BDP08_4887 (spirou_offline_udem)¶
This page was last modified: 2026-02-12 19:23:01.165990 (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=BDP08_4887
Target Information |
|
|---|---|
RA |
338.2617012 [deg] (Gaia EDR3) |
Dec |
9.37860496 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
3721.0 [K] (2021A&A…656A.162M) |
Spectral Type |
M0V (1986AJ…..92..139S) |
Proper Motion (RA) |
538.1796824 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
141.1487996 [mas/yr] (Gaia EDR3) |
Parallax |
77.03461201 [mas/yr] (Gaia EDR3) |
Radial Velocity |
-6.493 [mas/yr] (2018A&A…616A…7S) |
Aliases |
2MASS J22330225+0922410, AG+09 3160, ASCC 1089332, BD+08 4887, BPM 97364, DO 7833, G 18-56, G 28-4, GALEX 6376228696605329445, GCRV 73284, GEN# +0.00804887, GJ 863, Gaia DR1 2717105334899452032, Gaia DR2 2717105133036645760, Gaia EDR3 2717105133036645760, HIC 111313, HIP 111313, L 1149-27, LFT 1723, LHS 3828, LSPM J2233+0922, LTT 16614, MCC 208, NLTT 54142, PLX 5454, PLX 5454.00, PM 22305+0907, PM J22330+0922, PPM 173167, StKM 2-1624, TIC 418978178, TYC 1151-487-1, UBV 19275, UBV M 365, UCAC2 35131138, UCAC4 497-142295, USNO 680, USNO-B1.0 0993-00605514, VVO 114, WISEA J223302.61+092242.1, [HFE83] 1510, [R78b] 323, [RHG95] 3544, BD+08 4887, BDP08_4887, DO 7833, G 18-56, G 28-4, GJ 863, LHS 3828, UBV 19275, UBV M 365, UCAC2 35131138, [RHG95] 3544, 2MASSJ22330225+0922410, AG+093160, ASCC1089332, BD+084887, BPM97364, DO7833, G18-56, G28-4, GALEX6376228696605329445, GCRV73284, GEN#+0.00804887, GJ863, GaiaDR12717105334899452032, GaiaDR22717105133036645760, GaiaEDR32717105133036645760, HIC111313, HIP111313, L1149-27, LFT1723, LHS3828, LSPMJ2233+0922, LTT16614, MCC208, NLTT54142, PLX5454, PLX5454.00, PM22305+0907, PMJ22330+0922, PPM173167, StKM2-1624, TIC418978178, TYC1151-487-1, UBV19275, UBVM365, UCAC235131138, UCAC4497-142295, USNO680, USNO-B1.00993-00605514, VVO114, WISEAJ223302.61+092242.1, [HFE83]1510, [R78b]323, [RHG95]3544, BD+084887, BDP084887, DO7833, G18-56, G28-4, GJ863, LHS3828, UBV19275, UBVM365, UCAC235131138, [RHG95]3544 |
OBJECT name(s) in headers |
BD+08 4887 |
PI name(s) in headers |
Farbod Jahandar |
Project/Run name(s) in headers |
20BC30 |
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 |
-6508.51 \(\pm\) 3.98 m/s |
CCF FWHM |
7164.04 \(\pm\) 15.51 m/s |
Number of CCF files Total |
4 |
Number of CCF passed QC |
4 |
Number CCF files failed QC |
0 |
First ccf file [Mid exposure] |
2020-08-30 11:23:46.669 |
Last ccf file [Mid exposure] |
2020-08-30 11:30:05.661 |
Last processed [ccf] |
2025-02-23 19:23:56.160 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 19:23:04.157 |
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.