HD188088 (nirps_he_online_udem)

This page was last modified: 2025-10-02 20:40:58.126649 (UTC)

Back to the object table

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=HD188088

Target Information

RA

298.5733335 [deg] (Gaia DR3)

Dec

-23.9428973 [deg] (Gaia DR3)

Finder chart

[FINDER CHART]

Teff

6524.0 [K] (2024A&A…683A.125P)

Spectral Type

K3VaCN1 (1989ApJS…71..245K)

Proper Motion (RA)

-124.1669387 [mas/yr] (Gaia DR3)

Proper Motion (Dec)

-410.6807867 [mas/yr] (Gaia DR3)

Parallax

70.70095857 [mas/yr] (Gaia DR3)

Radial Velocity

-5.266 [mas/yr] (2017AJ….154..120F)

Aliases

HD 188088, ** ALP 33A, CABS 171, CCABS 139, CD-24 15668, Ci 20 1172, CNS5 4923, CPD-24 6848, CSI-24 15668 21, EUVE J1954-23.9, GC 27542, GCRV 12238, GEN# +1.00188088, GJ 770, HIC 97944, HIP 97944, HR 7578, IDS 19483-2411 A, IRAS 19512-2404, LTT 7861, 2MASS J19541775-2356275, N30 4399, NLTT 48390, PLX 4686, PLX 4686.00, PMC 90-93 6604, PPM 270417, 1RXS J195417.7-235628, SAO 188692, SBC9 1182, SKY# 37280, StKM 2-1422, TIC 241967968, TYC 6891-1773-1, UBV M 24240, UBV 16923, UCAC4 331-202951, UGP 479, uvby98 100188088, V* V4200 Sgr, WDS J19543-2356A, WEB 17233, YZ 114 13860, [GKL99] 377, Gaia DR2 6863535898551993472, Gaia DR3 6863535898551993472, HD_188088, J1954-23, HD188088, **ALP33A, CABS171, CCABS139, CD-2415668, Ci201172, CNS54923, CPD-246848, CSI-241566821, EUVEJ1954-23.9, GC27542, GCRV12238, GEN#+1.00188088, GJ770, HIC97944, HIP97944, HR7578, IDS19483-2411A, IRAS19512-2404, LTT7861, 2MASSJ19541775-2356275, N304399, NLTT48390, PLX4686, PLX4686.00, PMC90-936604, PPM270417, 1RXSJ195417.7-235628, SAO188692, SBC91182, SKY#37280, StKM2-1422, TIC241967968, TYC6891-1773-1, UBVM24240, UBV16923, UCAC4331-202951, UGP479, uvby98100188088, V*V4200Sgr, WDSJ19543-2356A, WEB17233, YZ11413860, [GKL99]377, GaiaDR26863535898551993472, GaiaDR36863535898551993472, HD188088, J1954-23

OBJECT name(s) in headers

J1954-23

OB Name(s) in headers

J1954-23

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

2025-09-13

2025-09-14 01:18:46.543

2025-09-14 01:18:46.543

1

0

1.200

1.005

300.958

300.958

418.482

556.414

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

../../../_images/debug_tcorr_map_plot_HD188088_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_HD188088_nirps_he_online_udem.png

Maximum saturation level measured at time of extraction

Measured effective readout noise before extraction

../../../_images/debug_effron_plot_HD188088_nirps_he_online_udem.png

Measured effective readout noise before extraction

APERO Processing Debug Plot

../../../_images/debug_version_plot_HD188088_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_HD188088_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.