HD195094 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:41:48.464904 (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=HD195094

Target Information

RA

307.4747591 [deg] (Gaia EDR3)

Dec

-18.58354497 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

8913.0 [K] (2012A&A…537A.120Z (via spirou@rali))

Spectral Type

A1V (1988MSS…C04….0H)

Proper Motion (RA)

29.05787637 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-81.32583884 [mas/yr] (Gaia EDR3)

Parallax

14.01927556 [mas/yr] (Gaia EDR3)

Radial Velocity

-12.4 [mas/yr] (2006AstL…32..759G)

Aliases

* 12 Cap A, * omi Cap A, ADS 13902 A, BD-19 5831, CCDM J20299-1835A, GC 28503, GSC 06333-02130, HD 195094, HIC 101123, HIP 101123, HR 7830, IDS 20242-1855 A, 2MASS J20295391-1834593, PPM 237509, ROT 2984, SAO 163626, SKY# 38780, TIC 72429235, TYC 6333-2130-1, UBV 17760, UBV M 24874, uvby98 100195094 A, WDS J20299-1835A, YZ 108 8789, Gaia DR1 6860821646719117952, Gaia EDR3 6860821651019024896, Gaia DR2 6860821651019024896, *12CapA, *omiCapA, ADS13902A, BD-195831, CCDMJ20299-1835A, GC28503, GSC06333-02130, HD195094, HIC101123, HIP101123, HR7830, IDS20242-1855A, 2MASSJ20295391-1834593, PPM237509, ROT2984, SAO163626, SKY#38780, TIC72429235, TYC6333-2130-1, UBV17760, UBVM24874, uvby98100195094A, WDSJ20299-1835A, YZ1088789, GaiaDR16860821646719117952, GaiaEDR36860821651019024896, GaiaDR26860821651019024896, HR7830, HR 7830, ADS 13902 A, OMICAPA, ADS13902A

OBJECT name(s) in headers

omiCapA

PI name(s) in headers

QSO Team

Project/Run name(s) in headers

25BQ58, 25AQ58, 20AQ58, 20BQ58, 21AQ58, 21BQ58, 22AQ58, 22BQ58, 23AQ58, 23BQ58, 24AQ58, 24BQ58, 19AQ58, 19BQ58

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_HD195094_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

297692.91 \(\pm\) 5216.37 m/s

CCF FWHM

5882.43 \(\pm\) 71408.25 m/s

Number of CCF files Total

72

Number of CCF passed QC

72

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-04-21 15:10:49.397

Last ccf file [Mid exposure]

2025-11-03 04:54:09.828

Last processed [ccf]

2026-01-07 12:18:14.590

Version [ccf]

0.7.294,0.7.292,0.7.295,0.7.293

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HD195094_spirou_offline_udem_file_list.txt

2026-02-12 20:41:59.979

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_HD195094_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_HD195094_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD195094_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD195094_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_HD195094_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.