Search Results - "Hosseinzadeh, Griffin"
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Bumpy Declining Light Curves Are Common in Hydrogen-poor Superluminous Supernovae
Published in The Astrophysical journal (01-07-2022)“…Abstract Recent work has revealed that the light curves of hydrogen-poor (Type I) superluminous supernovae (SLSNe), thought to be powered by magnetar central…”
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2
Luminous Supernovae: Unveiling a Population between Superluminous and Normal Core-collapse Supernovae
Published in The Astrophysical journal (01-12-2022)“…Abstract Stripped-envelope core-collapse supernovae can be divided into two broad classes: the common Type Ib/c supernovae (SNe Ib/c), powered by the…”
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3
Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger
Published in Nature (London) (02-11-2017)“…Optical to near-infrared observations of a transient coincident with the detection of the gravitational-wave signature of a binary neutron-star merger and a…”
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FLEET: A Redshift-agnostic Machine Learning Pipeline to Rapidly Identify Hydrogen-poor Superluminous Supernovae
Published in The Astrophysical journal (01-11-2020)“…Over the past decade wide-field optical time-domain surveys have increased the discovery rate of transients to the point that 10% are being spectroscopically…”
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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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6
High-resolution Spectroscopy of SN 2023ixf’s First Week: Engulfing the Asymmetric Circumstellar Material
Published in The Astrophysical journal (01-10-2023)“…Abstract We present a series of high-resolution echelle spectra of SN 2023ixf in M101, obtained nightly during the first week or so after discovery using PEPSI…”
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Photometrically Classified Superluminous Supernovae from the Pan-STARRS1 Medium Deep Survey: A Case Study for Science with Machine-learning-based Classification
Published in The Astrophysical journal (01-09-2022)“…Abstract With the upcoming Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), it is expected that only ∼0.1% of all transients will be…”
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1ES 1927+654: An AGN Caught Changing Look on a Timescale of Months
Published in The Astrophysical journal (20-09-2019)“…We study the sudden optical and ultraviolet (UV) brightening of 1ES 1927+654, which until now was known as a narrow-line active galactic nucleus (AGN). 1ES…”
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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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Late-time Hubble Space Telescope Observations of a Hydrogen-poor Superluminous Supernova Reveal the Power-law Decline of a Magnetar Central Engine
Published in The Astrophysical journal (01-11-2021)“…Abstract The light-curve diversity of hydrogen-poor superluminous supernovae (SLSNe) has kept open the possibility that multiple power sources account for the…”
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SuperRAENN: A Semisupervised Supernova Photometric Classification Pipeline Trained on Pan-STARRS1 Medium-Deep Survey Supernovae
Published in The Astrophysical journal (01-12-2020)“…Automated classification of supernovae (SNe) based on optical photometric light-curve information is essential in the upcoming era of wide-field time domain…”
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12
Optical Observations and Modeling of the Superluminous Supernova 2018lfe
Published in The Astrophysical journal (01-05-2022)“…Abstract We present optical imaging and spectroscopy of SN 2018lfe, which we classify as a Type I superluminous supernova (SLSN-I) at a redshift of z = 0.3501…”
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SN 2019ehk: A Double-peaked Ca-rich Transient with Luminous X-Ray Emission and Shock-ionized Spectral Features
Published in The Astrophysical journal (01-08-2020)“…We present panchromatic observations and modeling of the Calcium-rich supernova (SN) 2019ehk in the star-forming galaxy M100 (d 16.2 Mpc) starting 10 hr after…”
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14
Energetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star
Published in Nature (London) (09-11-2017)“…Observations of an event (several energetic eruptions leading to a terminal explosion that is surprisingly hydrogen-rich) with the spectrum of a supernova do…”
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Still Brighter than Pre-explosion, SN 2012Z Did Not Disappear: Comparing Hubble Space Telescope Observations a Decade Apart
Published in The Astrophysical journal (01-02-2022)“…Abstract Type Iax supernovae (SNe Iax) represent the largest class of peculiar white dwarf supernovae. The type Iax SN 2012Z in NGC 1309 is the only white…”
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Early Spectroscopy and Dense Circumstellar Medium Interaction in SN 2023ixf
Published in Astrophysical journal. Letters (01-10-2023)“…Abstract We present the optical spectroscopic evolution of SN 2023ixf seen in subnight cadence spectra from 1.18 to 15 days after explosion. We identify…”
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Type Ibn Supernovae Show Photometric Homogeneity and Spectral Diversity at Maximum Light
Published in The Astrophysical journal (20-02-2017)“…Type Ibn supernovae (SNe) are a small yet intriguing class of explosions whose spectra are characterized by low-velocity helium emission lines with little to…”
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Short-lived Circumstellar Interaction in the Low-luminosity Type IIP SN 2016bkv
Published in The Astrophysical journal (01-07-2018)“…While interaction with circumstellar material is known to play an important role in Type IIn supernovae (SNe), analyses of the more common SNe IIP and IIL have…”
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SN 2016iet: The Pulsational or Pair Instability Explosion of a Low-metallicity Massive CO Core Embedded in a Dense Hydrogen-poor Circumstellar Medium
Published in The Astrophysical journal (20-08-2019)“…We present optical photometry and spectroscopy of SN 2016iet (=Gaia16bvd=PS17brq), an unprecedented Type I supernova (SN I) at z = 0.0676 with no obvious…”
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Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants
Published in The Astrophysical journal (01-05-2021)“…Abstract The diversity of Type II supernovae (SNe II) is thought to be driven mainly by differences in their progenitor’s hydrogen-rich (H-rich) envelope mass,…”
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