HLTAU (spirou_offline_udem)

This page was last modified: 2026-02-12 20:47:17.055876 (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=HLTAU

Target Information

RA

67.91029972 [deg] (UCAC4)

Dec

18.23280139 [deg] (UCAC4)

Finder chart

[FINDER CHART]

Teff

4450.0 [K] (HEADER[CFHT])

Spectral Type

K5 (2004ApJ…616..998W)

Proper Motion (RA)

4.199999809 [mas/yr] (UCAC4)

Proper Motion (Dec)

-15.30000019 [mas/yr] (UCAC4)

Parallax

0.0 [mas/yr] (UCAC4)

Radial Velocity

nan [mas/yr] (None)

Aliases

** HER 10B, 2MASS J04313843+1813576, 2XMM J043138.4+181357, AAVSO 0425+18B, AKARI-IRC-V1 J0431384+181357, EPIC 210690913, GBS-VLA J043138.42+181357.3, GSC 01269-01065, HBC 49, HH 150, Haro 6-14, JCMTSE J043138.3+181356, JCMTSF J043138.3+181356, JP11 5275, SDSS J043138.46+181357.8, SSV LDN 1551 1, TIC 353752575, UCAC2 38202581, UCAC4 542-009387, V* HL Tau, WDS J04317+1814B, WISE J043138.43+181357.5, WISEA J043138.48+181357.6, XEST 22-043, [BFR2003] 35, [FGM2003] 29, [FGM2003] S19, [FK83] LDN 1551 11, [GBA2007] 1319, [GMM2009] Tau L1551 2, ** HER 10B, HBC 49, HH 150, HLTAU, HLTau, JP11 5275, SSV LDN 1551 1, UCAC2 38202581, [GMM2009] Tau L1551 2, hl tau, **HER10B, 2MASSJ04313843+1813576, 2XMMJ043138.4+181357, AAVSO0425+18B, AKARI-IRC-V1J0431384+181357, EPIC210690913, GBS-VLAJ043138.42+181357.3, GSC01269-01065, HBC49, HH150, Haro6-14, JCMTSEJ043138.3+181356, JCMTSFJ043138.3+181356, JP115275, SDSSJ043138.46+181357.8, SSVLDN15511, TIC353752575, UCAC238202581, UCAC4542-009387, V*HLTau, WDSJ04317+1814B, WISEJ043138.43+181357.5, WISEAJ043138.48+181357.6, XEST22-043, [BFR2003]35, [FGM2003]29, [FGM2003]S19, [FK83]LDN155111, [GBA2007]1319, [GMM2009]TauL15512, **HER10B, HBC49, HH150, HLTAU, HLTau, JP115275, SSVLDN15511, UCAC238202581, [GMM2009]TauL15512, hltau

OBJECT name(s) in headers

HLTau

PI name(s) in headers

Claire Moutou, Jean-Francois Donati

Project/Run name(s) in headers

18BE99, 18BD50, 20BP40

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_HLTAU_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

276445.95 \(\pm\) 15726.81 m/s

CCF FWHM

4199.11 \(\pm\) 2970.84 m/s

Number of CCF files Total

28

Number of CCF passed QC

28

Number CCF files failed QC

0

First ccf file [Mid exposure]

2018-09-22 14:18:18.854

Last ccf file [Mid exposure]

2020-09-22 13:28:36.168

Last processed [ccf]

2025-04-29 20:38:53.072

Version [ccf]

0.7.292,0.7.293

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HLTAU_spirou_offline_udem_file_list.txt

2026-02-12 20:47:22.970

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_HLTAU_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_HLTAU_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HLTAU_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HLTAU_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_HLTAU_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.