output
19932026
most citedThe Gaia mission

7.1k citations

Showing 2016 · astro-ph.HEShow all

48 papers · 2 filters

astro-ph.HE2016★ 6 cited

Testing the axion-conversion hypothesis of 3.5 keV emission with polarization

Yan Gong, Xuelei Chen, Hua Feng

The recently measured 3.5 keV line in a number of galaxy clusters, the Andromeda galaxy (M31) and the Milky Way (MW) center can be well accounted for by a scenario in which dark ma…

astro-ph.HE2016★ 21 cited

Revisiting the structure and spectrum of the magnetic-reconnection-heated corona in luminous AGNs

J. Y. Liu, ErLin Qiao, B. F. Liu

It is believed that the hard X-ray emission in the luminous active galactic nuclei (AGNs) is from the hot corona above the cool accretion disk. However, the formation of the corona…

astro-ph.HE2016★ 102 cited

Gamma-ray burst progenitors

Andrew Levan, Paul Crowther, Richard de Grijs +3

We review our current understanding of the progenitors of both long and short duration gamma-ray bursts (GRBs). Constraints can be derived from multiple directions, and we use thre…

astro-ph.HE2016★ 60 cited

Ultraluminous X-ray bursts in two ultracompact companions to nearby elliptical galaxies

Jimmy A. Irwin, W. Peter Maksym, Gregory R. Sivakoff +8

An X-ray flaring source was found near the galaxy NGC 4697. Two flares were seen, separated by four years. The flux increased by a factor of 90 on a timescale of about one minute.…

astro-ph.HE2016★ 30 cited

Evidence for magnetar formation in broad-lined type Ic supernovae 1998bw and 2002ap

L. J. Wang, H. Yu, L. D. Liu +6

Broad-lined type Ic supernovae (SNe Ic-BL) are peculiar stellar explosions that distinguish themselves from ordinary SNe. Some SNe Ic-BL are associated with long-duration (\gtrsim…

astro-ph.HE2016★ 35 cited

A New Measurement of the Spectral Lag of Gamma-Ray Bursts and its Implications for Spectral Evolution Behaviors

Lang Shao, Bin-Bin Zhang, Fu-Ri Wang +9

We carry out a systematical study of the spectral lag properties of 50 single-pulsed Gamma-Ray Bursts (GRBs) detected by Fermi/GBM. By dividing the light curves into multiple conse…

astro-ph.HE2016★ 50 cited

The second closest gamma-ray burst: sub-luminous GRB 111005A with no supernova in a super-solar metallicity environment

Michał J. Michałowski, Dong Xu, Jamie Stevens +17

We report the detection of the radio afterglow of a long gamma-ray burst (GRB) 111005A at 5-345 GHz, including the very long baseline interferometry observations with the positiona…

astro-ph.HE2016★ 21 cited

Curvature of the spectral energy distribution, the dominant process for inverse Compton component and other jet properties in Fermi 2LAC blazars

R. Xue, D. Luo, L. M. Du +7

We fit the spectral energy distributions (SEDs) of members of a large sample of Fermi 2LAC blazars to synchrotron and inverse Compton (IC) models. Our main results are as follows.…

astro-ph.HE2016★ 72 cited

NuSTAR observations of WISE J1036+0449, a Galaxy at z obscured by hot dust

C. Ricci, R. J. Assef, D. Stern +34

Hot, Dust-Obscured Galaxies (Hot DOGs), selected from the WISE all sky infrared survey, host some of the most powerful Active Galactic Nuclei (AGN) known, and might represent an im…

astro-ph.HE2016★ 26 cited

Very Bright Prompt and Reverse Shock Emission of GRB 140512A

Xiao-Li Huang, Li-Ping Xin, Shuang-Xi Yi +5

We report our observations of very bright prompt optical and reverse shock (RS) optical emission of GRB 140512A and analyze its multi-wavelength data observed with the {\em Swift}…

astro-ph.HE2016★ 9 cited

Highly polarized components of integrated pulse profiles

P. F. Wang, J. L. Han

Highly polarized components of pulse profiles are investigated by analyzing observational data and simulating the emission processes. The highly polarized components appear at the…

astro-ph.HE2016★ 12 cited

The intrinsic line width of the Fe Ka line of AGN

Jiren Liu

X-ray fluorescent lines are unique features of the reflection spectrum of the cold torus when irradiated by the central AGN. Their intrinsic line widths can be used to probe the li…

astro-ph.HE2016★ 6 cited

Time-Variable Aluminum Absorption in the Polar AR Ursae Majoris, and an Updated Estimate for the Mass of the White Dwarf

