DN_TAU (spirou_offline_udem)

This page was last modified: 2026-02-12 19:41:05.223215 (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=DN_TAU

Target Information

RA

68.86410202 [deg] (Gaia DR2)

Dec

24.24960745 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

3805.0 [K] (via spdrs@apikipiha)

Spectral Type

M1:Ve (1977ApJ…214..747H)

Proper Motion (RA)

6.054573777 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-20.77133084 [mas/yr] (Gaia DR2)

Parallax

7.79905153 [mas/yr] (Gaia DR2)

Radial Velocity

17.408199 [mas/yr] (2020AJ….160..120J)

Aliases

GSC 01829-00026, AKARI-IRC-V1 J0435273+241458, AP J04352737+2414589, CSI+24-04324, 2E 1100, 2E 0432.4+2409, EPIC 247776947, GALEX J043527.3+241458, GCRV 55208, GEN# +6.20078065, HBC 65, IRAS F04324+2408, IRAS 04324+2408, 2MASS J04352737+2414589, MHA 259-18, PDS 10, PSCz P04324+2408, SSTtau 043527.3+241458, SV* SVS 1084, TIC 268511247, UBV 4405, UCAC2 40304135, V* DN Tau, WISEA J043527.37+241458.6, WISE J043527.37+241458.7, XEST 12-OM-077, XEST 12-040, [ABG2007] 1753, [FK83] LDN 1529 35, [GBA2007] 1839, Gaia DR2 147606657186323712, Gaia DR3 147606657186323712, DNTau, GSC01829-00026, AKARI-IRC-V1J0435273+241458, APJ04352737+2414589, CSI+24-04324, 2E1100, 2E0432.4+2409, EPIC247776947, GALEXJ043527.3+241458, GCRV55208, GEN#+6.20078065, HBC65, IRASF04324+2408, IRAS04324+2408, 2MASSJ04352737+2414589, MHA259-18, PDS10, PSCzP04324+2408, SSTtau043527.3+241458, SV*SVS1084, TIC268511247, UBV4405, UCAC240304135, V*DNTau, WISEAJ043527.37+241458.6, WISEJ043527.37+241458.7, XEST12-OM-077, XEST12-040, [ABG2007]1753, [FK83]LDN152935, [GBA2007]1839, GaiaDR2147606657186323712, GaiaDR3147606657186323712, DNTau

OBJECT name(s) in headers

DNTau

PI name(s) in headers

Jean-Francois Donati

Project/Run name(s) in headers

23BP45

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_DN_TAU_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

17499.15 \(\pm\) 205.22 m/s

CCF FWHM

14992.51 \(\pm\) 252.15 m/s

Number of CCF files Total

131

Number of CCF passed QC

131

Number CCF files failed QC

0

First ccf file [Mid exposure]

2023-11-03 13:01:48.492

Last ccf file [Mid exposure]

2023-12-29 10:30:33.502

Last processed [ccf]

2025-02-23 15:19:46.263

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_DN_TAU_spirou_offline_udem_file_list.txt

2026-02-12 19:41:26.452

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_DN_TAU_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_DN_TAU_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_DN_TAU_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_DN_TAU_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_DN_TAU_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.