Search Publications

An Embedded X-Ray Source Shines through the Aspherical AT 2018cow: Revealing the Inner Workings of the Most Luminous Fast-evolving Optical Transients
DOI: 10.3847/1538-4357/aafa01 Bibcode: 2019ApJ...872...18M

Berger, E.; Hurley, K.; Götz, D. +42 more

We present the first extensive radio to γ-ray observations of a fast-rising blue optical transient, AT 2018cow, over its first ∼100 days. AT 2018cow rose over a few days to a peak luminosity L pk ∼ 4 × 1044 erg s-1, exceeding that of superluminous supernovae (SNe), before declining as L ∝ t -2. Initial s…

2019 The Astrophysical Journal
INTEGRAL XMM-Newton 225
A Decade of Gamma-Ray Bursts Observed by Fermi-LAT: The Second GRB Catalog
DOI: 10.3847/1538-4357/ab1d4e Bibcode: 2019ApJ...878...52A

Troja, E.; Caraveo, P. A.; Mirabal, N. +120 more

The Large Area Telescope (LAT) aboard the Fermi spacecraft routinely observes high-energy emission from gamma-ray bursts (GRBs). Here we present the second catalog of LAT-detected GRBs, covering the first 10 yr of operations, from 2008 to 2018 August 4. A total of 186 GRBs are found; of these, 91 show emission in the range 30-100 MeV (17 of which …

2019 The Astrophysical Journal
INTEGRAL 198
Follow-up of the Neutron Star Bearing Gravitational-wave Candidate Events S190425z and S190426c with MMT and SOAR
DOI: 10.3847/2041-8213/ab271c Bibcode: 2019ApJ...880L...4H

Reichart, D. E.; Berger, E.; Chornock, R. +23 more

On 2019 April 25.346 and 26.640 UT the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo gravitational-wave (GW) observatory announced the detection of the first candidate events in Observing Run 3 that contained at least one neutron star (NS). S190425z is a likely binary neutron star (BNS) merger at d L = 156 ± 41 …

2019 The Astrophysical Journal
INTEGRAL 78
Prompt Emission Polarimetry of Gamma-Ray Bursts with the AstroSat CZT Imager
DOI: 10.3847/1538-4357/ab40b7 Bibcode: 2019ApJ...884..123C

Rao, A. R.; Bhalerao, Varun; Mate, Sujay +10 more

X-ray and gamma-ray polarization measurements of the prompt emission of gamma-ray bursts (GRBs) are believed to be extremely important for testing various models of GRBs. So far, the available measurements of hard X-ray polarization of GRB prompt emission have not significantly constrained the GRB models, particularly because of the difficulty of …

2019 The Astrophysical Journal
INTEGRAL 78
On High-energy Particles in Accretion Disk Coronae of Supermassive Black Holes: Implications for MeV Gamma-rays and High-energy Neutrinos from AGN Cores
DOI: 10.3847/1538-4357/ab2715 Bibcode: 2019ApJ...880...40I

Inoue, Susumu; Inoue, Yoshiyuki; Doi, Akihiro +1 more

Recent observations with ALMA have revealed evidence for nonthermal synchrotron emission from the core regions of two nearby Seyfert galaxies. This suggests that the coronae of accretion disks in active galactic nuclei (AGNs) can be conducive to the acceleration of nonthermal electrons, in addition to the hot, thermal electrons responsible for the…

2019 The Astrophysical Journal
INTEGRAL 72
Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo
DOI: 10.3847/1538-4357/ab4b48 Bibcode: 2019ApJ...886...75A

Lee, H. M.; Williams, D.; Hurley, K. +1196 more

We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitation…

2019 The Astrophysical Journal
INTEGRAL 31
SN 2016coi (ASASSN-16fp): An Energetic H-stripped Core-collapse Supernova from a Massive Stellar Progenitor with Large Mass Loss
DOI: 10.3847/1538-4357/ab3e37 Bibcode: 2019ApJ...883..147T

Hurley, K.; Challis, P.; Stanek, K. Z. +26 more

We present comprehensive observations and analysis of the energetic H-stripped SN 2016coi (a.k.a. ASASSN-16fp), spanning the γ-ray through optical and radio wavelengths, acquired within the first hours to ∼420 days post explosion. Our observational campaign confirms the identification of He in the supernova (SN) ejecta, which we interpret to be ca…

2019 The Astrophysical Journal
INTEGRAL XMM-Newton 30
On the High-energy Emissions of Compact Objects Observed with INTEGRAL SPI: Event Selection Impact on Source Spectra and Scientific Results for the Bright Sources Crab Nebula, GS 2023+338 and MAXI J1820+070
DOI: 10.3847/1538-4357/aaf1c9 Bibcode: 2019ApJ...870...92R

Jourdain, Elisabeth; Roques, Jean-Pierre

The Spectrometer on INTEGRAL (SPI) instrument has observed the hard X-ray sky from 20 keV up to a few MeV for more than 15 yr. In this energy domain, the main emitters are compact objects for which SPI provides spectral information of prime interest. Recently, two transient sources reached very unusual flux levels and have been detected up to a fe…

2019 The Astrophysical Journal
INTEGRAL 24
A Search for Gravitationally Lensed Gamma-Ray Bursts in the Data of the Interplanetary Network and Konus-Wind
DOI: 10.3847/1538-4357/aaf645 Bibcode: 2019ApJ...871..121H

Zhang, X.; Hurley, K.; von Kienlin, A. +19 more

We examine a sample of 2301 gamma-ray bursts, detected by Konus-Wind in the triggered mode between 1994 and 2017 and localized by the interplanetary network (IPN), for evidence of gravitational lensing. We utilize all the available gamma-ray burst (GRB) data: time histories, localizations, and energy spectra. We employ common IPN techniques to fin…

2019 The Astrophysical Journal
INTEGRAL 20
The Galactic Bulge Diffuse Emission in Broadband X-Rays with NuSTAR
DOI: 10.3847/1538-4357/ab4590 Bibcode: 2019ApJ...884..153P

Wik, Daniel R.; Krivonos, Roman; Perez, Kerstin

The diffuse hard X-ray emission that fills the Galactic center, bulge, and ridge is believed to arise from unresolved populations of X-ray binary systems. However, the identity of the dominant class of accreting objects in each region remains unclear. Recent studies of Fe line properties and the low-energy (<10 keV) X-ray continuum of the bulge…

2019 The Astrophysical Journal
INTEGRAL 19