s

CCF FWHM

5310.69 \(\pm\) 29.25 m/s

Number of CCF files Total

120

Number of CCF passed QC

120

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-02-14 15:46:23.325

Last ccf file [Mid exposure]

2020-01-28 16:04:24.278

Last processed [ccf]

2025-02-23 21:16:50.585

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_GL581_spirou_offline_udem_file_list.txt

2026-02-12 20:25:32.560

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_GL581_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_GL581_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_GL581_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_GL581_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_GL581_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.