GJ4063 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:01:14.783487 (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=GJ4063

Target Information

RA

278.6530414 [deg] (Gaia DR2)

Dec

40.12310663 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

3419.0 [K] (2022MNRAS.516.3802C)

Spectral Type

M4V (2011ApJS..197…19K)

Proper Motion (RA)

57.72563445 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-206.3225987 [mas/yr] (Gaia DR2)

Parallax

91.85449204 [mas/yr] (Gaia DR2)

Radial Velocity

12.533 [mas/yr] (2018A&A…616A…7S)

Aliases

2MASS J18343664+4007266, ASCC 421007, GJ 4063, Gaia DR2 2110165780975185792, Karmn J18346+401, LP 229-17, LSPM J1834+4007, NLTT 46690, PM J18346+4007W, StKM 2-1382, TIC 289527642, TYC 3109-1699-1, UCAC2 45843486, UCAC4 651-063412, USNO-B1.0 1301-00298017, WISEA J183436.71+400724.2, WISEP J183436.70+400724.3, [GAL2014] J18346+4007, [RHG95] 2921, ASCC 421007, GJ 4063, GJ4063, LP 229-17, UCAC2 45843486, [RHG95] 2921, 2MASSJ18343664+4007266, ASCC421007, GJ4063, GaiaDR22110165780975185792, KarmnJ18346+401, LP229-17, LSPMJ1834+4007, NLTT46690, PMJ18346+4007W, StKM2-1382, TIC289527642, TYC3109-1699-1, UCAC245843486, UCAC4651-063412, USNO-B1.01301-00298017, WISEAJ183436.71+400724.2, WISEPJ183436.70+400724.3, [GAL2014]J18346+4007, [RHG95]2921, ASCC421007, GJ4063, GJ4063, LP229-17, UCAC245843486, [RHG95]2921

OBJECT name(s) in headers

GJ4063

PI name(s) in headers

Andres Carmona, Jean-Francois Donati, Etienne Artigau

Project/Run name(s) in headers

24BF13, 20AP40, 20BP40, 21AP40, 21BP40, 22AP40, 22BF10, 23AF13, 23AD98, 23BF12, 24AC25, 24AF17, 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_GJ4063_spirou_offline_udem.png

CCF stats

Mask used

GL699_neg.fits

CCF systemic velocity

12834.23 \(\pm\) 14.29 m/s

CCF FWHM

5396.96 \(\pm\) 40.52 m/s

Number of CCF files Total

1134

Number of CCF passed QC

1134

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-09-18 08:06:04.617

Last ccf file [Mid exposure]

2024-11-20 04:54:55.414

Last processed [ccf]

2025-02-23 20:53:32.801

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_GJ4063_spirou_offline_udem_file_list.txt

2026-02-12 20:04:23.102

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_GJ4063_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_GJ4063_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_GJ4063_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_GJ4063_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_GJ4063_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.