Search Results - "Fox, O D"
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The X-ray counterpart to the gravitational-wave event GW170817
Published in Nature (London) (02-11-2017)“…Detection of X-ray emission at a location coincident with the kilonova transient of the gravitational-wave event GW170817 provides the missing observational…”
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Delayed Circumstellar Interaction for Type Ia SN 2015cp Revealed by an HST Ultraviolet Imaging Survey
Published in The Astrophysical journal (20-01-2019)“…The nature and role of the binary companion of carbon-oxygen white dwarf stars that explode as Type Ia supernovae (SNe Ia) are not yet fully understood. Past…”
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3
Predicting the Presence of Companions for Stripped-envelope Supernovae: The Case of the Broad-lined Type Ic SN 2002ap
Published in The Astrophysical journal (20-06-2017)“…Many young, massive stars are found in close binaries. Using population synthesis simulations we predict the likelihood of a companion star being present when…”
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Extensive HST ultraviolet spectra and multiwavelength observations of SN 2014J in M82 indicate reddening and circumstellar scattering by typical dust
Published in Monthly notices of the Royal Astronomical Society (01-10-2014)“…SN 2014J in M82 is the closest detected Type Ia supernova (SN Ia) in at least 28 yr and perhaps in 410 yr. Despite its small distance of 3.3 Mpc, SN 2014J is…”
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EXTENSIVE SPECTROSCOPY AND PHOTOMETRY OF THE TYPE IIP SUPERNOVA 2013ej
Published in The Astrophysical journal (01-05-2016)“…ABSTRACT We present extensive optical (UBV RI, , and open CCD) and near-infrared (ZY JH) photometry for the very nearby Type IIP SN 2013ej extending from +1 to…”
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500 days of SN 2013dy: spectra and photometry from the ultraviolet to the infrared
Published in Monthly notices of the Royal Astronomical Society (01-10-2015)“…SN 2013dy is a Type Ia supernova (SN Ia) for which we have compiled an extraordinary data set spanning from 0.1 to ∼ 500 d after explosion. We present 10…”
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JWST NIRSpec Observations of Supernova 1987A—From the Inner Ejecta to the Reverse Shock
Published in Astrophysical journal. Letters (01-06-2023)“…Abstract We present initial results from JWST NIRSpec integral field unit observations of the nearby supernova SN 1987A. The observations provide the first…”
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A long-lived neutron star merger remnant in GW170817: constraints and clues from X-ray observations
Published in Monthly notices of the Royal Astronomical Society (21-02-2019)Get full text
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9
Discovery of an Apparent Red, High-velocity Type Ia Supernova at z = 2.9 with JWST
Published in Astrophysical journal. Letters (01-08-2024)“…Abstract We present the James Webb Space Telescope (JWST) discovery of SN 2023adsy, a transient object located in a host galaxy JADES-GS+53.13485−27.82088 with…”
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Discovery of a Relativistic Stripped-envelope Type Ic-BL Supernova at z = 2.83 with JWST
Published in Astrophysical journal. Letters (01-09-2024)“…Abstract We present James Webb Space Telescope (JWST) NIRCam and NIRSpec observations of a Type Ic supernova (SN Ic) and its host galaxy…”
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A detailed study of the optical attenuation of gamma-ray bursts in the Swift era
Published in Monthly notices of the Royal Astronomical Society (21-05-2015)“…We present optical and near-infrared (NIR) photometry of 28 gamma-ray bursts (GRBs) detected by the Swift satellite and rapidly observed by the Reionization…”
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The Foundation Supernova Survey: motivation, design, implementation, and first data release
Published in Monthly notices of the Royal Astronomical Society (01-03-2018)“…Abstract The Foundation Supernova Survey aims to provide a large, high-fidelity, homogeneous, and precisely calibrated low-redshift Type Ia supernova (SN Ia)…”
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Near-infrared Supernova Ia Distances: Host Galaxy Extinction and Mass-step Corrections Revisited
Published in The Astrophysical journal (01-12-2021)“…Abstract We present optical and near-infrared (NIR, Y - , J - , H- band) observations of 42 Type Ia supernovae (SNe Ia) discovered by the untargeted…”
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14
Confined dense circumstellar material surrounding a regular type II supernova
Published in Nature physics (01-05-2017)“…With the advent of new wide-field, high-cadence optical transient surveys, our understanding of the diversity of core-collapse supernovae has grown…”
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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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Ultraviolet diversity of Type Ia Supernovae
Published in Monthly notices of the Royal Astronomical Society (11-09-2016)“…Ultraviolet (UV) observations of Type Ia supernovae (SNe Ia) probe the outermost layers of the explosion, and UV spectra of SNe Ia are expected to be extremely…”
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Observations of the planetary nebula SMP LMC 058 with the JWST MIRI medium resolution spectrometer
Published in Monthly notices of the Royal Astronomical Society (01-08-2023)“…ABSTRACT During the commissioning of JWST, the medium-resolution spectrometer (MRS) on the mid-infrared instrument (MIRI) observed the planetary nebula SMP LMC…”
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18
PTF11kx: A Type Ia Supernova with Hydrogen Emission Persisting after 3.5 Years
Published in The Astrophysical journal (10-07-2017)“…The optical transient PTF11kx exhibited both the characteristic spectral features of Type Ia supernovae (SNe Ia) and the signature of ejecta interacting with…”
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SALT3-NIR: Taking the Open-source Type Ia Supernova Model to Longer Wavelengths for Next-generation Cosmological Measurements
Published in The Astrophysical journal (01-11-2022)“…Abstract A large fraction of Type Ia supernova (SN Ia) observations over the next decade will be in the near-infrared (NIR), at wavelengths beyond the reach of…”
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Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987A
Published in Science (American Association for the Advancement of Science) (23-02-2024)“…The nearby Supernova 1987A was accompanied by a burst of neutrino emission, which indicates that a compact object (a neutron star or black hole) was formed in…”
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