HD34751A (nirps_ha_online_udem)

This page was last modified: 2025-06-17 16:11:21.429508 (UTC)

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Contents

• Target info

• Spectrum

• LBL

• CCF

• Time series

• Debug

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=HD34751A

Target Information
RA	79.69599325 [deg] (Gaia DR2)
Dec	-21.393916 [deg] (Gaia DR2)
Finder chart	[FINDER CHART]
Teff	4653.0 [K] (2018MNRAS.479.1332M)
Spectral Type	K6Vk (2006AJ….132..161G)
Proper Motion (RA)	-137.0546728 [mas/yr] (Gaia DR2)
Proper Motion (Dec)	-36.93975905 [mas/yr] (Gaia DR2)
Parallax	48.94803178 [mas/yr] (Gaia DR2)
Radial Velocity	26.986 [mas/yr] (2018A&A…616A…7S)
Aliases	HD 34751, ** DON 101A, BD-21 1131, CCDM J05188-2124A, CSI-21 1131 1, GCRV 3170, GEN# +1.00034751, GJ 199 A, GSC 05914-01173, HD 34751A, HIC 24783, HIP 24783, IDS 05146-2130 A, 2MASS J05184718-2123376, MCC 114, NSV 16283, PLX 1213.1, PPM 725047, 1RXS J051847.5-212335, TIC 408191404, TYC 5914-1173-1, UBV M 10837, UGP 110, VVO 53, WDS J05189-2124A, WEB 4796, WISEA J051847.17-212337.8, WISE J051847.08-212337.7, [RHG95] 905, Gaia DR2 2962193318618221056, Gaia DR3 2962193318618221056, Gaia DR1 2962193314320452352, HD34751, **DON101A, BD-211131, CCDMJ05188-2124A, CSI-2111311, GCRV3170, GEN#+1.00034751, GJ199A, GSC05914-01173, HD34751A, HIC24783, HIP24783, IDS05146-2130A, 2MASSJ05184718-2123376, MCC114, NSV16283, PLX1213.1, PPM725047, 1RXSJ051847.5-212335, TIC408191404, TYC5914-1173-1, UBVM10837, UGP110, VVO53, WDSJ05189-2124A, WEB4796, WISEAJ051847.17-212337.8, WISEJ051847.08-212337.7, [RHG95]905, GaiaDR22962193318618221056, GaiaDR32962193318618221056, GaiaDR12962193314320452352
OBJECT name(s) in headers	GJ199A
OB Name(s) in headers	GJ199A-5h18, GJ199B-5h18
PI name(s) in headers	UNKNOWN
Project/Run name(s) in headers	112.25P7.001

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
2024-01-26	2024-01-27 02:53:33.051	2024-01-27 02:53:33.051	1	0	1.260	1.045	897.301	897.301	126.827	221.270	OBJ_SKY	1 [download]	0 [download]	Extracted 2D files	Telluric corrected 2D files
2024-01-29	2024-01-30 03:39:43.075	2024-01-30 03:39:43.075	1	0	1.260	1.145	897.301	897.301	170.830	266.968	OBJ_SKY	1 [download]	0 [download]	Extracted 2D files	Telluric corrected 2D files
2024-01-30	2024-01-31 03:09:55.312	2024-01-31 03:09:55.312	1	0	1.260	1.091	897.301	897.301	166.294	260.483	OBJ_SKY	1 [download]	0 [download]	Extracted 2D files	Telluric corrected 2D files
2024-03-06	2024-03-07 02:21:57.937	2024-03-07 02:21:57.937	1	0	1.260	1.387	897.301	897.301	136.144	229.656	OBJ_SKY	1 [download]	0 [download]	Extracted 2D files	Telluric corrected 2D files
2024-12-19	2024-12-20 02:37:05.932	2024-12-20 02:37:05.932	1	0	1.260	1.089	997.621	997.621	181.978	284.451	OBJ_SKY	1 [download]	0 [download]	Extracted 2D files	Telluric corrected 2D files

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.