IOTCYG (spirou_test_07)

This page was last modified: 2025-07-09 16:23:28.242976 (UTC)

Back to the object table

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=IOTCYG

Target Information

RA

292.4266376 [deg] (Gaia DR2)

Dec

51.73032873 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

7500.0 [K] (2016A&A…589A..83G)

Spectral Type

A5V (2010A&A…521A…5C)

Proper Motion (RA)

20.07199665 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

127.5134244 [mas/yr] (Gaia DR2)

Parallax

27.06034939 [mas/yr] (Gaia DR2)

Radial Velocity

-19.5 [mas/yr] (1953GCRV..C……0W)

Aliases

* 10 Cyg, * iot Cyg, * iot02 Cyg, 2MASS J19294236+5143472, AG+51 1322, BD+51 2605, CEL 4776, FK5 733, GC 26947, GCRV 11936, GEN# +1.00184006, GSC 03555-02112, Gaia DR2 2136270970157966464, HD 184006, HIC 95853, HIP 95853, HR 7420, IRAS 19284+5137, JP11 3110, KIC 12650049, N30 4326, PLX 4570, PLX 4570.00, PMC 90-93 522, PPM 37459, ROT 2809, SAO 31702, SKY# 36306, TD1 24876, TIC 424870548, TYC 3555-2112-1, UBV 16566, UBV M 23857, WEB 16783, YZ 51 6043, uvby98 100184006, * 10 Cyg, BD+51 2605, CEL 4776, FK5 733, HD184006, HIC 95853, HIP 95853, HR 7420, IOTCYG, JP11 3110, PMC 90-93 522, PPM 37459, ROT 2809, SAO 31702, UBV 16566, UBV M 23857, YZ 51 6043, iotCyg, *10Cyg, *iotCyg, *iot02Cyg, 2MASSJ19294236+5143472, AG+511322, BD+512605, CEL4776, FK5733, GC26947, GCRV11936, GEN#+1.00184006, GSC03555-02112, GaiaDR22136270970157966464, HD184006, HIC95853, HIP95853, HR7420, IRAS19284+5137, JP113110, KIC12650049, N304326, PLX4570, PLX4570.00, PMC90-93522, PPM37459, ROT2809, SAO31702, SKY#36306, TD124876, TIC424870548, TYC3555-2112-1, UBV16566, UBVM23857, WEB16783, YZ516043, uvby98100184006, *10Cyg, BD+512605, CEL4776, FK5733, HD184006, HIC95853, HIP95853, HR7420, IOTCYG, JP113110, PMC90-93522, PPM37459, ROT2809, SAO31702, UBV16566, UBVM23857, YZ516043, iotCyg

OBJECT name(s) in headers

iotCyg

PI name(s) in headers

QSO Team

Project/Run name(s) in headers

20AQ58, 20BQ58

Spectrum

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

../../../_images/spec_plot_IOTCYG_spirou_test_07.png

Spectrum Information

DPRTYPES

OBJ_DARK

Total number raw files

2

First raw files

2020-08-01 09:11:56.601

Last raw files

2020-08-10 09:32:35.958

Total number PP files

2

Number PP files passed QC

2

Number PP files failed QC

0

First pp file [Mid exposure]

2020-08-01 09:11:56.601

Last pp file [Mid exposure]

2020-08-10 09:32:35.958

Last processed [pp]

2025-04-15 13:17:05.971

Version [pp]

0.7.293

Total number ext files

2

Number ext files passed QC

2

Number ext files failed QC

0

First ext file [Mid exposure]

2020-08-01 09:11:56.601

Last ext file [Mid exposure]

2020-08-10 09:32:35.958

Last processed [ext]

2025-04-15 15:33:42.975

Version [ext]

0.7.293

Total number tcorr files

2

Number tcorr files passed QC

2

Number tcorr files failed QC

0

First tcorr file [Mid exposure]

2020-08-01 09:11:56.601

Last tcorr file [Mid exposure]

2020-08-10 09:32:35.958

Last processed [tcorr]

2025-04-15 16:26:19.043

Version [tcorr]

0.7.293

Median SNR Y

289.66 \(\pm\) 0.96

Median SNR H

340.89 \(\pm\) 4.88

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_IOTCYG_spirou_test_07_file_list.txt

2025-07-09 16:23:31.065

Extracted 1D spectra

ext1d_IOTCYG_spirou_test_07_file_list.txt

2025-07-09 16:23:31.065

Telluric corrected 2D spectra

tcorr2d_IOTCYG_spirou_test_07_file_list.txt

2025-07-09 16:23:31.065

Telluric corrected 1D spectra

tcorr1d_IOTCYG_spirou_test_07_file_list.txt

2025-07-09 16:23:31.065

Extracted 2D header file

ext2d_header_IOTCYG_spirou_test_07_file.csv

2025-07-09 16:23:31.064

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

2020-08-01

2020-08-01 09:11:56.601

2020-08-01 09:11:56.601

1

1

0.560

1.178

50.147

50.147

288.244

348.034

OBJ_DARK

1 [download]

1 [download]

Extracted 2D files

Telluric corrected 2D files

2020-08-10

2020-08-10 09:32:35.958

2020-08-10 09:32:35.958

1

1

0.650

1.204

50.147

50.147

291.068

333.742

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_IOTCYG_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_IOTCYG_spirou_test_07.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_IOTCYG_spirou_test_07.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_IOTCYG_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_IOTCYG_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.