GJ669B (spirou_offline_udem)¶
This page was last modified: 2026-02-12 19:57:31.230608 (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=GJ669B
Target Information |
|
|---|---|
RA |
259.9695667 [deg] (Gaia EDR3) |
Dec |
26.50231875 [deg] (Gaia EDR3) |
Finder chart |
|
Teff |
3145.0 [K] (2020ApJ…892…31B) |
Spectral Type |
M4.5V (1991ApJS…77..417K) |
Proper Motion (RA) |
-226.0399234 [mas/yr] (Gaia EDR3) |
Proper Motion (Dec) |
354.9842992 [mas/yr] (Gaia EDR3) |
Parallax |
92.9583053 [mas/yr] (Gaia EDR3) |
Radial Velocity |
-34.6 [mas/yr] (2012ApJ…758…56S) |
Aliases |
** OSV 5B, 1ES 1717+26.5, 2E 3884, 2E 1717.9+2632, 2MASS J17195298+2630026, CCDM J17199+2630B, CSI+26-17179 1, CSV 7640, CXOMP J171952.9+263003, G 170-34, GALEX 6375349012143277863, GCRV 67008, GEN# +9.80170034, GJ 669 B, Gaia DR2 4574048021719712640, Gaia EDR3 4574048021719712640, HAT 239-00513, IDS 17159+2635 B, Karmn J17198+265, LSPM J1719+2630W, LTT 15140, NLTT 44615, PM J17198+2630, RX J1719.8+2629, Ross 867, StKM 2-1312b, TIC 257798328, UCAC4 583-056829, USNO 645, USNO-B1.0 1165-00279417, V* V639 Her, WDS J17199+2629B, WISE J171952.80+263006.3, WISEA J171952.80+263006.3, [FS2003] 0887, [GKL99] 342, [RHG95] 2745, [ZEH2003] RX J1719.8+2629 2, ** OSV 5B, 2E 3884, CSI+26-17179 1, CSV 7640, GJ 669 B, GJ669B, Ross 867, [RHG95] 2745, [ZEH2003] RX J1719.8+2629 2, **OSV5B, 1ES1717+26.5, 2E3884, 2E1717.9+2632, 2MASSJ17195298+2630026, CCDMJ17199+2630B, CSI+26-171791, CSV7640, CXOMPJ171952.9+263003, G170-34, GALEX6375349012143277863, GCRV67008, GEN#+9.80170034, GJ669B, GaiaDR24574048021719712640, GaiaEDR34574048021719712640, HAT239-00513, IDS17159+2635B, KarmnJ17198+265, LSPMJ1719+2630W, LTT15140, NLTT44615, PMJ17198+2630, RXJ1719.8+2629, Ross867, StKM2-1312b, TIC257798328, UCAC4583-056829, USNO645, USNO-B1.01165-00279417, V*V639Her, WDSJ17199+2629B, WISEJ171952.80+263006.3, WISEAJ171952.80+263006.3, [FS2003]0887, [GKL99]342, [RHG95]2745, [ZEH2003]RXJ1719.8+26292, **OSV5B, 2E3884, CSI+26-171791, CSV7640, GJ669B, GJ669B, Ross867, [RHG95]2745, [ZEH2003]RXJ1719.8+26292 |
OBJECT name(s) in headers |
GJ669B |
PI name(s) in headers |
Julien Morin |
Project/Run name(s) in headers |
19AF26 |
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 |
GL699_neg.fits |
CCF systemic velocity |
-34103.90 \(\pm\) 3.61 m/s |
CCF FWHM |
9628.48 \(\pm\) 29.61 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] |
2019-04-25 13:21:00.179 |
Last ccf file [Mid exposure] |
2019-04-25 14:02:47.974 |
Last processed [ccf] |
2025-02-23 21:11:55.188 |
Version [ccf] |
0.7.292 |
Request |
|---|
CCF Downloads |
File URL |
Uploaded |
|---|---|---|
CCF Table |
2026-02-12 19:57:33.398 |
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.