Frequency of Solar-Like Systems and of Ice and Gas Giants Beyond the Snow Line from High-Magnification Microlensing Events in 2005-2008

Autor: Gould, A, Dong, S, Gaudi, Bs, Udalski, A, Bond, Ia, Greenhill, J, Street, Ra, Dominik, M, Sumi, T, Szymanski, Mk, Han, C, Allen, W, Bolt, G, Bos, M, Christie, Gw, Depoy, Dl, Drummond, J, Eastman, Jd, Gal-Yam, A, Higgins, D, Janczak, J, Kaspi, S, Kozllowski, S, Lee, C, Mallia, F, Maury, A, Maoz, D, Mccormick, J, Monard, Lag, Moorhouse, D, Morgan, N, Natusch, T, Ofek, Eo, Park, B, Pogge, Rw, Polishook, D, Santallo, R, Shporer, A, Spector, O, Thornley, G, Yee, Jc, Kubiak, M, Pietrzynski, G, Soszynski, I, Szewczyk, O, Wyrzykowski, E, Ulaczyk, K, Poleski, R, Abe, F, Bennett, Dp, Botzler, Cs, Douchin, D, Freeman, M, Fukui, A, Furusawa, K, Hearnshaw, Jb, Hosaka, S, Itow, Y, Kamiya, K, Kilmartin, Pm, Korpela, A, Lin, W, Ling, Ch, Makita, S, Masuda, K, Matsubara, Y, Miyake, N, Muraki, Y, Nagaya, M, Nishimoto, K, Ohnishi, K, Okumura, T, Perrott, Yc, Philpott, L, Rattenbury, N, Saito, To, Sako, T, Sullivan, Dj, Sweatman, Wl, Tristram, Pj, Von Seggern, Ev, Yock, Pcm, Albrow, M, Batista, V, Beaulieu, Jp, Brillant, S, Caldwell, J, Calitz, Jj, Cassan, A, Cole, A, Cook, K, Coutures, C, Dieters, S, Dominis Prester, D, Donatowicz, J, Fouque, P, Hill, K, Hoffman, M, Jablonski, F, Kane, Sr, Kains, N, Kubas, D, Marquette, J, Martin, R, Martioli, E, Meintjes, P, Menzies, J, Pedretti, E, Pollard, K, Sahu, Kc, Vinter, C, Wambsganss, J, Watson, R, Williams, A, Zub, M, Allan, A, Bode, Mf, Bramich, Dm, Burgdorf, Mj, Clay, N, Fraser, S, Hawkins, E, Horne, K, Kerins, E, Lister, Ta, Mottram, C, Saunders, Es, Snodgrass, C, Steele, Ia, Tsapras, Y, Jorgensen, Ug, Anguita, T, Bozza, V, Calchi Novati, S, Harpsoe, K, Hinse, Tc, Hundertmark, M, Kjaergaard, P, Liebig, C, Mancini, L, Masi, G, Mathiasen, M, Rahvar, S, Ricci, D, Scarpetta, G, Southworth, J, Surdej, J, Thone, Cc

Publikováno v: Astrophysical Journal
Artículos CONICYT
CONICYT Chile
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We present the first measurement of planet frequency beyond the "snow line" for planet/star mass-ratios[-4.5200) microlensing events during 2005-8. The sample host stars have typical mass M_host 0.5 Msun, and detection is sensitive to planets over a

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