HD221830 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:46:36.100738 (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=HD221830

Target Information

RA

353.8731062 [deg] (Gaia DR2)

Dec

31.01827009 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

5666.0 [K] (2015A&A…573A..67P)

Spectral Type

G2 (1985ApJS…59..197B)

Proper Motion (RA)

539.7859455 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

254.155434 [mas/yr] (Gaia DR2)

Parallax

29.90200317 [mas/yr] (Gaia DR2)

Radial Velocity

-112.284 [mas/yr] (2018A&A…616A…7S)

Aliases

LHS 3976, ** LDS 6405A, AG+30 2647, AGKR 21113, AP J23352889+3101017, ASCC 645645, BD+30 4982, BD+30 4982A, Ci 20 1435, GC 32800, GCRV 14794, GEN# +1.00221830, HD 221830, HIC 116421, HIP 116421, IRAS 23329+3044, LFT 1804, LSPM J2335+3101, LTT 16942, 2MASS J23352889+3101017, NLTT 57309, PLX 5706, PMC 90-93 4626, PPM 88952, SAO 73358, SKY# 44635, SPOCS 1023, TIC 366036237, TYC 2766-652-1, UBV 20280, UBV M 27109, USNO-B1.0 1210-00590759, uvby98 100221830, WDS J23355+3101A, WEB 20566, WISEA J233529.39+310104.2, Gaia DR2 2871338405070839040, Gaia DR3 2871338405072089088, LHS3976, **LDS6405A, AG+302647, AGKR21113, APJ23352889+3101017, ASCC645645, BD+304982, BD+304982A, Ci201435, GC32800, GCRV14794, GEN#+1.00221830, HD221830, HIC116421, HIP116421, IRAS23329+3044, LFT1804, LSPMJ2335+3101, LTT16942, 2MASSJ23352889+3101017, NLTT57309, PLX5706, PMC90-934626, PPM88952, SAO73358, SKY#44635, SPOCS1023, TIC366036237, TYC2766-652-1, UBV20280, UBVM27109, USNO-B1.01210-00590759, uvby98100221830, WDSJ23355+3101A, WEB20566, WISEAJ233529.39+310104.2, GaiaDR22871338405070839040, GaiaDR32871338405072089088

OBJECT name(s) in headers

HD 221830

PI name(s) in headers

Ryan Cloutier

Project/Run name(s) in headers

22BC27

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_HD221830_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-111594.56 \(\pm\) 0.00 m/s

CCF FWHM

8670.37 \(\pm\) 0.00 m/s

Number of CCF files Total

1

Number of CCF passed QC

1

Number CCF files failed QC

0

First ccf file [Mid exposure]

2022-11-11 07:36:59.290

Last ccf file [Mid exposure]

2022-11-11 07:36:59.290

Last processed [ccf]

2025-02-23 16:21:10.374

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HD221830_spirou_offline_udem_file_list.txt

2026-02-12 20:46:37.876

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_HD221830_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_HD221830_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD221830_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD221830_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_HD221830_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.