activity
19972015
most citedCosmological Imprint of an Energy Component with General Equation of State

3.7k citations · 4.1k across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.IM2015★ 27 cited

FATS: Feature Analysis for Time Series

Isadora Nun, Pavlos Protopapas, Brandon Sim +4

In this paper, we present the FATS (Feature Analysis for Time Series) library. FATS is a Python library which facilitates and standardizes feature extraction for time series data.…

astro-ph.SR2010★ 8 cited

The TAOS Project Stellar Variability II. Detection of 15 Variable Stars

S. Mondal, C. C. Lin, W. P. Chen +20

The Taiwanese-American Occultation Survey (TAOS) project has collected more than a billion photometric measurements since 2005 January. These sky survey data-covering timescales fr…

astro-ph.EP2010★ 31 cited

The TAOS Project: Upper Bounds on the Population of Small KBOs and Tests of Models of Formation and Evolution of the Outer Solar System

F. B. Bianco, Z. -W. Zhang, M. J. Lehner +23

We have analyzed the first 3.75 years of data from TAOS, the Taiwanese American Occultation Survey. TAOS monitors bright stars to search for occultations by Kuiper Belt Objects (KB…

astro-ph.SR2009★ 8 cited

The TAOS Project Stellar Variability I. Detection of Low-Amplitude delta Scuti Stars

D. -W. Kim, P. Protopapas, C. Alcock +22

We analyzed data accumulated during 2005 and 2006 by the Taiwan-American Occultation Survey (TAOS) in order to detect short-period variable stars (periods of <~ 1 hour) such as del…

astro-ph.EP2009★ 16 cited

Upper Limits on the Number of Small Bodies in Sedna-Like Orbits by the TAOS Project

J. -H. Wang, M. J. Lehner, Z. -W. Zhang +21

We present the results of a search for occultation events by objects at distances between 100 and 1000 AU in lightcurves from the Taiwanese-American Occultation Survey (TAOS). We s…

astro-ph.SR2009★ 3 cited

A Close Binary Star Resolved from Occultation by 87 Sylvia

Chi-Long Lin, Zhi-Wei Zhang, W. P. Chen +22

The star BD+29 1748 was resolved to be a close binary from its occultation by the asteroid 87 Sylvia on 2006 December 18 UT. Four telescopes were used to observe this event at two…