Multi-star calibration in starphotometry

We explored the improvement in starphotometry accuracy using a multi-star Langley calibration in lieu of the more traditional one-star Langley approach. Our goal was a 0.01 calibration-constant repeatability accuracy, at an operational sea-level facility such as our Arctic site at Eureka. Multi-star...

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Main Authors: Ivănescu, Liviu, O'Neill, Norman T.
Format: Text
Language:English
Published: 2023
Subjects:
Online Access:https://doi.org/10.5194/egusphere-2023-1383
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1383/
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spelling ftcopernicus:oai:publications.copernicus.org:egusphere112648 2024-01-21T10:03:43+01:00 Multi-star calibration in starphotometry Ivănescu, Liviu O'Neill, Norman T. 2023-12-22 application/pdf https://doi.org/10.5194/egusphere-2023-1383 https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1383/ eng eng doi:10.5194/egusphere-2023-1383 https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1383/ eISSN: Text 2023 ftcopernicus https://doi.org/10.5194/egusphere-2023-1383 2023-12-25T17:24:18Z We explored the improvement in starphotometry accuracy using a multi-star Langley calibration in lieu of the more traditional one-star Langley approach. Our goal was a 0.01 calibration-constant repeatability accuracy, at an operational sea-level facility such as our Arctic site at Eureka. Multi-star calibration errors were systematically smaller than single-star errors and, in the mid-spectrum, approached the 0.01 target for an observing period of 2.5 h. Filtering out coarse-mode (supermicrometre) contributions appears mandatory for improvements. Spectral vignetting, likely linked to significant UV/blue spectrum errors at large air mass, may be due to a limiting field of view and/or sub-optimal telescope collimation. Starphotometer measurements acquired by instruments that have been designed to overcome such effects may improve future star magnitude catalogues and consequently starphotometry accuracy. Text Arctic Copernicus Publications: E-Journals Arctic Eureka ENVELOPE(-85.940,-85.940,79.990,79.990)
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description We explored the improvement in starphotometry accuracy using a multi-star Langley calibration in lieu of the more traditional one-star Langley approach. Our goal was a 0.01 calibration-constant repeatability accuracy, at an operational sea-level facility such as our Arctic site at Eureka. Multi-star calibration errors were systematically smaller than single-star errors and, in the mid-spectrum, approached the 0.01 target for an observing period of 2.5 h. Filtering out coarse-mode (supermicrometre) contributions appears mandatory for improvements. Spectral vignetting, likely linked to significant UV/blue spectrum errors at large air mass, may be due to a limiting field of view and/or sub-optimal telescope collimation. Starphotometer measurements acquired by instruments that have been designed to overcome such effects may improve future star magnitude catalogues and consequently starphotometry accuracy.
format Text
author Ivănescu, Liviu
O'Neill, Norman T.
spellingShingle Ivănescu, Liviu
O'Neill, Norman T.
Multi-star calibration in starphotometry
author_facet Ivănescu, Liviu
O'Neill, Norman T.
author_sort Ivănescu, Liviu
title Multi-star calibration in starphotometry
title_short Multi-star calibration in starphotometry
title_full Multi-star calibration in starphotometry
title_fullStr Multi-star calibration in starphotometry
title_full_unstemmed Multi-star calibration in starphotometry
title_sort multi-star calibration in starphotometry
publishDate 2023
url https://doi.org/10.5194/egusphere-2023-1383
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1383/
long_lat ENVELOPE(-85.940,-85.940,79.990,79.990)
geographic Arctic
Eureka
geographic_facet Arctic
Eureka
genre Arctic
genre_facet Arctic
op_source eISSN:
op_relation doi:10.5194/egusphere-2023-1383
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1383/
op_doi https://doi.org/10.5194/egusphere-2023-1383
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