GL378 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:13:05.653206 (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=GL378

Target Information

RA

150.5864197 [deg] (Gaia EDR3)

Dec

48.08224673 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

3744.0 [K] (2021A&A…656A.162M)

Spectral Type

M1V (1986AJ…..92..139S)

Proper Motion (RA)

-633.0735513 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-1474.827096 [mas/yr] (Gaia EDR3)

Parallax

66.84477938 [mas/yr] (Gaia EDR3)

Radial Velocity

-9.778 [mas/yr] (2018A&A…616A…7S)

Aliases

2MASS J10022184+4805209, ASCC 327190, BD+48 1829, G 146-6, G 195-54, GCRV 61040, GEN# +0.04801829, GJ 378, Gaia DR2 823228721066990720, Gaia EDR3 823228721067307392, HIC 49189, HIP 49189, L 1687-13, LFT 695, LHS 278, LSPM J1002+4805, LTT 12682, MCC 562, NLTT 23220, PLX 2370.1, PLX 2370.10, PM 09592+4821, PM J10023+4805, StKM 2-605, TIC 252470070, TYC 3437-85-1, UCAC4 691-049924, USNO-B1.0 1380-00252535, WEB 9109, WISEA J100221.10+480504.5, Zkh 136, [RHG95] 1575, ASCC 327190, BD+48 1829, GJ 378, GL378, Gl378, HIC 49189, HIP 49189, LFT 695, LHS 278, WEB 9109, [RHG95] 1575, 2MASSJ10022184+4805209, ASCC327190, BD+481829, G146-6, G195-54, GCRV61040, GEN#+0.04801829, GJ378, GaiaDR2823228721066990720, GaiaEDR3823228721067307392, HIC49189, HIP49189, L1687-13, LFT695, LHS278, LSPMJ1002+4805, LTT12682, MCC562, NLTT23220, PLX2370.1, PLX2370.10, PM09592+4821, PMJ10023+4805, StKM2-605, TIC252470070, TYC3437-85-1, UCAC4691-049924, USNO-B1.01380-00252535, WEB9109, WISEAJ100221.10+480504.5, Zkh136, [RHG95]1575, ASCC327190, BD+481829, GJ378, GL378, Gl378, HIC49189, HIP49189, LFT695, LHS278, WEB9109, [RHG95]1575

OBJECT name(s) in headers

Gl378

PI name(s) in headers

Melissa Hobson

Project/Run name(s) in headers

19BF33

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_GL378_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-9820.83 \(\pm\) 9.15 m/s

CCF FWHM

7001.96 \(\pm\) 57.35 m/s

Number of CCF files Total

9

Number of CCF passed QC

9

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-12-05 14:59:54.232

Last ccf file [Mid exposure]

2020-01-28 12:17:03.748

Last processed [ccf]

2025-02-23 20:23:04.186

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_GL378_spirou_offline_udem_file_list.txt

2026-02-12 20:13:09.059

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_GL378_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_GL378_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_GL378_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_GL378_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_GL378_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.