Results 31 to 40 of about 3,685,182 (335)
Extreme Magnification Microlensing Event OGLE-2008-BLG-279: Strong
Limits on Planetary Companions to the Lens Star [PDF]
, 2009 We analyze the extreme high-magnification microlensing event
OGLE-2008-BLG-279, which peaked at a maximum magnification of A ~ 1600 on 30
May 2008.A. Cassan, A. Cole, A. Fukui, A. Gould, A. Maury, A. Shporer, A. Udalski, A. V. Korpela, A. Williams, B. -G. Park, B. S. Gaudi, Batista, Bennett, Bond, C. -U. Lee, C. Coutures, C. H. Ling, C. Han, Claret, Cox, D. Higgins, D. J. Sullivan, D. Kubas, D. L. DePoy, D. Maoz, D. P. Bennett, D. Polishook, Demarque, Dong, Dong, F. Abe, F. Mallia, G. Pietrzyński, G. W. Christie, Gaudi, Gaudi, Gaudi, Gould, Gould, Gould, Griest, Hardy, Holz, I. A. Bond, I. Soszyński, Ida, Ida, J. -P. Beaulieu, J. B. Hearnshaw, J. C. Bird, J. C. Yee, J. Comparat, J. D. Eastman, J. Greenhill, J. McCormick, J. Menzies, J. Wambsganss, Janczak, K. Furusawa, K. Horne, K. Kamiya, K. Masuda, K. Nishimoto, K. Ohnishi, K. Ulaczyk, L. A. G. Monard, L. Skuljan, Laughlin, M. Bos, M. D. Albrow, M. K. Szymański, M. Kubiak, M. Nagaya, M. Zub, N. J. Rattenbury, N. Kains, N. Miyake, O. Spector, O. Szewczyk, P. C. M. Yock, P. Fouqué, P. J. Tristram, P. M. Kilmartin, Poindexter, R. Martin, R. Poleski, R. Santallo, R. W. Pogge, Rhie, S. Dieters, S. Hosaka, S. Kaspi, S. Kozłowski, S. Makita, Subo Dong, T. Natusch, T. Sako, T. Sumi, To. Saito, Udalski, V. Batista, W. Allen, W. L. Sweatman, W. Lin, Wozniak, Y. C. Perrott, Y. Itow, Y. Matsubara, Y. Muraki, Yee, Yoo, Ł. Wyrzykowski +111 morecore +7 more sourcesRecruitment Disruption and the Role of Unaffected Populations for Potential Recovery After the Pinna nobilis Mass Mortality Event
Frontiers in Marine Science, 2020 A devastating mass mortality event (MME) very likely caused by the protozoan Haplosporidium pinnae first detected in 2016 in the Western Mediterranean Sea, is pushing the endemic bivalve Pinna nobilis to near extinction. Populations recovery, if possible,D. Kersting, M. Vázquez‐Luis, B. Mourre, F. Z. Belkhamssa, Elvira Álvarez, T. Bakran-Petricioli, C. Barberá, Agustín Barrajón, E. Cortés, S. Deudero, J. R. García-March, S. Giacobbe, F. Giménez-Casalduero, Luis González, S. Jiménez-Gutiérrez, S. Kipson, J. Llorente, D. Moreno, P. Prado, J. Pujol, Jordi Sánchez, A. Spinelli, J. M. Valencia, N. Vicente, I. Hendriks +24 moresemanticscholar +1 more sourceMOA-2009-BLG-387Lb: A massive planet orbiting an M dwarf [PDF]
, 2011 We report the discovery of a planet with a high planet-to-star mass ratio in
the microlensing event MOA-2009-BLG-387, which exhibited pronounced deviations
over a 12-day interval, one of the longest for any planetary event. The host is
an M dwarf, with a A. Allan, A. Cassan, A. Cole, A. Fukui, A. Gal-Yam, A. Gould, A. Korpela, A. Maury, A. Shporer, A. Williams, Afonso, Albrow, Albrow, Albrow, Albrow, An, An, An, B. Monard, B. S. Gaudi, B.-G. Park, Beaulieu, Bennett, Bennett, Bensby, Bessel, Bond, Boss, C. Coutures, C. H. Ling, C. Han, C. Liebig, C. S. Botzler, C. Snodgrass, C. Vinter, C.