G_145M11 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:24:45.521506 (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=G_145M11

Target Information

RA

316.2847433 [deg] (Gaia EDR3)

Dec

14.59108915 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

4100.0 [K] (HEADER[CFHT])

Spectral Type

M2.5 (1997PASP..109..643P)

Proper Motion (RA)

510.8303958 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-3.29316609 [mas/yr] (Gaia EDR3)

Parallax

25.12651708 [mas/yr] (Gaia EDR3)

Radial Velocity

-23.75 [mas/yr] (2018yCat.1345….0G)

Aliases

** LDS 1050B, ** NSN 740A, 2MASS J21050772+1435280, ASCC 990769, CSI+14-21028, G 144-60, G 145-11, GEN# +9.80144060, Gaia DR2 1760208512800938752, Gaia EDR3 1760208512800938752, L 1216-21, LHS 3621, LP 516-29, LSPM J2105+1435, LTT 16167, NLTT 50489, PLX 5069.01, PM J21051+1435, TIC 125699207, UBV M 42727, UCAC2 37097352, UCAC4 523-142262, USNO 84, USNO-B1.0 1045-00598991, WDS J21051+1435A, WDS J21058+1432C, WISEA J210508.14+143527.9, [GAL2014] J21051+1435, ASCC 990769, G_145M11, LHS 3621, LP 516-29, UBV M 42727, UCAC2 37097352, USNO 84, **LDS1050B, **NSN740A, 2MASSJ21050772+1435280, ASCC990769, CSI+14-21028, G144-60, G145-11, GEN#+9.80144060, GaiaDR21760208512800938752, GaiaEDR31760208512800938752, L1216-21, LHS3621, LP516-29, LSPMJ2105+1435, LTT16167, NLTT50489, PLX5069.01, PMJ21051+1435, TIC125699207, UBVM42727, UCAC237097352, UCAC4523-142262, USNO84, USNO-B1.01045-00598991, WDSJ21051+1435A, WDSJ21058+1432C, WISEAJ210508.14+143527.9, [GAL2014]J21051+1435, ASCC990769, G145M11, LHS3621, LP516-29, UBVM42727, UCAC237097352, USNO84

OBJECT name(s) in headers

G 145-11

PI name(s) in headers

Farbod Jahandar

Project/Run name(s) in headers

20BC30

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_G_145M11_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-24350.98 \(\pm\) 5.64 m/s

CCF FWHM

7019.64 \(\pm\) 8.22 m/s

Number of CCF files Total

4

Number of CCF passed QC

4

Number CCF files failed QC

0

First ccf file [Mid exposure]

2020-09-01 09:05:45.752

Last ccf file [Mid exposure]

2020-09-01 09:21:08.205

Last processed [ccf]

2025-02-23 19:22:15.927

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_G_145M11_spirou_offline_udem_file_list.txt

2026-02-12 20:24:48.172

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_G_145M11_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_G_145M11_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_G_145M11_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_G_145M11_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_G_145M11_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.