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1.
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A White Paper on keV Sterile Neutrino Dark Matter
/ Drewes, M. (Munich, Tech. U.) ; Lasserre, T. (Munich, Tech. U.) ; Merle, A. (Munich, Max Planck Inst.) ; Mertens, S. (LBL, Berkeley ; KIT, Karlsruhe) ; Adhikari, R. (Jamia Millia Islamia) ; Agostini, M. (Gran Sasso) ; Ky, N.Anh (Hanoi, Inst. Phys. ; Vietnam Natl. U.) ; Araki, T. (Saitama U.) ; Archidiacono, M. (Aarhus U.) ; Bahr, M. (UC, Santa Barbara) et al.
We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting views and insights from all disciplines involved - cosmology, astrophysics, nuclear, and particle physics - in each case viewed from both theoretical and experimental/observational perspectives. After reviewing the role of active neutrinos in particle physics, astrophysics, and cosmology, we focus on sterile neutrinos in the context of the Dark Matter puzzle. [...]
arXiv:1602.04816; FERMILAB-PUB-16-068-T.-
2017-01-13 - 239 p.
- Published in : JCAP 01 (2017) 025
Fulltext: PDF; External link: Fermilab Accepted Manuscript
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2.
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Classical novae from the POINT-AGAPE microlensing survey of M31; 2 Rate and statistical characteristics of the nova population
/ Darnley, M J ; Bode, M F ; Kerins, E ; Newsam, A M ; An, J ; Baillon, Paul ; Belokurov, V ; Novati, S C ; Carr, B J ; Creze, M et al.
We report the results of our statistical study of the POINT-AGAPE CNe catalogue. The first Sloan $r'$ and $i'$ analysis of the MMRD relationship in M31 is performed using the resulting POINT-AGAPE CN catalogue. [...]
astro-ph/0509493.-
Geneva : CERN, 2006 - 15 p.
- Published in : Mon. Not. R. Astron. Soc. 369 (2006) 257-271
Access to fulltext document: PDF; External link: astro-ph/0509493 PDF
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3.
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Automated Detection of Classical Novae with Neural Networks
/ Feeney, S. (Cambridge U., Inst. of Astron.) ; Belokurov, V. (Cambridge U., Inst. of Astron.) ; Evans, N.W. (Cambridge U., Inst. of Astron.) ; An, J. (Cambridge U., Inst. of Astron.) ; Hewett, Paul C. (Cambridge U., Inst. of Astron.) ; Bode, M. (Liverpool John Moores U., ARI) ; Darnley, M. (Liverpool John Moores U., ARI) ; Kerins, E. (Liverpool John Moores U., ARI) ; Baillon, P. (CERN) ; Carr, Bernard J. (Queen Mary, U. of London, Math. Sci.) et al.
The POINT-AGAPE collaboration surveyed M31 with the primary goal of optical detection of microlensing events, yet its data catalogue is also a prime source of lightcurves of variable and transient objects, including classical novae (CNe). A reliable means of identification, combined with a thorough survey of the variable objects in M31, provides an excellent opportunity to locate and study an entire galactic population of CNe. [...]
astro-ph/0504236.-
Geneva : CERN, 2005 - 28 p.
- Published in : Astron. J. 130 (2005) 84-94
Access to fulltext document: PDF; Fulltext: PDF; External link: astro-ph/0504236 PDF
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4.
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POINT-AGAPE Pixel Lensing Survey of M31 : Evidence for a MACHO contribution to Galactic Halos
/ Calchi Novati, Sebastiano ; Paulin-Henriksson, S. ; An, J. ; Baillon, P. ; Belokurov, V. ; Carr, Bernard J. ; Creze, M. ; Evans, N.W. ; Giraud-Heraud, Y. ; Gould, A. et al.
