PHILEO (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:54:05.192564 (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=PHILEO
Target Information |
|
|---|---|
RA |
169.1649414 [deg] (Gaia DR2) |
Dec |
-3.651760885 [deg] (Gaia DR2) |
Finder chart |
|
Teff |
8200.0 [K] (2018MNRAS.474.5287A) |
Spectral Type |
A5V (1999MSS…C05….0H) |
Proper Motion (RA) |
-111.2071397 [mas/yr] (Gaia DR2) |
Proper Motion (Dec) |
-37.04191885 [mas/yr] (Gaia DR2) |
Parallax |
17.44031722 [mas/yr] (Gaia DR2) |
Radial Velocity |
-3.0 [mas/yr] (2006AstL…32..759G) |
Aliases |
* 74 Leo, * phi Leo, ** SHJ 121A, 2MASS J11163972-0339056, BD-02 3315, BDS 5729 A, CCDM J11166-0339A, FK5 1292, GC 15511, GCRV 6915, GEN# +1.00098058, GSC 04925-01610, Gaia DR2 3789997584304629248, HD 98058, HIC 55084, HIP 55084, HR 4368, IDS 11116-0307 A, IRAS 11141-0322, JP11 2044, N30 2648, PLX 2620, PLX 2620.00, PMC 90-93 890, PPM 194304, ROT 1676, SAO 138102, SKY# 21474, TIC 443616529, TYC 4925-1610-1, UBV 10278, UBV M 16945, WDS J11167-0339A, WEB 9934, YZ 93 4264, [HFE83] 786, uvby98 100098058, * 74 Leo, ** SHJ 121A, BD-02 3315, BDS 5729 A, GCRV 6915, HD 98058, HIC 55084, HIP 55084, HR 4368, JP11 2044, PHILEO, PMC 90-93 890, ROT 1676, UBV 10278, UBV M 16945, WEB 9934, YZ 93 4264, [HFE83] 786, phiLeo, *74Leo, *phiLeo, **SHJ121A, 2MASSJ11163972-0339056, BD-023315, BDS5729A, CCDMJ11166-0339A, FK51292, GC15511, GCRV6915, GEN#+1.00098058, GSC04925-01610, GaiaDR23789997584304629248, HD98058, HIC55084, HIP55084, HR4368, IDS11116-0307A, IRAS11141-0322, JP112044, N302648, PLX2620, PLX2620.00, PMC90-93890, PPM194304, ROT1676, SAO138102, SKY#21474, TIC443616529, TYC4925-1610-1, UBV10278, UBVM16945, WDSJ11167-0339A, WEB9934, YZ934264, [HFE83]786, uvby98100098058, *74Leo, **SHJ121A, BD-023315, BDS5729A, GCRV6915, HD98058, HIC55084, HIP55084, HR4368, JP112044, PHILEO, PMC90-93890, ROT1676, UBV10278, UBVM16945, WEB9934, YZ934264, [HFE83]786, phiLeo |
OBJECT name(s) in headers |
phiLeo |
PI name(s) in headers |
QSO Team, Matt Wilson |
Project/Run name(s) in headers |
25BQ58, 25AQ58, 24BQ58, 20BQ58, 20AQ58, 21AQ58, 21BQ58, 22AQ58, 22BQ58, 23AQ58, 23BQ58, 24AQ58, 18BE93, 19AQ58, 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 |
299751.65 \(\pm\) 3550.32 m/s |
CCF FWHM |
10120.58 \(\pm\) 95300.03 m/s |
Number of CCF files Total |
71 |
Number of CCF passed QC |
71 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2018-12-19 11:24:05.804 |
Last ccf file [Mid exposure] |
2025-12-04 16:02:46.651 |
Last processed [ccf] |
2026-01-07 12:03:07.949 |
Version [ccf] |
0.7.292,0.7.295,0.7.293 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:54:19.283 |
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.