GQLUP (spirou_offline_udem)

This page was last modified: 2026-02-12 20:25:13.355254 (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=GQLUP

Target Information

RA

237.3003643 [deg] (Gaia DR2)

Dec

-35.65150548 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

4192.0 [K] (2017A&A…602A..33F)

Spectral Type

K7Ve (1977ApJ…214..747H)

Proper Motion (RA)

-14.25716365 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-23.59603804 [mas/yr] (Gaia DR2)

Parallax

6.586778354 [mas/yr] (Gaia DR2)

Radial Velocity

-3.6 [mas/yr] (2017A&A…602A..33F)

Aliases

** FMR 242A, ** NHR 8A, 2MASS J15491210-3539051, AAVSO 1542-35, AKARI-IRC-V1 J1549120-353905, CD-35 10525, GEN# -0.03510525, GSC 07340-00177, Gaia DR2 6011522757643074304, HBC 250, Hen 3-1106, IRAS 15459-3529, IRAS F15459-3529, JP11 310, PDS 74, SV* BV 1387, Sz 75, THA 15-7, TIC 442623945, UCAC2 16630543, UCAC3 109-183258, UCAC4 272-081159, V* GQ Lup, V* GQ Lup B, WDS J15492-3539A, WDS J15492-3539Aa,Ab, WISE J154912.09-353905.2, WISEA J154912.09-353905.2, WRAY 15-1362, [KWS97] Lupus 1 56, ** FMR 242Aa, ** NHR 8Aa, GQLUP, GQLup, JP11 310, PDS 74, SV* BV 1387, Sz 75, UCAC2 16630543, WDS J15492-3539Aa, **FMR242A, **NHR8A, 2MASSJ15491210-3539051, AAVSO1542-35, AKARI-IRC-V1J1549120-353905, CD-3510525, GEN#-0.03510525, GSC07340-00177, GaiaDR26011522757643074304, HBC250, Hen3-1106, IRAS15459-3529, IRASF15459-3529, JP11310, PDS74, SV*BV1387, Sz75, THA15-7, TIC442623945, UCAC216630543, UCAC3109-183258, UCAC4272-081159, V*GQLup, V*GQLupB, WDSJ15492-3539A, WDSJ15492-3539Aa,Ab, WISEJ154912.09-353905.2, WISEAJ154912.09-353905.2, WRAY15-1362, [KWS97]Lupus156, **FMR242Aa, **NHR8Aa, GQLUP, GQLup, JP11310, PDS74, SV*BV1387, Sz75, UCAC216630543, WDSJ15492-3539Aa

OBJECT name(s) in headers

GQLup

PI name(s) in headers

Jean-Francois Donati

Project/Run name(s) in headers

20AP40, 20BP40, 19AP40

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_GQLUP_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-2457.38 \(\pm\) 188.12 m/s

CCF FWHM

11415.15 \(\pm\) 393.43 m/s

Number of CCF files Total

129

Number of CCF passed QC

129

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-06-14 07:34:44.291

Last ccf file [Mid exposure]

2020-08-11 05:56:32.991

Last processed [ccf]

2025-02-23 21:01:01.606

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_GQLUP_spirou_offline_udem_file_list.txt

2026-02-12 20:25:35.476

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_GQLUP_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_GQLUP_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_GQLUP_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_GQLUP_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_GQLUP_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.