GJ490B (spirou_offline_udem)

This page was last modified: 2026-02-12 19:57:31.166944 (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=GJ490B

Target Information

RA

194.4123023 [deg] (Gaia DR2)

Dec

35.22137986 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

3136.0 [K] (2018MNRAS.475.1960F)

Spectral Type

M4.5V (2013AJ….145..102L)

Proper Motion (RA)

-284.5769984 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-140.7310876 [mas/yr] (Gaia DR2)

Parallax

49.54748393 [mas/yr] (Gaia DR2)

Radial Velocity

-6.78 [mas/yr] (2018MNRAS.475.1960F)

Aliases

** BWL 35Ba,Bb, ** LDS 5764B, 2MASS J12573935+3513194, ASCC 494776, BD+36 2322B, BPS BS 16466-0079, CCDM J12577+3514B, CSI+35-12553, G 164-31, GALEX 2491196617905933870, GEN# +0.03602322B, GJ 490 B, Gaia DR2 1515952176488266496, Gaia EDR3 1515952176488266496, LSPM J1257+3513W, NLTT 32438, NSV 6039, PM J12576+3513W, TIC 165916579, TYC 2534-825-2, UCAC4 627-047803, USNO 324, USNO-B1.0 1252-00202773, WDS J12576+3514B, WDS J12576+3514Ba,Bb, WISEA J125739.08+351317.7, [RHG95] 2036, [ZEH2003] RX J1257.6+3513 1, ** BWL 35Ba,Bb, ASCC 494776, BD+36 2322B, GJ 490 B, GJ490B, NSV 6039, [RHG95] 2036, [ZEH2003] RX J1257.6+3513 1, **BWL35Ba,Bb, **LDS5764B, 2MASSJ12573935+3513194, ASCC494776, BD+362322B, BPSBS16466-0079, CCDMJ12577+3514B, CSI+35-12553, G164-31, GALEX2491196617905933870, GEN#+0.03602322B, GJ490B, GaiaDR21515952176488266496, GaiaEDR31515952176488266496, LSPMJ1257+3513W, NLTT32438, NSV6039, PMJ12576+3513W, TIC165916579, TYC2534-825-2, UCAC4627-047803, USNO324, USNO-B1.01252-00202773, WDSJ12576+3514B, WDSJ12576+3514Ba,Bb, WISEAJ125739.08+351317.7, [RHG95]2036, [ZEH2003]RXJ1257.6+35131, **BWL35Ba,Bb, ASCC494776, BD+362322B, GJ490B, GJ490B, NSV6039, [RHG95]2036, [ZEH2003]RXJ1257.6+35131

OBJECT name(s) in headers

GJ490B

PI name(s) in headers

Julien Morin

Project/Run name(s) in headers

19AF26

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_GJ490B_spirou_offline_udem.png

CCF stats

Mask used

GL699_neg.fits

CCF systemic velocity

-4667.79 \(\pm\) 187.27 m/s

CCF FWHM

50282.04 \(\pm\) 150.21 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]

2019-04-24 09:49:28.376

Last ccf file [Mid exposure]

2019-04-24 10:51:36.363

Last processed [ccf]

2025-02-23 21:12:14.047

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_GJ490B_spirou_offline_udem_file_list.txt

2026-02-12 19:57:33.454

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_GJ490B_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_GJ490B_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_GJ490B_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_GJ490B_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_GJ490B_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.