output
20022015
most citedThe Five-Hundred-Meter Aperture Spherical Radio Telescope (FAST) Project

872 citations

Showing 2015Show all

50 papers · 1 filter

astro-ph.GA2015155 cited

Calibration of the optical mass proxy for clusters of galaxies and an update of the WHL12 cluster catalog

Z. L. Wen, J. L. Han

Accurately determining the mass of galaxy clusters is fundamental for many studies on cosmology and galaxy evolution. We collect and rescale the cluster masses of 1191 clusters of…

astro-ph.IM20157 cited

A Practical Deconvolution Computation Algorithm to Extract 1D Spectra from 2D Images of Optical Fiber Spectroscopy

Guangwei Li, Haotong Zhang, Zhongrui Bai

Bolton and Schlegel presented a promising deconvolution method to extract 1D spectra from a 2D optical fiber spectral CCD image. The method could eliminate the PSF difference betwe…

astro-ph.SR201526 cited

An independent test of the photometric selection of white dwarf candidates using LAMOST DR3

N. P. Gentile Fusillo, A. Rebassa-Mansergas, B. T. Gänsicke +7

In Gentile Fusillo et al. (2015) we developed a selection method for white dwarf candidates which makes use of photometry, colours and proper motions to calculate a probability of…

astro-ph.EP201536 cited

Using the Rossiter-McLaughlin effect to observe the transmission spectrum of Earth's atmosphere

Fei Yan, Robert A. E. Fosbury, Monika G. Petr-Gotzens +2

Due to stellar rotation, the observed radial velocity of a star varies during the transit of a planet across its surface, a phenomenon known as the Rossiter-McLaughlin (RM) effect.…

astro-ph.SR201515 cited

Optical observations of a SN 2002cx-like peculiar supernova SN 2013en in UGC 11369

Zheng-Wei Liu, Jujia Zhang, Fabrizio Ciabattari +7

We present optical observations of a SN 2002cx-like supernova SN 2013en in UGC 11369, spanning from a phase near maximum light (t= +1 d) to t= +60 d with respect to the R-band maxi…

astro-ph.CO2015

Combining time delays and image positions for quadruple lenses: a moment approach

Hans Witt, Shude Mao

Time delays in gravitational lenses can be used to determine the Hubble constant and the lens potential. In future surveys, many gravitational lenses can be discovered, and their t…