TOIM772 (nirps_ha_online_udem)

This page was last modified: 2026-03-19 16:00:40.719650 (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=TOIM772

Target Information

RA

190.1913967 [deg] (Gaia DR3)

Dec

-21.8727832 [deg] (Gaia DR3)

Finder chart

[FINDER CHART]

Teff

5144.0 [K] (2024A&A…683A.125P)

Spectral Type

None (None)

Proper Motion (RA)

-29.71778133 [mas/yr] (Gaia DR3)

Proper Motion (Dec)

-11.63587814 [mas/yr] (Gaia DR3)

Parallax

7.316676863 [mas/yr] (Gaia DR3)

Radial Velocity

-15.12 [mas/yr] (2018yCat.1345….0G)

Aliases

TYC 6110-1007-1, 2MASS J12404596-2152217, TIC 286864983, TOI-772, Gaia DR2 3502914269362946688, Gaia DR3 3502914269362946688, Gaia DR1 3502914269362946688, TOI-772A, TOIM772A, TYC6110-1007-1, 2MASSJ12404596-2152217, TIC286864983, TOI-772, GaiaDR23502914269362946688, GaiaDR33502914269362946688, GaiaDR13502914269362946688, TOI-772A, TOIM772A

OBJECT name(s) in headers

TOI-772A

OB Name(s) in headers

TOI-772A-12h40

PI name(s) in headers

UNKNOWN

Project/Run name(s) in headers

116.297P.001

Spectrum

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

../../../_images/spec_plot_TOIM772_nirps_ha_online_udem.png

Spectrum Information

DPRTYPES

OBJ_SKY

Total number raw files

8

Number of rejected files

0

First raw files

2026-03-04 04:45:15.506

Last raw files

2026-03-17 03:48:12.287

Total number PP files

8

Number PP files passed QC

8

Number PP files failed QC

0

First pp file [Mid exposure]

2026-03-04 04:45:15.506

Last pp file [Mid exposure]

2026-03-17 03:48:12.287

Last processed [pp]

2026-03-19 14:27:02.627

Version [pp]

0.7.296

Total number ext files

8

Number ext files passed QC

8

Number ext files failed QC

0

First ext file [Mid exposure]

2026-03-04 04:45:15.506

Last ext file [Mid exposure]

2026-03-17 03:48:12.287

Last processed [ext]

2026-03-19 15:02:52.279

Version [ext]

0.7.296

Total number tcorr files

8

Number tcorr files passed QC

8

Number tcorr files failed QC

0

First tcorr file [Mid exposure]

2026-03-04 04:45:15.506

Last tcorr file [Mid exposure]

2026-03-17 03:48:12.287

Last processed [tcorr]

2026-03-19 15:07:31.549

Version [tcorr]

0.7.296

Median SNR Y

22.28 \(\pm\) 9.49

Median SNR H

34.50 \(\pm\) 11.49

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_TOIM772_nirps_ha_online_udem_file_list.txt

2026-03-19 16:00:47.073

Extracted 1D spectra

ext1d_TOIM772_nirps_ha_online_udem_file_list.txt

2026-03-19 16:00:47.074

Telluric corrected 2D spectra

tcorr2d_TOIM772_nirps_ha_online_udem_file_list.txt

2026-03-19 16:00:47.076

Telluric corrected 1D spectra

tcorr1d_TOIM772_nirps_ha_online_udem_file_list.txt

2026-03-19 16:00:47.077

Extracted 2D header file

ext2d_header_TOIM772_nirps_ha_online_udem_file.csv

2026-03-19 16:00:47.070

LBL (TOIM772_TOIM772)

This section presents the LBL results for TOIM772_TOIM772. 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_TOIM772_TOIM772_nirps_ha_online_udem.png

LBL stats

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

2.49, 5.36, 6.07 m/s

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

101.77, 137.92, 158.44 m/s

Number of lbl.rdb Measurements

8

Number of lbl.rdb Spurious Low Points

0

Number of lbl.rdb Spurious High Points

0

Number of Nights

3

Number of Reset RV Points

1

Systemic Velocity

-124135.92 m/s

Velocity Domain considered valid

-124569.79 to -123666.39 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_TOIM772_TOIM772.rdb

2026-03-19 15:39:18.954

RDB2 file

lbl2_TOIM772_TOIM772.rdb

2026-03-19 15:39:37.877

LBL (TOIM772_HD85512)

This section presents the LBL results for TOIM772_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_TOIM772_HD85512_nirps_ha_online_udem.png

LBL stats

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

11.41, 14.80, 16.54 m/s

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

35.31, 47.67, 61.81 m/s

Number of lbl.rdb Measurements

8

Number of lbl.rdb Spurious Low Points

0

Number of lbl.rdb Spurious High Points

0

Number of Nights

3

Number of Reset RV Points

0

Systemic Velocity

-15274.65 m/s

Velocity Domain considered valid

-15457.80 to -15094.49 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_TOIM772_HD85512.rdb

2026-03-19 15:40:03.106

RDB2 file

lbl2_TOIM772_HD85512.rdb

2026-03-19 15:40:13.796

CCF

This section presents the APERO CCF results for this object.

../../../_images/ccf_plot_TOIM772_nirps_ha_online_udem.png

CCF stats

Mask used

GJ9425_neg.fits

CCF systemic velocity

-15279.11 \(\pm\) 165.98 m/s

CCF FWHM

9703.87 \(\pm\) 226.49 m/s

Number of CCF files Total

8

Number of CCF passed QC

8

Number CCF files failed QC

0

First ccf file [Mid exposure]

2026-03-04 04:45:15.506

Last ccf file [Mid exposure]

2026-03-17 03:48:12.287

Last processed [ccf]

2026-03-19 15:09:25.664

Version [ccf]

0.7.296

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_TOIM772_nirps_ha_online_udem_file_list.txt

2026-03-19 16:00:52.234

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

2026-03-03

2026-03-04 04:45:15.506

2026-03-04 05:12:22.893

3

3

0.410

1.102

802.555

2407.666

36.128

50.430

OBJ_SKY

3 [download]

3 [download]

Extracted 2D files

Telluric corrected 2D files

2026-03-15

2026-03-16 06:15:55.675

2026-03-16 06:29:29.368

2

2

0.945

1.014

802.555

1605.110

19.586

31.224

OBJ_SKY

2 [download]

2 [download]

Extracted 2D files

Telluric corrected 2D files

2026-03-16

2026-03-17 03:21:04.901

2026-03-17 03:48:12.287

3

3

1.463

1.179

802.555

2407.666

18.548

28.802

OBJ_SKY

3 [download]

3 [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_TOIM772_nirps_ha_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_TOIM772_nirps_ha_online_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_TOIM772_nirps_ha_online_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_TOIM772_nirps_ha_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_TOIM772_nirps_ha_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.