HD144579 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:41:36.243033 (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=HD144579

Target Information

RA

241.2333681 [deg] (Gaia EDR3)

Dec

39.15674358 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

5140.0 [K] (2021AJ….161..134H)

Spectral Type

G8V (2009ApJ…694.1085V)

Proper Motion (RA)

-570.8715972 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

52.63317555 [mas/yr] (Gaia EDR3)

Parallax

69.64054505 [mas/yr] (Gaia EDR3)

Radial Velocity

-59.442 [mas/yr] (2018A&A…616A…7S)

Aliases

LHS 3152, ** WNO 47A, AG+39 1556, AGKR 14350, ASCC 499773, BD+39 2947, CCDM J16049+3909A, Ci 20 965, GC 21623, GCRV 9256, GEN# +1.00144579, GJ 611 A, HD 144579, HIC 78775, HIP 78775, IDS 16013+3926 A, IRAS 16031+3917, LFT 1247, LSPM J1604+3909E, LTT 14788, 2MASS J16045689+3909234, NLTT 41938, PLX 3650, PPM 79018, SAO 65065, SKY# 29032, SPOCS 683, TIC 24089803, TYC 3061-1027-1, UBV 13642, UBV M 21161, USNO-B1.0 1291-00256810, uvby98 100144579, VVO 371, WDS J16048+3910A, WEB 13319, WISEA J160456.29+390923.9, Gaia DR2 1379500756257031808, Gaia EDR3 1379500756257031808, Gaia DR1 1379500751961664640, LHS3152, **WNO47A, AG+391556, AGKR14350, ASCC499773, BD+392947, CCDMJ16049+3909A, Ci20965, GC21623, GCRV9256, GEN#+1.00144579, GJ611A, HD144579, HIC78775, HIP78775, IDS16013+3926A, IRAS16031+3917, LFT1247, LSPMJ1604+3909E, LTT14788, 2MASSJ16045689+3909234, NLTT41938, PLX3650, PPM79018, SAO65065, SKY#29032, SPOCS683, TIC24089803, TYC3061-1027-1, UBV13642, UBVM21161, USNO-B1.01291-00256810, uvby98100144579, VVO371, WDSJ16048+3910A, WEB13319, WISEAJ160456.29+390923.9, GaiaDR21379500756257031808, GaiaEDR31379500756257031808, GaiaDR11379500751961664640

OBJECT name(s) in headers

HD 144579

PI name(s) in headers

Ryan Cloutier

Project/Run name(s) in headers

21AC33

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_HD144579_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-58807.28 \(\pm\) 2.50 m/s

CCF FWHM

7274.49 \(\pm\) 3.30 m/s

Number of CCF files Total

2

Number of CCF passed QC

2

Number CCF files failed QC

0

First ccf file [Mid exposure]

2021-02-21 15:35:29.681

Last ccf file [Mid exposure]

2021-02-21 16:15:54.091

Last processed [ccf]

2025-02-23 18:30:59.751

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HD144579_spirou_offline_udem_file_list.txt

2026-02-12 20:41:37.865

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_HD144579_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_HD144579_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD144579_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD144579_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_HD144579_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.