HD7895 (spirou_offline_udem)¶
This page was last modified: 2026-02-12 20:47:11.451937 (UTC)
Back to the object table
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=HD7895
Target Information |
|
|---|---|
RA |
19.67316706 [deg] (Gaia EDR3) |
Dec |
-0.8686919886 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
5266.0 [K] (2018MNRAS.479.1332M) |
Spectral Type |
K1V (1967AJ…..72.1334C) |
Proper Motion (RA) |
432.5638418 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
-253.3574733 [mas/yr] (Gaia EDR3) |
Parallax |
36.398541 [mas/yr] (Gaia EDR3) |
Radial Velocity |
16.37 [mas/yr] (2018A&A…619A..81H) |
Aliases |
CCDM J01187-0052A, ** EGN 1, ** HJ 5453A, ADS 1057 A, AG-01 114, AGKR 1123, BD-01 167, Ci 20 94, CSI-01 167 1, GC 1582, GCRV 754, GEN# +1.00007895A, G 70-51, G 271-32, GJ 56.3 A, GJ 9052 A, HD 7895, HIC 6130, HIP 6130, IDS 01135-0123 A, LFT 124, LHS 1230, LPM 68, LTT 723, 2MASS J01184107-0052030, NLTT 4362, PLX 269, PM J01186-0052N, PM 01161-0108, PPM 174875, SAO 129219, SDSS J011841.13-005205.9, SKY# 1978, SRS 3710, TIC 248391508, TYC 4682-1278-1, UBV 1396, UBV M 8091, UCAC4 446-001679, uvby98 100007895 A, WDS J01187-0052A, WDS J01187-0052Aa,Ab, WEB 1377, WISEA J011841.39-005205.8, 2XMM J011841.2-005204, YZC 21 243, YZ 0 3339, YZ 91 243, Gaia EDR3 2533723670313663872, Gaia DR1 2533723666018385408, Gaia DR2 2533723670313663872, CCDMJ01187-0052A, **EGN1, **HJ5453A, ADS1057A, AG-01114, AGKR1123, BD-01167, Ci2094, CSI-011671, GC1582, GCRV754, GEN#+1.00007895A, G70-51, G271-32, GJ56.3A, GJ9052A, HD7895, HIC6130, HIP6130, IDS01135-0123A, LFT124, LHS1230, LPM68, LTT723, 2MASSJ01184107-0052030, NLTT4362, PLX269, PMJ01186-0052N, PM01161-0108, PPM174875, SAO129219, SDSSJ011841.13-005205.9, SKY#1978, SRS3710, TIC248391508, TYC4682-1278-1, UBV1396, UBVM8091, UCAC4446-001679, uvby98100007895A, WDSJ01187-0052A, WDSJ01187-0052Aa,Ab, WEB1377, WISEAJ011841.39-005205.8, 2XMMJ011841.2-005204, YZC21243, YZ03339, YZ91243, GaiaEDR32533723670313663872, GaiaDR12533723666018385408, GaiaDR22533723670313663872 |
OBJECT name(s) in headers |
HD 7895, HD 7895 |
PI name(s) in headers |
Ryan Cloutier |
Project/Run name(s) in headers |
21BC28, 22BC27 |
Spectrum¶
This section presents the observation after extraction,with and without telluric correction.
LBL¶
No LBL reduction found
CCF¶
This section presents the APERO CCF results for this object.
CCF stats |
|
|---|---|
Mask used |
GL846_neg.fits |
CCF systemic velocity |
17750.85 \(\pm\) 28.74 m/s |
CCF FWHM |
8178.23 \(\pm\) 228.04 m/s |
Number of CCF files Total |
2 |
Number of CCF passed QC |
2 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2021-09-23 08:09:57.381 |
Last ccf file [Mid exposure] |
2022-11-11 08:45:51.862 |
Last processed [ccf] |
2025-02-23 17:36:12.312 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 20:47:13.299 |
Time series¶
This section deals with providing the time series information for this object
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.