HD146868 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:41:36.686000 (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=HD146868

Target Information

RA

243.7380712 [deg] (Gaia EDR3)

Dec

60.67175125 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

5610.0 [K] (2018MNRAS.479.1332M)

Spectral Type

G4 (1985ApJS…59..197B)

Proper Motion (RA)

27.98359267 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

445.8771931 [mas/yr] (Gaia EDR3)

Parallax

32.3407343 [mas/yr] (Gaia EDR3)

Radial Velocity

-17.95 [mas/yr] (2018MNRAS.479.1332M)

Aliases

G 240-11, ** LDS 1434A, AG+60 1009, ASCC 133663, BD+61 1574, CCDM J16150+6040A, Ci 18 2179, Ci 20 978, GC 21889, GEN# +1.00146868, G 225-52, G 226-2, HD 146868, HIC 79629, HIP 79629, IDS 16134+6056 A, LSPM J1614+6040, LTT 14852, 2MASS J16145709+6040109, NLTT 42399, PLX 3700, PPM 19789, SAO 17004, TIC 198160324, TYC 4189-1345-1, USNO-B1.0 1506-00225794, uvby98 100146868, WDS J16150+6040A, WISEA J161457.12+604015.9, WISE J161457.13+604015.8, Gaia DR2 1625058605098521600, Gaia EDR3 1625058605098521600, Gaia DR1 1625058600802062208, G240-11, **LDS1434A, AG+601009, ASCC133663, BD+611574, CCDMJ16150+6040A, Ci182179, Ci20978, GC21889, GEN#+1.00146868, G225-52, G226-2, HD146868, HIC79629, HIP79629, IDS16134+6056A, LSPMJ1614+6040, LTT14852, 2MASSJ16145709+6040109, NLTT42399, PLX3700, PPM19789, SAO17004, TIC198160324, TYC4189-1345-1, USNO-B1.01506-00225794, uvby98100146868, WDSJ16150+6040A, WISEAJ161457.12+604015.9, WISEJ161457.13+604015.8, GaiaDR21625058605098521600, GaiaEDR31625058605098521600, GaiaDR11625058600802062208

OBJECT name(s) in headers

HD 146868

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_HD146868_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-17391.83 \(\pm\) 8.50 m/s

CCF FWHM

8571.99 \(\pm\) 192.84 m/s

Number of CCF files Total

3

Number of CCF passed QC

3

Number CCF files failed QC

0

First ccf file [Mid exposure]

2021-03-20 15:51:59.790

Last ccf file [Mid exposure]

2022-01-28 16:21:03.508

Last processed [ccf]

2025-02-23 18:30:49.454

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HD146868_spirou_offline_udem_file_list.txt

2026-02-12 20:41:38.797

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_HD146868_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_HD146868_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD146868_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD146868_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_HD146868_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.