HD157347 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:41:42.950722 (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=HD157347

Target Information

RA

260.7139087 [deg] (Gaia DR2)

Dec

-2.388643085 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

5630.0 [K] (2021AJ….161..134H)

Spectral Type

G3V (2003AJ….126.2048G)

Proper Motion (RA)

48.70731348 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-108.0826657 [mas/yr] (Gaia DR2)

Parallax

50.85907333 [mas/yr] (Gaia DR2)

Radial Velocity

-35.861 [mas/yr] (2018A&A…616A…7S)

Aliases

** RAG 9A, 2MASS J17225127-0223173, AG-02 1040, BD-02 4343, GC 23493, GCRV 26109, GEN# +1.00157347, GSC 05071-00891, Gaia DR1 4367026298788236288, Gaia DR2 4367026303085396352, HD 157347, HIC 85042, HIP 85042, HR 6465, IRAS 17202-0220, PPM 180049, RAVE J172251.3-022317, SAO 141642, SKY# 31358, SPOCS 752, TD1 20332, TIC 59476871, TYC 5071-891-1, UBV 14811, UBV M 22147, WDS J17229-0223A, WEB 14362, YZ 92 5866, uvby98 100157347, ** RAG 9A, BD-02 4343, HD157347, HD_157347, HIC 85042, HIP 85042, HR 6465, SPOCS 752, UBV 14811, UBV M 22147, YZ 92 5866, **RAG9A, 2MASSJ17225127-0223173, AG-021040, BD-024343, GC23493, GCRV26109, GEN#+1.00157347, GSC05071-00891, GaiaDR14367026298788236288, GaiaDR24367026303085396352, HD157347, HIC85042, HIP85042, HR6465, IRAS17202-0220, PPM180049, RAVEJ172251.3-022317, SAO141642, SKY#31358, SPOCS752, TD120332, TIC59476871, TYC5071-891-1, UBV14811, UBVM22147, WDSJ17229-0223A, WEB14362, YZ925866, uvby98100157347, **RAG9A, BD-024343, HD157347, HD157347, HIC85042, HIP85042, HR6465, SPOCS752, UBV14811, UBVM22147, YZ925866

OBJECT name(s) in headers

HD157347

PI name(s) in headers

Lauren Weiss

Project/Run name(s) in headers

19AH28

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_HD157347_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-35119.91 \(\pm\) 75.86 m/s

CCF FWHM

8403.10 \(\pm\) 415.86 m/s

Number of CCF files Total

33

Number of CCF passed QC

33

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-04-16 11:38:31.396

Last ccf file [Mid exposure]

2019-06-19 12:14:38.455

Last processed [ccf]

2025-02-23 21:08:23.814

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HD157347_spirou_offline_udem_file_list.txt

2026-02-12 20:41:48.806

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_HD157347_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_HD157347_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD157347_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD157347_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_HD157347_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.