AGAPEROS: Searches for microlensing in the LMC with the Pixel Method; 1, Data treatment and pixel light curves production

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. This preferred mass is quite s...

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Detalles Bibliográficos
Autores principales: Melchior, A.-L., Afonso, C., Ansari, R., Aubourg, E., Baillon, P., Bareyre, P., Bauer, F., Beaulieu, J.-Ph., Bouquet, A., Brehin, S., Cavalier, F., Char, S., Couchot, F., Coutures, C., Ferlet, R., Fernandez, J., Gaucherel, C., Giraud-Heraud, Y., Glicenstein, J.-F., Goldman, B., Gondolo, P., Gros, M., Guibert, J., Gry, C., Hardin, D., Kaplan, J., de Kat, J., Lachieze-Rey, M., Laurent, B., Lesquoy, E., Magneville, Ch., Mansoux, B., Marquette, J.-B., Maurice, E., Milsztajn, A., Moniez, M., Moreau, O., Moscoso, L., Palanque-Delabrouille, N., Perdereau, O., Prevot, L., Renault, C., Queinnec, F., Rich, J., Spiro, M., Vigroux, L., Zylberajch, S., Vidal-Madjar, A.
Lenguaje:eng
Publicado: 1998
Materias:
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1051/aas:1999439
http://cds.cern.ch/record/341780

Internet

https://dx.doi.org/10.1051/aas:1999439
http://cds.cern.ch/record/341780

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