BDP07_2692 (nirps_he_online_udem)¶
This page was last modified: 2025-02-27 01:13:05.971846 (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=BDP07_2692
Target Information |
|
|---|---|
RA |
206.8677924 [deg] (Gaia DR2) |
Dec |
6.315179418 [deg] (Gaia DR2) |
Finder chart |
|
Teff |
4342.0 [K] (2019AJ….158..138S (via nirps-client@maestria)) |
Spectral Type |
K7Ve (2015A&A…577A.128A) |
Proper Motion (RA) |
-509.4402426 [mas/yr] (Gaia DR2) |
Proper Motion (Dec) |
-111.0215273 [mas/yr] (Gaia DR2) |
Parallax |
31.91661997 [mas/yr] (Gaia DR2) |
Radial Velocity |
-30.67 [mas/yr] (2018yCat.1345….0G) |
Aliases |
LHS 2801, AG+06 1649, ASCC 1045992, BD+07 2692, Ci 20 808, GCRV 64362, GEN# +0.00702692, G 65-2, HIC 67291, HIP 67291, Karmn J13474+063, LFT 1038, LSPM J1347+0618, LTT 14023, 2MASS J13472878+0618564, MCC 698, NLTT 35241, PM 13448+0634, TIC 379137299, TYC 314-947-1, UBV M 322, UCAC2 33939654, USNO-B1.0 0963-00225857, uvby98 000702692, VVO 216, WEB 11842, WISEA J134728.43+061855.2, Wolf 504, Gaia DR3 3721114933170707328, Gaia DR2 3721114933170707328, BDP07_2692, LHS 2801, LHS_2801, LHS2801, BD+07 2692, BD+07_2692, BDP07 2692, BDP07_2692, LHS2801, AG+061649, ASCC1045992, BD+072692, Ci20808, GCRV64362, GEN#+0.00702692, G65-2, HIC67291, HIP67291, KarmnJ13474+063, LFT1038, LSPMJ1347+0618, LTT14023, 2MASSJ13472878+0618564, MCC698, NLTT35241, PM13448+0634, TIC379137299, TYC314-947-1, UBVM322, UCAC233939654, USNO-B1.00963-00225857, uvby98000702692, VVO216, WEB11842, WISEAJ134728.43+061855.2, Wolf504, GaiaDR33721114933170707328, GaiaDR23721114933170707328, BDP072692, LHS2801, LHS2801, LHS2801, BD+072692, BD+072692, BDP072692, BDP072692 |
OBJECT name(s) in headers |
TIC379137299 |
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 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2025-02-18 |
2025-02-19 09:28:02.046 |
2025-02-19 09:28:02.046 |
1 |
0 |
-1.000 |
1.254 |
997.621 |
997.621 |
34.586 |
65.417 |
OBJ_SKY |
||||
2025-02-20 |
2025-02-21 09:21:33.116 |
2025-02-21 09:21:33.116 |
1 |
0 |
-1.000 |
1.255 |
997.621 |
997.621 |
35.883 |
67.448 |
OBJ_SKY |
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.
Shape QC plot¶
Shape parameters varying in time.dx is a shift along the order, dy is a shift across orders, [[A,B],[C,D]] is an affine transformation matrix.
wfpdrift plot¶
Wavelength solution absolute CCF FP Drift [km/s]
Wave cavity (c0) plot¶
Wave cavity polynomial coeffs=0
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.