HD143006 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:40:04.921928 (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=HD143006

Target Information

RA

239.6537524 [deg] (Gaia DR2)

Dec

-22.95431844 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

5956.0 [K] (2015A&A…573A..67P)

Spectral Type

G5IVe (2016MNRAS.461..794P)

Proper Motion (RA)

-10.88162421 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-20.96063291 [mas/yr] (Gaia DR2)

Parallax

6.020738347 [mas/yr] (Gaia DR2)

Radial Velocity

-3.26 [mas/yr] (2018yCat.1345….0G)

Aliases

1RXS J155837.1-225724, 2MASS J15583692-2257153, BD-22 4059, CD-22 11272, CPD-22 6099, EM* StHA 118, EPIC 204281210, EPIC 204281213, GLMP 441, GSC 06779-00305, Gaia DR1 6237190608636038656, Gaia DR2 6237190612936085120, HBC 608, HD 143006, Hen 3-1126, IRAS 15556-2248, PPM 264939, RX J155837.0-225711, SAO 183986, SPOCS 680, TIC 12658445, TYC 6779-305-1, USco 43, V* V1149 Sco, WISEA J155836.90-225715.3, YZ 112 11238, [DML87] 387, BD-22 4059, CPD-22 6099, EM* StHA 118, GLMP 441, HD143006, HD_143006, SPOCS 680, 1RXSJ155837.1-225724, 2MASSJ15583692-2257153, BD-224059, CD-2211272, CPD-226099, EM*StHA118, EPIC204281210, EPIC204281213, GLMP441, GSC06779-00305, GaiaDR16237190608636038656, GaiaDR26237190612936085120, HBC608, HD143006, Hen3-1126, IRAS15556-2248, PPM264939, RXJ155837.0-225711, SAO183986, SPOCS680, TIC12658445, TYC6779-305-1, USco43, V*V1149Sco, WISEAJ155836.90-225715.3, YZ11211238, [DML87]387, BD-224059, CPD-226099, EM*StHA118, GLMP441, HD143006, HD143006, SPOCS680

OBJECT name(s) in headers

HD143006

PI name(s) in headers

Lauren Weiss

Project/Run name(s) in headers

19AH28

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_HD143006_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-1049.53 \(\pm\) 128.62 m/s

CCF FWHM

16000.59 \(\pm\) 439.71 m/s

Number of CCF files Total

8

Number of CCF passed QC

8

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-02-16 14:42:10.547

Last ccf file [Mid exposure]

2019-04-20 13:23:53.229

Last processed [ccf]

2025-02-23 21:16:03.740

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HD143006_spirou_offline_udem_file_list.txt

2026-02-12 20:40:07.443

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_HD143006_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_HD143006_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD143006_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD143006_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_HD143006_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.