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19942026
most citedDiscovery of a Cool Planet of 5.5 Earth Masses Through Gravitational Microlensing

596 citations · 9.7k across the 249 of their papers we have counts for

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Showing 2017Show all

19 papers · 1 filter

astro-ph.EP2017★ 36 cited

OGLE-2016-BLG-1190Lb: First Spitzer Bulge Planet Lies Near the Planet/Brown-Dwarf Boundary

Y. -H. Ryu, J. C. Yee, A. Udalski +106

We report the discovery of OGLE-2016-BLG-1190Lb, which is likely to be the first Spitzer microlensing planet in the Galactic bulge/bar, an assignation that can be confirmed by two…

astro-ph.EP2017★ 30 cited

OGLE-2015-BLG-1459L: The Challenges of Exo-Moon Microlensing

K. -H. Hwang, A. Udalski, I. A. Bond +57

We show that dense OGLE and KMTNet -band survey data require four bodies (sources plus lenses) to explain the microlensing light curve of OGLE-2015-BLG-1459. However, these can…

astro-ph.EP2017★ 27 cited

An Isolated Microlens Observed from K2, Spitzer and Earth

Wei Zhu, A. Udalski, C. Huang +50

We present the result of microlensing event MOA-2016-BLG-290, which received observations from the two-wheel Kepler (K2), Spitzer, as well as ground-based observatories. A joint an…

astro-ph.EP2017★ 15 cited

OGLE-2016-BLG-0263L\lowercase{b}: Microlensing Detection of a Very Low-mass Binary Companion Through a Repeating Event Channel

C. Han, A. Udalski, A. Gould +51

We report the discovery of a planet-mass companion to the microlens OGLE-2016-BLG-0263L. Unlike most low-mass companions that were detected through perturbations to the smooth and…

astro-ph.SR2017★ 9 cited

Ground-based parallax confirmed by Spitzer: binary microlensing event MOA-2015-BLG-020

Tianshu Wang, Wei Zhu, Shude Mao +83

We present the analysis of the binary gravitational microlensing event MOA-2015-BLG-020. The event has a fairly long timescale (about 63 days) and thus the light curve deviates sig…

astro-ph.EP2017★ 25 cited

The First Planetary Microlensing Event with Two Microlensed Source Stars

D. P. Bennett, A. Udalski, C. Han +64

We present the analysis of microlensing event MOA-2010-BLG-117, and show that the light curve can only be explained by the gravitational lensing of a binary source star system by a…

astro-ph.HE2017

Analysis of solar gamma rays and solar neutrons detected on March 7th and September 25th of 2011 by Ground Level Neutron Telescopes, SEDA-FIB and FERMI-LAT

Y. Muraki, J. F. Valdes-Galicia, L. X. Gonzalez +16

At the 33rd ICRC, we reported the possible detection of solar gamma rays by a ground level detector and later re-examined this event. On March 7, 2011, the solar neutron telescope…

astro-ph.SR2017★ 5 cited

The First Eclipsing Binary Catalogue from the MOA-II database

M. C. A. Li, N. J. Rattenbury, A. Bond +25

We present the first catalogue of eclipsing binaries in two MOA fields towards the Galactic bulge, in which over 8,000 candidates, mostly contact and semi-detached binaries of peri…

astro-ph.SR2017

Application of Coupled Harmonic Oscillator model to Solar Activity and El Niño Phenomena

Yasushi Muraki

The solar activity provides an important impact not only on the intensity of cosmic rays but also on the earth environment. In this paper, a coupled oscillator model is proposed to…

astro-ph.SR2017★ 14 cited

OGLE-2016-BLG-1469L: Microlensing Binary Composed of Brown Dwarfs

C. Han, A. Udalski, T. Sumi +50

We report the discovery of a binary composed of two brown dwarfs, based on the analysis of the microlensing event OGLE-2016-BLG-1469. Thanks to detection of both finite-source and…

astro-ph.EP2017★ 45 cited

MOA-2016-BLG-227Lb: A Massive Planet Characterized by Combining Lightcurve Analysis and Keck AO Imaging

Naoki Koshimoto, Yossi Shvartzvald, David Bennett +55

We report the discovery of a microlensing planet --- MOA-2016-BLG-227Lb --- with a large planet/host mass ratio of . This event was located near the …

astro-ph.EP2017★ 10 cited

MOA Data Reveal a New Mass, Distance, and Relative Proper Motion for Planetary System OGLE-2015-BLG-0954L

D. P. Bennett, I. A. Bond, F. Abe +26

We present the MOA Collaboration light curve data for planetary microlensing event OGLE-2015-BLG-0954, which was previously announced in a paper by the KMTNet and OGLE Collaboratio…

astro-ph.SR2017★ 17 cited

OGLE-2016-BLG-1003: First Resolved Caustic-crossing Binary-source Event Discovered by Second-generation Microlensing Surveys

Y. K. Jung, A. Udalski, I. A. Bond +50

We report the analysis of the first resolved caustic-crossing binary-source microlensing event OGLE-2016-BLG-1003. The event is densely covered by the round-the-clock observations…

astro-ph.EP2017★ 10 cited

OGLE-2013-BLG-0132Lb and OGLE-2013-BLG-1721Lb: Two Saturn-mass Planets Discovered around M-dwarfs

Przemek Mroz, A. Udalski, I. A. Bond +37

We present the discovery of two planetary systems consisting of a Saturn-mass planet orbiting an M-dwarf, which were detected in faint microlensing events OGLE-2013-BLG-0132 and OG…

astro-ph.EP2017★ 21 cited

A companion on the planet/brown dwarf mass boundary on a wide orbit discovered by gravitational microlensing

R. Poleski, A. Udalski, I. A. Bond +40

We present the discovery of a substellar companion to the primary host lens in the microlensing event MOA-2012-BLG-006. The companion-to-host mass ratio is 0.016, corresponding to…

astro-ph.EP2017★ 17 cited

OGLE-2013-BLG-1761Lb: A Massive Planet Around an M/K Dwarf

Y. Hirao, A. Udalski, T. Sumi +37

We report the discovery and the analysis of the planetary microlensing event, OGLE-2013-BLG-1761. There are some degenerate solutions in this event because the planetary anomaly is…

astro-ph.EP2017★ 7 cited

MOA-2012-BLG-505Lb: A super-Earth mass planet probably in the Galactic bulge

Masayuki Nagakane, Takahiro Sumi, Naoki Koshimoto +27

We report the discovery of a super-Earth mass planet in the microlensing event MOA-2012-BLG-505. This event has the second shortest event timescale of days whe…

astro-ph.EP2017★ 84 cited

The Lowest Mass Ratio Planetary Microlens: OGLE 2016-BLG-1195Lb

I. A. Bond, D. P. Bennett, T. Sumi +37

We report discovery of the lowest mass ratio exoplanet to be found by the microlensing method in the light curve of the event OGLE~2016--BLG--1195. This planet revealed itself as a…

hep-ex2017★ 43 cited

Measurement of forward photon production cross-section in proton-proton collisions at = 13 TeV with the LHCf detector

O. Adriani, E. Berti, L. Bonechi +24

In this paper, we report the production cross-section of forward photons in the pseudorapidity regions of and , measured by the LHCf experiment w…