HERSCHEL36 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:47:12.339482 (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=HERSCHEL36

Target Information

RA

270.9180101 [deg] (Gaia DR2)

Dec

-24.37858121 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

8000.0 [K] (HEADER[CFHT])

Spectral Type

O7:V (2014ApJS..211…10S)

Proper Motion (RA)

2.018438477 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-2.048522455 [mas/yr] (Gaia DR2)

Parallax

0.9017957926 [mas/yr] (Gaia DR2)

Radial Velocity

-3.0 [mas/yr] (1953GCRV..C……0W)

Aliases

** AEN 1A, ** SBE 1, 2MASS J18034033-2422427, ALS 4589, CD-24 13806, CPD-24 6137, Cl* NGC 6530 CDZ 53, Cl* NGC 6530 SCB 144, Cl* NGC 6530 VAJ 105, Cl* NGC 6530 ZCW 134, GCRV 10486, GOS G005.97-01.17 01, Gaia DR2 4066021251107926272, LS 4589, NAME Her 36, NAME Herschel 36, NGC 6530 177, NSV 10081, TIC 406748532, UCAC4 329-121973, WDS J18037-2423A, WDS J18037-2423Aa,Ab, [KA2010] 0/I 25, ** AEN 1A, ALS 4589, CPD-24 6137, Cl* NGC 6530 CDZ 53, Cl* NGC 6530 SCB 144, Cl* NGC 6530 VAJ 105, Cl* NGC 6530 ZCW 134, HERSCHEL36, Herschel 36, Herschel36, NGC 6530 177, **AEN1A, **SBE1, 2MASSJ18034033-2422427, ALS4589, CD-2413806, CPD-246137, Cl*NGC6530CDZ53, Cl*NGC6530SCB144, Cl*NGC6530VAJ105, Cl*NGC6530ZCW134, GCRV10486, GOSG005.97-01.1701, GaiaDR24066021251107926272, LS4589, NAMEHer36, NAMEHerschel36, NGC6530177, NSV10081, TIC406748532, UCAC4329-121973, WDSJ18037-2423A, WDSJ18037-2423Aa,Ab, [KA2010]0/I25, **AEN1A, ALS4589, CPD-246137, Cl*NGC6530CDZ53, Cl*NGC6530SCB144, Cl*NGC6530VAJ105, Cl*NGC6530ZCW134, HERSCHEL36, Herschel36, Herschel36, NGC6530177

OBJECT name(s) in headers

Herschel36

PI name(s) in headers

Sheng-Yuan Liu

Project/Run name(s) in headers

19BT09

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_HERSCHEL36_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

295624.02 \(\pm\) 1709.39 m/s

CCF FWHM

2624.86 \(\pm\) 323.14 m/s

Number of CCF files Total

4

Number of CCF passed QC

4

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-10-09 04:58:39.979

Last ccf file [Mid exposure]

2019-10-09 05:12:19.293

Last processed [ccf]

2025-02-23 20:41:51.282

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HERSCHEL36_spirou_offline_udem_file_list.txt

2026-02-12 20:47:14.992

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_HERSCHEL36_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_HERSCHEL36_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HERSCHEL36_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HERSCHEL36_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_HERSCHEL36_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.