Search Results - "Lunnan, R."
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HOST-GALAXY PROPERTIES OF 32 LOW-REDSHIFT SUPERLUMINOUS SUPERNOVAE FROM THE PALOMAR TRANSIENT FACTORY
Published in The Astrophysical journal (10-10-2016)“…ABSTRACT We present ultraviolet through near-infrared photometry and spectroscopy of the host galaxies of all superluminous supernovae (SLSNe) discovered by…”
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Far-ultraviolet to Near-infrared Spectroscopy of a Nearby Hydrogen-poor Superluminous Supernova Gaia16apd
Published in The Astrophysical journal (01-05-2017)“…We report the first maximum-light far-ultraviolet (FUV) to near-infrared (NIR) spectra (1000 − 1.62 m, rest) of a hydrogen-poor superluminous supernova,…”
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SHORT GRB 130603B: DISCOVERY OF A JET BREAK IN THE OPTICAL AND RADIO AFTERGLOWS, AND A MYSTERIOUS LATE-TIME X-RAY EXCESS
Published in The Astrophysical journal (10-01-2014)“…We present radio, optical/NIR, and X-ray observations of the afterglow of the short-duration Swift and Konus-Wind GRB 130603B, and uncover a break in the radio…”
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4
Revisiting Optical Tidal Disruption Events with iPTF16axa
Published in The Astrophysical journal (10-06-2017)“…We report the discovery by the intermediate Palomar Transient Factory (iPTF) of a candidate tidal disruption event (TDE) iPTF16axa at z = 0.108 and present its…”
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Results from a Systematic Survey of X-Ray Emission from Hydrogen-poor Superluminous SNe
Published in The Astrophysical journal (01-09-2018)“…We present the results from a sensitive X-ray survey of 26 nearby hydrogen-poor superluminous supernovae (SLSNe-I) with Swift, Chandra, and XMM. This data set…”
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Supernova Photometric Classification Pipelines Trained on Spectroscopically Classified Supernovae from the Pan-STARRS1 Medium-deep Survey
Published in The Astrophysical journal (10-10-2019)“…Photometric classification of supernovae (SNe) is imperative as recent and upcoming optical time-domain surveys, such as the Large Synoptic Survey Telescope…”
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THE AFTERGLOW AND EARLY-TYPE HOST GALAXY OF THE SHORT GRB 150101B AT z = 0.1343
Published in The Astrophysical journal (20-12-2016)“…ABSTRACT We present the discovery of the X-ray and optical afterglows of the short-duration GRB 150101B, pinpointing the event to an early-type host galaxy at…”
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X-Rays from the Location of the Double-humped Transient ASASSN-15lh
Published in The Astrophysical journal (10-02-2017)“…We present the detection of persistent soft X-ray radiation with -1042 erg s-1 at the location of the extremely luminous, double-humped transient ASASSN-15lh…”
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Far-UV HST Spectroscopy of an Unusual Hydrogen-poor Superluminous Supernova: SN2017egm
Published in The Astrophysical journal (10-05-2018)“…SN2017egm is the closest (z = 0.03) H-poor superluminous supernova (SLSN-I) detected to date, and a rare example of an SLSN-I in a massive, metal-rich galaxy…”
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Two New Calcium-rich Gap Transients in Group and Cluster Environments
Published in The Astrophysical journal (10-02-2017)“…We present the Palomar Transient Factory discoveries and the photometric and spectroscopic observations of PTF11kmb and PTF12bho. We show that both transients…”
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iPTF 16asu: A Luminous, Rapidly Evolving, and High-velocity Supernova
Published in The Astrophysical journal (20-12-2017)“…Wide-field surveys are discovering a growing number of rare transients whose physical origin is not yet well understood. Here we present optical and UV data…”
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The Hydrogen-poor Superluminous Supernovae from the Zwicky Transient Facility Phase I Survey. II. Light-curve Modeling and Characterization of Undulations
Published in The Astrophysical journal (01-01-2023)“…Abstract We present analysis of the light curves (LCs) of 77 hydrogen-poor superluminous supernovae (SLSNe I) discovered during the Zwicky Transient Facility…”
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HYDROGEN-POOR SUPERLUMINOUS SUPERNOVAE AND LONG-DURATION GAMMA-RAY BURSTS HAVE SIMILAR HOST GALAXIES
Published in The Astrophysical journal (01-06-2014)“…We present optical spectroscopy and optical/near-IR photometry of 31 host galaxies of hydrogen-poor superluminous supernovae (SLSNe), including 15 events from…”
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A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary
Published in Science (American Association for the Advancement of Science) (12-10-2018)“…Compact neutron star binary systems are produced from binary massive stars through stellar evolution involving up to two supernova explosions. The final stages…”
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iPTF16fnl: A Faint and Fast Tidal Disruption Event in an E+A Galaxy
Published in The Astrophysical journal (20-07-2017)“…We present ground-based and Swift observations of iPTF16fnl, a likely tidal disruption event (TDE) discovered by the intermediate Palomar Transient Factory…”
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Hydrogen-poor Superluminous Supernovae with Late-time Hα Emission: Three Events From the Intermediate Palomar Transient Factory
Published in The Astrophysical journal (10-10-2017)“…Abstract We present observations of two new hydrogen-poor superluminous supernovae (SLSN-I), iPTF15esb and iPTF16bad, showing late-time H α emission with line…”
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A REVERSE SHOCK IN GRB 130427A
Published in The Astrophysical journal (20-10-2013)“…We present extensive radio and millimeter observations of the unusually bright GRB 130427A at z = 0.340, spanning 0.67-12 days after the burst. We combine…”
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TOWARD CHARACTERIZATION OF THE TYPE IIP SUPERNOVA PROGENITOR POPULATION: A STATISTICAL SAMPLE OF LIGHT CURVES FROM Pan-STARRS1
Published in The Astrophysical journal (01-02-2015)“…In recent years, wide-field sky surveys providing deep multiband imaging have presented a new path for indirectly characterizing the progenitor populations of…”
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An Empirical Study of Contamination in Deep, Rapid, and Wide-field Optical Follow-up of Gravitational Wave Events
Published in The Astrophysical journal (01-05-2018)“…We present an empirical study of contamination in wide-field optical follow-up searches of gravitational wave sources from Advanced LIGO/Virgo using dedicated…”
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Early Observations of the Type Ia Supernova iPTF 16abc: A Case of Interaction with Nearby, Unbound Material and/or Strong Ejecta Mixing
Published in The Astrophysical journal (10-01-2018)“…Early observations of Type Ia supernovae (SNe Ia) provide a unique probe of their progenitor systems and explosion physics. Here we report the intermediate…”
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