GJ1105 (spirou_offline_udem)

This page was last modified: 2026-02-12 19:50:43.258892 (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=GJ1105

Target Information

RA

119.5542083 [deg] (Gaia EDR3)

Dec

41.3006425 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

3324.0 [K] (2022MNRAS.516.3802C)

Spectral Type

M3.5Ve (2013AJ….145..102L)

Proper Motion (RA)

216.8662245 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-687.6148518 [mas/yr] (Gaia EDR3)

Parallax

112.9926779 [mas/yr] (Gaia EDR3)

Radial Velocity

-20.94 [mas/yr] (2018MNRAS.475.1960F)

Aliases

2MASS J07581269+4118134, ASCC 402755, G 111-47, GEN# +9.80111047, GJ 1105, Gaia DR2 922225002820369152, Gaia EDR3 922225002820369152, HIC 38956, HIP 38956, Karmn J07582+413, LHS 1963, LSPM J0758+4118, NLTT 18699, PLX 1875.01, PM J07582+4118, TIC 371272665, TYC 2968-1142-1, UBV M 53745, UCAC2 46137824, UCAC4 657-049582, USNO 133, USNO-B1.0 1313-00192853, Zkh 115, [RHG95] 1247, ASCC 402755, GJ 1105, GJ1105, HIC 38956, HIP 38956, LHS 1963, UBV M 53745, UCAC2 46137824, [RHG95] 1247, 2MASSJ07581269+4118134, ASCC402755, G111-47, GEN#+9.80111047, GJ1105, GaiaDR2922225002820369152, GaiaEDR3922225002820369152, HIC38956, HIP38956, KarmnJ07582+413, LHS1963, LSPMJ0758+4118, NLTT18699, PLX1875.01, PMJ07582+4118, TIC371272665, TYC2968-1142-1, UBVM53745, UCAC246137824, UCAC4657-049582, USNO133, USNO-B1.01313-00192853, Zkh115, [RHG95]1247, ASCC402755, GJ1105, GJ1105, HIC38956, HIP38956, LHS1963, UBVM53745, UCAC246137824, [RHG95]1247

OBJECT name(s) in headers

GJ1105

PI name(s) in headers

Etienne Artigau, Andres Carmona, Jean-Francois Donati

Project/Run name(s) in headers

25BC08, 25AF23, 24BF13, 24BC05, 20BP40, 21AP40, 21BP40, 22AP40, 22BF10, 23AF13, 24AC25, 19BP40, 20AP40

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_GJ1105_spirou_offline_udem.png

CCF stats

Mask used

GL699_neg.fits

CCF systemic velocity

-20684.84 \(\pm\) 13.78 m/s

CCF FWHM

5312.97 \(\pm\) 41.04 m/s

Number of CCF files Total

851

Number of CCF passed QC

851

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-09-18 15:06:49.134

Last ccf file [Mid exposure]

2025-11-01 12:00:40.191

Last processed [ccf]

2026-01-07 12:19:12.945

Version [ccf]

0.7.294,0.7.292,0.7.295,0.7.293

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_GJ1105_spirou_offline_udem_file_list.txt

2026-02-12 19:52:38.062

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_GJ1105_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_GJ1105_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_GJ1105_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_GJ1105_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_GJ1105_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.