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1.
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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.
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Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies and the Distant Universe
/ Blanton, Michael R. (Stanford U., Phys. Dept.) ; Bershady, Matthew A. (Wisconsin U., Madison, Astron.) ; Abolfathi, Bela ; Albareti, Franco D. (Madrid, Autonoma U. ; Madrid, IFT) ; Allende Prieto, Carlos ; Almeida, Andres ; Alonso-García, Javier ; Anders, Friedrich (Potsdam, Astrophys. Inst.) ; Anderson, Scott F. (LLNL, Livermore) ; Andrews, Brett et al.
We describe the Sloan Digital Sky Survey IV (SDSS-IV), a project encompassing three major spectroscopic programs. The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is observing hundreds of thousands of Milky Way stars at high resolution and high signal-to-noise ratio in the near-infrared. [...]
arXiv:1703.00052.-
2017
- Published in : Astron. J. 154 (2017) 28
Fulltext: PDF;
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3.
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Constraint on neutrino masses from SDSS-III/BOSS Ly$\alpha$ forest and other cosmological probes
/ Palanque-Delabrouille, Nathalie (IRFU, SPP, Saclay ; LBL, Berkeley) ; Yèche, Christophe (IRFU, SPP, Saclay) ; Lesgourgues, Julien (ITPP, Lausanne ; CERN ; Annecy, LAPTH) ; Rossi, Graziano (IRFU, SPP, Saclay ; Sejong U.) ; Borde, Arnaud (IRFU, SPP, Saclay) ; Viel, Matteo (Trieste Observ. ; INFN, Trieste) ; Aubourg, Eric (APC, Paris) ; Kirkby, David (UC, Irvine) ; LeGoff, Jean-Marc (IRFU, SPP, Saclay) ; Rich, James (IRFU, SPP, Saclay) et al.
We present constraints on the parameters of the $\Lambda$CDM cosmological model in the presence of massive neutrinos, using the one-dimensional Ly$\alpha$ forest power spectrum obtained with the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey (SDSS) by Palanque-Delabrouille et al. (2013), complemented by additional cosmological probes. [...]
arXiv:1410.7244.-
2015-02-27 - 39 p.
- Published in : JCAP 02 (2015) 045
Preprint: PDF; External link: Preprint
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4.
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5.
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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.
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1998.
IN2P3 Publications database
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7.
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8.
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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.
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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.
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Experimental particle astrophysics
/ Spiro, Michel ; Aubourg, E
DAPNIA-SPP-97-011.-
Saclay : DAPNIA, 1998 - 24 p.
Fulltext: TIF; Published version from CERN: PDF;
In : 28th International Conference on High-energy Physics, Warsaw, Poland, 25 - 31 Jul 1996, pp.397-412
International Workshop on New Worlds in Astroparticle Physics, Faro, Portugal, 8 - 10 Sep 1996, pp.57-82
European School of High-Energy Physics, Carry-le-Rouet, France, 1 - 14 Sep 1996, pp.239-260 (CERN-1997-003)
- CERN library copies
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