GJ1151 (spirou_offline_udem)

This page was last modified: 2026-02-12 19:50:07.589459 (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=GJ1151

Target Information

RA

177.7301638 [deg] (Gaia EDR3)

Dec

48.3730998 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

3178.0 [K] (2022MNRAS.516.3802C)

Spectral Type

M4.5Ve (2013AJ….145..102L)

Proper Motion (RA)

-1545.068861 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-962.7239331 [mas/yr] (Gaia EDR3)

Parallax

124.3377749 [mas/yr] (Gaia EDR3)

Radial Velocity

-35.12 [mas/yr] (2018MNRAS.475.1960F)

Aliases

2MASS J11505787+4822395, G 122-49, GALEX 3858637239337622240, GEN# +9.80122049, GJ 1151, Gaia DR2 786834302079285632, Gaia EDR3 786834302080370304, ILT J115055.50+482225.2, Karmn J11509+483, LHS 316, LSPM J1150+4822, NLTT 28752, PLX 2739.01, PM 11485+4840, PM J11509+4822, StKM 2-769, TIC 11893637, UBV M 53759, UCAC4 692-050566, USNO 144, USNO-B1.0 1383-00239712, WISEA J115056.09+482228.4, Zkh 171, [RHG95] 1854, GJ 1151, GJ1151, LHS 316, UBV M 53759, [RHG95] 1854, 2MASSJ11505787+4822395, G122-49, GALEX3858637239337622240, GEN#+9.80122049, GJ1151, GaiaDR2786834302079285632, GaiaEDR3786834302080370304, ILTJ115055.50+482225.2, KarmnJ11509+483, LHS316, LSPMJ1150+4822, NLTT28752, PLX2739.01, PM11485+4840, PMJ11509+4822, StKM2-769, TIC11893637, UBVM53759, UCAC4692-050566, USNO144, USNO-B1.01383-00239712, WISEAJ115056.09+482228.4, Zkh171, [RHG95]1854, GJ1151, GJ1151, LHS316, UBVM53759, [RHG95]1854

OBJECT name(s) in headers

GJ1151

PI name(s) in headers

Jean-Francois Donati

Project/Run name(s) in headers

20AP40, 20BP40, 21AP40, 21BP40, 22AP40, 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_GJ1151_spirou_offline_udem.png

CCF stats

Mask used

GL699_neg.fits

CCF systemic velocity

-34995.38 \(\pm\) 9.73 m/s

CCF FWHM

5357.30 \(\pm\) 61.39 m/s

Number of CCF files Total

613

Number of CCF passed QC

613

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-12-10 14:48:06.619

Last ccf file [Mid exposure]

2022-06-13 06:37:23.542

Last processed [ccf]

2025-02-23 20:19:04.678

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_GJ1151_spirou_offline_udem_file_list.txt

2026-02-12 19:51:14.695

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_GJ1151_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_GJ1151_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_GJ1151_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_GJ1151_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_GJ1151_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.