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Microlensing of unresolved stars as a brown dwarf detection method

We describe a project of brown dwarf detection in the dark halo of a galaxy using the microlensing effect. We argue that monitoring pixels instead of stars could provide an enhancement in the number of detectable events. We estimate the detection efficiency with a Monte-Carlo simulation. We expect a...

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Detalles Bibliográficos
Autores principales: Bouquet, Alain, Kaplan, Jean, Melchior, Anne-Laure, Giraud-Heraud, Yannick, Baillon, Paul
Lenguaje:eng
Publicado: 1993
Materias:
Acceso en línea:http://cds.cern.ch/record/255911
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author Bouquet, Alain
Kaplan, Jean
Melchior, Anne-Laure
Giraud-Heraud, Yannick
Baillon, Paul
author_facet Bouquet, Alain
Kaplan, Jean
Melchior, Anne-Laure
Giraud-Heraud, Yannick
Baillon, Paul
author_sort Bouquet, Alain
collection CERN
description We describe a project of brown dwarf detection in the dark halo of a galaxy using the microlensing effect. We argue that monitoring pixels instead of stars could provide an enhancement in the number of detectable events. We estimate the detection efficiency with a Monte-Carlo simulation. We expect a ten-fold increase with respect to current experiments. To assess the feasibility of this method we have determined the photometric precision of a pixel by comparing several pictures of a same field in the LMC. To be published in the Proceeding of the workshop 'The dark side of the universe...', Roma, Juin 1993,
id cern-255911
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1993
record_format invenio
spelling cern-2559112023-03-14T18:53:25Zhttp://cds.cern.ch/record/255911engBouquet, AlainKaplan, JeanMelchior, Anne-LaureGiraud-Heraud, YannickBaillon, PaulMicrolensing of unresolved stars as a brown dwarf detection methodOther Fields of PhysicsWe describe a project of brown dwarf detection in the dark halo of a galaxy using the microlensing effect. We argue that monitoring pixels instead of stars could provide an enhancement in the number of detectable events. We estimate the detection efficiency with a Monte-Carlo simulation. We expect a ten-fold increase with respect to current experiments. To assess the feasibility of this method we have determined the photometric precision of a pixel by comparing several pictures of a same field in the LMC. To be published in the Proceeding of the workshop 'The dark side of the universe...', Roma, Juin 1993,We describe a project of brown dwarf detection in the dark halo of a galaxy using the microlensing effect. We argue that monitoring pixels instead of stars could provide an enhancement in the number of detectable events. We estimate the detection efficiency with a Monte-Carlo simulation. We expect a ten-fold increase with respect to current experiments. To assess the feasibility of this method we have determined the photometric precision of a pixel by comparing several pictures of a same field in the LMC. To be published in the Proceeding of the workshop 'The dark side of the universe...', Roma, Juin 1993,astro-ph/9312009oai:cds.cern.ch:2559111993
spellingShingle Other Fields of Physics
Bouquet, Alain
Kaplan, Jean
Melchior, Anne-Laure
Giraud-Heraud, Yannick
Baillon, Paul
Microlensing of unresolved stars as a brown dwarf detection method
title Microlensing of unresolved stars as a brown dwarf detection method
title_full Microlensing of unresolved stars as a brown dwarf detection method
title_fullStr Microlensing of unresolved stars as a brown dwarf detection method
title_full_unstemmed Microlensing of unresolved stars as a brown dwarf detection method
title_short Microlensing of unresolved stars as a brown dwarf detection method
title_sort microlensing of unresolved stars as a brown dwarf detection method
topic Other Fields of Physics
url http://cds.cern.ch/record/255911
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AT kaplanjean microlensingofunresolvedstarsasabrowndwarfdetectionmethod
AT melchiorannelaure microlensingofunresolvedstarsasabrowndwarfdetectionmethod
AT giraudheraudyannick microlensingofunresolvedstarsasabrowndwarfdetectionmethod
AT baillonpaul microlensingofunresolvedstarsasabrowndwarfdetectionmethod