Continuing Exploitation of the UK Investment in the JCMT
Lead Research Organisation:
CARDIFF UNIVERSITY
Department Name: School of Physics and Astronomy
Abstract
We propose that the UK continue to take a significant role in the operation and scientific exploitation of the James Clerk Maxwell telescope (JCMT). We request £200K per annum funding from STFC for a further 3 years from 1st April 2021 to 1st April 2024, which combined with the contributions from the universities will allow us to continue as roughly 20% partners with the East Asian Observatory (EAO), the lead operator, and Canada. The JCMT is the world's largest submm telescope and is likely to remain so until at least 2030. The period for which we now request funding will include the commissioning of new instrumentation, in particular a new camera which will increase the mapping speed of the telescope by at least a factor of 10.
The STFC contribution will allow the UK to continue to play a major role in the Large Programmes currently underway, many of which we are leading, as well as allowing us to initiate new programmes, all at a remarkably low cost. The EAO see the operation of the JCMT as the route to developing the skill base of their own communities via collaboration with the enormous expertise of the UK submm community. It has therefore set aside 50% of the total observing time on the JCMT for large-scale collaborative programmes defined and exploited by joint science teams drawn from all six partner countries. The UK community therefore will gain access to effectively 60% of the total science output of the JCMT at a total cost of £600K over 3 years. As well as producing excellent science, access to the JCMT gives the only direct UK access to the Event Horizon Telescope, with its ability to image the regions immediately around black holes, and the wide-field imaging capability of the JCMT puts UK astronomers in a strong position to leverage time on the Atacama Large Millimetre Array and the James Webb Space Telescope.
The STFC contribution will allow the UK to continue to play a major role in the Large Programmes currently underway, many of which we are leading, as well as allowing us to initiate new programmes, all at a remarkably low cost. The EAO see the operation of the JCMT as the route to developing the skill base of their own communities via collaboration with the enormous expertise of the UK submm community. It has therefore set aside 50% of the total observing time on the JCMT for large-scale collaborative programmes defined and exploited by joint science teams drawn from all six partner countries. The UK community therefore will gain access to effectively 60% of the total science output of the JCMT at a total cost of £600K over 3 years. As well as producing excellent science, access to the JCMT gives the only direct UK access to the Event Horizon Telescope, with its ability to image the regions immediately around black holes, and the wide-field imaging capability of the JCMT puts UK astronomers in a strong position to leverage time on the Atacama Large Millimetre Array and the James Webb Space Telescope.
Planned Impact
The JCMT has a strong history of public outreach, which will continue. The public has a very positive view of astronomy research, and astronomy outreach attracts young people to study STEM subjects at school and university.
Because this is a collaboration with four East Asian countries - China, Japan, Korea and Taiwan - it will enable UK universities and scientists to develop closer ties with scientists and research institutions in these four very strong economies. There are strong opportunities for student exchange, both outward for UK students and inwards for Asian students coming to the UK.
UK PhD students and early-career researchers will have the opportunity of working with cutting-edge technology, both with the hardware at the telescope and with the software used to analyse the data. There is significant opportunity for this training to result in spinout activity in other areas, for example the UK creative industries in the case of software and imaging technology in the case of hardware.
Because this is a collaboration with four East Asian countries - China, Japan, Korea and Taiwan - it will enable UK universities and scientists to develop closer ties with scientists and research institutions in these four very strong economies. There are strong opportunities for student exchange, both outward for UK students and inwards for Asian students coming to the UK.
UK PhD students and early-career researchers will have the opportunity of working with cutting-edge technology, both with the hardware at the telescope and with the software used to analyse the data. There is significant opportunity for this training to result in spinout activity in other areas, for example the UK creative industries in the case of software and imaging technology in the case of hardware.
Organisations
People |
ORCID iD |
Stephen Eales (Principal Investigator) |
Publications
Dye S
(2022)
A high-resolution investigation of the multiphase ISM in a galaxy during the first two billion years
in Monthly Notices of the Royal Astronomical Society
Könyves V
(2023)
A low-mass hub-filament with double centre revealed in NGC 2071-North
in Monthly Notices of the Royal Astronomical Society
Torne P
(2023)
A Search for Pulsars around Sgr A* in the First Event Horizon Telescope Data Set
in The Astrophysical Journal
Stach S
(2021)
An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: halo masses for submillimetre galaxies
in Monthly Notices of the Royal Astronomical Society
Kwon W
(2022)
B-fields in Star-forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main
in The Astrophysical Journal
Hagimoto M.
(2023)
Bright Extragalactic ALMA Redshift Survey (BEARS) III: Detailed study of emission lines from 71 Herschel targets
in arXiv e-prints
Broderick A
(2022)
Characterizing and Mitigating Intraday Variability: Reconstructing Source Structure in Accreting Black Holes with mm-VLBI
in The Astrophysical Journal Letters
Scholte D
(2023)
Cold gas mass measurements for the era of large optical spectroscopic surveys
in Monthly Notices of the Royal Astronomical Society
Greaves J
(2023)
Comment on "Phosphine in the Venusian Atmosphere: A Strict Upper Limit From SOFIA GREAT Observations" by Cordiner et al.
in Geophysical Research Letters
Prather B
(2023)
Comparison of Polarized Radiative Transfer Codes Used by the EHT Collaboration
in The Astrophysical Journal
Kocherlakota P
(2021)
Constraints on black-hole charges with the 2017 EHT observations of M87*
in Physical Review D
Bains W
(2022)
Constraints on the Production of Phosphine by Venusian Volcanoes
in Universe
Relaño M
(2022)
Dust grain size evolution in local galaxies: a comparison between observations and simulations
in Monthly Notices of the Royal Astronomical Society
Arzoumanian D
(2021)
Dust polarized emission observations of NGC 6334 BISTRO reveals the details of the complex but organized magnetic field structure of the high-mass star-forming hub-filament network
in Astronomy & Astrophysics
Gupta A
(2022)
Effects of Magnetic Field Orientations in Dense Cores on Gas Kinematics in Protostellar Envelopes
in The Astrophysical Journal
Doi Y
(2021)
Erratum: "The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333" (2020, ApJ, 899, 28)
in The Astrophysical Journal
Janssen M
(2021)
Event Horizon Telescope observations of the jet launching and collimation in Centaurus A
in Nature Astronomy
Ward-Thompson D
(2023)
First BISTRO Observations of the Dark Cloud Taurus L1495A-B10: The Role of the Magnetic Field in the Earliest Stages of Low-mass Star Formation
in The Astrophysical Journal
Ward-Thompson Derek
(2023)
First BISTRO observations of the dark cloud Taurus L1495A-B10: the role of the magnetic field in the earliest stages of low-mass star formation
in arXiv e-prints
Event Horizon Telescope Collaboration
(2022)
First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
in The Astrophysical Journal Letters
Event Horizon Telescope Collaboration
(2022)
First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multiwavelength Observations, Data Processing, and Calibration
in The Astrophysical Journal Letters
Event Horizon Telescope Collaboration
(2022)
First Sagittarius A* Event Horizon Telescope Results. III. Imaging of the Galactic Center Supermassive Black Hole
in The Astrophysical Journal Letters
Event Horizon Telescope Collaboration
(2022)
First Sagittarius A* Event Horizon Telescope Results. IV. Variability, Morphology, and Black Hole Mass
in The Astrophysical Journal Letters