A consolidated grant for Sheffield Astrophysics 2018-2021
Lead Research Organisation:
University of Sheffield
Department Name: Physics and Astronomy
Abstract
The aim of this proposal is to support a programme of internationally excellent research in astrophysics at Sheffield, building on our recent research achievements, and tied to the exploitation of leading international facilities supported by STFC and UKSA.
Planned Impact
The main ways in which our research makes an impact outside the academic community is via our knowledge exchange and outreach activities. To summarise:
1. Knowledge exchange. This is primarily based on the building of the ULTRACAM and HiPERCAM instruments, which has lead to the development of new new CCD detector, data acquisition and cooling systems, as well as stimulating a project to develop new techniques to use 3D printing build rigid, lightweight support structure for astronomical instruments.
2. Outreach. Over the last 5 years members of the Sheffield astrophsyics group have delivered 126 talks to schools and astronomical societies, have held 70 in-house workshops for school students, and been involved in 15 press releases, all based on their research activities.
Details are given in our Impact Plan that is included as an attachment.
1. Knowledge exchange. This is primarily based on the building of the ULTRACAM and HiPERCAM instruments, which has lead to the development of new new CCD detector, data acquisition and cooling systems, as well as stimulating a project to develop new techniques to use 3D printing build rigid, lightweight support structure for astronomical instruments.
2. Outreach. Over the last 5 years members of the Sheffield astrophsyics group have delivered 126 talks to schools and astronomical societies, have held 70 in-house workshops for school students, and been involved in 15 press releases, all based on their research activities.
Details are given in our Impact Plan that is included as an attachment.
Organisations
Publications
Schaffenroth V
(2021)
A quantitative in-depth analysis of the prototype sdB+BD system SDSS J08205+0008 revisited in the Gaia era
in Monthly Notices of the Royal Astronomical Society
Schneider F
(2018)
The VLT-FLAMES Tarantula Survey XXIX. Massive star formation in the local 30 Doradus starburst
in Astronomy & Astrophysics
Scholtz J
(2021)
The impact of ionized outflows from z ~ 2.5 quasars is not through instantaneous in situ quenching: the evidence from ALMA and VLT/SINFONI
in Monthly Notices of the Royal Astronomical Society
Schootemeijer A
(2021)
A dearth of young and bright massive stars in the Small Magellanic Cloud
in Astronomy & Astrophysics
Sergison D
(2020)
Characterizing the i-band variability of YSOs over six orders of magnitude in time-scale
in Monthly Notices of the Royal Astronomical Society
Silvotti R
(2018)
The sdB pulsating star V391 Peg and its putative giant planet revisited after 13 years of time-series photometric data
in Astronomy & Astrophysics
Snaid S
(2018)
Flickering in AGB stars: probing the nature of accreting companions
in Monthly Notices of the Royal Astronomical Society
Spence R
(2018)
Quantifying the AGN-driven outflows in ULIRGs (QUADROS) III: measurements of the radii and kinetic powers of eight near-nuclear outflows
in Monthly Notices of the Royal Astronomical Society
Stanley F
(2018)
Deep ALMA photometry of distant X-ray AGN: improvements in star formation rate constraints, and AGN identification
in Monthly Notices of the Royal Astronomical Society
Stevance H
(2018)
Probing the rotational velocity of Galactic WO stars with spectropolarimetry
in Monthly Notices of the Royal Astronomical Society
Stevance H
(2019)
The 3D shape of Type IIb SN 2011hs
in Monthly Notices of the Royal Astronomical Society
Sun N
(2020)
The changing-type SN 2014C may come from an 11-M? star stripped by binary interaction and violent eruption
in Monthly Notices of the Royal Astronomical Society
Sun N
(2020)
Origins of Type Ibn SNe 2006jc/2015G in interacting binaries and implications for pre-SN eruptions
in Monthly Notices of the Royal Astronomical Society
Tadhunter C
(2018)
Quantifying the AGN-driven outflows in ULIRGs (QUADROS) - II. Evidence for compact outflow regions from HST [O III] imaging observations
in Monthly Notices of the Royal Astronomical Society
Tadhunter C
(2021)
A light echo from the warm outflow in the ULIRG F01004-2237 following a major flare in its optical continuum emission
in Monthly Notices of the Royal Astronomical Society
Tadhunter C
(2024)
An ALMA CO(1-0) survey of the 2Jy sample: large and massive molecular discs in radio AGN host galaxies
in Monthly Notices of the Royal Astronomical Society
Tehrani K
(2019)
Weighing Melnick 34: the most massive binary system known
in Monthly Notices of the Royal Astronomical Society
Urbano-Mayorgas J
(2019)
The host galaxies of luminous type 2 AGNs at z ~ 0.3-0.4
in Monthly Notices of the Royal Astronomical Society
Van Dyk S
(2019)
The Type II-plateau Supernova 2017eaw in NGC 6946 and Its Red Supergiant Progenitor
in The Astrophysical Journal
Walters K
(2020)
A binning-free method reveals a continuous relationship between galaxies' AGN power and offset from main sequence
in Monthly Notices of the Royal Astronomical Society
Wang ? L
(2019)
The Pre-He White Dwarf in the Post-mass Transfer Binary EL CVn
in The Astronomical Journal
Wild J
(2020)
Spectroscopic and photometric periods of six ultracompact accreting binaries
in Monthly Notices of the Royal Astronomical Society
Wright N
(2020)
The velocity structure of Cygnus OB2
in Monthly Notices of the Royal Astronomical Society
Wyrzykowski L
(2020)
Full orbital solution for the binary system in the northern Galactic disc microlensing event Gaia16aye
in Astronomy & Astrophysics
Xiao M
(2023)
The hidden side of cosmic star formation at z > 3 Bridging optically dark and Lyman-break galaxies with GOODS-ALMA
in Astronomy & Astrophysics
Yang ? Y
(2020)
The Young and Nearby Normal Type Ia Supernova 2018gv: UV-optical Observations and the Earliest Spectropolarimetry
in The Astrophysical Journal
Zhou L
(2020)
GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5
in Astronomy & Astrophysics
| Description | The award was used to fund a wide range of research that led to substantial progress in (a) understanding the links between the evolution actively accreting black holes and their host galaxies via far-IR observations taken with the Herschel satellite; (b) the way in which the most massive stars explode at the ends of their lives and the environments in which they do so; (c) the time variability of a range of astrophysical objects, and in particular compact stellar remnants. |
| Exploitation Route | The outcomes can and have been used to inform future research projects and applications for observing time on highly-oversubscribed observing facilities. |
| Sectors | Education Other |
| Description | The findings have been used to inform a variety of outreach activities, including talks to schools and amateur astronomy societies socities, as well as public lectures. |
| First Year Of Impact | 2018 |
| Sector | Other |
| Impact Types | Cultural Societal |
| Title | Parameters of 15 Cataclysmic Variables |
| Description | VizieR online Data Catalogue associated with article published in journal Monthly Notices of the Royal Astronomical Society with title ' The evolutionary status of Cataclysmic Variables: eclipse modelling of 15 systems.' (bibcode: 2019MNRAS.486.5535M) |
| Type Of Material | Database/Collection of data |
| Year Produced | 2022 |
| Provided To Others? | Yes |
| URL | https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/486/5535 |