Articles | Volume 16, issue 24
https://doi.org/10.5194/amt-16-6111-2023
https://doi.org/10.5194/amt-16-6111-2023
Research article
 | 
22 Dec 2023
Research article |  | 22 Dec 2023

Multi-star calibration in starphotometry

Liviu Ivănescu and Norman T. O'Neill

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Cited articles

Alekseeva, G. A., Arkharov, A. A., Galkin, V. D., Hagen-Thorn, E., Nikanorova, I., Novikov, V. V., Novopashenny, V., Pakhomov, V., Ruban, E., and Shchegolev, D.: The Pulkovo Spectrophotometric Catalog of Bright Stars in the Range from 320 TO 1080 NM, Balt. Astron., 5, 603–838, https://doi.org/10.1515/astro-1997-0311, 1996. a
Baibakov, K., O'Neill, N. T., Ivanescu, L., Duck, T. J., Perro, C., Herber, A., Schulz, K.-H., and Schrems, O.: Synchronous polar winter starphotometry and lidar measurements at a High Arctic station, Atmos. Meas. Tech., 8, 3789–3809, https://doi.org/10.5194/amt-8-3789-2015, 2015. a
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Dachs, J.: Lichtelektrische Sternphotometrie und Farbenindexmessungen durch Zählung von Photoelektronen, PhD thesis, Tübingen University, https://www.worldcat.org/title/249623335 (last access: 4 December 2023), 1960. a
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Short summary
The starphotometers' complex infrastructure prohibits calibration campaigns. On-site calibration procedures appear as the only practical solution. A multi-star approach overcomes site-specific sky transparency stability problems. Star selection strategies were proposed for mitigating some sources of errors. Data processing strategies and instrument design improvements appear necessary.