VV_CRA_NE (spirou_offline_udem)

This page was last modified: 2026-02-12 21:12:25.470719 (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=VV_CRA_NE

Target Information

RA

285.7781056 [deg] (Gaia DR2)

Dec

-37.21391385 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

4500.0 [K] (Approx from K7 spt)

Spectral Type

K7 (2011A&A…527A.119B)

Proper Motion (RA)

2.598713063 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-26.22503974 [mas/yr] (Gaia DR2)

Parallax

6.695192571 [mas/yr] (Gaia DR2)

Radial Velocity

-2.8709 [mas/yr] (2020AJ….160..120J)

Aliases

UCAC2 16068379, ** REP 48, AP J19030674-3712494, DENIS J190306.7-371249, HBC 291, Hen 3-1736, HGBS J190307.0-371250, IRAS 18597-3717, JCMTSE J190306.9-371248, JCMTSF J190306.9-371248, 2MASS J19030674-3712494, NAME VV CrA IRC, PSCz P18597-3717, SSTgbs J1903068-371249, SV* HV 4000, TIC 254080107, UCAC4 264-177392, V* VV CrA, VSST 4, WDS J19031-3713AB, WISEA J190306.78-371249.2, WISE J190306.80-371249.2, [CKR2003] MMS 24, [NWA2005] SMM 9, [SHK2011b] 4, [WGL92] iras 33, Gaia DR3 6719168132036642432, Gaia DR2 6719168132036642432, VV CrA NE, UCAC216068379, **REP48, APJ19030674-3712494, DENISJ190306.7-371249, HBC291, Hen3-1736, HGBSJ190307.0-371250, IRAS18597-3717, JCMTSEJ190306.9-371248, JCMTSFJ190306.9-371248, 2MASSJ19030674-3712494, NAMEVVCrAIRC, PSCzP18597-3717, SSTgbsJ1903068-371249, SV*HV4000, TIC254080107, UCAC4264-177392, V*VVCrA, VSST4, WDSJ19031-3713AB, WISEAJ190306.78-371249.2, WISEJ190306.80-371249.2, [CKR2003]MMS24, [NWA2005]SMM9, [SHK2011b]4, [WGL92]iras33, GaiaDR36719168132036642432, GaiaDR26719168132036642432, VVCrANE, VV_CRA_NE

OBJECT name(s) in headers

VV CrA NE

PI name(s) in headers

Evelyne Alecian

Project/Run name(s) in headers

24AF13

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_VV_CRA_NE_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

281401.47 \(\pm\) 12993.34 m/s

CCF FWHM

7502.39 \(\pm\) 3130.49 m/s

Number of CCF files Total

12

Number of CCF passed QC

12

Number CCF files failed QC

0

First ccf file [Mid exposure]

2024-04-25 13:22:24.907

Last ccf file [Mid exposure]

2024-06-24 11:42:18.837

Last processed [ccf]

2025-04-29 20:36:09.192

Version [ccf]

0.7.293

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_VV_CRA_NE_spirou_offline_udem_file_list.txt

2026-02-12 21:12:29.350

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_VV_CRA_NE_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_VV_CRA_NE_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_VV_CRA_NE_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_VV_CRA_NE_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_VV_CRA_NE_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.