HIP_41378 (spirou_offline_udem)

This page was last modified: 2025-08-26 17:02:29.215277 (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=HIP_41378

Target Information

RA

126.6158279 [deg] (Gaia DR2)

Dec

10.08037081 [deg] (Gaia DR2)

Finder chart

[FINDER CHART]

Teff

6251.0 [K] (2018AJ….155…21P)

Spectral Type

F8 (None)

Proper Motion (RA)

-48.14251486 [mas/yr] (Gaia DR2)

Proper Motion (Dec)

0.0593519777 [mas/yr] (Gaia DR2)

Parallax

9.37993946 [mas/yr] (Gaia DR2)

Radial Velocity

50.42 [mas/yr] (2018yCat.1345….0G)

Aliases

BD+10 1799, AG+10 1097, EPIC 211311380, GSC 00800-01325, HIC 41378, HIP 41378, K2-93, 2MASS J08262784+1004493, PPM 125260, SAO 97816, TIC 366443426, TYC 800-1325-1, YZ 10 3402, Gaia DR1 600698180468002688, Gaia DR3 600698184764497664, Gaia DR2 600698184764497664, BD+101799, AG+101097, EPIC211311380, GSC00800-01325, HIC41378, HIP41378, K2-93, 2MASSJ08262784+1004493, PPM125260, SAO97816, TIC366443426, TYC800-1325-1, YZ103402, GaiaDR1600698180468002688, GaiaDR3600698184764497664, GaiaDR2600698184764497664

OBJECT name(s) in headers

HIP 41378

PI name(s) in headers

Florian Debras

Project/Run name(s) in headers

22BD13

Spectrum

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

../../../_images/spec_plot_HIP_41378_spirou_offline_udem.png

Spectrum Information

DPRTYPES

OBJ_FP

Total number raw files

2

First raw files

2022-12-30 14:24:04.423

Last raw files

2022-12-30 14:38:55.924

Total number PP files

2

Number PP files passed QC

2

Number PP files failed QC

0

First pp file [Mid exposure]

2022-12-30 14:24:04.423

Last pp file [Mid exposure]

2022-12-30 14:38:55.924

Last processed [pp]

2025-07-26 18:30:37.201

Version [pp]

0.7.293

Total number ext files

2

Number ext files passed QC

2

Number ext files failed QC

0

First ext file [Mid exposure]

2022-12-30 14:24:04.423

Last ext file [Mid exposure]

2022-12-30 14:38:55.924

Last processed [ext]

2025-07-26 23:45:09.589

Version [ext]

0.7.293

Total number tcorr files

2

Number tcorr files passed QC

2

Number tcorr files failed QC

0

First tcorr file [Mid exposure]

2022-12-30 14:24:04.423

Last tcorr file [Mid exposure]

2022-12-30 14:38:55.924

Last processed [tcorr]

2025-07-27 09:32:48.788

Version [tcorr]

0.7.293

Median SNR Y

171.77 \(\pm\) 1.02

Median SNR H

205.29 \(\pm\) 1.04

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_HIP_41378_spirou_offline_udem_file_list.txt

2025-08-26 17:02:40.920

Extracted 1D spectra

ext1d_HIP_41378_spirou_offline_udem_file_list.txt

2025-08-26 17:02:40.962

Telluric corrected 2D spectra

tcorr2d_HIP_41378_spirou_offline_udem_file_list.txt

2025-08-26 17:02:41.016

Telluric corrected 1D spectra

tcorr1d_HIP_41378_spirou_offline_udem_file_list.txt

2025-08-26 17:02:41.102

Extracted 2D header file

ext2d_header_HIP_41378_spirou_offline_udem_file.csv

2025-08-26 17:02:40.833

LBL

No LBL reduction found

CCF

This section presents the APERO CCF results for this object.

../../../_images/ccf_plot_HIP_41378_spirou_offline_udem.png

CCF stats

Mask used

GL846_neg.fits

CCF systemic velocity

51611.33 \(\pm\) 6.83 m/s

CCF FWHM

10974.22 \(\pm\) 54.32 m/s

Number of CCF files Total

2

Number of CCF passed QC

2

Number CCF files failed QC

0

First ccf file [Mid exposure]

2022-12-30 14:24:04.423

Last ccf file [Mid exposure]

2022-12-30 14:38:55.924

Last processed [ccf]

2025-07-27 10:53:55.363

Version [ccf]

0.7.293

Request

CCF files

CCF Downloads

File URL

Uploaded

CCF Table

ccf_HIP_41378_spirou_offline_udem_file_list.txt

2025-08-26 17:02:44.076

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 8 (#71 1.08um)]

SNR[Order 35 (#44 1.75um)]

DPRTYPEs

ext_files

tcorr_files

Request ext files

Request tcorr files

2022-12-30

2022-12-30 14:24:04.423

2022-12-30 14:38:55.924

2

2

-9999.900

1.192

869.220

1738.440

171.772

205.293

OBJ_FP

2 [download]

2 [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_HIP_41378_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_HIP_41378_spirou_offline_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HIP_41378_spirou_offline_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HIP_41378_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_HIP_41378_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.