GAIA_DR3_6013525277553837312 (nirps_he_online_udem)

This page was last modified: 2026-03-12 22:28:40.840498 (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=GAIA_DR3_6013525277553837312

Target Information

RA

231.3726577 [deg] (Gaia DR3)

Dec

-36.40484319 [deg] (Gaia DR3)

Finder chart

[FINDER CHART]

Teff

nan [K] (None)

Spectral Type

None (None)

Proper Motion (RA)

-18.82488304 [mas/yr] (Gaia DR3)

Proper Motion (Dec)

-23.72386184 [mas/yr] (Gaia DR3)

Parallax

1.927591632 [mas/yr] (Gaia DR3)

Radial Velocity

14.06 [mas/yr] (2018yCat.1345….0G)

Aliases

EBLM J1525-36, Gaia DR2 6013525277553837312, Gaia DR3 6013525277553837312, J1525-36, EBLMJ1525-36, GaiaDR26013525277553837312, GaiaDR36013525277553837312, J1525-36

OBJECT name(s) in headers

J1525-36

OB Name(s) in headers

J1525-36

PI name(s) in headers

UNKNOWN

Project/Run name(s) in headers

116.28LL.001

Spectrum

This section presents the observation after extraction,with and without telluric correction.

../../../_images/spec_plot_GAIA_DR3_6013525277553837312_nirps_he_online_udem.png

Spectrum Information

DPRTYPES

OBJ_SKY

Total number raw files

1

Number of rejected files

0

First raw files

2026-03-12 09:01:28.111

Last raw files

2026-03-12 09:01:28.111

Total number PP files

1

Number PP files passed QC

1

Number PP files failed QC

0

First pp file [Mid exposure]

2026-03-12 09:01:28.111

Last pp file [Mid exposure]

2026-03-12 09:01:28.111

Last processed [pp]

2026-03-12 14:53:13.848

Version [pp]

0.7.296

Total number ext files

1

Number ext files passed QC

1

Number ext files failed QC

0

First ext file [Mid exposure]

2026-03-12 09:01:28.111

Last ext file [Mid exposure]

2026-03-12 09:01:28.111

Last processed [ext]

2026-03-12 15:54:58.428

Version [ext]

0.7.296

Total number tcorr files

1

Number tcorr files passed QC

1

Number tcorr files failed QC

0

First tcorr file [Mid exposure]

2026-03-12 09:01:28.111

Last tcorr file [Mid exposure]

2026-03-12 09:01:28.111

Last processed [tcorr]

2026-03-12 16:41:05.448

Version [tcorr]

0.7.296

Median SNR Y

37.89 \(\pm\) 0.00

Median SNR H

44.39 \(\pm\) 0.00

Request

Extracted 2D spectra

Extracted 1D spectra

Telluric corrected 2D spectra

Telluric corrected 1D spectra

2D Template (after telluric correction)

1D Template (after telluric correction)

Packaged extraction files (e.fits)

Packaged telluric corrected files (t.fits)

Packaged s1d extract+tcorr (s.fits)

Packaged velocity files (v.fits)

Packaged polarimetry files (p.fits)

Spectrum Downloads

File URL

Uploaded

Extracted 2D spectra

ext2d_GAIA_DR3_6013525277553837312_nirps_he_online_udem_file_list.txt

2026-03-12 22:28:55.921

Extracted 1D spectra

ext1d_GAIA_DR3_6013525277553837312_nirps_he_online_udem_file_list.txt

2026-03-12 22:28:56.099

Telluric corrected 2D spectra

tcorr2d_GAIA_DR3_6013525277553837312_nirps_he_online_udem_file_list.txt

2026-03-12 22:28:56.383

Telluric corrected 1D spectra

tcorr1d_GAIA_DR3_6013525277553837312_nirps_he_online_udem_file_list.txt

2026-03-12 22:28:56.641

Extracted 2D header file

ext2d_header_GAIA_DR3_6013525277553837312_nirps_he_online_udem_file.csv

2026-03-12 22:28:55.323

LBL

No LBL reduction found

CCF

This section presents the APERO CCF results for this object.

../../../_images/ccf_plot_GAIA_DR3_6013525277553837312_nirps_he_online_udem.png

CCF stats

Mask used

PROXIMA_neg.fits

CCF systemic velocity

298278.81 \(\pm\) 0.00 m/s

CCF FWHM

1272.99 \(\pm\) 0.00 m/s

Number of CCF files Total

1

Number of CCF passed QC

1

Number CCF files failed QC

0

First ccf file [Mid exposure]

2026-03-12 09:01:28.111

Last ccf file [Mid exposure]

2026-03-12 09:01:28.111

Last processed [ccf]

2026-03-12 16:48:20.995

Version [ccf]

0.7.296

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_GAIA_DR3_6013525277553837312_nirps_he_online_udem_file_list.txt

2026-03-12 22:28:59.330

Time series

This section deals with providing the time series information for this object

Obs Dir

First obs mid

Last obs mid

Number of ext

Number of tcorr

Seeing

Airmass

Mean Exptime

Total Exptime

SNR[Order 15 (#134 1.08um)]

SNR[Order 60 (#89 1.63um)]

DPRTYPEs

ext_files

tcorr_files

Request ext files

Request tcorr files

2026-03-11

2026-03-12 09:01:28.111

2026-03-12 09:01:28.111

1

1

0.490

1.008

897.301

897.301

37.886

44.394

OBJ_SKY

1 [download]

1 [download]

Extracted 2D files

Telluric corrected 2D files

Debug

This section has various debug plots from APERO products

Telluric map

../../../_images/debug_tcorr_map_plot_GAIA_DR3_6013525277553837312_nirps_he_online_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_GAIA_DR3_6013525277553837312_nirps_he_online_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_GAIA_DR3_6013525277553837312_nirps_he_online_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_GAIA_DR3_6013525277553837312_nirps_he_online_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_GAIA_DR3_6013525277553837312_nirps_he_online_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.