HD189733 (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:43:07.484848 (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=HD189733
Target Information |
|
|---|---|
RA |
300.1821223 [deg] (Gaia DR2) |
Dec |
22.70977592 [deg] (Gaia DR2) |
Finder chart |
|
Teff |
5070.0 [K] (2021AJ….161..134H) |
Spectral Type |
K2V (2003AJ….126.2048G) |
Proper Motion (RA) |
-3.294453262 [mas/yr] (Gaia DR2) |
Proper Motion (Dec) |
-250.2246974 [mas/yr] (Gaia DR2) |
Parallax |
50.56847245 [mas/yr] (Gaia DR2) |
Radial Velocity |
-2.317 [mas/yr] (2018A&A…616A…7S) |
Aliases |
** BAK 1A, 1RXS J200043.3+224240, 2MASS J20004370+2242391, AG+22 2072, ASCC 807144, BD+22 3887, EXO 195834+2234.6, GC 27741, GEN# +1.00189733, GJ 4130, GSC 02141-00972, Gaia DR1 1827242811876888960, Gaia DR2 1827242816201846144, HD 189733, HIC 98505, HIP 98505, LSPM J2000+2242, LTT 15851, NLTT 48568, PPM 110211, SAO 88060, SKY# 37530, SPOCS 3132, TIC 256364928, TYC 2141-972-1, USNO-B1.0 1127-00538857, V* V452 Vul, WDS J20007+2243A, WISEA J200043.63+224236.1, Wolf 864, YZ 22 7419, uvby98 100189733, ** BAK 1A, ASCC 807144, BD+22 3887, GJ 4130, HD 189733b, HD189733, HD189733B, HD_189733B, HIC 98505, HIP 98505, SAO 88060, Wolf 864, YZ 22 7419, HD189733, HD189733b, HD_189733b, HD_189733B, **BAK1A, 1RXSJ200043.3+224240, 2MASSJ20004370+2242391, AG+222072, ASCC807144, BD+223887, EXO195834+2234.6, GC27741, GEN#+1.00189733, GJ4130, GSC02141-00972, GaiaDR11827242811876888960, GaiaDR21827242816201846144, HD189733, HIC98505, HIP98505, LSPMJ2000+2242, LTT15851, NLTT48568, PPM110211, SAO88060, SKY#37530, SPOCS3132, TIC256364928, TYC2141-972-1, USNO-B1.01127-00538857, V*V452Vul, WDSJ20007+2243A, WISEAJ200043.63+224236.1, Wolf864, YZ227419, uvby98100189733, **BAK1A, ASCC807144, BD+223887, GJ4130, HD189733b, HD189733, HD189733B, HD189733B, HIC98505, HIP98505, SAO88060, Wolf864, YZ227419, HD189733, HD189733b, HD189733b, HD189733B |
OBJECT name(s) in headers |
HD189733, HD 189733b, HD 189733 |
PI name(s) in headers |
QSO Team, Florian Debras, Jean-Francois Donati, Emily Deibert, Romain Allart, Claire Moutou |
Project/Run name(s) in headers |
25BQ57, 24AF11, 25AQ57, 25AP45, 24BF15, 20AC01, 21BC16, 23AQ57, 23BQ57, 24AQ57, 24AC16, 24BQ57, 18BE99, 19AP40 |
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 |
-1755.41 \(\pm\) 60.85 m/s |
CCF FWHM |
8896.87 \(\pm\) 271.44 m/s |
Number of CCF files Total |
950 |
Number of CCF passed QC |
950 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2018-09-22 06:24:31.684 |
Last ccf file [Mid exposure] |
2025-11-30 06:10:34.944 |
Last processed [ccf] |
2026-01-07 12:06:28.377 |
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 20:45:15.204 |
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.