The Science Case for PILOT III: the Nearby Universe

PILOT (the Pathfinder for an International Large Optical Telescope is a proposed 2.5 m optical/infrared telescope to be located at DomeC on the Antarctic plateau. The atmospheric conditions at Dome C deliver a high sensitivity, high photometric precision, wide-field, high spatial resolution, and hig...

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Main Authors: Lawrence, J. S., Ashley, M. C. B., Bailey, J., Navascues, D. Barrado y, Bedding, T., Bland-Hawthorn, J., Bond, I., Bruntt, H., Burton, M. G., Cioni, M. -R., Eiroa, C., Epchtein, N., Kiss, L., Lagage, P. O., Minier, V., Mora, A., Olsen, K., Peri, P., Saunders, W., Stello, D., Storey, J. W. V., Tinney, C., Yock, P.
Format: Text
Language:unknown
Published: arXiv 2009
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.0905.4636
https://arxiv.org/abs/0905.4636
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spelling ftdatacite:10.48550/arxiv.0905.4636 2023-05-15T13:31:09+02:00 The Science Case for PILOT III: the Nearby Universe Lawrence, J. S. Ashley, M. C. B. Bailey, J. Navascues, D. Barrado y Bedding, T. Bland-Hawthorn, J. Bond, I. Bruntt, H. Burton, M. G. Cioni, M. -R. Eiroa, C. Epchtein, N. Kiss, L. Lagage, P. O. Minier, V. Mora, A. Olsen, K. Peri, P. Saunders, W. Stello, D. Storey, J. W. V. Tinney, C. Yock, P. 2009 https://dx.doi.org/10.48550/arxiv.0905.4636 https://arxiv.org/abs/0905.4636 unknown arXiv https://dx.doi.org/10.1071/as08051 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Solar and Stellar Astrophysics astro-ph.SR Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences article-journal Article ScholarlyArticle Text 2009 ftdatacite https://doi.org/10.48550/arxiv.0905.4636 https://doi.org/10.1071/as08051 2022-04-01T15:06:39Z PILOT (the Pathfinder for an International Large Optical Telescope is a proposed 2.5 m optical/infrared telescope to be located at DomeC on the Antarctic plateau. The atmospheric conditions at Dome C deliver a high sensitivity, high photometric precision, wide-field, high spatial resolution, and high-cadence imaging capability to the PILOT telescope. These capabilities enable a unique scientific potential for PILOT, which is addressed in this series of papers. The current paper presents a series of projects dealing with the nearby Universe that have been identified as key science drivers for the PILOT facility. Several projects are proposed that examine stellar populations in nearby galaxies and stellar clusters in order to gain insight into the formation and evolution processes of galaxies and stars. A series of projects will investigate the molecular phase of the Galaxy and explore the ecology of star formation, and investigate the formation processes of stellar and planetary systems. Three projects in the field of exoplanet science are proposed: a search for free-floating low-mass planets and dwarfs, a program of follow-up observations of gravitational microlensing events, and a study of infrared light-curves for previously discovered exoplanets. Three projects are also proposed in the field of planetary and space science: optical and near-infrared studies aimed at characterising planetary atmospheres, a study of coronal mass ejections from the Sun, and a monitoring program searching for small-scale Low Earth Orbit satellite debris items. : 27 pages, 16 figures (degraded quality), accepted for publication in PASA Text Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic The Antarctic Pasa ENVELOPE(26.733,26.733,67.850,67.850)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Solar and Stellar Astrophysics astro-ph.SR
Instrumentation and Methods for Astrophysics astro-ph.IM
FOS Physical sciences
spellingShingle Solar and Stellar Astrophysics astro-ph.SR
Instrumentation and Methods for Astrophysics astro-ph.IM
FOS Physical sciences
Lawrence, J. S.
Ashley, M. C. B.
Bailey, J.
Navascues, D. Barrado y
Bedding, T.
