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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author Ivănescu, Liviu
O'Neill, Norman T.
author_facet Ivănescu, Liviu
O'Neill, Norman T.
author_sort Ivănescu, Liviu
collection Copernicus Publications: E-Journals
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.
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op_doi https://doi.org/10.5194/egusphere-2023-1383
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spelling ftcopernicus:oai:publications.copernicus.org:egusphere112648 2025-01-16T20:33:11+00:00 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)
spellingShingle Ivănescu, Liviu
O'Neill, Norman T.
Multi-star calibration in starphotometry
title 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_short Multi-star calibration in starphotometry
title_sort multi-star calibration in starphotometry
url https://doi.org/10.5194/egusphere-2023-1383
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1383/