IMLUP (spirou_offline_udem)

This page was last modified: 2026-02-12 20:48:13.427193 (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=IMLUP

Target Information

RA

239.0382932 [deg] (Gaia EDR3)

Dec

-37.93514048 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

4146.0 [K] (2017A&A…602A..33F)

Spectral Type

M0e (1994AJ….108.1071H)

Proper Motion (RA)

-12.0586495 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-23.72668048 [mas/yr] (Gaia EDR3)

Parallax

6.417493723 [mas/yr] (Gaia EDR3)

Radial Velocity

-0.5 [mas/yr] (2017A&A…602A..33F)

Aliases

HIP 78053, ** HDS 2242, ** GHE 38A, CCDM J15562-3756AB, 2E 3526, 2E 1552.8-3747, GSC 07838-00962, HBC 605, HIC 78053, IRAS 15528-3747, 2MASS J15560921-3756057, PDS 75, 1RXS J155609.3-375556, SSTc2d J155609.2-375607, 1SWASP J155609.20-375605.9, Sz 82, THA 15-12, TIC 364203272, UCAC2 15776163, UCAC4 261-089667, V* IM Lup, WDS J15562-3756A, WDS J15562-3756Aa,Ab, WISEA J155609.19-375606.3, WISE J155609.20-375606.3, 2XMM J155609.2-375606, [KWS97] Lupus 2 24, Gaia EDR3 6010135758090335232, Gaia DR2 6010135758090335232, IM_LUP, HIP78053, **HDS2242, **GHE38A, CCDMJ15562-3756AB, 2E3526, 2E1552.8-3747, GSC07838-00962, HBC605, HIC78053, IRAS15528-3747, 2MASSJ15560921-3756057, PDS75, 1RXSJ155609.3-375556, SSTc2dJ155609.2-375607, 1SWASPJ155609.20-375605.9, Sz82, THA15-12, TIC364203272, UCAC215776163, UCAC4261-089667, V*IMLup, WDSJ15562-3756A, WDSJ15562-3756Aa,Ab, WISEAJ155609.19-375606.3, WISEJ155609.20-375606.3, 2XMMJ155609.2-375606, [KWS97]Lupus224, GaiaEDR36010135758090335232, GaiaDR26010135758090335232, IMLUP

OBJECT name(s) in headers

IMLup

PI name(s) in headers

Jean-Francois Donati

Project/Run name(s) in headers

22AP40

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_IMLUP_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

-774514.70 \(\pm\) 17583.59 m/s

CCF FWHM

2426.91 \(\pm\) 5182.12 m/s

Number of CCF files Total

120

Number of CCF passed QC

120

Number CCF files failed QC

0

First ccf file [Mid exposure]

2022-03-11 14:51:39.499

Last ccf file [Mid exposure]

2022-05-20 11:48:45.135

Last processed [ccf]

2025-02-23 16:52:16.631

Version [ccf]

0.7.292

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_IMLUP_spirou_offline_udem_file_list.txt

2026-02-12 20:48:30.196

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_IMLUP_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_IMLUP_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_IMLUP_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_IMLUP_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_IMLUP_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.