-U. Lee, Cumming, D. Dominis Prester, D. Douchin, D. Higgins, D. J. Sullivan, D. Kubas, D. L. DePoy, D. M. Bramich, D. Maoz, D. Moorhouse, D. P. Bennett, D. Polishook, D. Ricci, Dong, Dong, Doran, Dwek, E. Gorbikov, E. Martioli, E. O. Ofek, E. Pedretti, E. von Seggern, F. Abe, F. Finet, F. Grundahl, F. Jablonski, F. Mallia, F. V. Hessman, F. Zimmer, G. Bolt, G. Maier, G. Scarpetta, G. Thornley, G. W. Christie, Gaudi, Gould, Gould, Gould, Gould, Gould, Gould, Gould, Gould, Han, Han, Holtzman, I. A. Steele, I. Bond, Ida, J. An, J. B. Hearnshaw, J. C. Yee, J. Caldwell, J. D. Eastman, J. Donatowicz, J. Drummond, J. Greenhill, J. J. Calitz, J. Janczak, J. McCormick, J. Menzies, J. P. Beaulieu, J. Skottfelt, J. Southworth, J. Surdej, J. Wambsganss, J.-B. Marquette, Janczak, Johnson, K. C. Sahu, K. Cook, K. Furusawa, K. Harpsøe, K. Horne, K. Kamiya, K. Masuda, K. Nishimoto, K. Ohnishi, K. Pollard, Kennedy, Kervella, L. A. G. Monard, L. Mancini, Laughlin, M. Bos, M. D. Albrow, M. Dominik, M. Freeman, M. Glitrup, M. Hoffman, M. Hundertmark, M. J. Burgdorf, M. Mathiasen, M. Nagaya, M. Zub, N. Kains, N. Miyake, N. Morgan, N. Rattenbury, O. Spector, P. Browne, P. C. M. Yock, P. J. Tristram, P. M. Kilmartin, P. Meintjes, R. A. Street, R. Martin, R. Santallo, R. W. Pogge, R. Watson, S. Brillant, S. Calchi Novati, S. Dieters, S. Dong, S. Dreizler, S. Hosaka, S. Kaspi, S. Kozłowski, S. Makita, S. R. Kane, S. Rahvar, Smith, Sumi, T. C. Hinse, T. Natusch, T. Okumura, T. Sumi, To. Saito, U. G. Jørgensen, Udalski, V. Batista, V. Bozza, W. Allen, W. L. Sweatman, W. Lin, Wambsganss, Y. C. Perrott, Y. Itow, Y. Matsubara, Y. Muraki, Y. Tsapras, Yoo, Zheng, Zoccali +179 morecore +5 more sourcesLimits on Stellar and Planetary Companions in Microlensing Event
OGLE-1998-BUL-14 [PDF]
, 1999 We present the PLANET photometric data set for \ob14, a high magnification
($A_{\rm max}\sim 16$) event alerted by the OGLE collaboration toward the
Galactic bulge in 1998.(The PLANET Collaboration), A. Gould, A. Williams, B. S. Gaudi, Bertelli G., D. L. DePoy, Dominik M., J. A. R. Caldwell, J. Greenhill, J. Menzies, J.‐P. Beaulieu, K. C. Sahu, K. Hill, K. R. Pollard, M. D. Albrow, M. Dominik, P. D. Sackett, P. Vermaak, R. M. Naber, R. Martin, R. W. Pogge, R. Watson, Rhie S. H., S. Kane, Udalski A., Udalski A. +25 morecore +3 more sourcesSpeech as Noise Interference During a Mass Event
IOP Conference Series: Materials Science and Engineering, 2021 Abstract Participants of mass events are noise sources for surrounding area and perception of information. To rate the intelligibility of the signals of sound amplification systems and to design the instruments of the noise insolation, the methods of calculating the propagation of sound energy from distributed noise sources such as ...I L Shubin, A I Antonov, V I Ledenev, T S Yarovaya +3 moreopenaire +1 more sourceExtreme mass ratio inspiral rates: dependence on the massive black hole
mass [PDF]
, 2009 We study the rate at which stars spiral into a massive black hole (MBH) due
to the emission of gravitational waves (GWs), as a function of the mass M of
the MBH. In the context of our model, it is shown analytically that the rate
approximately depends on Alexander T, Alexander T, Alexander T Hopman C, Clovis Hopman, Eisenhauer F, Ferrarese L, Fiorito R, Freitag M, Freitag M, Freitag M, Gair J R, Gair J R, Gebhardt K, Gebhardt K, Genzel R, Gerssen J, Ghez A M, Ghez A M, Holley-Bockelmann K Sigurdsson S, Hopman C, Hopman C, Hopman C, Hopman C, Hopman C, Liu J-F, Miller J M, Miller J M, Miralda-Escudé J, Noyola E, O'Leary R M Kocsis B Loeb A, Perets H B, Rubbo L J, Sigurdsson S, Tremaine S, Yunes N, Zhang M +35 morecore +1 more source