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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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) |
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Open Polar |
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Copernicus Publications: E-Journals |
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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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1788694025225633792 |