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20032026
most citedThe Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617

1.9k citations · 17k across the 275 of their papers we have counts for

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Showing 2017 · astro-ph.HEShow all

7 papers · 2 filters

astro-ph.HE2017★ 15 cited

Chandra X-ray Constraints on the Candidate Ca-rich Gap Transient SN 2016hnk

P. H. Sell, K. Arur, T. J. Maccarone +4

We present a Chandra observation of SN 2016hnk, a candidate Ca-rich gap transient. This observation was specifically designed to test whether or not this transient was the result o…

astro-ph.HE2017★ 126 cited

The early detection and follow-up of the highly obscured Type II supernova 2016ija/DLT16am

L. Tartaglia, D. J. Sand, S. Valenti +45

We present our analysis of the Type II supernova DLT16am (SN~2016ija). The object was discovered during the ongoing (DLT40) one day cadence supernova search a…

astro-ph.HE2017★ 24 cited

2FGL J0846.0+2820: A new neutron star binary with a giant secondary and variable -ray emission

Samuel J. Swihart, Jay Strader, Tyrel J. Johnson +11

We present optical photometric and spectroscopic observations of the likely stellar counterpart to the unassociated \emph{Fermi}-Large Area Telescope (LAT) -ray source 2FGL J084…

astro-ph.HE2017★ 41 cited

An empirical limit on the kilonova rate from the DLT40 one day cadence Supernova Survey

Sheng Yang, Stefano Valenti, Enrico Cappellaro +6

Binary neutron star mergers are important to understand stellar evolution, the chemical enrichment of the universe via the r-process, the physics of short gamma-ray bursts, gravita…

astro-ph.HE2017★ 54 cited

SN 2016coi/ASASSN-16fp: An example of residual helium in a type Ic supernova?

S. J. Prentice, C. Ashall, P. A. Mazzali +35

The optical observations of Ic-4 supernova (SN) 2016coi/ASASSN-16fp, from to days after explosion, are presented along with analysis of its physical properties.…

astro-ph.HE2017★ 72 cited

Nebular-Phase Spectra of Nearby Type Ia Supernovae

Melissa L. Graham, Sahana Kumar, Griffin Hosseinzadeh +8

We present late-time spectra of eight Type Ia supernovae (SNe Ia) obtained at days after peak brightness using the Gemini South and Keck telescopes. All of the SNe Ia in our…