Sean M O’Brien
Scintillation-limited photometry with the 20-cm NGTS telescopes at Paranal Observatory
O’Brien, Sean M; Bayliss, Daniel; Osborn, James; Bryant, Edward M; McCormac, James; Wheatley, Peter J; Acton, Jack S; Alves, Douglas R; Anderson, David R; Burleigh, Matthew R; Casewell, Sarah L; Gill, Samuel; Goad, Michael R; Henderson, Beth A; Jackman, James AG; Lendl, Monika; Tilbrook, Rosanna H; Udry, Stéphane; Vines, Jose I; West, Richard G
Authors
Daniel Bayliss
Professor James Osborn james.osborn@durham.ac.uk
Professor
Edward M Bryant
James McCormac
Peter J Wheatley
Jack S Acton
Douglas R Alves
David R Anderson
Matthew R Burleigh
Sarah L Casewell
Samuel Gill
Michael R Goad
Beth A Henderson
James AG Jackman
Monika Lendl
Rosanna H Tilbrook
Stéphane Udry
Jose I Vines
Richard G West
Abstract
Ground-based photometry of bright stars is expected to be limited by atmospheric scintillation, although in practice observations are often limited by other sources of systematic noise. We analyse 122 nights of bright star (Gmag ≲ 11.5) photometry using the 20-cm telescopes of the Next-Generation Transit Survey (NGTS) at the Paranal Observatory in Chile. We compare the noise properties to theoretical noise models and we demonstrate that NGTS photometry of bright stars is indeed limited by atmospheric scintillation. We determine a median scintillation coefficient at the Paranal Observatory of CY=1.54, which is in good agreement with previous results derived from turbulence profiling measurements at the observatory. We find that separate NGTS telescopes make consistent measurements of scintillation when simultaneously monitoring the same field. Using contemporaneous meteorological data, we find that higher wind speeds at the tropopause correlate with a decrease in long-exposure (t = 10 s) scintillation. Hence, the winter months between June and August provide the best conditions for high-precision photometry of bright stars at the Paranal Observatory. This work demonstrates that NGTS photometric data, collected for searching for exoplanets, contains within it a record of the scintillation conditions at Paranal.
Citation
O’Brien, S. M., Bayliss, D., Osborn, J., Bryant, E. M., McCormac, J., Wheatley, P. J., Acton, J. S., Alves, D. R., Anderson, D. R., Burleigh, M. R., Casewell, S. L., Gill, S., Goad, M. R., Henderson, B. A., Jackman, J. A., Lendl, M., Tilbrook, R. H., Udry, S., Vines, J. I., & West, R. G. (2022). Scintillation-limited photometry with the 20-cm NGTS telescopes at Paranal Observatory. Monthly Notices of the Royal Astronomical Society, 509(4), 6111-6118. https://doi.org/10.1093/mnras/stab3399
Journal Article Type | Article |
---|---|
Acceptance Date | Nov 18, 2021 |
Online Publication Date | Nov 26, 2021 |
Publication Date | 2022-02 |
Deposit Date | Dec 17, 2021 |
Publicly Available Date | Jun 16, 2022 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 509 |
Issue | 4 |
Pages | 6111-6118 |
DOI | https://doi.org/10.1093/mnras/stab3399 |
Public URL | https://durham-repository.worktribe.com/output/1219339 |
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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
Copyright Statement
© The Author(s) 2021.
Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative
Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium,
provided the original work is properly cited.
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