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Title
The EROS-2 project has been designed to search for microlensing events towards any dense stellar field. The densest parts of the Galactic spiral arms have been monitored to maximize the microlensing signal expected from the stars of the Galactic disk...
We present the first results of the EMBLA survey (Extremely Metal-poor BuLge stars with AAOmega), aimed at finding metal-poor stars in the Milky Way bulge, where the oldest stars should now preferentially reside. EMBLA utilizes SkyMapper photometry t...
Fast radio bursts (FRBs) are one of the most tantalizing mysteries of the radio sky; their progenitors and origins remain unknown and until now no rapid multiwavelength follow-up of an FRB has been possible. New instrumentation has decreased the time...
The first stars are predicted to have formed within 200 million years after the Big Bang, initiating the cosmic dawn. A true first star has not yet been discovered, although stars with tiny amounts of elements heavier than helium ('metals') have been...
Henderson, Calen B.;Poleski, Radosław;Penny, Matthew;Street, Rachel A.;Bennett, David P.;Hogg, David W.;Gaudi, B. Scott;Zhu, W.;Barclay, T.;Barentsen, G.;Howell, S. B.;Mullally, F.;Udalski, A.;Szymański, M. K.;Skowron, J.;Mróz, P.;Kozłowski, S.;Wyrzykowski, Ł.;Pietrukowicz, P.;Soszyński, I.;Ulaczyk, K.;Pawlak, M.;Sumi, T.;Abe, F.;Asakura, Y.;Barry, R. K.;Bhattacharya, A.;Bond, I. A.;Donachie, M.;Freeman, M.;Fukui, A.;Hirao, Y.;Itow, Y.;Koshimoto, N.;Li, M. C. A.;Ling, C. H.;Masuda, K.;Matsubara, Y.;Muraki, Y.;Nagakane, M.;Ohnishi, K.;Oyokawa, H.;Rattenbury, N.;Saito, To.;Sharan, A.;Sullivan, D. J.;Tristram, P. J.;Yonehara, A.;Bachelet, E.;Bramich, D. M.;Cassan, A.;Dominik, M.;Jaimes, R. Figuera;Horne, K.;Hundertmark, M.;Mao, S.;Ranc, C.;Schmidt, R.;Snodgrass, C.;Steele, I. A.;Tsapras, Y.;Wambsganss, J.;Bozza, V.;Burgdorf, M. J.;Jørgensen, U. G.;Novati, S. Calchi;Ciceri, S.;D'Ago, G.;Evans, D. F.;Hessman, F. V.;Hinse, T. C.;Husser, T. -O.;Mancini, L.;Popovas, A.;Rabus, M.;Rahvar, S.;Scarpetta, G.;Skottfelt, J.;Southworth, J.;Unda-Sanzana, E.;Bryson, S. T.;Caldwell, D. A.;Haas, M. R.;Larson, K.;McCalmont, K.;Packard, M.;Peterson, C.;Putnam, D.;Reedy, L.;Ross, S.;Van Cleve, J. E.;Akeson, R.;Batista, V.;Beaulieu, J. -P.;Beichman, C. A.;Bryden, G.;Ciardi, D.;Cole, A.;Coutures, C.;Foreman-Mackey, D.;Fouqué, P.;Friedmann, M.;Gelino, C.;Kaspi, S.;Kerins, E.;Korhonen, H.;Lang, D.;Lee, C. -H.;Lineweaver, C. H.;Maoz, D.;Marquette, J. -B.;Mogavero, F.;Morales, J. C.;Nataf, D.;Pogge, R. W.;Santerne, A.;Shvartzvald, Y.;Suzuki, D.;Tamura, M.;Tisserand, P.;Wang, D.
$K2$'s Campaign 9 ($K2$C9) will conduct a $\sim$3.7 deg$^{2}$ survey toward the Galactic bulge from 7/April through 1/July of 2016 that will leverage the spatial separation between $K2$ and the Earth to facilitate measurement of the microlens paralla...