Search Results - "Berger, Edo"
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Short-Duration Gamma-Ray Bursts
Published in Annual review of astronomy and astrophysics (01-01-2014)“…Gamma-ray bursts (GRBs) display a bimodal duration distribution with a separation between the short- and long-duration bursts at about 2 s. The progenitors of…”
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Millisecond Magnetar Birth Connects FRB 121102 to Superluminous Supernovae and Long-duration Gamma-Ray Bursts
Published in The Astrophysical journal (20-05-2017)“…Subarcsecond localization of the repeating fast radio burst FRB 121102 revealed its coincidence with a dwarf host galaxy and a steady ("quiescent") nonthermal…”
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3
Fast Radio Bursts from Magnetars Born in Binary Neutron Star Mergers and Accretion Induced Collapse
Published in The Astrophysical journal (01-12-2019)“…Recently born magnetars are promising candidates for the engines powering fast radio bursts (FRBs). The focus thus far has been placed on millisecond magnetars…”
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THE OFFSET AND HOST LIGHT DISTRIBUTIONS OF LONG GAMMA-RAY BURSTS: A NEW VIEW FROM HST OBSERVATIONS OF SWIFT BURSTS
Published in The Astrophysical journal (01-02-2016)“…ABSTRACT We present the results of an extensive Hubble Space Telescope imaging study of 105, mostly Swift, long-duration gamma-ray bursts (LGRBs) spanning ,…”
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Detection and parameter estimation of gravitational waves from binary neutron-star mergers in real LIGO data using deep learning
Published in Physics letters. B (10-04-2021)“…One of the key challenges of real-time detection and parameter estimation of gravitational waves from compact binary mergers is the computational cost of…”
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Superluminous Supernovae in LSST: Rates, Detection Metrics, and Light-curve Modeling
Published in The Astrophysical journal (20-12-2018)“…We explore and demonstrate the capabilities of the upcoming Large Synoptic Survey Telescope (LSST) to study Type I superluminous supernovae (SLSNe). We fit the…”
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Does GW190425 Require an Alternative Formation Pathway than a Fast-merging Channel?
Published in The Astrophysical journal (01-09-2020)“…The LIGO/Virgo Scientific Collaboration (LVC) recently announced the detection of a compact object binary merger, GW190425, with a total mass of M and…”
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Impact of massive binary star and cosmic evolution on gravitational wave observations I: black hole–neutron star mergers
Published in Monthly notices of the Royal Astronomical Society (01-12-2021)“…ABSTRACT Mergers of black hole–neutron star (BHNS) binaries have now been observed by gravitational wave (GW) detectors with the recent announcement of…”
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Deep learning detection and classification of gravitational waves from neutron star-black hole mergers
Published in Physics letters. B (10-05-2023)“…The Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo Interferometer Collaborations have now detected all three classes of compact binary…”
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Nebular-phase Spectra of Superluminous Supernovae: Physical Insights from Observational and Statistical Properties
Published in The Astrophysical journal (20-01-2019)“…We study the spectroscopic evolution of superluminous supernovae (SLSNe) later than 100 days after maximum light. We present new data for Gaia16apd and SN…”
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Theoretical Models of Optical Transients. I. A Broad Exploration of the Duration-Luminosity Phase Space
Published in The Astrophysical journal (01-11-2017)“…The duration-luminosity phase space (DLPS) of optical transients is used, mostly heuristically, to compare various classes of transient events, to explore the…”
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Unveiling the engines of fast radio bursts, superluminous supernovae, and gamma-ray bursts
Published in Monthly notices of the Royal Astronomical Society (01-12-2018)Get full text
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The Pre-explosion Mass Distribution of Hydrogen-poor Superluminous Supernova Progenitors and New Evidence for a Mass-Spin Correlation
Published in The Astrophysical journal (01-07-2020)“…Despite indications that superluminous supernovae (SLSNe) originate from massive progenitors, the lack of a uniformly analyzed statistical sample has so far…”
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Magnetar Models of Superluminous Supernovae from the Dark Energy Survey: Exploring Redshift Evolution
Published in The Astrophysical journal (01-11-2021)“…Abstract Superluminous supernovae (SLSNe) are luminous transients that can be detected to high redshifts with upcoming optical time-domain surveys such as the…”
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EXTRAGALACTIC SYNCHROTRON TRANSIENTS IN THE ERA OF WIDE-FIELD RADIO SURVEYS. I. DETECTION RATES AND LIGHT CURVE CHARACTERISTICS
Published in The Astrophysical journal (20-06-2015)“…ABSTRACT The impending era of wide-field radio surveys has the potential to revolutionize our understanding of astrophysical transients. Here we evaluate the…”
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The Luminous and Double-peaked Type Ic Supernova 2019stc: Evidence for Multiple Energy Sources
Published in The Astrophysical journal (01-06-2021)“…Abstract We present optical photometry and spectroscopy of SN 2019stc (=ZTF19acbonaa), an unusual Type Ic supernova (SN Ic) at a redshift of z = 0.117. SN…”
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Investigating the Cosmological Rate of Compact Object Mergers from Isolated Massive Binary Stars
Published in The Astrophysical journal (01-11-2024)“…Abstract Gravitational-wave (GW) detectors are observing compact object mergers from increasingly far distances, revealing the redshift evolution of the binary…”
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The Binary Black Hole Merger Rate Deviates from the Cosmic Star Formation Rate: A Tug of War between Metallicity and Delay Times
Published in The Astrophysical journal (01-11-2024)“…Abstract Gravitational-wave detectors are now making it possible to investigate how the merger rate of binary black holes (BBHs) evolves with redshift. In this…”
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An Extensive Hubble Space Telescope Study of the Offset and Host Light Distributions of Type I Superluminous Supernovae
Published in The Astrophysical journal (01-02-2024)“…Abstract We present an extensive Hubble Space Telescope rest-frame UV imaging study of the locations of Type I superluminous supernovae (SLSNe) within their…”
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UNBOUND DEBRIS STREAMS AND REMNANTS RESULTING FROM THE TIDAL DISRUPTIONS OF STARS BY SUPERMASSIVE BLACK HOLES
Published in The Astrophysical journal (01-05-2016)“…ABSTRACT The kinetic energy of a star in orbit about a supermassive black hole is a significant fraction of its rest mass energy when its periapse is…”
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