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OGLE-2016-BLG-1266: A Probable Brown Dwarf/Planet Binary at the Deuterium Fusion Limit
Albrow, M. D.,Yee, J. C.,Udalski, A.,Novati, S. Calchi,Carey, S.,Henderson, C. B.,Beichman, C.,Bryden, G.,Gaudi, B. S.,Shvartzvald, Y.,Szymań,ski, M. K.,Mró,z, P.,Skowron, J.,Poleski, R.,So American Astronomical Society 2018 The Astrophysical journal Vol.858 No.2
Observation of ExclusiveγγProduction inpp¯Collisions ats=1.96TeV
Aaltonen, T.,Albrow, M. G.,Á,lvarez Gonzá,lez, B.,Amerio, S.,Amidei, D.,Anastassov, A.,Annovi, A.,Antos, J.,Apollinari, G.,Appel, J. A.,Arisawa, T.,Artikov, A.,Asaadi, J.,Ashmanskas, W.,Au American Physical Society 2012 Physical Review Letters Vol.108 No.8
Aaltonen, T.,Albrow, M. G.,Amerio, S.,Amidei, D.,Anastassov, A.,Annovi, A.,Antos, J.,Apollinari, G.,Appel, J. A.,Arisawa, T.,Artikov, A.,Asaadi, J.,Ashmanskas, W.,Auerbach, B.,Aurisano, A.,Azfar, F.,B American Physical Society 2017 Physical Review D Vol.96 No.9
<P>A measurement of the inclusive production cross section of isolated prompt photons in proton-antiproton collisions at center-of-mass energy root s = 1.96 TeV is presented. The results are obtained using the full Run II data sample collected with the Collider Detector at the Fermilab Tevatron, which corresponds to an integrated luminosity of 9.5 fb(-1). The cross section is measured as a function of photon transverse energy, E-T(gamma), in the range 30 < E-T(gamma) < 500 GeV and in the pseudorapidity region |eta(gamma)| < 1.0. The results are compared with predictions from parton-shower Monte Carlo models at leading order in QCD and from next-to-leading-order perturbative QCD calculations. The latter show good agreement with the measured cross section.</P>
Study of the energy dependence of the underlying event in proton-antiproton collisions
Aaltonen, T.,Albrow, M.,Amerio, S.,Amidei, D.,Anastassov, A.,Annovi, A.,Antos, J.,Apollinari, G.,Appel, J. A.,Arisawa, T.,Artikov, A.,Asaadi, J.,Ashmanskas, W.,Auerbach, B.,Aurisano, A.,Azfar, F.,Badg American Physical Society 2015 PHYSICAL REVIEW D - Vol.92 No.9
Measurement of central exclusiveπ+π−production inpp¯collisions ats=0.9and 1.96 TeV at CDF
Aaltonen, T.,Albrow, M. G.,Amerio, S.,Amidei, D.,Anastassov, A.,Annovi, A.,Antos, J.,Apollinari, G.,Appel, J. A.,Arisawa, T.,Artikov, A.,Asaadi, J.,Ashmanskas, W.,Auerbach, B.,Aurisano, A.,Azfar, F.,B American Physical Society 2015 PHYSICAL REVIEW D - Vol.91 No.9
Optimized search for single-top-quark production at the Fermilab Tevatron
Acosta, D.,Affolder, T.,Albrow, M. G.,Ambrose, D.,Amidei, D.,Anikeev, K.,Antos, J.,Apollinari, G.,Arisawa, T.,Artikov, A.,Ashmanskas, W.,Azfar, F.,Azzi-Bacchetta, P.,Bacchetta, N.,Bachacou, H.,Badgett American Physical Society 2004 PHYSICAL REVIEW D - Vol.69 No.5
MOA-2007-BLG-197: Exploring the brown dwarf desert
Ranc, C.,Cassan, A.,Albrow, M. D.,Kubas, D.,Bond, I. A.,Batista, V.,Beaulieu, J.-P.,Bennett, D. P.,Dominik, M.,Dong, Subo,Fouqué,, P.,Gould, A.,Greenhill, J.,Jørgensen, U. G.,Kains, N.,Menzies, EDP Sciences 2015 Astronomy and astrophysics Vol.580 No.-
Direct photon cross section with conversions at CDF
Acosta, D.,Affolder, T.,Albrow, M. G.,Ambrose, D.,Amidei, D.,Anikeev, K.,Antos, J.,Apollinari, G.,Arisawa, T.,Artikov, A.,Ashmanskas, W.,Azfar, F.,Azzi-Bacchetta, P.,Bacchetta, N.,Bachacou, H.,Badgett American Physical Society 2004 PHYSICAL REVIEW D - Vol.70 No.7
CAN THE MASSES OF ISOLATED PLANETARY-MASS GRAVITATIONAL LENSES BE MEASURED BY TERRESTRIAL PARALLAX?
Freeman, M.,Philpott, L. C.,Abe, F.,Albrow, M. D.,Bennett, D. P.,Bond, I. A.,Botzler, C. S.,Bray, J. C.,Cherrie, J. M.,Christie, G. W.,Dionnet, Z.,Gould, A.,Han, C.,Heyrovský,, D.,McCormick, J. IOP Publishing 2015 The Astrophysical journal Vol.799 No.2
<P>Recently Sumi et al. reported evidence for a large population of planetary-mass objects ( PMOs) that are either unbound or orbit host stars in orbits >= 10 AU. Their result was deduced from the statistical distribution of durations of gravitational microlensing events observed by the MOA collaboration during 2006 and 2007. Here we study the feasibility of measuring the mass of an individual PMO through microlensing by examining a particular event, MOA-2011-BLG-274. This event was unusual as the duration was short, the magnification high, the source-size effect large, and the angular Einstein radius small. Also, it was intensively monitored from widely separated locations under clear skies at low air masses. Choi et al. concluded that the lens of the event may have been a PMO but they did not attempt a measurement of its mass. We report here a re-analysis of the event using re-reduced data. We confirm the results of Choi et al. and attempt a measurement of the mass and distance of the lens using the terrestrial parallax effect. Evidence for terrestrial parallax is found at a 3 sigma level of confidence. The best fit to the data yields the mass and distance of the lens as 0.80 +/- 0.30 M-J and 0.80 +/- 0.25 kpc respectively. We exclude a host star to the lens out to a separation similar to 40 AU. Drawing on our analysis of MOA-2011-BLG-274 we propose observational strategies for future microlensing surveys to yield sharper results on PMOs including those down to super-Earth mass.</P>