HD113283 (nirps_he_online_udem)¶
This page was last modified: 2026-03-09 10:07:31.105615 (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=HD113283
Target Information |
|
|---|---|
RA |
198.8369564 [deg] (Gaia DR3) |
Dec |
-87.56137833 [deg] (Gaia DR3) |
Finder chart |
|
Teff |
5649.0 [K] (2011A&A…530A.138C) |
Spectral Type |
G5V (2006AJ….132..161G) |
Proper Motion (RA) |
-222.290438 [mas/yr] (Gaia DR3) |
Proper Motion (Dec) |
-156.1708701 [mas/yr] (Gaia DR3) |
Parallax |
40.47572676 [mas/yr] (Gaia DR3) |
Radial Velocity |
-4.72 [mas/yr] (2018yCat.1345….0G) |
Aliases |
LTT 5027, CD-86 85, CNS5 3262, CPC 22 1642, CPD-86 283, GC 17801, GCRV 63780, GEN# +1.00113283, HD 113283, HIC 64690, HIP 64690, IRAS 13054-8717, 2MASS J13152666-8733386, NLTT 32983, PLX 2988, PLX 2988.00, PPM 377545, SAO 258659, SKY# 24505, TIC 383473544, TYC 9516-1604-1, UBV 11774, uvby98 100113283, WEB 11440, Gaia DR2 5765846127180770432, Gaia DR3 5765846127180770432, Gaia DR1 5765846122884217600, HD_113283, J1315-87, LTT5027, CD-8685, CNS53262, CPC221642, CPD-86283, GC17801, GCRV63780, GEN#+1.00113283, HD113283, HIC64690, HIP64690, IRAS13054-8717, 2MASSJ13152666-8733386, NLTT32983, PLX2988, PLX2988.00, PPM377545, SAO258659, SKY#24505, TIC383473544, TYC9516-1604-1, UBV11774, uvby98100113283, WEB11440, GaiaDR25765846127180770432, GaiaDR35765846127180770432, GaiaDR15765846122884217600, HD113283, J1315-87 |
OBJECT name(s) in headers |
J1315-87 |
OB Name(s) in headers |
J1315-87 |
PI name(s) in headers |
UNKNOWN |
Project/Run name(s) in headers |
115.27UZ.001 |
Spectrum¶
This section presents the observation after extraction,with and without telluric correction.
LBL¶
No LBL reduction found
CCF¶
No CCF files found
Time series¶
This section deals with providing the time series information for this object
Obs Dir |
First obs mid |
Last obs mid |
Number of ext |
Number of tcorr |
Seeing |
Airmass |
Mean Exptime |
Total Exptime |
SNR[Order 15 (#134 1.08um)] |
SNR[Order 60 (#89 1.63um)] |
DPRTYPEs |
ext_files |
tcorr_files |
Request ext files |
Request tcorr files |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2025-04-28 |
2025-04-29 03:22:40.918 |
2025-04-29 03:22:40.918 |
1 |
0 |
-1.000 |
1.905 |
300.958 |
300.958 |
201.240 |
251.342 |
OBJ_FP |
||||
2025-05-18 |
2025-05-19 06:02:59.420 |
2025-05-19 06:02:59.420 |
1 |
0 |
0.780 |
1.963 |
300.958 |
300.958 |
171.908 |
221.401 |
OBJ_FP |
||||
2025-06-16 |
2025-06-17 02:16:26.236 |
2025-06-17 04:23:36.515 |
2 |
0 |
2.590 |
1.945 |
300.958 |
601.916 |
128.147 |
175.466 |
OBJ_FP |
||||
2025-06-19 |
2025-06-20 02:20:25.671 |
2025-06-20 02:20:25.671 |
1 |
0 |
1.180 |
1.924 |
300.958 |
300.958 |
140.087 |
189.662 |
OBJ_FP |
||||
2025-06-21 |
2025-06-22 02:44:36.666 |
2025-06-22 02:44:36.666 |
1 |
0 |
0.710 |
1.935 |
300.958 |
300.958 |
173.694 |
220.621 |
OBJ_FP |
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.