HD195094 (spirou_test_07)

This page was last modified: 2025-04-24 02:17:57.892311 (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=HD195094

Target Information

RA

307.4747591 [deg] (Gaia EDR3)

Dec

-18.58354497 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

8913.0 [K] (2012A&A…537A.120Z (via spirou@rali))

Spectral Type

A1V (1988MSS…C04….0H)

Proper Motion (RA)

29.05787637 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-81.32583884 [mas/yr] (Gaia EDR3)

Parallax

14.01927556 [mas/yr] (Gaia EDR3)

Radial Velocity

-12.4 [mas/yr] (2006AstL…32..759G)

Aliases

* 12 Cap A, * omi Cap A, ADS 13902 A, BD-19 5831, CCDM J20299-1835A, GC 28503, GSC 06333-02130, HD 195094, HIC 101123, HIP 101123, HR 7830, IDS 20242-1855 A, 2MASS J20295391-1834593, PPM 237509, ROT 2984, SAO 163626, SKY# 38780, TIC 72429235, TYC 6333-2130-1, UBV 17760, UBV M 24874, uvby98 100195094 A, WDS J20299-1835A, YZ 108 8789, Gaia DR1 6860821646719117952, Gaia EDR3 6860821651019024896, Gaia DR2 6860821651019024896, *12CapA, *omiCapA, ADS13902A, BD-195831, CCDMJ20299-1835A, GC28503, GSC06333-02130, HD195094, HIC101123, HIP101123, HR7830, IDS20242-1855A, 2MASSJ20295391-1834593, PPM237509, ROT2984, SAO163626, SKY#38780, TIC72429235, TYC6333-2130-1, UBV17760, UBVM24874, uvby98100195094A, WDSJ20299-1835A, YZ1088789, GaiaDR16860821646719117952, GaiaEDR36860821651019024896, GaiaDR26860821651019024896, HR7830, HR 7830, ADS 13902 A, OMICAPA, ADS13902A

OBJECT name(s) in headers

omiCapA

PI name(s) in headers

QSO Team

Spectrum

This section presents the observation after extraction,with and without telluric correction.

../../../_images/spec_plot_HD195094_spirou_test_07.png

Spectrum Information

DPRTYPES

OBJ_DARK

Total number raw files

3

First raw files

2020-07-30 10:33:20.601

Last raw files

2020-10-07 06:38:35.335

Total number PP files

3

Number PP files passed QC

3

Number PP files failed QC

0

First pp file [Mid exposure]

2020-07-30 10:33:20.601

Last pp file [Mid exposure]

2020-10-07 06:38:35.335

Last processed [pp]

2025-04-15 12:17:54.652

Version [pp]

0.7.293

Total number ext files

3

Number ext files passed QC

3

Number ext files failed QC

0

First ext file [Mid exposure]

2020-07-30 10:33:20.601

Last ext file [Mid exposure]

2020-10-07 06:38:35.335

Last processed [ext]

2025-04-15 13:00:37.524

Version [ext]

0.7.293

Total number tcorr files

3

Number tcorr files passed QC

3

Number tcorr files failed QC

0

First tcorr file [Mid exposure]

2020-07-30 10:33:20.601

Last tcorr file [Mid exposure]

2020-10-07 06:38:35.335

Last processed [tcorr]

2025-04-15 13:15:52.757

Version [tcorr]

0.7.293

Median SNR Y

235.78 \(\pm\) 4.35

Median SNR H

262.20 \(\pm\) 3.49

Request

Extracted 2D spectra

Extracted 1D spectra

Telluric corrected 2D spectra

Telluric corrected 1D spectra

2D Template (after telluric correction)

1D Template (after telluric correction)

Packaged extraction files (e.fits)

Packaged telluric corrected files (t.fits)

Packaged s1d extract+tcorr (s.fits)

Packaged velocity files (v.fits)

Packaged polarimetry files (p.fits)

Spectrum Downloads

File URL

Uploaded

Extracted 2D spectra

ext2d_HD195094_spirou_test_07_file_list.txt

2025-04-24 02:18:03.056

Extracted 1D spectra

ext1d_HD195094_spirou_test_07_file_list.txt

2025-04-24 02:18:03.056

Telluric corrected 2D spectra

tcorr2d_HD195094_spirou_test_07_file_list.txt

2025-04-24 02:18:03.056

Telluric corrected 1D spectra

tcorr1d_HD195094_spirou_test_07_file_list.txt

2025-04-24 02:18:03.057

Extracted 2D header file

ext2d_header_HD195094_spirou_test_07_file.csv

2025-04-24 02:18:03.055

LBL

No LBL reduction found

CCF

No CCF files found

Time series

This section deals with providing the time series information for this object

Obs Dir

First obs mid

Last obs mid

Number of ext

Number of tcorr

Seeing

Airmass

Mean Exptime

Total Exptime

SNR[Order 8 (#71 1.08um)]

SNR[Order 35 (#44 1.75um)]

DPRTYPEs

ext_files

tcorr_files

Request ext files

Request tcorr files

2020-07-30

2020-07-30 10:33:20.601

2020-07-30 10:33:20.601

1

1

-9999.900

1.277

300.884

300.884

226.353

271.051

OBJ_DARK

1 [download]

1 [download]

Extracted 2D files

Telluric corrected 2D files

2020-08-10

2020-08-10 10:02:44.557

2020-08-10 10:02:44.557

1

1

0.460

1.283

289.740

289.740

235.779

262.199

OBJ_DARK

1 [download]

1 [download]

Extracted 2D files

Telluric corrected 2D files

2020-10-07

2020-10-07 06:38:35.335

2020-10-07 06:38:35.335

1

1

0.510

1.308

289.740

289.740

239.104

260.820

OBJ_DARK

1 [download]

1 [download]

Extracted 2D files

Telluric corrected 2D files

Debug

This section has various debug plots from APERO products

Telluric map

../../../_images/debug_tcorr_map_plot_HD195094_spirou_test_07.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_HD195094_spirou_test_07.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD195094_spirou_test_07.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD195094_spirou_test_07.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_HD195094_spirou_test_07.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.