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CERN Document Server 找到 5 筆記錄  檢索需時 0.65 秒. 
1.
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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2.
A Candidate M31/M32 Intergalactic Microlensing Event / POINT-AGAPE Collaboration
We report the discovery of a microlensing candidate projected 2'54" from the center of M32, on the side closest to M31. The blue color (R-I= 0.00 +/- 0.14) of the source argues strongly that it lies in the disk of M31, while the proximity of the line of sight to M32 implies that this galaxy is the most likely host of the lens. [...]
astro-ph/0206387.- Columbus, OH : Ohio State Univ., 2002 - 13 p. - Published in : Astrophys. J. 576 (2002) L121-L124 Access to fulltext document: PDF; External link: astro-ph/0206387 PDF
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3.
A Short Timescale Candidate Microlensing Event in the POINT-AGAPE Pixel Lensing Survey of M31 / POINT-AGAPE Collaboration
We report the discovery of a short-duration microlensing candidate in the northern field of the POINT-AGAPE pixel lensing survey towards M31. The full-width half-maximum timescale is very short, just 1.8 days. [...]
astro-ph/0102080.- 2001 - 20 p. - Published in : Astrophys. J. 553 (2001) 2 Access to fulltext document: 0102080.fig4 - PS.GZ; 0102080 - PDF; 0102080.fig1 - PS.GZ; External link: astro-ph/0102080 PDF
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4.
AgapeZ1 : a Large Amplification Microlensing Event or an Odd Variable Star Towards the Inner Bulge of M31 / Ansari, R. (Orsay, LAL) ; Auriere, M. (Pic du Midi Observ.) ; Baillon, P. (CERN) ; Bouquet, A. (College de France) ; Coupinot, G. (Pic du Midi Observ.) ; Coutures, Ch. (DAPNIA, Saclay) ; Ghesquiere, C. (College de France) ; Giraud-Heraud, Y. (College de France) ; Gondolo, P. (Munich, Max Planck Inst.) ; Hecquet, J. (Midi-Pyrenees Observ.) et al.
AgapeZ1 is the brightest and the shortest duration microlensing candidate event found in the Agape data. It occured only 42" from the center of M31. [...]
astro-ph/9812334; PCC-98-23; PCC-98-23.- Paris : Collège de France. Lab. Phys. Corpusc. Cosmol., 1999 - 4 p. - Published in : Astron. Astrophys. 344 (1999) L49 Access to fulltext document: PDF; External link: astro-ph/9812334 PDF
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5.
AGAPE : a search for dark matter towards M31 by microlensing effects on unresolved stars / Ansari, R. (Orsay) ; Auriere, M. ; Baillon, P. (CERN) ; Bouquet, A. ; Coupinot, G. ; Coutures, Ch. ; Ghesquiere, C. ; Giraud-Heraud, Y. ; Gondolo, P. ; Hecquet, J. et al.
M31 is a very tempting target for a microlensing search of compact objects in galactic haloes. It is the nearest large galaxy, it probably has its own dark halo, and its tilted position with respect to the line of sight provides an unmistakable signature of microlensing. [...]
astro-ph/9607040; LPC-96-33; LPC-96-33.- Caen : Caen Univ. Lab. Phys. Corpusc., 1996 - 15 p. - Published in : Astron.Astrophys.: 324 (1997) , pp. 843-856 Access to fulltext document: 9607040.fig09b_n - PS.GZ; 9607040.fig02 - PS.GZ; 9607040.fig01 - PS.GZ; 9607040.fig06 - PS.GZ; 9607040.fig04 - PS.GZ; 9607040.fig08 - PS.GZ; 9607040 - PDF; 9607040.fig14 - PS.GZ; 9607040.fig15 - PS.GZ; 9607040.fig11 - PS.GZ; 9607040.fig12 - PS.GZ; 9607040.fig13 - PS.GZ; 9607040.fig07a - PS.GZ; 9607040.fig07b - PS.GZ; 9607040.fig13_n - PS.GZ; 9607040.fig09a_n - PS.GZ; 9607040.fig10a - PS.GZ; 9607040.fig10b - PS.GZ; 9607040.fig08_n - PS.GZ; 9607040.fig03a - PS.GZ; 9607040.fig03c - PS.GZ; 9607040.fig03b - PS.GZ; 9607040.fig05b - PS.GZ; 9607040.fig05a - PS.GZ; External link: astro-ph/9607040 PDF
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