Search Results - "de Jaeger, T."
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A measurement of the Hubble constant from Type II supernovae
Published in Monthly notices of the Royal Astronomical Society (20-06-2020)“…ABSTRACT Progressive increases in the precision of the Hubble-constant measurement via Cepheid-calibrated Type Ia supernovae (SNe Ia) have shown a discrepancy…”
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A 5 per cent measurement of the Hubble–Lemaître constant from Type II supernovae
Published in Monthly notices of the Royal Astronomical Society (02-07-2022)“…ABSTRACT The most stringent local measurement of the Hubble–Lemaître constant from Cepheid-calibrated Type Ia supernovae (SNe Ia) differs from the value…”
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3
A surge of light at the birth of a supernova
Published in Nature (London) (22-02-2018)“…The discovery of a newly born type IIb supernova reveals a rapid brightening at optical wavelengths that corresponds to the shock-breakout phase of the…”
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The effects of varying colour–luminosity relations on Type Ia supernova science
Published in Monthly notices of the Royal Astronomical Society (01-12-2021)“…ABSTRACT The success of Type Ia supernova (SN Ia) distance standardization for cosmology relies on a single global linear relationship between their peak…”
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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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A Type II Supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS Surveys
Published in The Astrophysical journal (01-02-2017)“…Abstract The coming era of large photometric wide-field surveys will increase the detection rate of supernovae by orders of magnitude. Such numbers will…”
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JWST Low-resolution MIRI Spectral Observations of SN 2021aefx: High-density Burning in a Type Ia Supernova
Published in Astrophysical journal. Letters (01-03-2023)“…Abstract We present a JWST/MIRI low-resolution mid-infrared (MIR) spectroscopic observation of the normal Type Ia supernova (SN Ia) SN 2021aefx at +323 days…”
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The delay of shock breakout due to circumstellar material evident in most type II supernovae
Published in Nature astronomy (01-10-2018)“…Type II supernovae (SNe II) originate from the explosion of hydrogen-rich supergiant massive stars. Their first electromagnetic signature is the shock breakout…”
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JWST MIRI/Medium Resolution Spectrograph (MRS) Observations and Spectral Models of the Underluminous Type Ia Supernova 2022xkq
Published in The Astrophysical journal (01-02-2024)“…Abstract We present a JWST mid-infrared (MIR) spectrum of the underluminous Type Ia Supernova (SN Ia) 2022xkq, obtained with the medium-resolution spectrometer…”
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A JWST Medium-resolution MIRI Spectrum and Models of the Type Ia Supernova 2021aefx at +415 days
Published in The Astrophysical journal (01-11-2024)“…Abstract We present a JWST MIRI medium-resolution spectrometer spectrum (5–27 μ m) of the Type Ia supernova (SN Ia) SN 2021aefx at +415 days past B -band…”
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SN 2011hs: a fast and faint Type IIb supernova from a supergiant progenitor
Published in Monthly notices of the Royal Astronomical Society (01-04-2014)“…Observations spanning a large wavelength range, from X-ray to radio, of the Type IIb supernova (SN) 2011hs are presented, covering its evolution during the…”
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ASAS-SN search for optical counterparts of gravitational-wave events from the third observing run of Advanced LIGO/Virgo
Published in Monthly notices of the Royal Astronomical Society (01-01-2022)“…ABSTRACT We report on the search for electromagnetic counterparts to the nine gravitational-wave events with a >60 per cent probability of containing a neutron…”
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Optical/γ-ray blazar flare correlations: understanding the high-energy emission process using ASAS-SN and Fermi light curves
Published in Monthly notices of the Royal Astronomical Society (01-03-2023)“…ABSTRACT Using blazar light curves from the optical All-Sky Automated Survey for Supernovae (ASAS-SN) and the γ-ray Fermi-LAT telescope, we performed the most…”
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The rise-time of Type II supernovae
Published in Monthly notices of the Royal Astronomical Society (01-08-2015)“…We investigate the early-time light curves of a large sample of 223 Type II supernovae (SNe II) from the Sloan Digital Sky Survey and the Supernova Legacy…”
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The Berkeley Sample of Type II Supernovae: BVRI Light Curves and Spectroscopy of 55 SNe II
Published in Monthly notices of the Royal Astronomical Society (01-12-2019)“…In this work, BVRI light curves of 55 Type II supernovae (SNe II) from the Lick Observatory Supernova Search programme obtained with the Katzman Automatic…”
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Observed Type II supernova colours from the Carnegie Supernova Project-I
Published in Monthly notices of the Royal Astronomical Society (01-06-2018)Get full text
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The Spectroscopic Classification of Astronomical Transients (SCAT) Survey: Overview, Pipeline Description, Initial Results, and Future Plans
Published in Publications of the Astronomical Society of the Pacific (01-12-2022)“…Abstract We present the Spectroscopic Classification of Astronomical Transients (SCAT) survey, which is dedicated to spectrophotometric observations of…”
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Multiple flares in the changing-look AGN NGC 5273
Published in Monthly notices of the Royal Astronomical Society (23-03-2023)“…ABSTRACT NGC 5273 is a known optical and X-ray variable AGN. We analyse new and archival IR, optical, UV, and X-ray data in order to characterize its long-term…”
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Studying Type II supernovae as cosmological standard candles using the Dark Energy Survey
Published in Monthly notices of the Royal Astronomical Society (2020)“…ABSTRACT Despite vast improvements in the measurement of the cosmological parameters, the nature of dark energy and an accurate value of the Hubble constant…”
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SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
Published in Monthly notices of the Royal Astronomical Society (01-12-2017)“…AbstractAlthough Type Ia supernova cosmology has now reached a mature state, it is important to develop as many independent methods as possible to understand…”
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