activity
19972016
most citedOn X-ray variability in narrow line and broad line AGNs

84 citations · 155 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2016★ 24 cited

The peculiar velocities in the Galactic outer disk--hints of the elliptical disk and the perturbation of the spiral structures

Hai-Jun Tian, Chao Liu, Jun-Chen Wan +7

We present the peculiar in-plane velocities derived from the LAMOST red clump stars. From the variations of the in-plane velocity with the Galactocentric radius for the young and o…

astro-ph.GA2015★ 24 cited

The stellar kinematics in the solar neighborhood from LAMOST data

Hai-Jun Tian, Chao Liu, Jeffrey L. Carlin +6

We use about 200,000 FGK type main-sequence stars from the LAMOST DR1 data to map the local stellar kinematics. With the velocity de-projection technique, we are able to derive the…

astro-ph2007★ 23 cited

Two novel approaches for photometric redshift estimation based on SDSS and 2MASS databases

Dan Wang, Yan-Xia Zhang, Chao Liu +1

We investigate two training-set methods: support vector machines (SVMs) and Kernel Regression (KR) for photometric redshift estimation with the data from the Sloan Digital Sky Surv…

astro-ph2006

The DWT Power Spectrum of the two-degree Field Galaxy Redshift Survey

Yan-Chuan Cai, Jun Pan, Yong-Heng Zhao +2

The power spectrum of the two-degree Field Galaxy Redshift Survey (2dFGRS) sample is estimated with the discrete wavelet transform (DWT) method. The DWT power spectra within $0.04…

astro-ph2003

Black Hole -- Bulge Relation for Narrow-Line Objects

Bian Weihao, Zhao Yongheng

It has been thought that narrow-line Seyfert 1 galaxies are likely to be in the early stages of the evolution of active galaxies. To test this suggestion, the ratios of the central…

astro-ph2003★ 84 cited

On X-ray variability in narrow line and broad line AGNs

W. Bian, Y. Zhao

We assembled a sample of broad line and narrow lines AGNs observed by ASCA, whose excess variances have been determined. The central black hole masses in this sample can be obtaine…