Exoplanets from the arctic: The first wide-field survey at 80°N

Located within 10° of the North Pole, northern Ellesmere Island offers continuous darkness in the winter months. This capability can greatly enhance the detection efficiency of planetary transit surveys and other time domain astronomy programs. We deployed two wide-field cameras at 80°N, near Eureka...

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Published in:The Astronomical Journal
Main Authors: Law, N.M., Carlberg, R., Salbi, P., Ngan, W.-H.W., Ahmadi, A., Steinbring, E., Murowinski, R., Sivanandam, S., Kerzendorf, W.
Format: Article in Journal/Newspaper
Language:English
Published: 2013
Subjects:
Online Access:https://doi.org/10.1088/0004-6256/145/3/58
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spelling ftnrccanada:oai:cisti-icist.nrc-cnrc.ca:cistinparc:21269943 2023-05-15T14:58:43+02:00 Exoplanets from the arctic: The first wide-field survey at 80°N Law, N.M. Carlberg, R. Salbi, P. Ngan, W.-H.W. Ahmadi, A. Steinbring, E. Murowinski, R. Sivanandam, S. Kerzendorf, W. 2013 text https://doi.org/10.1088/0004-6256/145/3/58 https://nrc-publications.canada.ca/eng/view/object/?id=38e7268f-99bb-4bee-9410-4d6d7c08dc0f https://nrc-publications.canada.ca/fra/voir/objet/?id=38e7268f-99bb-4bee-9410-4d6d7c08dc0f eng eng issn:0004-6256 Astronomical Journal, Volume: 145, Issue: 3, Publication date: 2013 doi:10.1088/0004-6256/145/3/58 article 2013 ftnrccanada https://doi.org/10.1088/0004-6256/145/3/58 2021-09-01T06:27:46Z Located within 10° of the North Pole, northern Ellesmere Island offers continuous darkness in the winter months. This capability can greatly enhance the detection efficiency of planetary transit surveys and other time domain astronomy programs. We deployed two wide-field cameras at 80°N, near Eureka, Nunavut, for a 152 hr observing campaign in 2012 February. The 16 megapixel camera systems were based on commercial f/1.2 lenses with 70 mm and 42 mm apertures, and they continuously imaged 504 and 1295 deg2, respectively. In total, the cameras took over 44,000 images and produced better than 1% precision light curves for approximately 10,000 stars. We describe a new high-speed astrometric and photometric data reduction pipeline designed for the systems, test several methods for the precision flat fielding of images from very-wide-angle cameras, and evaluate the cameras' image qualities. We achieved a scintillation-limited photometric precision of 1%-2% in each 10 s exposure. Binning the short exposures into 10 minute chunks provided a photometric stability of 2-3 mmag, sufficient for the detection of transiting exoplanets around the bright stars targeted by our survey. We estimate that the cameras, when operated over the full Arctic winter, will be capable of discovering several transiting exoplanets around bright (mV < 9.5) stars. © 2013. The American Astronomical Society. All rights reserved. Peer reviewed: Yes NRC publication: Yes Article in Journal/Newspaper Arctic Ellesmere Island Eureka Nunavut National Research Council Canada: NRC Publications Archive Arctic Ellesmere Island Eureka ENVELOPE(-85.940,-85.940,79.990,79.990) North Pole Nunavut The Astronomical Journal 145 3 58
institution Open Polar
collection National Research Council Canada: NRC Publications Archive
op_collection_id ftnrccanada
language English
description Located within 10° of the North Pole, northern Ellesmere Island offers continuous darkness in the winter months. This capability can greatly enhance the detection efficiency of planetary transit surveys and other time domain astronomy programs. We deployed two wide-field cameras at 80°N, near Eureka, Nunavut, for a 152 hr observing campaign in 2012 February. The 16 megapixel camera systems were based on commercial f/1.2 lenses with 70 mm and 42 mm apertures, and they continuously imaged 504 and 1295 deg2, respectively. In total, the cameras took over 44,000 images and produced better than 1% precision light curves for approximately 10,000 stars. We describe a new high-speed astrometric and photometric data reduction pipeline designed for the systems, test several methods for the precision flat fielding of images from very-wide-angle cameras, and evaluate the cameras' image qualities. We achieved a scintillation-limited photometric precision of 1%-2% in each 10 s exposure. Binning the short exposures into 10 minute chunks provided a photometric stability of 2-3 mmag, sufficient for the detection of transiting exoplanets around the bright stars targeted by our survey. We estimate that the cameras, when operated over the full Arctic winter, will be capable of discovering several transiting exoplanets around bright (mV < 9.5) stars. © 2013. The American Astronomical Society. All rights reserved. Peer reviewed: Yes NRC publication: Yes
format Article in Journal/Newspaper
author Law, N.M.
Carlberg, R.
Salbi, P.
Ngan, W.-H.W.
Ahmadi, A.
Steinbring, E.
Murowinski, R.
Sivanandam, S.
Kerzendorf, W.
spellingShingle Law, N.M.
Carlberg, R.
Salbi, P.
Ngan, W.-H.W.
Ahmadi, A.
Steinbring, E.
Murowinski, R.
Sivanandam, S.
Kerzendorf, W.
Exoplanets from the arctic: The first wide-field survey at 80°N
author_facet Law, N.M.
Carlberg, R.
Salbi, P.
Ngan, W.-H.W.
Ahmadi, A.
Steinbring, E.
Murowinski, R.
Sivanandam, S.
Kerzendorf, W.
author_sort Law, N.M.
title Exoplanets from the arctic: The first wide-field survey at 80°N
title_short Exoplanets from the arctic: The first wide-field survey at 80°N
title_full Exoplanets from the arctic: The first wide-field survey at 80°N
title_fullStr Exoplanets from the arctic: The first wide-field survey at 80°N
title_full_unstemmed Exoplanets from the arctic: The first wide-field survey at 80°N
title_sort exoplanets from the arctic: the first wide-field survey at 80°n
publishDate 2013
url https://doi.org/10.1088/0004-6256/145/3/58
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https://nrc-publications.canada.ca/fra/voir/objet/?id=38e7268f-99bb-4bee-9410-4d6d7c08dc0f
long_lat ENVELOPE(-85.940,-85.940,79.990,79.990)
geographic Arctic
Ellesmere Island
Eureka
North Pole
Nunavut
geographic_facet Arctic
Ellesmere Island
Eureka
North Pole
Nunavut
genre Arctic
Ellesmere Island
Eureka
Nunavut
genre_facet Arctic
Ellesmere Island
Eureka
Nunavut
op_relation issn:0004-6256
Astronomical Journal, Volume: 145, Issue: 3, Publication date: 2013
doi:10.1088/0004-6256/145/3/58
op_doi https://doi.org/10.1088/0004-6256/145/3/58
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