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20162022
most citedThe X-ray counterpart to the gravitational wave event GW 170817

888 citations · 2.3k across the 30 of their papers we have counts for

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Showing 2017Show all

10 papers · 1 filter

astro-ph.HE2017171 cited

The environment of the binary neutron star merger GW170817

A. J. Levan, J. D. Lyman, N. R. Tanvir +37

We present Hubble Space Telescope and Chandra imaging, combined with Very Large Telescope MUSE integral field spectroscopy of the counterpart and host galaxy of the first binary ne…

astro-ph.HE2017888 cited

The X-ray counterpart to the gravitational wave event GW 170817

E. Troja, L. Piro, H. van Eerten +31

A long-standing paradigm in astrophysics is that collisions- or mergers- of two neutron stars (NSs) form highly relativistic and collimated outflows (jets) powering gamma-ray burst…

astro-ph.HE201754 cited

X-ray Emission from SN 2012ca: A Type Ia-CSM Supernova Explosion in a Dense Surrounding Medium

C. D. Bochenek, Vikram. V. Dwarkadas, Jeffrey M. Silverman +4

X-ray emission is one of the signposts of circumstellar interaction in supernovae (SNe), but until now, it has been observed only in core-collapse SNe. The level of thermal X-ray e…

astro-ph.GA201712 cited

Probing gas and dust in the tidal tail of NGC 5221 with the type Ia supernova iPTF16abc

R. Ferretti, R. Amanullah, A. Goobar +8

Context. Type Ia supernovae (SNe Ia) can be used to address numerous questions in astrophysics and cosmology. Due to their well known spectral and photometric properties, SNe Ia ar…

astro-ph.SR201714 cited

Constraints on the Progenitor of SN 2010jl and Pre-Existing Hot Dust in its Surrounding Medium

Eli Dwek, Richard G. Arendt, Ori D. Fox +6

A search for the progenitor of SN~2010jl, an unusually luminous core-collapse supernova of Type~IIn, using pre-explosion {\it Hubble}/WFPC2 and {\it Spitzer}/IRAC images of the reg…

astro-ph.HE201742 cited

Optical and IR observations of SN 2013L, a Type IIn Supernova surrounded by asymmetric CSM

Jennifer E. Andrews, Nathan Smith, Curtis McCully +3

We present optical and NIR photometry and spectroscopy of SN 2013L for the first four years post-explosion. SN 2013L was a moderately luminous (M = -19.0) Type IIn supernova…