PI_02ORI (spirou_test_07)

This page was last modified: 2025-04-24 02:18:06.506388 (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=PI_02ORI

Target Information

RA

72.6530173 [deg] (Gaia DR2)

Dec

8.900053883 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

7500.0 [K] (2016A&A…589A..83G)

Spectral Type

A1Vn (None)

Proper Motion (RA)

1.337105405 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-27.98165285 [mas/yr] (Gaia DR2)

Parallax

17.51629856 [mas/yr] (Gaia DR2)

Radial Velocity

24.4 [mas/yr] (2006AstL…32..759G)

Aliases

* 2 Ori, * pi.02 Ori, 2MASS J04503674+0854004, AG+08 506, BD+08 777, CEL 472, GC 5892, GCRV 2846, GEN# +1.00030739, GSC 00683-01217, Gaia DR2 3289827339648726272, HD 30739, HGAM 346, HIC 22509, HIP 22509, HR 1544, IRAS 04478+0848, JP11 935, PLX 1082, PLX 1082.00, PPM 148045, ROT 684, SAO 112124, SKY# 7533, TD1 3609, TIC 399669624, TYC 683-1217-1, UBV 4648, UBV M 10369, WEB 4343, WISE J045036.73+085400.5, WISEA J045036.74+085400.4, YZ 8 1821, [SC93b] 6, uvby98 100030739, * 2 Ori, AG+08 506, BD+08 777, CEL 472, GC 5892, GCRV 2846, HD 30739, HGAM 346, HIC 22509, HIP 22509, HR 1544, JP11 935, PI.02ORI, PI_02ORI, ROT 684, SKY# 7533, TD1 3609, TYC 683-1217-1, UBV 4648, UBV M 10369, WEB 4343, YZ 8 1821, [SC93b] 6, pi.02Ori, *2Ori, *pi.02Ori, 2MASSJ04503674+0854004, AG+08506, BD+08777, CEL472, GC5892, GCRV2846, GEN#+1.00030739, GSC00683-01217, GaiaDR23289827339648726272, HD30739, HGAM346, HIC22509, HIP22509, HR1544, IRAS04478+0848, JP11935, PLX1082, PLX1082.00, PPM148045, ROT684, SAO112124, SKY#7533, TD13609, TIC399669624, TYC683-1217-1, UBV4648, UBVM10369, WEB4343, WISEJ045036.73+085400.5, WISEAJ045036.74+085400.4, YZ81821, [SC93b]6, uvby98100030739, *2Ori, AG+08506, BD+08777, CEL472, GC5892, GCRV2846, HD30739, HGAM346, HIC22509, HIP22509, HR1544, JP11935, PI.02ORI, PI02ORI, ROT684, SKY#7533, TD13609, TYC683-1217-1, UBV4648, UBVM10369, WEB4343, YZ81821, [SC93b]6, pi.02Ori

OBJECT name(s) in headers

pi.02Ori

PI name(s) in headers

QSO Team

Project/Run name(s) in headers

20BQ58

Spectrum

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

../../../_images/spec_plot_PI_02ORI_spirou_test_07.png

Spectrum Information

DPRTYPES

OBJ_DARK

Total number raw files

1

First raw files

2020-08-31 15:27:37.472

Last raw files

2020-08-31 15:27:37.472

Total number PP files

1

Number PP files passed QC

1

Number PP files failed QC

0

First pp file [Mid exposure]

2020-08-31 15:27:37.472

Last pp file [Mid exposure]

2020-08-31 15:27:37.472

Last processed [pp]

2025-04-15 12:18:58.866

Version [pp]

0.7.293

Total number ext files

1

Number ext files passed QC

1

Number ext files failed QC

0

First ext file [Mid exposure]

2020-08-31 15:27:37.472

Last ext file [Mid exposure]

2020-08-31 15:27:37.472

Last processed [ext]

2025-04-15 13:00:37.552

Version [ext]

0.7.293

Total number tcorr files

1

Number tcorr files passed QC

1

Number tcorr files failed QC

0

First tcorr file [Mid exposure]

2020-08-31 15:27:37.472

Last tcorr file [Mid exposure]

2020-08-31 15:27:37.472

Last processed [tcorr]

2025-04-15 13:15:52.783

Version [tcorr]

0.7.293

Median SNR Y

262.36 \(\pm\) 0.00

Median SNR H

291.71 \(\pm\) 0.00

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_PI_02ORI_spirou_test_07_file_list.txt

2025-04-24 02:18:10.503

Extracted 1D spectra

ext1d_PI_02ORI_spirou_test_07_file_list.txt

2025-04-24 02:18:10.503

Telluric corrected 2D spectra

tcorr2d_PI_02ORI_spirou_test_07_file_list.txt

2025-04-24 02:18:10.503

Telluric corrected 1D spectra

tcorr1d_PI_02ORI_spirou_test_07_file_list.txt

2025-04-24 02:18:10.503

Extracted 2D header file

ext2d_header_PI_02ORI_spirou_test_07_file.csv

2025-04-24 02:18:10.501

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

2020-08-31

2020-08-31 15:27:37.472

2020-08-31 15:27:37.472

1

1

0.430

1.059

61.291

61.291

262.361

291.715

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_PI_02ORI_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_PI_02ORI_spirou_test_07.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_PI_02ORI_spirou_test_07.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_PI_02ORI_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_PI_02ORI_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.