activity
20112022
most citedThe surface detector array of the Telescope Array experiment

399 citations · 1.3k across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.EP2022★ 32 cited

Less effective hydrodynamic escape of H-HO atmospheres on terrestrial planets orbiting pre-main sequence M dwarfs

Tatsuya Yoshida, Naoki Terada, Masahiro Ikoma +1

Terrestrial planets currently in the habitable zones around M dwarfs likely experienced a long-term runaway greenhouse condition because of a slow decline in host-stellar luminosit…

astro-ph.EP2021★ 16 cited

Polarimetric Properties of the Near--Sun Asteroid (155140) 2005 UD in Comparison with Other Asteroids and Meteoritic Samples

Masateru Ishiguro, Yoonsoo P. Bach, Jooyeon Geem +26

The investigation of asteroids near the Sun is important for understanding the final evolutionary stage of primitive solar system objects. A near-Sun asteroid, (155140) 2005 UD, ha…

astro-ph.EP2021★ 8 cited

A polarimetric study of asteroids in comet-like orbits

Jooyeon Geem, Masateru Ishiguro, Yoonsoo P. Bach +16

Context. Asteroids in comet-like orbits (ACOs) consist of asteroids and dormant comets. Due to their similar appearance, it is challenging to distinguish dormant comets from ACOs v…

astro-ph.EP2021★ 12 cited

Implications of High Polarization Degree for the Surface State of Ryugu

Daisuke Kuroda, Jooyeon Geem, Hiroshi Akitaya +19

The asteroid exploration project "Hayabusa2" has successfully returned samples from the asteroid (162173) Ryugu. In this study, we measured the linear polarization degrees of Ryugu…

astro-ph.EP2020★ 14 cited

HO-induced Greenhouse Warming on Oxidized Early Mars

Yuichi Ito, George L. Hashimoto, Yoshiyuki O. Takahashi +2

The existence of liquid water within an oxidized environment on early Mars has been inferred by the Mn-rich rocks found during recent explorations on Mars. The oxidized atmosphere…

astro-ph.EP2020★ 7 cited

Obliquity of an Earth-like planet from frequency modulation of its direct imaged lightcurve: mock analysis from general circulation model simulation

Yuta Nakagawa, Takanori Kodama, Masaki Ishiwatari +8

Direct-imaging techniques of exoplanets have made significant progress recently, and will eventually enable to monitor photometric and spectroscopic signals of earth-like habitable…

astro-ph.SR2019★ 8 cited

Diagnosing the Clumpy Protoplanetary Disk of the UXor Type Young Star GM Cephei

P. C. Huang, W. P. Chen, M. Mugrauer +29

UX Orionis stars (UXors) are Herbig Ae/Be or T Tauri stars exhibiting sporadic occultation of stellar light by circumstellar dust. GM\,Cephei is such a UXor in the young (~M…

astro-ph.EP2018★ 2 cited

Science Objectives of the Ganymede Laser Altimeter (GALA) for the JUICE Mission

Jun Kimura, Hauke Hussmann, Shunichi Kamata +11

Laser altimetry is a powerful tool for addressing the major objectives of planetary physics and geodesy, and have been applied in planetary explorations of the Moon, Mars, Mercury,…

astro-ph.SR2018★ 36 cited

Breaking the habit - the peculiar 2016 eruption of the unique recurrent nova M31N 2008-12a

M. Henze, M. J. Darnley, S. C. Williams +70

Since its discovery in 2008, the Andromeda galaxy nova M31N 2008-12a has been observed in eruption every single year. This unprecedented frequency indicates an extreme object, with…

astro-ph.EP2017★ 10 cited

Significantly high polarization degree of the very low-albedo asteroid (152679) 1998 KU

