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20032024
most citedThe Spectral Energy Distribution of Fermi bright blazars

1k citations · 5k across the 59 of their papers we have counts for

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8 papers · 1 filter

astro-ph.EP2016★ 15 cited

The Pan-STARRS 1 Discoveries of five new Neptune Trojans

Hsing Wen Lin, Ying-Tung Chen, Matthew J. Holman +16

In this work we report the detection of seven Neptune Trojans (NTs) in the Pan-STARRS 1 (PS1) survey. Five of these are new discoveries, consisting of four L4 Trojans and one L5 Tr…

astro-ph.EP2015★ 24 cited

Ground-based transit observations of the HAT-P-18, HAT-P-19, HAT-P-27/WASP-40 and WASP-21 systems

M. Seeliger, M. Kitze, R. Errmann +46

As part of our ongoing effort to investigate transit timing variations (TTVs) of known exoplanets, we monitored transits of the four exoplanets HAT-P-18b, HAT-P-19b, HAT-P-27b/WASP…

astro-ph.EP2013★ 51 cited

The TAOS Project: Results From Seven Years of Survey Data

Z. -W. Zhang, M. J. Lehner, J. -H. Wang +19

The Taiwanese-American Occultation Survey (TAOS) aims to detect serendipitous occultations of stars by small (about 1 km diameter) objects in the Kuiper Belt and beyond. Such event…

astro-ph.EP2013★ 57 cited

Multi-site campaign for transit timing variations of WASP-12 b: possible detection of a long-period signal of planetary origin

G. Maciejewski, D. Dimitrov, M. Seeliger +38

The transiting planet WASP-12 b was identified as a potential target for transit timing studies because a departure from a linear ephemeris was reported in the literature. Such dev…

astro-ph.EP2010★ 51 cited

Transit timing variation and activity in the WASP-10 planetary system

G. Maciejewski, D. Dimitrov, R. Neuhaeuser +13

Transit timing analysis may be an effective method of discovering additional bodies in extrasolar systems which harbour transiting exoplanets. The deviations from the Keplerian mot…

astro-ph.EP2010★ 14 cited

The TAOS Project: Statistical Analysis of Multi-Telescope Time Series Data

M. J. Lehner, N. K. Coehlo, Z. -W. Zhang +17

The Taiwanese-American Occultation Survey (TAOS) monitors fields of up to ~1000 stars at 5 Hz simultaneously with four small telescopes to detect occultation events from small (~1…