DX_CNC (spirou_offline_udem)

This page was last modified: 2026-02-12 19:41:43.447098 (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=DX_CNC

Target Information

RA

127.4500924 [deg] (Gaia EDR3)

Dec

26.77328597 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

3054.0 [K] (2021A&A…656A.162M)

Spectral Type

M6.5Ve (2004AJ….128.2460H)

Proper Motion (RA)

-1113.693547 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-612.1910728 [mas/yr] (Gaia EDR3)

Parallax

279.2496391 [mas/yr] (Gaia EDR3)

Radial Velocity

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

Aliases

GEN# +9.80051015, 8pc275.80, DX Cnc, PLX2016.0, PLX2016.01, GJ 1111, AP J08294949+2646348, GaiaDR3703790044252850688, UCAC2 41191231, [GKL99] 181, LSPM J0829+2646, TIC 3664898, LTT18058, V* DX Cnc, PM08269+2657, PM J08298+2646, Zkh 118, Karmn J08298+267, [GKL99]181, LHS 248, GaiaDR2703790044252850688, UCAC4584-042341, 2MASSJ08294949+2646348, LSPMJ0829+2646, UCAC4 584-042341, UCAC241191231, GJ 1111, USNO 311, LHS 248, USNO311, G51-15, USNO-B1.0 1167-00167383, KarmnJ08298+267, [RHG95]1326, GEN#+9.80051015, PLX 2016.0, [RHG95] 1326, PM 08269+2657, NLTT 19635, JP115934, JP11 5934, [RHG95] 1326, LTT 18058, JP115935, JP11 5934, Gaia DR3 703790044252850688, GaiaEDR3703790044252850688, APJ08294949+2646348, V*DXCnc, 8pc 275.80, NLTT19635, TIC3664898, JP11 5935, 2MASS J08294949+2646348, Zkh118, PLX 2016.01, DX_CNC, USNO-B1.01167-00167383, G 51-15, UCAC2 41191231, GJ1111, G 51-15, JP11 5935, LHS248, PMJ08298+2646, Gaia DR2 703790044252850688, Gaia EDR3 703790044252850688

OBJECT name(s) in headers

GJ1111

PI name(s) in headers

Andres Carmona, Etienne Artigau, Jean-Francois Donati

Project/Run name(s) in headers

25BF27, 25AF23, 24BC05, 23BF12, 23BC10, 24AC25, 24AF17, 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_DX_CNC_spirou_offline_udem.png

CCF stats

Mask used

GL699_neg.fits

CCF systemic velocity

11060.97 \(\pm\) 51.05 m/s

CCF FWHM

14743.00 \(\pm\) 168.19 m/s

Number of CCF files Total

324

Number of CCF passed QC

324

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-02-14 12:03:19.239

Last ccf file [Mid exposure]

2025-11-08 15:45:48.518

Last processed [ccf]

2026-01-07 12:14:30.805

Version [ccf]

0.7.292,0.7.295,0.7.293

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_DX_CNC_spirou_offline_udem_file_list.txt

2026-02-12 19:42:15.816

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_DX_CNC_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_DX_CNC_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_DX_CNC_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_DX_CNC_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_DX_CNC_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.