GJ1289 (spirou_offline_udem)

This page was last modified: 2026-02-12 19:51:45.027348 (UTC)

Back to the object table

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=GJ1289

Target Information

RA

355.7815092 [deg] (Gaia EDR3)

Dec

36.53631038 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

3238.0 [K] (2022MNRAS.516.3802C)

Spectral Type

M4.5V (2013AJ….145..102L)

Proper Motion (RA)

941.8406663 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-151.2715238 [mas/yr] (Gaia EDR3)

Parallax

119.5794052 [mas/yr] (Gaia EDR3)

Radial Velocity

-2.52 [mas/yr] (2018MNRAS.475.1960F)

Aliases

2MASS J23430628+3632132, CSI+36-23406, G 130-4, G 171-12, G 190-43, GALEX 6372217670673108177, GEN# +9.80130004, GJ 1289, Gaia DR2 2879455480941956736, Gaia EDR3 2879455480942629248, Karmn J23431+365, LHS 4003, LSPM J2343+3632, NLTT 57748, PLX 5741.21, PM J23431+3632, TIC 352593978, UBV M 53771, USNO 100, USNO 686, USNO-B1.0 1265-00549220, WISEA J234307.14+363211.5, Zkh 354, [RHG95] 3748, GJ 1289, GJ1289, LHS 4003, UBV M 53771, [RHG95] 3748, 2MASSJ23430628+3632132, CSI+36-23406, G130-4, G171-12, G190-43, GALEX6372217670673108177, GEN#+9.80130004, GJ1289, GaiaDR22879455480941956736, GaiaEDR32879455480942629248, KarmnJ23431+365, LHS4003, LSPMJ2343+3632, NLTT57748, PLX5741.21, PMJ23431+3632, TIC352593978, UBVM53771, USNO100, USNO686, USNO-B1.01265-00549220, WISEAJ234307.14+363211.5, Zkh354, [RHG95]3748, GJ1289, GJ1289, LHS4003, UBVM53771, [RHG95]3748

OBJECT name(s) in headers

GJ1289

PI name(s) in headers

Andres Carmona, Jean-Francois Donati, , QSO Team

Project/Run name(s) in headers

25BF27, 20AP40, 20BP40, 21AP40, 21BP40, 22AP40, 22BP45, 23AP45, 23BP45, 24AP45, 19AP40, 19BE99, 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_GJ1289_spirou_offline_udem.png

CCF stats

Mask used

GL699_neg.fits

CCF systemic velocity

-2358.27 \(\pm\) 11.90 m/s

CCF FWHM

5459.32 \(\pm\) 54.80 m/s

Number of CCF files Total

1313

Number of CCF passed QC

1313

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-05-15 14:29:51.099

Last ccf file [Mid exposure]

2025-10-13 07:38:45.783

Last processed [ccf]

2025-11-04 18:03:13.693

Version [ccf]

0.7.294,0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_GJ1289_spirou_offline_udem_file_list.txt

2026-02-12 19:55:58.155

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_GJ1289_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_GJ1289_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_GJ1289_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_GJ1289_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_GJ1289_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.