CDM52_9147 (nirps_he_online_udem)

This page was last modified: 2026-03-09 10:07:29.533081 (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=CDM52_9147

Target Information

RA

293.1380541 [deg] (Gaia DR2)

Dec

-51.98302585 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

5651.0 [K] (2020AJ….160…83S)

Spectral Type

None (None)

Proper Motion (RA)

-42.17660525 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

-92.63087642 [mas/yr] (Gaia DR2)

Parallax

9.019566186 [mas/yr] (Gaia DR2)

Radial Velocity

-14.27 [mas/yr] (2018yCat.1345….0G)

Aliases

CD-52 9147, CPC 19 7729, CPD-52 11467, GSC 08401-00665, 2MASS J19323320-5158575, PPM 774069, RAVE J193233.2-515857, TIC 406238813, TYC 8401-665-1, Gaia DR2 6645578368544928000, Gaia DR3 6645578368544928000, Gaia DR1 6645578364248973312, J1932-51, CD-529147, CPC197729, CPD-5211467, GSC08401-00665, 2MASSJ19323320-5158575, PPM774069, RAVEJ193233.2-515857, TIC406238813, TYC8401-665-1, GaiaDR26645578368544928000, GaiaDR36645578368544928000, GaiaDR16645578364248973312, J1932-51

OBJECT name(s) in headers

J1932-51

OB Name(s) in headers

J1932-51

PI name(s) in headers

UNKNOWN

Project/Run name(s) in headers

115.27UZ.001

Spectrum

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

LBL

No LBL reduction found

CCF

No CCF files found

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

2025-04-26

2025-04-27 09:22:21.598

2025-04-27 09:22:21.598

1

0

-1.000

1.091

300.958

300.958

43.581

54.670

OBJ_FP

1 [download]

0 [download]

Extracted 2D files

Telluric corrected 2D files

2025-06-21

2025-06-22 06:41:57.196

2025-06-22 06:41:57.196

1

0

1.100

1.087

300.958

300.958

38.059

47.845

OBJ_FP

1 [download]

0 [download]

Extracted 2D files

Telluric corrected 2D files

2025-06-24

2025-06-25 07:51:30.768

2025-06-25 07:51:30.768

1

0

2.670

1.154

300.958

300.958

9.653

12.188

OBJ_FP

1 [download]

0 [download]

Extracted 2D files

Telluric corrected 2D files

2025-06-29

2025-06-30 05:14:19.109

2025-06-30 05:14:19.109

1

0

1.470

1.090

300.958

300.958

33.099

42.226

OBJ_FP

1 [download]

0 [download]

Extracted 2D files

Telluric corrected 2D files

Debug

This section has various debug plots from APERO products

Telluric map

nirps_he_online_udem/object_pages/CDM52_9147/debug_tcorr_map_plot_CDM52_9147_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_CDM52_9147_nirps_he_online_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_CDM52_9147_nirps_he_online_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_CDM52_9147_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_CDM52_9147_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.