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CERN Document Server Encontrados 15 registros  1 - 10siguiente  ir al registro: La búsqueda tardó 0.74 segundos. 
1.
Euclid. I. Overview of the Euclid mission / Euclid Collaboration
The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015-2025 programme of the European Space Agency (ESA) that will provide high-resolution optical imaging, as well as near-infrared imaging and spectroscopy, over about 14,000 deg^2 of extragalactic sky. [...]
arXiv:2405.13491.- 2025-04 - 94 p. - Published in : Astron. Astrophys. 697 (2025) A1 Fulltext: 2405.13491 - PDF; publication - PDF;
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2.
Euclid Definition Study Report / Laureijs, R. (ESTEC, Noordwijk) ; Amiaux, J. (DAPNIA, Saclay) ; Arduini, S. (Paris U., VI-VII) ; Augueres, J.L. (DAPNIA, Saclay) ; Brinchmann, J. (Leiden U.) ; Cole, R. (University Coll. London) ; Cropper, M. (University Coll. London) ; Dabin, C. (CNES, Toulouse) ; Duvet, L. (ESTEC, Noordwijk) ; Ealet, A. (Marseille, CPPM) et al.
Euclid is a space-based survey mission from the European Space Agency designed to understand the origin of the Universe's accelerating expansion. [...]
arXiv:1110.3193 ; ESA-SRE(2011)12 ; ESA-SRE(2011)12. - 2011 - 116.
Preprint - Full text
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3.
OGLE 2004-BLG-254: a K2 III Galactic Bulge Giant spatially resolved by a single microlens / PLANET Collaboration
DAPNIA-2005-295. - 2005. - 11 p.
Fulltext - CERN library copies
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4.
Observation of Microlensing towards the Galactic Spiral Arms : EROS II 3 year survey . - extended version / EROS Collaboration
LAL-2002-79. - 2000. - 20 p.
Access to fulltext document
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5.
Measuring The Thickness Of The Magellanic Cloud Cepheid Population : Implications For Microlensing / Graff, D ; Bauer, F ; Afonso, C ; Albert, J N ; Andersen, J ; Ansari, R ; Aubourg, E ; Bareyre, P ; Beaulieu, J P ; Bouquet, A et al.
PCC-98-26. - 1998.
IN2P3 Publications database
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6.
EROS 2 proper motion survey : a field brown dwarf and an L dwarf companion to LHS 102 / EROS Collaboration
We report the discovery of two L dwarfs (the new spectral class defined for dwarfs cooler than the M type) in a two-epoch CCD proper motion survey of 413 square degrees, complemented by infrared photometry from DENIS. One of them has a strong lithium line and is therefore a brown dwarf. [...]
astro-ph/9905162.- 1999 - Published in : Astron. Astrophys. 351 (1999) L5 Access to fulltext document: 9905162.fig.3a - PS.GZ; 9905162.fig.3b - PS.GZ; 9905162 - PDF; External link: astro-ph/9905162 PDF
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7.
Observation of Microlensing towards the Galactic Spiral Arms : EROS II 2 year survey / EROS Collaboration
We present the analysis of the light curves of 8.5 million stars observed during two seasons by EROS (Experience de Recherche d'Objets Sombres), in the galactic plane away from the bulge. Three stars have been found that exhibit luminosity variations compatible with gravitational microlensing effects due to unseen objects. [...]
astro-ph/9903209; CERN-OPEN-99-069; LAL-99-12.- Geneva : CERN, 1999 - 11 p. - Published in : Astron. Astrophys. 351 (1999) 87 External link: Fulltext
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8.
AGAPEROS : Searches for microlensing in the LMC with the Pixel Method; 2, Selection of possible microlensing events / Melchior, A.L. (Queen Mary, U. of London ; College de France) ; Afonso, C (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Ansari, R (Orsay, LAL) ; Aubourg, E. (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Baillon, P. (CERN) ; Bareyre, P. (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Bauer, F. (CEA, DSM, Saclay ; DAPNIA, Saclay) ; Beaulieu, J.-Ph. (Paris, Inst. Astrophys.) ; Bouquet, A. (College de France) ; Brehin, S. (CEA, DSM, Saclay ; DAPNIA, Saclay) et al.
We apply the pixel method of analysis (sometimes called ``pixel lensing'') to a small subset of the EROS-1 microlensing observations of the bar of the Large Magellanic Cloud (LMC). The pixel method is designed to find microlensing events of unresolved source stars and had heretofore been applied only to M31 where essentially all sources are unresolved. [...]
astro-ph/9804321.- 1998 - 14 p. - Published in : Astron. Astrophys. 339 (1998) 658 Access to fulltext document: PDF; External link: astro-ph/9804321 PDF
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9.
AGAPEROS : Searches for microlensing in the LMC with the Pixel Method; 1, Data treatment and pixel light curves production / Melchior, A.-L. (Queen Mary, U. of London ; College de France ; Fermilab) ; Afonso, C. (DAPNIA, Saclay) ; Ansari, R. (Orsay, LAL) ; Aubourg, E. (DAPNIA, Saclay) ; Baillon, P. (CERN) ; Bareyre, P. (DAPNIA, Saclay) ; Bauer, F. (DAPNIA, Saclay) ; Beaulieu, J.-Ph. (Paris, Inst. Astrophys.) ; Bouquet, A. (College de France) ; Brehin, S. (DAPNIA, Saclay) et al.
The presence and abundance of MAssive Compact Halo Objects (MACHOs) towards the Large Magellanic Cloud (LMC) can be studied with microlensing searches. The 10 events detected by the EROS and MACHO groups suggest that objects with 0.5 Mo could fill 50% of the dark halo. [...]
astro-ph/9712236; FERMILAB-PUB-98-019-A; FERMILAB-PUB-98-019-A.- Batavia, IL : FERMILAB, 1999 - 13 p. - Published in : Astron. Astrophys. 134 (1999) 377-391 Access to fulltext document: PDF; Fulltext: PDF; External link: Fermilab Library Server (fulltext available)
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10.
The two EROS 4Kx8K CCD mosaic cameras / Bauer, F ; Adrianzyk, G ; Afonso, C ; Albert, J N ; Andersen, J ; Ansari, R ; Aubourg, E ; Aune, S ; Baranne, A ; Bareyre, P et al.
1997 - Published in : Nucl. Instrum. Methods Phys. Res., A 387 (1997) 286 Access to fulltext document: TIF PDF; - CERN library copies
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CERN Document Server : Encontrados 15 registros   1 - 10siguiente  ir al registro:
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