activity
20042026
most citedThe Chandra Deep Field-South Survey: 4 Ms Source Catalogs

581 citations · 4.1k across the 72 of their papers we have counts for

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Showing 2019Show all

8 papers · 1 filter

astro-ph.GA2019★ 12 cited

X-ray spectral variations of synchrotron peak in BL Lacs

Yijun Wang, Shifu Zhu, Yongquan Xue +3

The spectral energy distribution of blazars around the synchrotron peak can be well described by the log-parabolic model that has three parameters: peak energy (), pe…

astro-ph.HE2019★ 39 cited

A unified binary neutron star merger magnetar model for the Chandra X-ray transients CDF-S XT1 and XT2

Hui Sun, Ye Li, Binbin Zhang +4

Two bright X-ray transients were reported from the Chandra Deep Field South archival data, namely CDF-S XT1 and XT2. Whereas the nature of the former is not identified, the latter…

astro-ph.GA2019★ 2 cited

High Redshift Obscured Quasars and the Need for Optical to NIR, Massively Multiplexed, Spectroscopic Facilities

Andreea Petric, Mark Lacy, Stéphanie Juneau +15

Most bulge-dominated galaxies host black holes with masses that tightly correlate with the masses of their bulges. This may indicate that the black holes may regulate galaxy growth…

astro-ph.GA2019★ 6 cited

On the Origin of the Dramatic Spectral Variability of WPVS 007

Junyao Li, Mouyuan Sun, Tinggui Wang +2

We report the discovery of large-amplitude mid-infrared variabilities (MIR; mag) in the Wide-field Infrared Survey Explorer W1 and W2 bands of the low-luminosity narrow-…

astro-ph.GA2019★ 73 cited

The Host-Galaxy Properties of Type 1 Versus Type 2 Active Galactic Nuclei

Fan Zou, Guang Yang, William N. Brandt +1

The unified model of active galactic nuclei (AGNs) proposes that different AGN optical spectral types are caused by different viewing angles with respect to an obscuring 'torus'. T…

astro-ph.HE2019★ 130 cited

A magnetar-powered X-ray transient as the aftermath of a binary neutron-star merger

Y. Q. Xue, X. C. Zheng, Y. Li +14

Neutron star-neutron star mergers are known to be associated with short gamma-ray bursts. If the neutron star equation of state is sufficiently stiff, at least some of such mergers…