The POINT-AGAPE collaboration is carrying out a search for gravitational microlensing toward M31 to reveal galactic dark matter in the form of MACHOs (Massive Astrophysical Compact Halo Objects) in the halos of the Milky Way and M31. A high-threshold analysis of 3 years of data yields 6 bright, short--duration microlensing events, which are confronted to a simulation of the observations and the analysis. [...]
astro-ph/0504188.-
Geneva : CERN, 2005 - 20 p.
- Published in : Astron. Astrophys. 443 (2005) 911
Access to fulltext document: PDF; Preprint: PDF; External link: astro-ph/0504188 PDF
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5.
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The POINT-AGAPE survey II: An Unrestricted Search for Microlensing Events towards M31
/ Belokurov, V ; An, J ; Evans, N W ; Hewett, P C ; Baillon, Paul ; Novati, S C ; Carr, B J ; Creze, M ; Giraud-Héraud, Yannick ; Gould, A et al.
An automated search is carried out for microlensing events using a catalogue of 44554 variable superpixel lightcurves derived from our three-year monitoring program of M31. Each step of our candidate selection is objective and reproducible by a computer. [...]
astro-ph/0411186.-
Geneva : CERN, 2005 - 22 p.
- Published in : Mon. Not. R. Astron. Soc. 357 (2005) 17-37
Access to fulltext document: PDF; External link: astro-ph/0411186 PDF
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6.
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Classical novae from the POINT-AGAPE microlensing survey of M31 -- I. The nova catalogue
/ Darnley, Matt J. (Liverpool John Moores U., ARI) ; Bode, M.F. (Liverpool John Moores U., ARI) ; Kerins, E. (Liverpool John Moores U., ARI) ; Newsam, A.M. (Liverpool John Moores U., ARI) ; An, J. (Cambridge U., Inst. of Astron.) ; Baillon, P. (CERN) ; Calchi Novati, S. (Zurich U.) ; Carr, Bernard J. (Queen Mary, U. of London, Math. Sci.) ; Creze, M. (College de France ; Bretagne U.) ; Evans, N.W. (Cambridge U., Inst. of Astron.) et al.
The POINT-AGAPE survey is an optical search for gravitational microlensing events towards the Andromeda Galaxy (M31). As well as microlensing, the survey is sensitive to many different classes of variable stars and transients. [...]
astro-ph/0403447.-
2004 - 17 p.
- Published in : Mon. Not. R. Astron. Soc. 353 (2004) 571
Access to fulltext document: PDF; Fulltext: PDF; Oxford University Press Open Access article: PDF; External link: astro-ph/0403447 PDF
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7.
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The POINT-AGAPE Survey I: The Variable Stars in M31
/ An Jun Hong ; Evans, y N W ; Hewett, P C ; Baillon, Paul ; Calchi-Novati, S ; Carr, B J ; Creze, M ; Giraud-Héraud, Yannick ; Gould, A ; Jetzer, P et al.
The POINT-AGAPE collaboration has been monitoring M31 for three seasons with the Wide Field Camera on the Isaac Newton Telescope. In each season, data are taken for one hour per night for roughly sixty nights during the six months that M31 is visible [...]
astro-ph/0401374.-
Geneva : CERN, 2004
- Published in : Mon. Not. R. Astron. Soc. 351 (2004) 1071-1098
Access to fulltext document: PDF; External link: astro-ph/0401374 PDF
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8.
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9.
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10.
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The Point-Agape survey : No Need for Machos in M31 ?
/ POINT-AGAPE Collaboration
We have carried out a survey of the Andromeda galaxy for unresolved microlensing (pixel lensing). We present a subset of four short timescale microlensing candidates with high ratio of signal to noise, by imposing severe selection criteria: the source flux variation exceeds the flux of a R=21 magnitude star and the full-width half-maximum timescale is less than 25 days. [...]
astro-ph/0207025.-
2003 - 5 p.
- Published in : Astron. Astrophys. 405 (2003) 15
Access to fulltext document: PDF; Preprint: PDF; External link: astro-ph/0207025 PDF
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