Search Results - "Smartt, S. J"
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The ATLAS All-Sky Stellar Reference Catalog
Published in The Astrophysical journal (10-11-2018)“…The Asteroid Terrestrial-impact Last Alert System (ATLAS) observes most of the sky every night in search of dangerous asteroids. Its data are also used to…”
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The death of massive stars – I. Observational constraints on the progenitors of Type II-P supernovae
Published in Monthly notices of the Royal Astronomical Society (21-05-2009)“…We present the results of a 10.5-yr, volume-limited (28-Mpc) search for supernova (SN) progenitor stars. In doing so we compile all SNe discovered within this…”
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Nebular spectra of pair-instability supernovae
Published in Monthly notices of the Royal Astronomical Society (21-01-2016)“…If very massive stars (M ≳ 100 M⊙) can form and avoid too strong mass-loss during their evolution, they are predicted to explode as pair-instability supernovae…”
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AT2018kzr: the merger of an oxygen–neon white dwarf and a neutron star or black hole
Published in Monthly notices of the Royal Astronomical Society (01-09-2020)“…ABSTRACT We present detailed spectroscopic analysis of the extraordinarily fast-evolving transient AT2018kzr. The transient’s observed light curve showed a…”
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Design and Operation of the ATLAS Transient Science Server
Published in Publications of the Astronomical Society of the Pacific (01-08-2020)“…The Asteroid Terrestrial impact Last Alert System (ATLAS) system consists of two 0.5 m Schmidt telescopes with cameras covering 29 square degrees at plate…”
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Constraints on the presence of platinum and gold in the spectra of the kilonova AT2017gfo
Published in Monthly notices of the Royal Astronomical Society (01-09-2021)“…ABSTRACT Binary neutron star mergers are thought to be one of the dominant sites of production for rapid neutron capture elements, including platinum and gold…”
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The nebular spectra of SN 2012aw and constraints on stellar nucleosynthesis from oxygen emission lines
Published in Monthly notices of the Royal Astronomical Society (21-04-2014)“…We present nebular-phase optical and near-infrared spectroscopy of the Type IIP supernova SN 2012aw combined with non-local thermodynamic equilibrium radiative…”
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LONG-DURATION SUPERLUMINOUS SUPERNOVAE AT LATE TIMES
Published in The Astrophysical journal (20-01-2017)“…ABSTRACT Nebular-phase observations and spectral models of Type Ic superluminous supernovae (SLSNe) are presented. LSQ14an and SN 2015bn both display late-time…”
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The host galaxy and late-time evolution of the superluminous supernova PTF12dam
Published in Monthly notices of the Royal Astronomical Society (11-09-2015)“…Superluminous supernovae (SLSNe) of Type Ic have a tendency to occur in faint host galaxies which are likely to have low mass and low metallicity. PTF12dam is…”
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The tidal disruption event AT2017eqx: spectroscopic evolution from hydrogen rich to poor suggests an atmosphere and outflow
Published in Monthly notices of the Royal Astronomical Society (11-09-2019)“…ABSTRACT We present and analyse a new tidal disruption event (TDE), AT2017eqx at redshift z = 0.1089, discovered by Pan-STARRS and ATLAS. The position of the…”
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Constraining the physical properties of Type II-Plateau supernovae using nebular phase spectra
Published in Monthly notices of the Royal Astronomical Society (01-03-2012)“…We present a study of the nebular phase spectra of a sample of Type II-Plateau supernovae with identified progenitors or restrictive limits. The evolution of…”
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The VLT FLAMES Survey of Massive Stars: Rotation and Nitrogen Enrichment as the Key to Understanding Massive Star Evolution
Published in The Astrophysical journal (20-03-2008)“…Rotation has become an important element in evolutionary models of massive stars, specifically via the prediction of rotational mixing. Here we study a sample…”
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SN 2009md: another faint supernova from a low-mass progenitor
Published in Monthly notices of the Royal Astronomical Society (01-10-2011)“…We present adaptive optics imaging of the core-collapse supernova (SN) 2009md, which we use together with archival Hubble Space Telescope data to identify a…”
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Machine learning for transient discovery in Pan-STARRS1 difference imaging
Published in Monthly notices of the Royal Astronomical Society (01-05-2015)“…Efficient identification and follow-up of astronomical transients is hindered by the need for humans to manually select promising candidates from data streams…”
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The Luminous Type Ia Supernova 2022ilv and Its Early Excess Emission
Published in Astrophysical journal. Letters (01-02-2023)“…Abstract We present observations and analysis of the hostless and luminous Type Ia supernova 2022ilv, illustrating it is part of the 2003fg-like family, often…”
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Early observations of the nearby Type Ia supernova SN 2015F
Published in Monthly notices of the Royal Astronomical Society (01-02-2017)“…We present photometry and time series spectroscopy of the nearby Type Ia supernova (SN Ia) SN 2015F over -16 d to +80 d relative to maximum light, obtained as…”
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SN 2023emq: A Flash-ionized Ibn Supernova with Possible C iii Emission
Published in Astrophysical journal. Letters (01-12-2023)“…Abstract SN 2023emq is a fast-evolving transient initially classified as a rare Type Icn supernova (SN), interacting with a H- and He-free circumstellar medium…”
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Massive stars exploding in a He-rich circumstellar medium – IV. Transitional Type Ibn supernovae
Published in Monthly notices of the Royal Astronomical Society (11-05-2015)“…We present ultraviolet, optical and near-infrared data of the Type Ibn supernovae (SNe) 2010al and 2011hw. SN 2010al reaches an absolute magnitude at peak of M…”
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SN 2009jf: a slow-evolving stripped-envelope core-collapse supernova
Published in Monthly notices of the Royal Astronomical Society (01-10-2011)“…We present an extensive set of photometric and spectroscopic data for SN 2009jf, a nearby Type Ib supernova (SN), spanning from ∼20 d before B-band maximum to…”
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A low-energy core-collapse supernova without a hydrogen envelope
Published in Nature (04-06-2009)“…The final fate of massive stars depends on many factors. Theory suggests that some with initial masses greater than 25 to 30 solar masses end up as Wolf-Rayet…”
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