HD38678 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:46:46.157658 (UTC)

Back to the object table

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=HD38678

Target Information

RA

86.73885884 [deg] (Gaia DR2)

Dec

-14.82195344 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

8337.0 [K] (2003AJ….125.1598L)

Spectral Type

A2IV-V(n) (2006AJ….132..161G)

Proper Motion (RA)

-15.65974984 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-1.384821039 [mas/yr] (Gaia DR2)

Parallax

45.71714404 [mas/yr] (Gaia DR2)

Radial Velocity

24.7 [mas/yr] (2006AstL…32..759G)

Aliases

* zet Lep, * 14 Lep, BD-14 1232, FK5 219, GC 7247, GCRV 3591, GEN# +1.00038678, GJ 9190, GJ 217.1, GSC 05359-01778, HD 38678, HIC 27288, HIP 27288, HR 1998, IRAS 05446-1450, JP11 1259, 2MASS J05465735-1449189, N30 1240, PLX 1326, PLX 1326.00, PMC 90-93 157, PPM 216268, ROT 925, SACS 125, SAO 150801, SKY# 9500, TD1 5348, TIC 317132886, TYC 5359-1778-1, UBV 5925, UBV M 11498, uvby98 100038678, WEB 5364, YZ 104 1761, Gaia DR2 2996171698248345984, *zetLep, *14Lep, BD-141232, FK5219, GC7247, GCRV3591, GEN#+1.00038678, GJ9190, GJ217.1, GSC05359-01778, HD38678, HIC27288, HIP27288, HR1998, IRAS05446-1450, JP111259, 2MASSJ05465735-1449189, N301240, PLX1326, PLX1326.00, PMC90-93157, PPM216268, ROT925, SACS125, SAO150801, SKY#9500, TD15348, TIC317132886, TYC5359-1778-1, UBV5925, UBVM11498, uvby98100038678, WEB5364, YZ1041761, GaiaDR22996171698248345984, ZETLEP, zetLep, SAO 150801, SAO150801

OBJECT name(s) in headers

zetLep

PI name(s) in headers

QSO Team, Claire Moutou, Matt Wilson

Project/Run name(s) in headers

25BQ58, 25AQ58, 20BQ58, 21AQ58, 21BQ58, 22AQ58, 22BQ58, 23AQ58, 23BQ58, 24AQ58, 24BQ58, 18BE93, 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_HD38678_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

298257.93 \(\pm\) 3318.89 m/s

CCF FWHM

3944.04 \(\pm\) 68713.67 m/s

Number of CCF files Total

66

Number of CCF passed QC

66

Number CCF files failed QC

0

First ccf file [Mid exposure]

2018-09-26 14:37:26.701

Last ccf file [Mid exposure]

2025-11-27 11:38:34.730

Last processed [ccf]

2026-01-07 12:13:20.719

Version [ccf]

0.7.294,0.7.295,0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HD38678_spirou_offline_udem_file_list.txt

2026-02-12 20:46:55.937

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_HD38678_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_HD38678_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD38678_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD38678_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_HD38678_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.