HD199260 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:41:39.515210 (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=HD199260

Target Information

RA

314.1976666 [deg] (Gaia DR2)

Dec

-26.29666025 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

6284.0 [K] (2018AJ….155..111L)

Spectral Type

F6V (2006AJ….132..161G)

Proper Motion (RA)

95.10549809 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-65.00058274 [mas/yr] (Gaia DR2)

Parallax

46.97640367 [mas/yr] (Gaia DR2)

Radial Velocity

-15.546 [mas/yr] (2018A&A…616A…7S)

Aliases

1RXS J205647.0-261751, 2MASS J20564731-2617470, CD-26 15344, CPD-26 7133, GC 29213, GCRV 71630, GEN# +1.00199260, GJ 811, Gaia DR2 6802426038708609536, HD 199260, HIC 103389, HIP 103389, HR 8013, IRAS 20538-2629, NSV 13412, PLX 5007.01, PPM 271828, RBS 1708, SAO 189856, SKY# 39791, SPOCS 3155, SRS 44502, TD1 27452, TIC 29495621, TYC 6931-1018-1, UBV 18104, UBV M 25271, WEB 18796, YZ 116 14506, uvby98 100199260, CPD-26 7133, GJ 811, HD199260, HD_199260, HR 8013, RBS 1708, SRS 44502, UBV 18104, UBV M 25271, 1RXSJ205647.0-261751, 2MASSJ20564731-2617470, CD-2615344, CPD-267133, GC29213, GCRV71630, GEN#+1.00199260, GJ811, GaiaDR26802426038708609536, HD199260, HIC103389, HIP103389, HR8013, IRAS20538-2629, NSV13412, PLX5007.01, PPM271828, RBS1708, SAO189856, SKY#39791, SPOCS3155, SRS44502, TD127452, TIC29495621, TYC6931-1018-1, UBV18104, UBVM25271, WEB18796, YZ11614506, uvby98100199260, CPD-267133, GJ811, HD199260, HD199260, HR8013, RBS1708, SRS44502, UBV18104, UBVM25271

OBJECT name(s) in headers

HD199260

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_HD199260_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-13100.24 \(\pm\) 262405.23 m/s

CCF FWHM

17892.95 \(\pm\) 11124.78 m/s

Number of CCF files Total

15

Number of CCF passed QC

15

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-06-15 14:57:33.518

Last ccf file [Mid exposure]

2019-06-19 12:21:47.362

Last processed [ccf]

2025-02-23 20:59:36.022

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HD199260_spirou_offline_udem_file_list.txt

2026-02-12 20:41:43.317

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_HD199260_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_HD199260_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD199260_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD199260_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_HD199260_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.