An adaptive 2 m class telescope for a microlensing search from Antarctica

We describe the scientific rationale and the preliminary optomechanical design for a 2 m class telescope designed to achieve ground layer correction over a ≈15 arcmin Field of View (FoV) to be located at the Dome-C site. The proposed science case is the detection of microlensing events in and by glo...

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Main Authors: R. Ragazzoni, C. Arcidiacono, G. Bono, E. Diolaiti, J. Farinato, A. Moore, A. Riccardi, P. Salinari, R. Soci, E. Vernet, F. Casoli, F. Paletou, BUSSO, Maurizio Maria, TOSTI, Gino
Other Authors: Giard, Martin, R., Ragazzoni, C., Arcidiacono, G., Bono, Busso, Maurizio Maria, E., Diolaiti, J., Farinato, A., Moore, A., Riccardi, P., Salinari, R., Soci, Tosti, Gino, E., Vernet, F., Casoli, F., Paletou
Format: Conference Object
Language:unknown
Published: 2005
Subjects:
Online Access:http://hdl.handle.net/11391/994391
http://adsabs.harvard.edu/abs/2005EAS.14.161R
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spelling ftuniperugiairis:oai:research.unipg.it:11391/994391 2024-02-11T09:58:13+01:00 An adaptive 2 m class telescope for a microlensing search from Antarctica R. Ragazzoni C. Arcidiacono G. Bono E. Diolaiti J. Farinato A. Moore A. Riccardi P. Salinari R. Soci E. Vernet F. Casoli F. Paletou BUSSO, Maurizio Maria TOSTI, Gino Giard, Martin R., Ragazzoni C., Arcidiacono G., Bono Busso, Maurizio Maria E., Diolaiti J., Farinato A., Moore A., Riccardi P., Salinari R., Soci Tosti, Gino E., Vernet F., Casoli F., Paletou 2005 http://hdl.handle.net/11391/994391 http://adsabs.harvard.edu/abs/2005EAS.14.161R unknown info:eu-repo/semantics/altIdentifier/wos/WOS:000231723200024 ispartofbook:EAS Publications Series volume:14 firstpage:161 lastpage:167 numberofpages:6 journal:EAS PUBLICATIONS SERIES http://hdl.handle.net/11391/994391 info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-33749256094 http://adsabs.harvard.edu/abs/2005EAS.14.161R info:eu-repo/semantics/conferenceObject 2005 ftuniperugiairis 2024-01-24T17:51:13Z We describe the scientific rationale and the preliminary optomechanical design for a 2 m class telescope designed to achieve ground layer correction over a ≈15 arcmin Field of View (FoV) to be located at the Dome-C site. The proposed science case is the detection of microlensing events in and by globular clusters and nearby galaxies that, for a high probability of success, requires exceptional seeing (≈0.2 arcsec or better) and a large target density (the centre of a globular cluster with a corresponding telescope FoV of ≈15 arcmin). This approach can capitalise on some of the unique qualities already observed above the Dome-C site, namely that the atmospheric turbulence is largely limited to a ground layer of small thickness only, a relatively low Greenwood frequency and uniterrupted sky coverage during the winter months for objects such as the globular cluster 47-Tuc. Further to the central science case of microlensing the telescope could provide a technological testbed for future telescopes and, given the unique atmospheric properties witnessed already during previous site testing compaigns, has the chance to provide a large amount of data (based on accurate and continuous light curves lasting several months) for fields of research outside that of microlensing. Details of the specific concepts of adaptive optics to be adopted for this telescope are outlined. Conference Object Antarc* Antarctica IRIS Università degli Studi di Perugia
institution Open Polar
collection IRIS Università degli Studi di Perugia
op_collection_id ftuniperugiairis
language unknown
description We describe the scientific rationale and the preliminary optomechanical design for a 2 m class telescope designed to achieve ground layer correction over a ≈15 arcmin Field of View (FoV) to be located at the Dome-C site. The proposed science case is the detection of microlensing events in and by globular clusters and nearby galaxies that, for a high probability of success, requires exceptional seeing (≈0.2 arcsec or better) and a large target density (the centre of a globular cluster with a corresponding telescope FoV of ≈15 arcmin). This approach can capitalise on some of the unique qualities already observed above the Dome-C site, namely that the atmospheric turbulence is largely limited to a ground layer of small thickness only, a relatively low Greenwood frequency and uniterrupted sky coverage during the winter months for objects such as the globular cluster 47-Tuc. Further to the central science case of microlensing the telescope could provide a technological testbed for future telescopes and, given the unique atmospheric properties witnessed already during previous site testing compaigns, has the chance to provide a large amount of data (based on accurate and continuous light curves lasting several months) for fields of research outside that of microlensing. Details of the specific concepts of adaptive optics to be adopted for this telescope are outlined.
author2 Giard, Martin
R., Ragazzoni
C., Arcidiacono
G., Bono
Busso, Maurizio Maria
E., Diolaiti
J., Farinato
A., Moore
A., Riccardi
P., Salinari
R., Soci
Tosti, Gino
E., Vernet
F., Casoli
F., Paletou
format Conference Object
author R. Ragazzoni
C. Arcidiacono
G. Bono
E. Diolaiti
J. Farinato
A. Moore
A. Riccardi
P. Salinari
R. Soci
E. Vernet
F. Casoli
F. Paletou
BUSSO, Maurizio Maria
TOSTI, Gino
spellingShingle R. Ragazzoni
C. Arcidiacono
G. Bono
E. Diolaiti
J. Farinato
A. Moore
A. Riccardi
P. Salinari
R. Soci
E. Vernet
F. Casoli
F. Paletou
BUSSO, Maurizio Maria
TOSTI, Gino
An adaptive 2 m class telescope for a microlensing search from Antarctica
author_facet R. Ragazzoni
C. Arcidiacono
G. Bono
E. Diolaiti
J. Farinato
A. Moore
A. Riccardi
P. Salinari
R. Soci
E. Vernet
F. Casoli
F. Paletou
BUSSO, Maurizio Maria
TOSTI, Gino
author_sort R. Ragazzoni
title An adaptive 2 m class telescope for a microlensing search from Antarctica
title_short An adaptive 2 m class telescope for a microlensing search from Antarctica
title_full An adaptive 2 m class telescope for a microlensing search from Antarctica
title_fullStr An adaptive 2 m class telescope for a microlensing search from Antarctica
title_full_unstemmed An adaptive 2 m class telescope for a microlensing search from Antarctica
title_sort adaptive 2 m class telescope for a microlensing search from antarctica
publishDate 2005
url http://hdl.handle.net/11391/994391
http://adsabs.harvard.edu/abs/2005EAS.14.161R
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation info:eu-repo/semantics/altIdentifier/wos/WOS:000231723200024
ispartofbook:EAS Publications Series
volume:14
firstpage:161
lastpage:167
numberofpages:6
journal:EAS PUBLICATIONS SERIES
http://hdl.handle.net/11391/994391
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-33749256094
http://adsabs.harvard.edu/abs/2005EAS.14.161R
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