HD136378 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:40:03.684093 (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=HD136378

Target Information

RA

230.1094582 [deg] (Gaia EDR3)

Dec

0.2435334907 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

5186.0 [K] (2018MNRAS.479.1332M)

Spectral Type

K1V (1999MSS…C05….0H)

Proper Motion (RA)

132.2311526 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-254.2802622 [mas/yr] (Gaia EDR3)

Parallax

23.28139911 [mas/yr] (Gaia EDR3)

Radial Velocity

-7.76 [mas/yr] (2018MNRAS.479.1332M)

Aliases

G 15-17, AG+00 1843, ASCC 1142937, BD+00 3346, CCDM J15204+0014A, GEN# +1.00136378, HD 136378, HIC 75069, HIP 75069, IDS 15153+0036 A, LSPM J1520+0014, LTT 14559, 2MASS J15202613+0014407, NLTT 39941, PPM 161468, SAO 120952, TIC 461311923, TYC 336-530-1, UBV M 20707, UCAC2 31877213, USNO-B1.0 0902-00244747, uvby98 100136378, WDS J15204+0015A, WISEA J152026.21+001438.2, YZC 21 3916, YZ 0 3916, Gaia DR2 4418850954729363584, Gaia EDR3 4418850954729363584, Gaia DR1 4418850954729363584, G15-17, AG+001843, ASCC1142937, BD+003346, CCDMJ15204+0014A, GEN#+1.00136378, HD136378, HIC75069, HIP75069, IDS15153+0036A, LSPMJ1520+0014, LTT14559, 2MASSJ15202613+0014407, NLTT39941, PPM161468, SAO120952, TIC461311923, TYC336-530-1, UBVM20707, UCAC231877213, USNO-B1.00902-00244747, uvby98100136378, WDSJ15204+0015A, WISEAJ152026.21+001438.2, YZC213916, YZ03916, GaiaDR24418850954729363584, GaiaEDR34418850954729363584, GaiaDR14418850954729363584

OBJECT name(s) in headers

HD 136378

PI name(s) in headers

Ryan Cloutier

Project/Run name(s) in headers

21AC33, 22AC25

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_HD136378_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-7422.88 \(\pm\) 63.05 m/s

CCF FWHM

8444.69 \(\pm\) 130.22 m/s

Number of CCF files Total

5

Number of CCF passed QC

5

Number CCF files failed QC

0

First ccf file [Mid exposure]

2021-03-04 15:51:17.130

Last ccf file [Mid exposure]

2022-03-17 14:56:51.837

Last processed [ccf]

2025-02-23 18:31:28.919

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HD136378_spirou_offline_udem_file_list.txt

2026-02-12 20:40:05.993

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_HD136378_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_HD136378_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD136378_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD136378_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_HD136378_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.