activity
19982026
most citedSolar 8B and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data

1k citations · 23k across the 396 of their papers we have counts for

collaborators
Showing 2012Show all

22 papers · 1 filter

astro-ph.EP2012★ 46 cited

MOA-2010-BLG-073L: An M-Dwarf with a Substellar Companion at the Planet/Brown Dwarf Boundary

R. A. Street, J. -Y. Choi, Y. Tsapras +129

We present an analysis of the anomalous microlensing event, MOA-2010-BLG-073, announced by the Microlensing Observations in Astrophysics survey on 2010-03-18. This event was remark…

astro-ph.CO2012★ 79 cited

Search for solar axions in XMASS, a large liquid-xenon detector

K. Abe, K. Hieda, K. Hiraide +43

XMASS, a low-background, large liquid-xenon detector, was used to search for solar axions that would be produced by bremsstrahlung and Compton effects in the Sun. With an exposure…

astro-ph.CO2012★ 52 cited

Light WIMP search in XMASS

K. Abe, K. Hieda, K. Hiraide +43

A search for light dark matter using low-threshold data from the single phase liquid xenon scintillation detector XMASS, has been conducted. Using the entire 835 kg inner volume as…

astro-ph.SR2012★ 16 cited

MOA-2010-BLG-523: "Failed Planet" = RS CVn Star

A. Gould, J. C. Yee, I. A. Bond +116

The Galactic bulge source MOA-2010-BLG-523S exhibited short-term deviations from a standard microlensing lightcurve near the peak of an Amax ~ 265 high-magnification microlensing e…

astro-ph.EP2012★ 20 cited

MOA-2010-BLG-311: A planetary candidate below the threshold of reliable detection

J. C. Yee, L. -W. Hung, I. A. Bond +123

We analyze MOA-2010-BLG-311, a high magnification (A_max>600) microlensing event with complete data coverage over the peak, making it very sensitive to planetary signals. We fit th…

astro-ph.SR2012★ 9 cited

Using Orbital Effects to Break the Close/wide Degeneracy in Binary-lens Microlensing Events

I. -G. Shin, T. Sumi, A. Udalski +37

Microlensing can provide an important tool to study binaries, especially those composed of faint or dark objects. However, accurate analysis of binary-lens light curves is often ha…

astro-ph.SR2012★ 22 cited

Microlensig Binaries with Candidate Brown Dwarf Companions

I. -G. Shin, C. Han, A. Gould +152

Brown dwarfs are important objects because they may provide a missing link between stars and planets, two populations that have dramatically different formation history. In this pa…

hep-ex2012★ 39 cited

Measurement of zero degree inclusive photon energy spectra for 900 GeV proton-proton collisions at LHC

O. Adriani, L. Bonechi, M. Bongi +25

The inclusive photon energy spectra measured by the Large Hadron Collider forward (LHCf) experiment in the very forward region of LHC proton-proton collisions at 900 Ge…

astro-ph.EP2012★ 19 cited

A possible binary system of a stellar remnant in the high magnification gravitational microlensing event OGLE-2007-BLG-514

N. Miyake, A. Udalski, T. Sumi +78

We report the extremely high magnification (A > 1000) binary microlensing event OGLE-2007-BLG-514. We obtained good coverage around the double peak structure in the light curve via…

hep-ex2012★ 99 cited

Evidence for the Appearance of Atmospheric Tau Neutrinos in Super-Kamiokande

Kamiokande Collaboration

Super-Kamiokande atmospheric neutrino data were fit with an unbinned maximum likelihood method to search for the appearance of tau leptons resulting from the interactions of oscill…

hep-ex2012★ 46 cited

Search for Proton Decay into Muon plus Neutral Kaon in Super-Kamiokande I, II, and III

