GY92_214 (spirou_offline_udem)¶
This page was last modified: 2025-01-17 00:08:19.138619 (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=GY92_214
Target Information |
|
|---|---|
RA |
246.789293 [deg] (2003yCat.2246….0C) |
Dec |
-24.621881 [deg] (2003yCat.2246….0C) |
Finder chart |
|
Teff |
nan [K] (None) |
Spectral Type |
None (None) |
Proper Motion (RA) |
nan [mas/yr] (None) |
Proper Motion (Dec) |
nan [mas/yr] (None) |
Parallax |
nan [mas/yr] (None) |
Radial Velocity |
nan [mas/yr] (None) |
Aliases |
2MASS J16270943-2437187, ALMA J162709.41-243718.9, AP J16270943-2437187, BBRCG 23, BKLT J162709-243718, CRBR 2407.8-3033, DROXO 38, Elia 2-29, EPIC 203868595, GBS-VLA J162709.41-243719.0, HGBS J162709.5-243723, ISO-Oph 108, JCMTLSG J162709.1-243719, JCMTSE J162709.4-243720, JCMTSF J162709.4-243720, LFAM 27, ROXA 8, ROXN 22, ROX C15, SSTc2d J162709.4-243719, SSTc2d J162709.4-243718, TIC 175629501, WISEA J162709.42-243719.1, WISE J162709.41-243718.9, WL 15, WLY 1-7, 2XMM J162709.4-243718, YLW 7, YLW 7A, [AMD2002] J162709-243718, [CG2010] IRAS 16240-2430(E), [EDJ2009] 871, [EES2009] Oph-emb 16, [GY92] 214, [HL2013] 246.78918-24.62184, [IKT2001] 23, [INT2003] BF-26, [JJK2008] J162709.40-243718.6, [JJK2008] SMM J162709-24372, [JWM2000] SMM J16271-2437b, [MAN98] E-MM6, [SKS95] 162407.9-243037, [SSG2006] MMS009, YLW_7, GY92_214, GY92-214, 2MASSJ16270943-2437187, ALMAJ162709.41-243718.9, APJ16270943-2437187, BBRCG23, BKLTJ162709-243718, CRBR2407.8-3033, DROXO38, Elia2-29, EPIC203868595, GBS-VLAJ162709.41-243719.0, HGBSJ162709.5-243723, ISO-Oph108, JCMTLSGJ162709.1-243719, JCMTSEJ162709.4-243720, JCMTSFJ162709.4-243720, LFAM27, ROXA8, ROXN22, ROXC15, SSTc2dJ162709.4-243719, SSTc2dJ162709.4-243718, TIC175629501, WISEAJ162709.42-243719.1, WISEJ162709.41-243718.9, WL15, WLY1-7, 2XMMJ162709.4-243718, YLW7, YLW7A, [AMD2002]J162709-243718, [CG2010]IRAS16240-2430(E), [EDJ2009]871, [EES2009]Oph-emb16, [GY92]214, [HL2013]246.78918-24.62184, [IKT2001]23, [INT2003]BF-26, [JJK2008]J162709.40-243718.6, [JJK2008]SMMJ162709-24372, [JWM2000]SMMJ16271-2437b, [MAN98]E-MM6, [SKS95]162407.9-243037, [SSG2006]MMS009, YLW7, GY92214, GY92-214 |
OBJECT name(s) in headers |
GY92-214 |
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 8 (#71 1.08um)] |
SNR[Order 35 (#44 1.75um)] |
DPRTYPEs |
ext_files |
tcorr_files |
Request ext files |
Request tcorr files |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2019-05-14 |
2019-05-14 12:03:26.865 |
2019-05-14 12:45:38.186 |
8 |
0 |
0.599 |
1.463 |
300.884 |
2407.072 |
2.400 |
7.864 |
POLAR_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.
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.