Bland-Hawthorn, J.
Bond, I.
Bruntt, H.
Burton, M. G.
Cioni, M. -R.
Eiroa, C.
Epchtein, N.
Kiss, L.
Lagage, P. O.
Minier, V.
Mora, A.
Olsen, K.
Peri, P.
Saunders, W.
Stello, D.
Storey, J. W. V.
Tinney, C.
Yock, P.
The Science Case for PILOT III: the Nearby Universe
topic_facet Solar and Stellar Astrophysics astro-ph.SR
Instrumentation and Methods for Astrophysics astro-ph.IM
FOS Physical sciences
description PILOT (the Pathfinder for an International Large Optical Telescope is a proposed 2.5 m optical/infrared telescope to be located at DomeC on the Antarctic plateau. The atmospheric conditions at Dome C deliver a high sensitivity, high photometric precision, wide-field, high spatial resolution, and high-cadence imaging capability to the PILOT telescope. These capabilities enable a unique scientific potential for PILOT, which is addressed in this series of papers. The current paper presents a series of projects dealing with the nearby Universe that have been identified as key science drivers for the PILOT facility. Several projects are proposed that examine stellar populations in nearby galaxies and stellar clusters in order to gain insight into the formation and evolution processes of galaxies and stars. A series of projects will investigate the molecular phase of the Galaxy and explore the ecology of star formation, and investigate the formation processes of stellar and planetary systems. Three projects in the field of exoplanet science are proposed: a search for free-floating low-mass planets and dwarfs, a program of follow-up observations of gravitational microlensing events, and a study of infrared light-curves for previously discovered exoplanets. Three projects are also proposed in the field of planetary and space science: optical and near-infrared studies aimed at characterising planetary atmospheres, a study of coronal mass ejections from the Sun, and a monitoring program searching for small-scale Low Earth Orbit satellite debris items. : 27 pages, 16 figures (degraded quality), accepted for publication in PASA
format Text
author Lawrence, J. S.
Ashley, M. C. B.
Bailey, J.
Navascues, D. Barrado y
Bedding, T.
Bland-Hawthorn, J.
Bond, I.
Bruntt, H.
Burton, M. G.
Cioni, M. -R.
Eiroa, C.
Epchtein, N.
Kiss, L.
Lagage, P. O.
Minier, V.
Mora, A.
Olsen, K.
Peri, P.
Saunders, W.
Stello, D.
Storey, J. W. V.
Tinney, C.
Yock, P.
author_facet Lawrence, J. S.
Ashley, M. C. B.
Bailey, J.
Navascues, D. Barrado y
Bedding, T.
Bland-Hawthorn, J.
Bond, I.
Bruntt, H.
Burton, M. G.
Cioni, M. -R.
Eiroa, C.
Epchtein, N.
Kiss, L.
Lagage, P. O.
Minier, V.
Mora, A.
Olsen, K.
Peri, P.
Saunders, W.
Stello, D.
Storey, J. W. V.
Tinney, C.
Yock, P.
author_sort Lawrence, J. S.
title The Science Case for PILOT III: the Nearby Universe
title_short The Science Case for PILOT III: the Nearby Universe
title_full The Science Case for PILOT III: the Nearby Universe
title_fullStr The Science Case for PILOT III: the Nearby Universe
title_full_unstemmed The Science Case for PILOT III: the Nearby Universe
title_sort science case for pilot iii: the nearby universe
publisher arXiv
publishDate 2009
url https://dx.doi.org/10.48550/arxiv.0905.4636
https://arxiv.org/abs/0905.4636
long_lat ENVELOPE(26.733,26.733,67.850,67.850)
geographic Antarctic
The Antarctic
Pasa
geographic_facet Antarctic
The Antarctic
Pasa
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_relation https://dx.doi.org/10.1071/as08051
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.0905.4636
https://doi.org/10.1071/as08051
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