Yu Bai, Stephen Justham, JiFeng Liu +3

We present spectra of the extreme polar AR Ursae Majoris (AR UMa) which display a clear Al I absorption doublet, alongside spectra taken less than a year earlier in which that feat…

astro-ph.HE2016★ 182 cited

The Spectral Energy Distributions of Fermi Blazars

J. H. Fan, J. H. Yang, Y. Liu +7

(Abridged) In this paper, multi-wavelength data are compiled for a sample of 1425 Fermi blazars to calculate their spectral energy distributions (SEDs). A parabolic function, $\log…

astro-ph.HE2016★ 1 cited

Sharp Chandra View of ROSAT All-Sky Survey Bright Sources: I. Improvement of Positional Accuracy

Shuang Gao, Song Wang, Jifeng Liu

The ROSAT All-Sky Survey (RASS) represents one of the most complete and sensitive soft X-ray all-sky surveys to date. However, the deficient positional accuracy of the RASS Bright…

astro-ph.HE2016★ 23 cited

Solving the 56Ni puzzle of magnetar-powered broad-lined type Ic supernovae

Ling-Jun Wang, Yan-Hui Han, Dong Xu +4

Broad-lined type Ic supernovae (SNe Ic-BL) are of great importance because their association with long-duration gamma-ray bursts (LGRBs) holds the key to deciphering the central en…

astro-ph.HE2016★ 25 cited

The History of GRB Outflows: Ejection Lorentz Factor and Radiation Location of X-Ray Flares

Hui-Jun Mu, Da-Bin Lin, Shao-Qiang Xi +6

We present time-resolved spectral analysis of the steep decay segments of 29 bright X-ray flares of gamma-ray bursts (GRBs) observed with the Swift/X-ray telescope, and model their…

astro-ph.HE2016★ 33 cited

Rotational evolution of magnetars in the presence of a fallback disk

H. Tong, W. Wang, X. W. Liu +1

Magnetars may have strong surface dipole field. Observationally, two magnetars may have passive fallback disks. In the presence of a fallback disk, the rotational evolution of magn…

astro-ph.HE2016★ 7 cited

GRB 110530A: Peculiar Broad Bump and Delayed Plateau in Early Optical Afterglows

Shu-Qing Zhong, Li-Ping Xin, En-Wei Liang +7

We report our very early optical observations of GRB 110530A and investigate its jet properties together with its X-ray afterglow data. A peculiar broad onset bump followed by a pl…

astro-ph.HE2016★ 15 cited

The radiative efficiency of relativistic jet and wind: A case study of GRB 070110

Shuang Du, Hou-Jun Lü, Shu-Qing Zhong +1

A rapidly spinning, strongly magnetized neutron star is invoked as the central engine for some Gamma-ray bursts (GRBs), especially, the internal plateau feature of X-ray afte…

astro-ph.HE2016★ 12 cited

Similarity of Jet Radiation between Flat Spectrum Radio Quasars and GeV Narrow-Line Seyfert 1 Galaxies: A Universal - Correlation

Yong-Kai Zhu, Jin Zhang, Hai-Ming Zhang +4

By modeling the broadband spectral energy distributions (SEDs) of a typical flat spectrum radio quasar (FSRQ, 3C 279) and two GeV narrow-line Seyfert 1 galaxies (NLS1s, PMN J0948+0…

astro-ph.HE2016★ 29 cited

Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities

Weimin Yuan, Lorenzo Amati, John K. Cannizzo +10

High-redshift Gamma-Ray Bursts (GRBs) beyond redshift are potentially powerful tools to probe the distant early Universe. Their detections in large numbers and at truly hig…

astro-ph.HE2016★ 38 cited

Prospects for constraining the spin of the massive black hole at the Galactic center via the relativistic motion of a surrounding star

Qingjuan Yu, Fupeng Zhang, Youjun Lu

In this paper, we investigate the quality of constraining the spin of the massive black hole (MBH) at the Galactic center (GC) by using full general relativistic simulations of the…

astro-ph.HE2016★ 3 cited

Three X-ray Flares Near Primary Eclipse of the RS CVn Binary XY UMa

Hang Gong, Rachel Osten, Thomas Maccarone +3

We report on an archival X-ray observation of the eclipsing RS CVn binary XY UMa ( 0.48d). In two ACIS observations spanning 200 ks and almost…