New generation sky surveys, exotic transients and gravitational wave sources
Lead Research Organisation:
University of Oxford
Department Name: Oxford Physics
Abstract
Supernovae create the heavy elements we see in the entire visible Universe. While stars evolve over millions or billions of years, a supernova explosion happens in seconds and the glowing remnant lasts for years. We aim to understand how these explosions happen and how they create the neutron stars, pulsars and black holes in our galaxy. In 2017 a breakthrough discovery was made when the first electromagnetic counterpart to a gravitational wave source was found. Termed a 'kilonova', this was the result of a pair of merging neutron stars and the optical and infrared light arose from the radioactive decay of heavy elements (which we call r-process elements). These elements are heavier than iron and such neutron star mergers may be responsible for all these heavy elements. Our projects will find more of these, and the combination of gravitational waves and electromagnetic signals opens up a new window on the Universe
Organisations
People |
ORCID iD |
Stephen Smartt (Principal Investigator) |
Publications
Aamer A
(2024)
A precursor plateau and pre-maximum [O ii ] emission in the superluminous SN2019szu: a pulsational pair-instability candidate
in Monthly Notices of the Royal Astronomical Society
Gillanders J
(2023)
Modelling the spectra of the kilonova AT2017gfo - II: Beyond the photospheric epochs
in Monthly Notices of the Royal Astronomical Society
Kilpatrick C
(2023)
SN 2023ixf in Messier 101: A Variable Red Supergiant as the Progenitor Candidate to a Type II Supernova
in The Astrophysical Journal Letters
Moore T
(2023)
SN 2022jli: A Type Ic Supernova with Periodic Modulation of Its Light Curve and an Unusually Long Rise
in The Astrophysical Journal Letters
Nicholl M
(2023)
AT 2022aedm and a New Class of Luminous, Fast-cooling Transients in Elliptical Galaxies
in The Astrophysical Journal Letters
Pursiainen M
(2023)
SN 2023emq: A Flash-ionized Ibn Supernova with Possible C iii Emission
in The Astrophysical Journal Letters
Pursiainen M
(2023)
SN 2023emq: a flash-ionised Ibn supernova with possible CIII emissio
Smartt S
(2024)
GW190425: Pan-STARRS and ATLAS coverage of the skymap and limits on optical emission associated with FRB 20190425A
in Monthly Notices of the Royal Astronomical Society
Srivastav S
(2023)
Unprecedented Early Flux Excess in the Hybrid 02es-like Type Ia Supernova 2022ywc Indicates Interaction with Circumstellar Material
in The Astrophysical Journal Letters