GL102 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:15:14.142438 (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=GL102

Target Information

RA

38.40512931 [deg] (Gaia DR2)

Dec

24.92422568 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

3335.0 [K] (2021A&A…656A.162M)

Spectral Type

M3.5Ve (2015AJ….149..106D)

Proper Motion (RA)

48.81816802 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-676.1670258 [mas/yr] (Gaia DR2)

Parallax

100.2834518 [mas/yr] (Gaia DR2)

Radial Velocity

-6.21 [mas/yr] (2018MNRAS.475.1960F)

Aliases

UCAC4 575-005505, CSI+24-02307, GALEX 6403346950463161832, GEN# +6.10010102, G 36-24, GJ 102, JP11 5108, Karmn J02336+249, LFT 215, LHS 1417, L 1305-10, LP 354-46, LSPM J0233+2455, LTT 10844, 2MASS J02333717+2455392, NLTT 8312, PLX 514, PLX 514.00, PM 02307+2443, PM J02336+2455, RX J0233.6+2455, 1RXS J023336.5+245549, TIC 22750743, USNO-B1.0 1149-00029723, USNO 408, WISEA J023337.21+245530.5, Zkh 42, [GKL99] 67, [RHG95] 453, [ZEH2003] RX J0233.6+2455 3, Gaia DR3 102162639019033600, Gaia DR2 102162639019033600, GL102, GL_102, UCAC4575-005505, CSI+24-02307, GALEX6403346950463161832, GEN#+6.10010102, G36-24, GJ102, JP115108, KarmnJ02336+249, LFT215, LHS1417, L1305-10, LP354-46, LSPMJ0233+2455, LTT10844, 2MASSJ02333717+2455392, NLTT8312, PLX514, PLX514.00, PM02307+2443, PMJ02336+2455, RXJ0233.6+2455, 1RXSJ023336.5+245549, TIC22750743, USNO-B1.01149-00029723, USNO408, WISEAJ023337.21+245530.5, Zkh42, [GKL99]67, [RHG95]453, [ZEH2003]RXJ0233.6+24553, GaiaDR3102162639019033600, GaiaDR2102162639019033600, GL 102, GL102

OBJECT name(s) in headers

Gl102

PI name(s) in headers

Etienne Artigau, Jean-Francois Donati

Project/Run name(s) in headers

24BC12, 22BP45, 23AP45, 23BP45, 24AP45

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_GL102_spirou_offline_udem.png

CCF stats

Mask used

GL699_neg.fits

CCF systemic velocity

-5975.87 \(\pm\) 16.34 m/s

CCF FWHM

6733.28 \(\pm\) 58.77 m/s

Number of CCF files Total

519

Number of CCF passed QC

519

Number CCF files failed QC

0

First ccf file [Mid exposure]

2022-11-02 12:12:50.380

Last ccf file [Mid exposure]

2024-12-23 08:21:56.304

Last processed [ccf]

2025-02-23 16:23:50.632

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_GL102_spirou_offline_udem_file_list.txt

2026-02-12 20:16:07.149

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_GL102_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_GL102_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_GL102_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_GL102_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_GL102_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.