72_OPH (spirou_offline_udem)¶
This page was last modified: 2026-02-12 19:23:27.085794 (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=72_OPH
Target Information |
|
|---|---|
RA |
271.8371583 [deg] (Gaia EDR3) |
Dec |
9.564197857 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
8299.0 [K] (2012A&A…537A.120Z) |
Spectral Type |
A5V (2003AJ….126.2048G) |
Proper Motion (RA) |
-61.80433681 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
79.0043939 [mas/yr] (Gaia EDR3) |
Parallax |
38.12630611 [mas/yr] (Gaia EDR3) |
Radial Velocity |
-23.9 [mas/yr] (2007AN….328..889K) |
Aliases |
* 72 Oph, ** STT 342A, 1RXS J180719.8+093411, 2MASS J18072099+0933497, ADS 11076 A, AG+09 2155, AKARI-IRC-V1 J1807209+093350, BD+09 3564, CCDM J18073+0934A, CSI+09 3564 1, FK5 680, GC 24695, GCRV 10566, GEN# +1.00165777A, GJ 9615 A, GSC 01012-01661, Gaia DR2 4482432246130215296, Gaia EDR3 4482432246132106496, HD 165777, HIC 88771, HIP 88771, HR 6771, IDS 18026+0933 A, IRAS 18049+0933, JP11 2934, N30 4025, PLX 4147, PMC 90-93 484, PPM 165207, ROT 2551, Renson 46702, SAO 123142, SKY# 32929, TD1 21675, TIC 24592444, TYC 1012-1661-1, UBV 15405, UBV M 22638, WDS J18073+0934A, WEB 15039, YZ 9 8299, uvby98 100165777 A, * 72 Oph, ** STT 342A, 72_OPH, BD+09 3564, CSI+09 3564 1, FK5 680, GJ 9615 A, HIC 88771, HIP 88771, HR 6771, JP11 2934, PMC 90-93 484, ROT 2551, UBV 15405, UBV M 22638, YZ 9 8299, *72Oph, **STT342A, 1RXSJ180719.8+093411, 2MASSJ18072099+0933497, ADS11076A, AG+092155, AKARI-IRC-V1J1807209+093350, BD+093564, CCDMJ18073+0934A, CSI+0935641, FK5680, GC24695, GCRV10566, GEN#+1.00165777A, GJ9615A, GSC01012-01661, GaiaDR24482432246130215296, GaiaEDR34482432246132106496, HD165777, HIC88771, HIP88771, HR6771, IDS18026+0933A, IRAS18049+0933, JP112934, N304025, PLX4147, PMC90-93484, PPM165207, ROT2551, Renson46702, SAO123142, SKY#32929, TD121675, TIC24592444, TYC1012-1661-1, UBV15405, UBVM22638, WDSJ18073+0934A, WEB15039, YZ98299, uvby98100165777A, *72Oph, **STT342A, 72OPH, BD+093564, CSI+0935641, FK5680, GJ9615A, HIC88771, HIP88771, HR6771, JP112934, PMC90-93484, ROT2551, UBV15405, UBVM22638, YZ98299 |
OBJECT name(s) in headers |
|
PI name(s) in headers |
Emily Deibert |
Project/Run name(s) in headers |
20AC01 |
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 |
296567.47 \(\pm\) 7149.71 m/s |
CCF FWHM |
141615.04 \(\pm\) 78475.85 m/s |
Number of CCF files Total |
112 |
Number of CCF passed QC |
112 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2020-07-03 10:27:42.748 |
Last ccf file [Mid exposure] |
2020-07-25 10:29:23.784 |
Last processed [ccf] |
2025-02-23 19:47:23.902 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 19:23:51.125 |
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.