STRESS STEREO TRansiting Exoplanet and Stellar Survey

Research output: Contribution to conference (unpublished) › Paper › peer-review

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STRESS STEREO TRansiting Exoplanet and Stellar Survey. / Sangaralingam, Vinothini; Stevens, Ian; Spreckley, S; Debosscher, J.

2010. 434-439 Paper presented at Proceedings of the International Astronomical Union, .

Research output: Contribution to conference (unpublished) › Paper › peer-review

Harvard

Sangaralingam, V, Stevens, I, Spreckley, S & Debosscher, J 2010, 'STRESS STEREO TRansiting Exoplanet and Stellar Survey', Paper presented at Proceedings of the International Astronomical Union, 1/01/10 pp. 434-439. https://doi.org/10.1017/S174392130999305X

APA

Sangaralingam, V., Stevens, I., Spreckley, S., & Debosscher, J. (2010). STRESS STEREO TRansiting Exoplanet and Stellar Survey. 434-439. Paper presented at Proceedings of the International Astronomical Union, . https://doi.org/10.1017/S174392130999305X

Vancouver

Sangaralingam V, Stevens I, Spreckley S, Debosscher J. STRESS STEREO TRansiting Exoplanet and Stellar Survey. 2010. Paper presented at Proceedings of the International Astronomical Union, . https://doi.org/10.1017/S174392130999305X

Author

Sangaralingam, Vinothini ; Stevens, Ian ; Spreckley, S ; Debosscher, J. / STRESS STEREO TRansiting Exoplanet and Stellar Survey. Paper presented at Proceedings of the International Astronomical Union, .6 p.

Bibtex

@conference{ec8a7499765c4cafad65d3a257867523,
title = "STRESS STEREO TRansiting Exoplanet and Stellar Survey",
abstract = "The Heliospheric Imager (HI) instruments on board the two STEREO (Solar TErrestrial RElations Observatory) spacecraft provides an excellent opportunity for space based stellar photometry. The HI instruments provide a wide area coverage (20° × 20° for the two HI-1 instruments and 70° × 70° for the two HI-2 instruments) and long continuous periods of observations (20 days and 70 days respectively). Using HI-1A which has a pass band of 6500{\AA} to 7500{\AA} and a cadence of 40 minutes, we have gathered photometric information for more than a million stars brighter than 12th magnitude for a period of two years. Here we present some early results from this study on a range of variable stars and the future prospects for the data.",
keywords = "stars: variables, survey, etc, methods: data analysis, techniques: image processing",
author = "Vinothini Sangaralingam and Ian Stevens and S Spreckley and J Debosscher",
year = "2010",
month = jan,
day = "1",
doi = "10.1017/S174392130999305X",
language = "English",
pages = "434--439",
note = "Proceedings of the International Astronomical Union ; Conference date: 01-01-2010",

}

RIS

TY - CONF

T1 - STRESS STEREO TRansiting Exoplanet and Stellar Survey

AU - Sangaralingam, Vinothini

AU - Stevens, Ian

AU - Spreckley, S

AU - Debosscher, J

PY - 2010/1/1

Y1 - 2010/1/1

N2 - The Heliospheric Imager (HI) instruments on board the two STEREO (Solar TErrestrial RElations Observatory) spacecraft provides an excellent opportunity for space based stellar photometry. The HI instruments provide a wide area coverage (20° × 20° for the two HI-1 instruments and 70° × 70° for the two HI-2 instruments) and long continuous periods of observations (20 days and 70 days respectively). Using HI-1A which has a pass band of 6500Å to 7500Å and a cadence of 40 minutes, we have gathered photometric information for more than a million stars brighter than 12th magnitude for a period of two years. Here we present some early results from this study on a range of variable stars and the future prospects for the data.

AB - The Heliospheric Imager (HI) instruments on board the two STEREO (Solar TErrestrial RElations Observatory) spacecraft provides an excellent opportunity for space based stellar photometry. The HI instruments provide a wide area coverage (20° × 20° for the two HI-1 instruments and 70° × 70° for the two HI-2 instruments) and long continuous periods of observations (20 days and 70 days respectively). Using HI-1A which has a pass band of 6500Å to 7500Å and a cadence of 40 minutes, we have gathered photometric information for more than a million stars brighter than 12th magnitude for a period of two years. Here we present some early results from this study on a range of variable stars and the future prospects for the data.

KW - stars: variables, survey, etc

KW - methods: data analysis

KW - techniques: image processing

U2 - 10.1017/S174392130999305X

DO - 10.1017/S174392130999305X

M3 - Paper

SP - 434

EP - 439

T2 - Proceedings of the International Astronomical Union

Y2 - 1 January 2010

ER -