GJ872A (nirps_ha_online_udem)

This page was last modified: 2025-06-17 16:06:18.041764 (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=GJ872A

Target Information
RA	341.6742772 [deg] (Gaia DR2)
Dec	12.17076258 [deg] (Gaia DR2)
Finder chart	[FINDER CHART]
Teff	6167.0 [K] (2013MNRAS.435..952S)
Spectral Type	F6V (2001AJ….121.2148G)
Proper Motion (RA)	236.5564656 [mas/yr] (Gaia DR2)
Proper Motion (Dec)	-494.8929558 [mas/yr] (Gaia DR2)
Parallax	62.39938245 [mas/yr] (Gaia DR2)
Radial Velocity	-5.853 [mas/yr] (2018A&A…616A…7S)
Aliases	LHS 3851, * ksi Peg, * ksi Peg A, * 46 Peg, ** HJ 301A, ADS 16261 A, AG+11 2850, AKARI-IRC-V1 J2246417+121018, ASCC 996971, BD+11 4875, BD+11 4875A, CCDM J22467+1211A, Ci 20 1381, CSI+11 4875 1, GC 31778, GCRV 14308, GEN# +1.00215648, GJ 872 A, HD 215648, HIC 112447, HIP 112447, HR 8665, IDS 22417+1139 A, IRAS 22442+1154, IRC +10522, JP11 3532, LFT 1735, LSPM J2246+1210W, LTT 16693, 2MASS J22464156+1210228, NLTT 54819, PLX 5516, PM 22442+1155, PPM 141833, ROT 3316, SAO 108165, SKY# 43286, SPOCS 984, TD1 29336, TIC 60716322, TYC 1155-2186-1, UBV 19514, UBV M 26609, USNO-B1.0 1021-00758035, uvby98 100215648, WDS J22467+1210A, WEB 20055, WISEA J224641.79+121017.4, WISE J224641.75+121017.0, YZ 11 9091, Gaia DR2 2719475542666622976, Gaia DR3 2719475542667772416, GJ_872_A, LHS 3851, LHS_3851, LHS3851, * ksi Peg, * ksi_Peg, * ksiPeg, *_ksi Peg, *_ksi_Peg, *_ksiPeg, *ksi Peg, *ksi_Peg, *ksiPeg, * ksi Peg A, * ksi Peg_A, * ksi PegA, * ksi_Peg A, * ksi_Peg_A, * ksi_PegA, * ksiPeg A, * ksiPeg_A, * ksiPegA, *_ksi Peg A, *_ksi Peg_A, *_ksi PegA, *_ksi_Peg A, *_ksi_Peg_A, *_ksi_PegA, *_ksiPeg A, *_ksiPeg_A, *_ksiPegA, *ksi Peg A, *ksi Peg_A, *ksi PegA, *ksi_Peg A, *ksi_Peg_A, *ksi_PegA, *ksiPeg A, *ksiPeg_A, *ksiPegA, GJ 872 A, GJ 872_A, GJ 872A, GJ_872 A, GJ_872_A, GJ_872A, GJ872 A, GJ872_A, GJ872A, GL 872 A, GL 872_A, GL 872A, GL_872 A, GL_872_A, GL_872A, GL872 A, GL872_A, GL872A, HD 215648, HD_215648, HD215648, HR 8665, HR_8665, HR8665, LHS3851, *ksiPeg, *ksiPegA, *46Peg, **HJ301A, ADS16261A, AG+112850, AKARI-IRC-V1J2246417+121018, ASCC996971, BD+114875, BD+114875A, CCDMJ22467+1211A, Ci201381, CSI+1148751, GC31778, GCRV14308, GEN#+1.00215648, GJ872A, HD215648, HIC112447, HIP112447, HR8665, IDS22417+1139A, IRAS22442+1154, IRC+10522, JP113532, LFT1735, LSPMJ2246+1210W, LTT16693, 2MASSJ22464156+1210228, NLTT54819, PLX5516, PM22442+1155, PPM141833, ROT3316, SAO108165, SKY#43286, SPOCS984, TD129336, TIC60716322, TYC1155-2186-1, UBV19514, UBVM26609, USNO-B1.01021-00758035, uvby98100215648, WDSJ22467+1210A, WEB20055, WISEAJ224641.79+121017.4, WISEJ224641.75+121017.0, YZ119091, GaiaDR22719475542666622976, GaiaDR32719475542667772416, GJ872A, LHS3851, LHS3851, LHS3851, *ksiPeg, *ksiPeg, *ksiPeg, *ksiPeg, *ksiPeg, *ksiPeg, *ksiPeg, *ksiPeg, *ksiPeg, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, *ksiPegA, GJ872A, GJ872A, GJ872A, GJ872A, GJ872A, GJ872A, GJ872A, GJ872A, GJ872A, GL872A, GL872A, GL872A, GL872A, GL872A, GL872A, GL872A, GL872A, GL872A, HD215648, HD215648, HD215648, HR8665, HR8665, HR8665
OBJECT name(s) in headers	GJ872A
OB Name(s) in headers	GJ872A-22h46, GJ872B-22h46
PI name(s) in headers	UNKNOWN
Project/Run name(s) in headers	111.24ZU.001, 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
2023-06-24	2023-06-25 08:45:24.769	2023-06-25 08:46:48.369	2	0	1.360	1.351	72.453	144.906	241.127	320.346	OBJ_SKY	2 [download]	0 [download]	Extracted 2D files	Telluric corrected 2D files
2023-06-27	2023-06-28 09:21:51.027	2023-06-28 09:36:59.515	3	0	1.650	1.340	347.402	1042.207	203.566	235.896	OBJ_SKY	3 [download]	0 [download]	Extracted 2D files	Telluric corrected 2D files
2023-08-26	2023-08-27 06:09:50.597	2023-08-27 06:09:50.597	1	0	2.180	1.375	897.301	897.301	443.064	615.465	OBJ_SKY	1 [download]	0 [download]	Extracted 2D files	Telluric corrected 2D files
2023-08-31	2023-09-01 05:07:14.996	2023-09-01 05:22:23.432	2	0	0.995	1.340	897.301	1794.603	359.181	587.991	OBJ_SKY	2 [download]	0 [download]	Extracted 2D files	Telluric corrected 2D files
2023-11-02	2023-11-03 02:56:20.452	2023-11-03 02:56:20.452	1	0	1.260	1.604	897.301	897.301	180.241	283.611	OBJ_SKY	1 [download]	0 [download]	Extracted 2D files	Telluric corrected 2D files
2024-11-10	2024-11-11 01:33:37.389	2024-11-11 01:33:37.389	1	0	1.260	1.425	997.621	997.621	869.034	1091.007	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.