Kamiokande Collaboration, C. Regis, K. Abe +104

We have searched for proton into muon plus neutral kaon using data from a 91.7 kiloton-year exposure of Super-Kamiokande-I, a 49.2 kiloton-year exposure of Super-Kamiokande-II, and…

astro-ph.EP2012★ 77 cited

MOA-2010-BLG-477Lb: constraining the mass of a microlensing planet from microlensing parallax, orbital motion and detection of blended light

E. Bachelet, I. -G. Shin, C. Han +138

Microlensing detections of cool planets are important for the construction of an unbiased sample to estimate the frequency of planets beyond the snow line, which is where giant pla…

hep-ex2012★ 50 cited

Measurement of forward neutral pion transverse momentum spectra for = 7TeV proton-proton collisions at LHC

O. Adriani, L. Bonechi, M. Bongi +26

The inclusive production rate of neutral pions in the rapidity range greater than has been measured by the Large Hadron Collider forward (LHCf) experiment during LHC $\sqrt…

astro-ph.EP2012★ 27 cited

A New Type of Ambiguity in the Planet and Binary Interpretations of Central Perturbations of High-Magnification Gravitational Microlensing Events

J. -Y. Choi, I. -G. Shin, C. Han +118

High-magnification microlensing events provide an important channel to detect planets. Perturbations near the peak of a high-magnification event can be produced either by a planet…

astro-ph.IM2012★ 13 cited

The JEM-EUSO Mission: Status and Prospects in 2011

EUSO Collaboration, J. H. Adams, S. Ahmad +256

Contributions of the JEM-EUSO Collaboration to the 32nd International Cosmic Ray Conference, Beijing, August, 2011.

astro-ph.SR2012★ 36 cited

Characterizing Low-Mass Binaries From Observation of Long Time-scale Caustic-crossing Gravitational Microlensing Events

I. -G. Shin, C. Han, J. -Y. Choi +119

Despite astrophysical importance of binary star systems, detections are limited to those located in small ranges of separations, distances, and masses and thus it is necessary to u…

astro-ph.EP2012★ 25 cited

OGLE-2008-BLG-510: first automated real-time detection of a weak microlensing anomaly - brown dwarf or stellar binary?

V. Bozza, M. Dominik, N. J. Rattenbury +103

The microlensing event OGLE-2008-BLG-510 is characterised by an evident asymmetric shape of the peak, promptly detected by the ARTEMiS system in real time. The skewness of the ligh…

hep-ex2012★ 37 cited

Search for GUT Monopoles at Super-Kamiokande

Kamiokande Collaboration, K. Ueno, K. Abe +109

GUT monopoles captured by the Sun's gravitation are expected to catalyze proton decays via the Callan-Rubakov process. In this scenario, protons, which initially decay into pions,…

astro-ph.EP2012★ 99 cited

Planetary and Other Short Binary Microlensing Events from the MOA Short Event Analysis

D. P. Bennett, T. Sumi, I. A. Bond +22

We present the analysis of four candidate short duration binary microlensing events from the 2006-2007 MOA Project short event analysis. These events were discovered as a byproduct…

hep-ex2012★ 91 cited

Search for Nucleon Decay into Charged Anti-lepton plus Meson in Super-Kamiokande I and II

Kamiokande Collaboration, H. Nishino, K. Abe +105

Searches for a nucleon decay into a charged anti-lepton (e^+ or μ^+) plus a light meson (π^0, π^-, η, ρ^0, ρ^-, ω) were performed using the Super-Kamiokande I and II data. Twelve n…

hep-ex2012

Results from LHCf Experiment

Alessia Tricomi

The LHCf experiment has taken data in 2009 and 2010 p-p collisions at LHC at TeV and TeV. The measurement of the forward neutral particle spectra pr…

astro-ph.EP2012★ 235 cited

MOA-2011-BLG-293Lb: A test of pure survey microlensing planet detections

J. C. Yee, Y. Shvartzvald, A. Gal-Yam +10

Because of the development of large-format, wide-field cameras, microlensing surveys are now able to monitor millions of stars with sufficient cadence to detect planets. These new…