V1057CYG (spirou_offline_udem)

This page was last modified: 2026-02-12 21:12:24.990764 (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=V1057CYG

Target Information

RA

314.7238735 [deg] (Gaia DR2)

Dec

44.25786821 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

2100.0 [K] (HEADER[CFHT])

Spectral Type

F7/G3I/IIe (2003ApJ…595..384H)

Proper Motion (RA)

-2.79307162 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-3.813038634 [mas/yr] (Gaia DR2)

Parallax

1.0864028 [mas/yr] (Gaia DR2)

Radial Velocity

nan [mas/yr] (None)

Aliases

2MASS J20585371+4415283, AAVSO 2055+43, ATO J314.7238+44.2578, CSI+44-20571 2, EM* LkHA 190, EM* UHA 94, GEN# +6.20038190, GSC 03179-01055, Gaia DR2 2162235662383047040, HBC 300, HBHA 4204-02, JP11 5293, JP11 5439, MSX6C G085.4897-01.0466, SV* SON 7817, TIC 329612015, UCAC4 672-087538, V* V1057 Cyg, WISE J205853.71+441528.2, WISEA J205853.72+441528.3, [KW97] 53-38, [PCC93] 435, [RGS2011] J205853.74+441528.3, uvby98 610300300, CSI+44-20571 2, EM* LkHA 190, EM* UHA 94, JP11 5293, JP11 5439, SV* SON 7817, V1057CYG, V1057Cyg, 2MASSJ20585371+4415283, AAVSO2055+43, ATOJ314.7238+44.2578, CSI+44-205712, EM*LkHA190, EM*UHA94, GEN#+6.20038190, GSC03179-01055, GaiaDR22162235662383047040, HBC300, HBHA4204-02, JP115293, JP115439, MSX6CG085.4897-01.0466, SV*SON7817, TIC329612015, UCAC4672-087538, V*V1057Cyg, WISEJ205853.71+441528.2, WISEAJ205853.72+441528.3, [KW97]53-38, [PCC93]435, [RGS2011]J205853.74+441528.3, uvby98610300300, CSI+44-205712, EM*LkHA190, EM*UHA94, JP115293, JP115439, SV*SON7817, V1057CYG, V1057Cyg

OBJECT name(s) in headers

V1057Cyg

PI name(s) in headers

Michihiro Takami

Project/Run name(s) in headers

19AT02

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_V1057CYG_spirou_offline_udem.png

CCF stats

Mask used

GL905_neg.fits

CCF systemic velocity

293440.83 \(\pm\) 156482.87 m/s

CCF FWHM

34026.74 \(\pm\) 49504.50 m/s

Number of CCF files Total

12

Number of CCF passed QC

12

Number CCF files failed QC

0

First ccf file [Mid exposure]

2019-04-15 15:06:01.136

Last ccf file [Mid exposure]

2019-06-16 11:44:00.362

Last processed [ccf]

2025-02-23 20:58:58.437

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_V1057CYG_spirou_offline_udem_file_list.txt

2026-02-12 21:12:28.442

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_V1057CYG_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_V1057CYG_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_V1057CYG_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_V1057CYG_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_V1057CYG_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.