Search Results - "Horst, Chuck"
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M31N 2008-12a-THE REMARKABLE RECURRENT NOVA IN M31: PANCHROMATIC OBSERVATIONS OF THE 2015 ERUPTION
Published in The Astrophysical journal (20-12-2016)“…ABSTRACT The Andromeda Galaxy recurrent nova M31N 2008-12a had been observed in eruption 10 times, including yearly eruptions from 2008 to 2014. With a…”
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Breaking the Habit: The Peculiar 2016 Eruption of the Unique Recurrent Nova M31N 2008-12a
Published in The Astrophysical journal (10-04-2018)“…Since its discovery in 2008, the Andromeda galaxy nova M31N 2008-12a has been observed in eruption every single year. This unprecedented frequency indicates an…”
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What Does the Geometry of the Hβ BLR Depend On?
Published in The Astrophysical journal (01-05-2023)“…We combine our dynamical modeling black-hole mass measurements from the Lick AGN Monitoring Project 2016 sample with measured cross-correlation time lags and…”
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PTF11iqb: cool supergiant mass-loss that bridges the gap between Type IIn and normal supernovae
Published in Monthly notices of the Royal Astronomical Society (11-05-2015)“…The supernova (SN) PTF11iqb was initially classified as a Type IIn event caught very early after explosion. It showed narrow Wolf–Rayet (WR) spectral features…”
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Superluminous supernovae at redshifts of 2.05 and 3.90
Published in Nature (London) (08-11-2012)“…The identification of two superluminous supernovae at redshifts of 2.05 and 3.90 extends the present technological redshift limit on supernova detection and…”
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TYPE II SUPERNOVA ENERGETICS AND COMPARISON OF LIGHT CURVES TO SHOCK-COOLING MODELS
Published in The Astrophysical journal (20-03-2016)“…ABSTRACT During the first few days after explosion, Type II supernovae (SNe) are dominated by relatively simple physics. Theoretical predictions regarding…”
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Photometric Observations of the 2017 Outburst of Recurrent Nova M31N 2007-10b
Published 23-10-2018“…Research Notes of the American Astronomical Society, 2, 190 M31 is an ideal laboratory for observing and studying recurrent novae. To date, there have been 18…”
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The Lick AGN Monitoring Project 2016: Dynamical Modeling of Velocity-resolved Hβ Lags in Luminous Seyfert Galaxies
Published in The Astrophysical journal (01-05-2022)“…We have modeled the velocity-resolved reverberation response of the H β broad emission line in nine Seyfert 1 galaxies from the Lick Active Galactic Nucleus…”
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The Lick AGN Monitoring Project 2016: Velocity-resolved Hβ Lags in Luminous Seyfert Galaxies
Published in The Astrophysical journal (01-01-2022)“…We carried out spectroscopic monitoring of 21 low-redshift Seyfert 1 galaxies using the Kast double spectrograph on the 3 m Shane telescope at Lick Observatory…”
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REVERBERATION MAPPING OF THE KEPLER FIELD AGN KA1858+4850
Published in The Astrophysical journal (01-11-2014)“…KA1858+4850 is a narrow-line Seyfert 1 galaxy at redshift 0.078 and is among the brightest active galaxies monitored by the Kepler mission. We have carried out…”
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Breaking the habit - the peculiar 2016 eruption of the unique recurrent nova M31N 2008-12a
Published 01-03-2018“…Since its discovery in 2008, the Andromeda galaxy nova M31N 2008-12a has been observed in eruption every single year. This unprecedented frequency indicates an…”
Get full text
Journal Article -
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PTF11iqb: Cool supergiant mass loss that bridges the gap between Type IIn and normal supernovae
Published 12-01-2015“…PTF11iqb was initially classified as a TypeIIn event caught very early after explosion. It showed narrow Wolf-Rayet (WR) spectral features on day 2, but the…”
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Journal Article -
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M31N 2008-12a - the remarkable recurrent nova in M31: Pan-chromatic observations of the 2015 eruption
Published 29-08-2016“…The Andromeda Galaxy recurrent nova M31N 2008-12a had been observed in eruption ten times, including yearly eruptions from 2008-2014. With a measured…”
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Journal Article -
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Type II supernova energetics and comparison of light curves to shock-cooling models
Published 30-11-2015“…During the first few days after explosion, Type II supernovae (SNe) are dominated by relatively simple physics. Theoretical predictions regarding early-time SN…”
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Reverberation Mapping of the Kepler-Field AGN KA1858+4850
Published 29-08-2014“…2014ApJ...795...38P KA1858+4850 is a narrow-line Seyfert 1 galaxy at redshift 0.078 and is among the brightest active galaxies monitored by the Kepler mission…”
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Discovery and Early Multi-Wavelength Measurements of the Energetic Type Ic Supernova PTF12gzk: A Massive-Star Explosion in a Dwarf Host Galaxy
Published 23-09-2013“…We present the discovery and extensive early-time observations of the Type Ic supernova (SN) PTF12gzk. Our finely sampled light curves show a rise of 0.8mag…”
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Collaborative workspaces to accelerate discovery
Published 05-04-2017“…By applying a display ecology to the {\em Deeper, Wider, Faster} proactive, simultaneous telescope observing campaign, we have shown a dramatic reduction in…”
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Super-luminous supernovae at redshifts of 2.05 and 3.90
Published 08-11-2012“…Nature, 491, 228 (2012) A rare class of `super-luminous' supernovae that are about ten or more times more luminous at their peaks than other types of luminous…”
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What Does the Virial Coefficient of the \Hb Broad-Line Region Depend On?
Published 13-04-2023“…We combine our dynamical modeling black hole mass measurements from the Lick AGN Monitoring Project 2016 sample with measured cross-correlation time lags and…”
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Journal Article