HD176232 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:41:38.075834 (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=HD176232

Target Information

RA

284.695518 [deg] (Gaia DR2)

Dec

13.90644774 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

8129.0 [K] (1973ApJ…183…95A)

Spectral Type

A7VpSrEu_Ksn (1995ApJS…99..135A)

Proper Motion (RA)

0.3254550772 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-47.2688812 [mas/yr] (Gaia DR2)

Parallax

13.37100177 [mas/yr] (Gaia DR2)

Radial Velocity

17.298 [mas/yr] (2018A&A…616A…7S)

Aliases

* 10 Aql, 2MASS J18584691+1354239, AAVSO 1854+13, AG+13 1865, BD+13 3838, CSV 8073, GC 26064, GCRV 11426, GEN# +1.00176232, GSC 01051-01778, Gaia DR1 4506321708923235456, Gaia DR2 4506321713245405184, HD 176232, HIC 93179, HIP 93179, HR 7167, N30 4210, PPM 135566, ROT 2697, Renson 49160, SAO 104303, SKY# 35017, TD1 23623, TIC 299000970, TYC 1051-1778-1, UBV 16118, UBV M 23370, V* V1286 Aql, WEB 16146, YZ 13 6942, uvby98 100176232, * 10 Aql, BD+13 3838, CSV 8073, HD176232, HD_176232, HIC 93179, HIP 93179, HR 7167, ROT 2697, UBV 16118, UBV M 23370, YZ 13 6942, *10Aql, 2MASSJ18584691+1354239, AAVSO1854+13, AG+131865, BD+133838, CSV8073, GC26064, GCRV11426, GEN#+1.00176232, GSC01051-01778, GaiaDR14506321708923235456, GaiaDR24506321713245405184, HD176232, HIC93179, HIP93179, HR7167, N304210, PPM135566, ROT2697, Renson49160, SAO104303, SKY#35017, TD123623, TIC299000970, TYC1051-1778-1, UBV16118, UBVM23370, V*V1286Aql, WEB16146, YZ136942, uvby98100176232, *10Aql, BD+133838, CSV8073, HD176232, HD176232, HIC93179, HIP93179, HR7167, ROT2697, UBV16118, UBVM23370, YZ136942

OBJECT name(s) in headers

HD176232

PI name(s) in headers

Claire Moutou

Project/Run name(s) in headers

18BE99

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_HD176232_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

17923.10 \(\pm\) 91.83 m/s

CCF FWHM

10697.34 \(\pm\) 126.02 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]

2018-09-23 07:09:16.573

Last ccf file [Mid exposure]

2018-09-23 07:32:24.779

Last processed [ccf]

2025-02-23 21:24:26.899

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HD176232_spirou_offline_udem_file_list.txt

2026-02-12 20:41:40.927

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_HD176232_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_HD176232_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD176232_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD176232_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_HD176232_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.