Daisuke Kuroda, Masateru Ishiguro, Makoto Watanabe +7

We present a unique and significant polarimetric result regarding the near-Earth asteroid (152679) 1998 KU , which has a very low geometric albedo. From our observatio…

astro-ph.EP2017★ 25 cited

Polarimetric Study of Near-Earth Asteroid (1566) Icarus

Masateru Ishiguro, Daisuke Kuroda, Makoto Watanabe +13

We conducted a polarimetric observation of the fast-rotating near-Earth asteroid (1566) Icarus at large phase (Sun-asteroid-observer's) angles = 57 deg--141deg around the 2015 s…

astro-ph.EP2014★ 6 cited

Near-infrared Brightness of the Galilean Satellites Eclipsed in Jovian Shadow: A New Technique to Investigate Jovian Upper Atmosphere

K. Tsumura, K. Arimatsu, E. Egami +12

We have discovered that Europa, Ganymede and Callisto are bright around 1.5 μm even when not directly lit by sunlight, based on observations from the Hubble Space Telescope and the…

astro-ph.HE2013★ 50 cited

Search for correlations of the arrival directions of ultra-high energy cosmic ray with extragalactic objects as observed by the telescope array experiment

T. Abu-Zayyad, R. Aida, M. Allen +141

We search for correlations between positions of extragalactic objects and arrival directions of Ultra-High Energy Cosmic Rays (UHECRs) with primary energy EeV as observe…

astro-ph.HE2013★ 1 cited

Energy Spectrum of Ultra-High Energy Cosmic Rays Observed with the Telescope Array Using a Hybrid Technique

T. Abu-Zayyad, R. Aida, M. Allen +141

We measure the spectrum of cosmic rays with energies greater than eV with the Fluorescence Detectors (FDs) and the Surface Detectors (SDs) of the Telescope Array Experi…

astro-ph.HE2013★ 1 cited

The Energy Spectrum of Ultra-High-Energy Cosmic Rays Measured by the Telescope Array FADC Fluorescence Detectors in Monocular Mode

The Telescope Array Collaboration, T. Abu-Zayyad, R. Aida +141

We present a measurement of the energy spectrum of ultra-high-energy cosmic rays performed by the Telescope Array experiment using monocular observations from its two new FADC-base…

astro-ph.HE2013★ 50 cited

Upper limit on the flux of photons with energies above 10^19 eV using the Telescope Array surface detector

T. Abu-Zayyad, R. Aida, M. Allen +138

We search for ultra-high energy photons by analyzing geometrical properties of shower fronts of events registered by the Telescope Array surface detector. By making use of an event…

astro-ph.HE2012★ 71 cited

Search for Anisotropy of Ultra-High Energy Cosmic Rays with the Telescope Array Experiment

T. Abu-Zayyad, R. Aida, M. Allen +139

We study the anisotropy of Ultra-High Energy Cosmic Ray (UHECR) events collected by the Telescope Array (TA) detector in the first 40 months of operation. Following earlier studies…

astro-ph.HE2012★ 264 cited

The Cosmic Ray Energy Spectrum Observed with the Surface Detector of the Telescope Array Experiment

T. Abu-Zayyad, R. Aida, M. Allen +137

The Telescope Array (TA) collaboration has measured the energy spectrum of ultra-high energy cosmic rays with primary energies above 1.6 x 10^(18) eV. This measurement is based upo…

astro-ph.IM2012★ 43 cited

The Energy Spectrum of Telescope Array's Middle Drum Detector and the Direct Comparison to the High Resolution Fly's Eye Experiment

T. Abu-Zayyad, R. Aida, M. Allen +137

The Telescope Array's Middle Drum fluorescence detector was instrumented with telescopes refurbished from the High Resolution Fly's Eye's HiRes-1 site. The data observed by Middle…

astro-ph.IM2012★ 399 cited

The surface detector array of the Telescope Array experiment

T. Abu-Zayyad, R. Aida, M. Allen +134

The Telescope Array (TA) experiment, located in the western desert of Utah,USA, is designed for observation of extensive air showers from extremely high energy cosmic rays. The exp…

astro-ph.IM2011★ 274 cited

New air fluorescence detectors employed in the Telescope Array experiment

H. Tokuno, Y. Tameda, M. Takeda +134

Since 2007, the Telescope Array (TA) experiment, based in Utah, USA, has been observing ultra high energy cosmic rays to understand their origins. The experiment involves a surface…