IOTCYG (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:48:08.371891 (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 |
|
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, HD184006 |
PI name(s) in headers |
QSO Team, Claire Moutou, Rosine Lallement |
Project/Run name(s) in headers |
25BQ58, 25AQ58, 20AQ58, 20BQ58, 21AQ58, 21BQ58, 22AQ58, 23AQ58, 23BQ58, 24AQ58, 24BQ58, 18BE93, 19AQ58, 19BF14, 19BQ58 |
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.
CCF stats |
|
|---|---|
Mask used |
GL846_neg.fits |
CCF systemic velocity |
299923.00 \(\pm\) 3146.87 m/s |
CCF FWHM |
13971.70 \(\pm\) 96256.62 m/s |
Number of CCF files Total |
66 |
Number of CCF passed QC |
66 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2018-09-25 08:33:09.265 |
Last ccf file [Mid exposure] |
2025-11-06 05:15:28.618 |
Last processed [ccf] |
2026-01-07 12:15:55.781 |
Version [ccf] |
0.7.294,0.7.292,0.7.295,0.7.293 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:48:20.555 |
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¶
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¶
Maximum saturation level measured at time of extraction
Measured effective readout noise before extraction¶
Measured effective readout noise before extraction
APERO Processing Debug Plot¶
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¶
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.