Search Results - "Siebert, M R"
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Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source
Published in Science (American Association for the Advancement of Science) (22-12-2017)“…On 17 August 2017, the Laser Interferometer Gravitational-Wave Observatory (LIGO) and the Virgo interferometer detected gravitational waves (GWs) emanating…”
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Discovery and follow-up of ASASSN-19dj: an X-ray and UV luminous TDE in an extreme post-starburst galaxy
Published in Monthly notices of the Royal Astronomical Society (01-01-2021)“…ABSTRACT We present observations of ASASSN-19dj, a nearby tidal disruption event (TDE) discovered in the post-starburst galaxy KUG 0810+227 by the All-Sky…”
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SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances
Published in The Astrophysical journal (01-12-2021)“…Abstract A spectral-energy distribution (SED) model for Type Ia supernovae (SNe Ia) is a critical tool for measuring precise and accurate distances across a…”
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A Spectroscopic Model of the Type Ia Supernova–Host-galaxy Mass Correlation from SALT3
Published in The Astrophysical journal (01-07-2023)“…Abstract The unknown cause of the correlation between Type Ia supernova (SN Ia) Hubble residuals and their host-galaxy masses (the “mass step”) may bias…”
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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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Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis
Published in Science (American Association for the Advancement of Science) (22-12-2017)“…On 17 August 2017, gravitational waves (GWs) were detected from a binary neutron star merger, GW170817, along with a coincident short gamma-ray burst, GRB…”
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Electromagnetic evidence that SSS17a is the result of a binary neutron star merger
Published in Science (American Association for the Advancement of Science) (22-12-2017)“…Eleven hours after the detection of gravitational wave source GW170817 by the Laser Interferometer Gravitational-Wave Observatory and Virgo Interferometers, an…”
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Should Type Ia Supernova Distances Be Corrected for Their Local Environments?
Published in The Astrophysical journal (10-11-2018)“…Recent analyses suggest that distance residuals measured from Type Ia supernovae (SNe Ia) are correlated with local host galaxy properties within a few…”
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Early spectra of the gravitational wave source GW170817: Evolution of a neutron star merger
Published in Science (American Association for the Advancement of Science) (22-12-2017)“…On 17 August 2017, Swope Supernova Survey 2017a (SSS17a) was discovered as the optical counterpart of the binary neutron star gravitational wave event…”
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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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A possible distance bias for type Ia supernovae with different ejecta velocities
Published in Monthly notices of the Royal Astronomical Society (21-04-2020)“…ABSTRACT After correcting for their light-curve shape and colour, Type Ia supernovae (SNe Ia) are precise cosmological distance indicators. However, there…”
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Investigating the diversity of Type Ia supernova spectra with the open-source relational data base kaepora
Published in Monthly notices of the Royal Astronomical Society (01-07-2019)“…Abstract We present a public, open-source relational data base (we name kaepora) containing a sample of 4975 spectra of 777 Type Ia supernovae (SNe Ia). Since…”
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The Foundation Supernova Survey: Measuring Cosmological Parameters with Supernovae from a Single Telescope
Published in The Astrophysical journal (10-08-2019)“…Measurements of the dark energy equation-of-state parameter, w, have been limited by uncertainty in the selection effects and photometric calibration of z <…”
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The Early Phases of Supernova 2020pni: Shock Ionization of the Nitrogen-enriched Circumstellar Material
Published in The Astrophysical journal (01-02-2022)“…Abstract We present multiwavelength observations of the Type II SN 2020pni. Classified at ∼1.3 days after explosion, the object showed narrow (FWHM intensity…”
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Cosmological Results from the RAISIN Survey: Using Type Ia Supernovae in the Near Infrared as a Novel Path to Measure the Dark Energy Equation of State
Published in The Astrophysical journal (01-07-2022)“…Abstract Type Ia supernovae (SNe Ia) are more precise standardizable candles when measured in the near-infrared (NIR) than in the optical. With this…”
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YSE-PZ: A Transient Survey Management Platform that Empowers the Human-in-the-loop
Published in Publications of the Astronomical Society of the Pacific (01-06-2023)“…Abstract The modern study of astrophysical transients has been transformed by an exponentially growing volume of data. Within the last decade, the transient…”
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Discovery of Highly Blueshifted Broad Balmer and Metastable Helium Absorption Lines in a Tidal Disruption Event
Published in The Astrophysical journal (10-07-2019)“…We report the discovery of nonstellar hydrogen Balmer and metastable helium absorption lines accompanying a transient, high-velocity (0.05c) broad absorption…”
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To TDE or not to TDE: the luminous transient ASASSN-18jd with TDE-like and AGN-like qualities
Published in Monthly notices of the Royal Astronomical Society (11-05-2020)“…ABSTRACT We present the discovery of ASASSN-18jd (AT 2018bcb), a luminous optical/ultraviolet(UV)/X-ray transient located in the nucleus of the galaxy…”
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Progenitor and close-in circumstellar medium of type II supernova 2020fqv from high-cadence photometry and ultra-rapid UV spectroscopy
Published in Monthly notices of the Royal Astronomical Society (30-03-2022)“…ABSTRACT We present observations of SN 2020fqv, a Virgo-cluster type II core-collapse supernova (CCSN) with a high temporal resolution light curve from the…”
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