UMON (spirou_offline_udem)

This page was last modified: 2026-02-12 21:12:25.592344 (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=UMON

Target Information

RA

112.6977619 [deg] (Gaia DR2)

Dec

-9.776871634 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

5719.0 [K] (2014AJ….147..137L)

Spectral Type

G8/K0Ib/II (1999MSS…C05….0H)

Proper Motion (RA)

-10.12402559 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

3.267905643 [mas/yr] (Gaia DR2)

Parallax

0.9160545006 [mas/yr] (Gaia DR2)

Radial Velocity

34.6 [mas/yr] (1953GCRV..C……0W)

Aliases

2MASS J07304746-0946366, AAVSO 0726-09, BD-09 2085, GC 10054, GCRV 5005, GEN# +1.00059693, GSC 05400-04699, GSC2 S1031232880, Gaia DR2 3035408251728251520, HD 59693, HERZ 12707, HIC 36521, HIP 36521, IRAS 07284-0940, MSX5C G226.1409+04.1531, MSX6C G226.1416+04.1537, PLX 1777, PLX 1777.00, PPM 190345, RAFGL 1135, SAO 134775, SKY# 13755, TIC 6423203, TYC 5400-4699-1, UCAC3 161-67065, V* U Mon, WEB 7265, YZ 99 2696, [LTY2003] NIRS 07284-0940, BD-09 2085, GCRV 5005, HD 59693, HIC 36521, HIP 36521, UMON, UMon, WEB 7265, YZ 99 2696, 2MASSJ07304746-0946366, AAVSO0726-09, BD-092085, GC10054, GCRV5005, GEN#+1.00059693, GSC05400-04699, GSC2S1031232880, GaiaDR23035408251728251520, HD59693, HERZ12707, HIC36521, HIP36521, IRAS07284-0940, MSX5CG226.1409+04.1531, MSX6CG226.1416+04.1537, PLX1777, PLX1777.00, PPM190345, RAFGL1135, SAO134775, SKY#13755, TIC6423203, TYC5400-4699-1, UCAC3161-67065, V*UMon, WEB7265, YZ992696, [LTY2003]NIRS07284-0940, BD-092085, GCRV5005, HD59693, HIC36521, HIP36521, UMON, UMon, WEB7265, YZ992696

OBJECT name(s) in headers

UMon

PI name(s) in headers

Claire Moutou

Project/Run name(s) in headers

18BE99

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_UMON_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

300013.27 \(\pm\) 129745.62 m/s

CCF FWHM

130891.73 \(\pm\) 56902.18 m/s

Number of CCF files Total

16

Number of CCF passed QC

16

Number CCF files failed QC

0

First ccf file [Mid exposure]

2018-09-26 15:21:22.938

Last ccf file [Mid exposure]

2018-10-26 15:46:43.803

Last processed [ccf]

2025-02-23 21:22:14.889

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_UMON_spirou_offline_udem_file_list.txt

2026-02-12 21:12:30.497

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_UMON_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_UMON_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_UMON_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_UMON_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_UMON_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.