DOTAU (spirou_offline_udem)

This page was last modified: 2026-02-12 19:41:39.040713 (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=DOTAU

Target Information

RA

69.61914697 [deg] (Gaia DR2)

Dec

26.18031703 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

3736.0 [K] (2020AJ….160..120J)

Spectral Type

M1Ve (1977ApJ…214..747H)

Proper Motion (RA)

6.128117983 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-21.33953845 [mas/yr] (Gaia DR2)

Parallax

7.174606407 [mas/yr] (Gaia DR2)

Radial Velocity

16.55 [mas/yr] (2019AJ….157..196K)

Aliases

GaiaDR2148449913884294528, GaiaDR3148449913884294528, DOTAU, DO_TAU, DO TAU, UCAC2 40978501, AKARI-IRC-V1 J0438285+261048, AP J04382858+2610494, CSI+26-04354, EPIC 248049475, GCRV 55265, HBC 67, HH 230, IRAS 04353+2604, ITG 7, JCMTSE J043828.8+261050, JCMTSF J043828.8+261050, Kim 1-20, LAMOST J043828.58+261049.2, 2MASS J04382858+2610494, MHA 259-15, SSTc2d J043828.6+261049, SSTtau 043828.5+261049, SV* SVS 1086, TIC 150002984, UBV 4459, V* DO Tau, WDS J04385+2611C, WISEA J043828.58+261049.4, WISE J043828.58+261049.4, [OMK98] 34, [TNS87] 3, Gaia DR2 148449913884294528, Gaia DR3 148449913884294528, DO_TAU, UCAC240978501, AKARI-IRC-V1J0438285+261048, APJ04382858+2610494, CSI+26-04354, EPIC248049475, GCRV55265, HBC67, HH230, IRAS04353+2604, ITG7, JCMTSEJ043828.8+261050, JCMTSFJ043828.8+261050, Kim1-20, LAMOSTJ043828.58+261049.2, 2MASSJ04382858+2610494, MHA259-15, SSTc2dJ043828.6+261049, SSTtau043828.5+261049, SV*SVS1086, TIC150002984, UBV4459, V*DOTau, WDSJ04385+2611C, WISEAJ043828.58+261049.4, WISEJ043828.58+261049.4, [OMK98]34, [TNS87]3

OBJECT name(s) in headers

DOTau, DO Tau

PI name(s) in headers

Jean-Francois Donati

Project/Run name(s) in headers

25BP45, 20BP40, 23AP45, 23BP45, 24AP45, 20AP40

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_DOTAU_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

16701.26 \(\pm\) 727.74 m/s

CCF FWHM

17656.15 \(\pm\) 674.76 m/s

Number of CCF files Total

314

Number of CCF passed QC

314

Number CCF files failed QC

0

First ccf file [Mid exposure]

2020-02-19 06:57:36.252

Last ccf file [Mid exposure]

2025-11-13 13:56:33.538

Last processed [ccf]

2026-01-07 12:20:01.477

Version [ccf]

0.7.294,0.7.295,0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_DOTAU_spirou_offline_udem_file_list.txt

2026-02-12 19:42:09.619

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_DOTAU_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_DOTAU_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_DOTAU_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_DOTAU_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_DOTAU_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.