ROSS_555 (spirou_offline_udem)

This page was last modified: 2026-02-12 20:53:51.932401 (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=ROSS_555

Target Information

RA

27.95543446 [deg] (Gaia EDR3)

Dec

-10.80586698 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

3998.0 [K] (2019ApJ…878..134K)

Spectral Type

M3.5 (1985ApJS…59..197B)

Proper Motion (RA)

568.6177622 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-539.3835152 [mas/yr] (Gaia EDR3)

Parallax

58.24092077 [mas/yr] (Gaia EDR3)

Radial Velocity

-11.1 [mas/yr] (2016A&A…596A.116S)

Aliases

2MASS J01514865-1048120, CSI-11-01493, Ci 20 130, G 271-168, G 272-109, GCRV 1039, GJ 78, Gaia DR2 2460983348274381696, Gaia EDR3 2460983348274381696, HIC 8691, HIP 8691, Karmn J01518-108, LFT 166, LHS 1303, LPM 88, LTT 996, NLTT 6243, PLX 386.2, PLX 386.20, PM 01493-1103, PM J01518-1048, Ross 555, TIC 24924439, TYC 5278-815-1, UCAC4 396-002213, WEB 1833, WISEA J015149.09-104818.2, [RHG95] 339, Ci 20 130, GCRV 1039, GJ 78, HIC 8691, HIP 8691, LFT 166, LHS 1303, LPM 88, LTT 996, NLTT 6243, PLX 386.2, PLX 386.20, ROSS_555, Ross 555, WEB 1833, [RHG95] 339, 2MASSJ01514865-1048120, CSI-11-01493, Ci20130, G271-168, G272-109, GCRV1039, GJ78, GaiaDR22460983348274381696, GaiaEDR32460983348274381696, HIC8691, HIP8691, KarmnJ01518-108, LFT166, LHS1303, LPM88, LTT996, NLTT6243, PLX386.2, PLX386.20, PM01493-1103, PMJ01518-1048, Ross555, TIC24924439, TYC5278-815-1, UCAC4396-002213, WEB1833, WISEAJ015149.09-104818.2, [RHG95]339, Ci20130, GCRV1039, GJ78, HIC8691, HIP8691, LFT166, LHS1303, LPM88, LTT996, NLTT6243, PLX386.2, PLX386.20, ROSS555, Ross555, WEB1833, [RHG95]339

OBJECT name(s) in headers

Ross 555

PI name(s) in headers

Farbod Jahandar

Project/Run name(s) in headers

19BC31

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.

../../../_images/ccf_plot_ROSS_555_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-10494.09 \(\pm\) 10.60 m/s

CCF FWHM

6675.91 \(\pm\) 32.08 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]

2019-11-14 09:02:42.177

Last ccf file [Mid exposure]

2019-11-14 09:09:17.837

Last processed [ccf]

2025-02-23 20:23:44.395

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_ROSS_555_spirou_offline_udem_file_list.txt

2026-02-12 20:53:54.243

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

../../../_images/debug_tcorr_map_plot_ROSS_555_spirou_offline_udem.png

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

../../../_images/debug_extsmax_plot_ROSS_555_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_ROSS_555_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_ROSS_555_spirou_offline_udem.png

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

../../../_images/debug_mjd_cdt_plot_ROSS_555_spirou_offline_udem.png

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.