TOI1130 (nirps_he_online_udem)

This page was last modified: 2025-06-03 04:02:10.730296 (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=TOI1130

Target Information

RA

286.376006 [deg] (Gaia EDR3)

Dec

-41.43764374 [deg] (Gaia EDR3)

Finder chart

[FINDER CHART]

Teff

4236.0 [K] (2019AJ….158..138S (via spirou@rali))

Spectral Type

None (None)

Proper Motion (RA)

12.57910622 [mas/yr] (Gaia EDR3)

Proper Motion (Dec)

-27.46876281 [mas/yr] (Gaia EDR3)

Parallax

17.12120845 [mas/yr] (Gaia EDR3)

Radial Velocity

-8.01 [mas/yr] (2018yCat.1345….0G)

Aliases

2MASS J19053021-4126151, TIC 254113311, TOI-1130, TYC 7925-2200-1, Gaia EDR3 6715688452614516736, Gaia DR2 6715688452614516736, TOIM1130, TOI1130, 2MASSJ19053021-4126151, TIC254113311, TOI-1130, TYC7925-2200-1, GaiaEDR36715688452614516736, GaiaDR26715688452614516736, TOIM1130, TOI1130

OBJECT name(s) in headers

TOI-1130

OB Name(s) in headers

TOI-1130_01_06_05h00UT, TOI-1130_02_07_05h20UT_HAM

PI name(s) in headers

UNKNOWN

Project/Run name(s) in headers

112.25P3.004, 112.25P3.002

Spectrum

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

../../../_images/spec_plot_TOI1130_nirps_he_online_udem.png

Spectrum Information

DPRTYPES

OBJ_SKY

Total number raw files

84

First raw files

2024-07-03 05:26:56.710

Last raw files

2025-06-02 08:43:41.316

Total number PP files

84

Number PP files passed QC

84

Number PP files failed QC

0

First pp file [Mid exposure]

2024-07-03 05:26:56.710

Last pp file [Mid exposure]

2025-06-02 08:43:41.316

Last processed [pp]

2025-06-03 00:03:27.965

Version [pp]

0.7.292,0.7.294

Total number ext files

84

Number ext files passed QC

84

Number ext files failed QC

0

First ext file [Mid exposure]

2024-07-03 05:26:56.710

Last ext file [Mid exposure]

2025-06-02 08:43:41.316

Last processed [ext]

2025-06-03 00:35:14.659

Version [ext]

0.7.292,0.7.294

Total number tcorr files

84

Number tcorr files passed QC

84

Number tcorr files failed QC

0

First tcorr file [Mid exposure]

2024-07-03 05:26:56.710

Last tcorr file [Mid exposure]

2025-06-02 08:43:41.316

Last processed [tcorr]

2025-06-03 00:51:26.539

Version [tcorr]

0.7.292,0.7.294

Median SNR Y

28.10 \(\pm\) 6.72

Median SNR H

48.17 \(\pm\) 8.38

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_TOI1130_nirps_he_online_udem_file_list.txt

2025-06-03 04:02:22.470

Extracted 1D spectra

ext1d_TOI1130_nirps_he_online_udem_file_list.txt

2025-06-03 04:02:22.471

Telluric corrected 2D spectra

tcorr2d_TOI1130_nirps_he_online_udem_file_list.txt

2025-06-03 04:02:22.473

Telluric corrected 1D spectra

tcorr1d_TOI1130_nirps_he_online_udem_file_list.txt

2025-06-03 04:02:22.474

Extracted 2D header file

ext2d_header_TOI1130_nirps_he_online_udem_file.csv

2025-06-03 04:02:22.437

LBL (TOI1130_TOI1130)

This section presents the LBL results for TOI1130_TOI1130. The first object is the target we measure RVs for the second is the “friend” or “template” that was used to calculate those RVs.

../../../_images/lbl_plot_TOI1130_TOI1130_nirps_he_online_udem.png

LBL stats

RV Uncertainty lbl.rdb (25, 50, 75 percentile)

4.90, 5.42, 6.17 m/s

RV Absolute Deviation lbl.rdb (25, 50, 75 percentile)

23.27, 40.43, 52.95 m/s

Number of lbl.rdb Measurements

84

Number of lbl.rdb Spurious Low Points

0

Number of lbl.rdb Spurious High Points

0

Number of Nights

2

Number of Reset RV Points

0

Systemic Velocity

-7743.01 m/s

Velocity Domain considered valid

-7954.46 to -7565.35 m/s

LBL Version

0.65.002

Request

LBL fits files

lbl_rdb files

lbl2_rdb files

lbl_drift files

lbl2_drift files

lbl_fits files

LBL Downloads

File URL

Uploaded

RDB file

lbl_TOI1130_TOI1130.rdb

2025-06-03 02:31:03.192

RDB2 file

lbl2_TOI1130_TOI1130.rdb

2025-06-03 02:31:06.168

LBL (TOI1130_HD85512)

This section presents the LBL results for TOI1130_HD85512. The first object is the target we measure RVs for the second is the “friend” or “template” that was used to calculate those RVs.

../../../_images/lbl_plot_TOI1130_HD85512_nirps_he_online_udem.png

LBL stats

RV Uncertainty lbl.rdb (25, 50, 75 percentile)

10.29, 12.49, 13.75 m/s

RV Absolute Deviation lbl.rdb (25, 50, 75 percentile)

33.36, 50.12, 92.98 m/s

Number of lbl.rdb Measurements

84

Number of lbl.rdb Spurious Low Points

0

Number of lbl.rdb Spurious High Points

0

Number of Nights

2

Number of Reset RV Points

0

Systemic Velocity

-7712.51 m/s

Velocity Domain considered valid

-7956.38 to -7530.40 m/s

LBL Version

0.65.002

Request

LBL fits files

lbl_rdb files

lbl2_rdb files

lbl_drift files

lbl2_drift files

lbl_fits files

LBL Downloads

File URL

Uploaded

RDB file

lbl_TOI1130_HD85512.rdb

2025-06-03 02:31:58.764

RDB2 file

lbl2_TOI1130_HD85512.rdb

2025-06-03 02:32:00.368

CCF

This section presents the APERO CCF results for this object.

../../../_images/ccf_plot_TOI1130_nirps_he_online_udem.png

CCF stats

Mask used

GJ9425_neg.fits

CCF systemic velocity

-7732.27 \(\pm\) 67.18 m/s

CCF FWHM

6945.25 \(\pm\) 72.33 m/s

Number of CCF files Total

84

Number of CCF passed QC

84

Number CCF files failed QC

0

First ccf file [Mid exposure]

2024-07-03 05:26:56.710

Last ccf file [Mid exposure]

2025-06-02 08:43:41.316

Last processed [ccf]

2025-06-03 00:55:54.913

Version [ccf]

0.7.292,0.7.294

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_TOI1130_nirps_he_online_udem_file_list.txt

2025-06-03 04:02:47.189

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

2024-07-02

2024-07-03 05:26:56.710

2024-07-03 08:55:00.778

41

41

1.260

1.174

300.958

12339.286

25.672

44.920

OBJ_SKY

41 [download]

41 [download]

Extracted 2D files

Telluric corrected 2D files

2025-06-01

2025-06-02 05:05:13.041

2025-06-02 08:43:41.316

43

43

0.754

1.053

300.958

12941.203

32.103

51.425

OBJ_SKY

43 [download]

43 [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_TOI1130_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_TOI1130_nirps_he_online_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_TOI1130_nirps_he_online_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_TOI1130_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_TOI1130_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.