Astrophysics and Cosmology Research at the JBCA 2020-2023
Lead Research Organisation:
University of Manchester
Department Name: Physics and Astronomy
Abstract
This grant supports the research of the Jodrell Bank Centre for Astrophysics at the University of Manchester. Our research is a divided into 3 groups. There are too many specific proposals to describe in detail, do below we have given a brief layman's explanation of the work being carried out by the three groups.
Cosmology: This is the study of the Universe as a whole. The main aim is to understand the processes by which the large scale feature of the Universe formed and to constrain the various different kinds of matter that existed within it. These include dark matter and dark energy which are thought to constitute more than 95% of the total. We do this by comparison to observations of weak and strong gravitational lensing which is the distortion of light predicted to be caused by massive objects in Einstein' Theory of General Relativity, the cosmic microwave background which is the faint emission of radiation created at the time when protons and electrons come together to form hydrogen and the emission given off by neutral hydrogen atoms in galaxies. The research we propose here involves both theory and observation as well as the development of the technology necessary to make the observations possible.
Sun, Stars and Galaxies: The researchers in this group study a wide range of astrophysical processes that are reasonable for the formation and evolution of the objects in the name of the group. Specific key areas that the group is interested in are the formation of stars much larger than the Sun and the subsequent evolution, the properties of the so-called interstellar medium (ISM) which comprises molecules not bound to stars and the magnetic fields that permeate space.
Pulsars and Time Domain Astrophysics: The focus of this group is astrophysical signatures that are changing with time- things which come on and off, often with some kind of regularity. These include Pulsars which are a non-standard star type, known as a neutron star, which is a dead star supported by the quantum pressure of neutrons. The radio emission from these objects pulses on an off with extraordinary regularity allowing them to acts cosmic clocks. The constantly measuring these clocks as the neutron stars spin and move through space, often impacted on by a companion star, allows the most precise constraints on the nature of gravity outside the solar system. Other phenomena studied by this group include Nova explosions, other variable stars, and variability induced by the lensing effects of one star passing in front of another, called microlensing.
Cosmology: This is the study of the Universe as a whole. The main aim is to understand the processes by which the large scale feature of the Universe formed and to constrain the various different kinds of matter that existed within it. These include dark matter and dark energy which are thought to constitute more than 95% of the total. We do this by comparison to observations of weak and strong gravitational lensing which is the distortion of light predicted to be caused by massive objects in Einstein' Theory of General Relativity, the cosmic microwave background which is the faint emission of radiation created at the time when protons and electrons come together to form hydrogen and the emission given off by neutral hydrogen atoms in galaxies. The research we propose here involves both theory and observation as well as the development of the technology necessary to make the observations possible.
Sun, Stars and Galaxies: The researchers in this group study a wide range of astrophysical processes that are reasonable for the formation and evolution of the objects in the name of the group. Specific key areas that the group is interested in are the formation of stars much larger than the Sun and the subsequent evolution, the properties of the so-called interstellar medium (ISM) which comprises molecules not bound to stars and the magnetic fields that permeate space.
Pulsars and Time Domain Astrophysics: The focus of this group is astrophysical signatures that are changing with time- things which come on and off, often with some kind of regularity. These include Pulsars which are a non-standard star type, known as a neutron star, which is a dead star supported by the quantum pressure of neutrons. The radio emission from these objects pulses on an off with extraordinary regularity allowing them to acts cosmic clocks. The constantly measuring these clocks as the neutron stars spin and move through space, often impacted on by a companion star, allows the most precise constraints on the nature of gravity outside the solar system. Other phenomena studied by this group include Nova explosions, other variable stars, and variability induced by the lensing effects of one star passing in front of another, called microlensing.
Planned Impact
The range of research we undertake and the world-class facilities within and in close association with JBCA (the Jodrell Bank Discovery Centre, e-MERLIN, the Lovell Telescope, the ALMA ARC and the SKA HQ) will provide key pathways to increasing our already strong impact on UK and global industry, the next generation of scientists and engineers, and the general public. The University's investment in the Jodrell Bank site combined with significant external funding (e.g. from Heritage Lottery Fund) will enable us to expand its use as an iconic venue for public and industrial engagement. The programme described here formed a key part of the School's submission for REF2014, helping it to be ranked highest in the REF for physics impact with 83% at 4* and 17% at 3*. Our outreach \& public engagement programme is extremely strong and continues to grow, particularly through its work with the University's award-winning Jodrell Bank Discovery Centre and the BBC. With the recent decision on SKA HQ location and our strong research work in this area, there is also growing impact in both outreach and industrial engagement in this area.
Our "Pathways to Impact" statement in the case for support outlines things that we have done in recent times under the headings of "Outreach and Public Engagement" and "Industrial and economic impact". We list some highlights below.
- Jodcast: Podcast run by students with 7000 regular listeners.
- 215000 Twitter and 18000 Facebook followers
- Stargazing live, Pulsar Hunters, Science Programmes presented by Danielle George
- JB Discovery centre with 190000 visitors per year
- Award winning Bluedot Festivals
- Industry contracts for SKA work including CISCO, AASL, NPL, AEON, Critical Software, MMI, GEANT
- Newton programme for Radio Astronomy in Africa.
Our "Pathways to Impact" statement in the case for support outlines things that we have done in recent times under the headings of "Outreach and Public Engagement" and "Industrial and economic impact". We list some highlights below.
- Jodcast: Podcast run by students with 7000 regular listeners.
- 215000 Twitter and 18000 Facebook followers
- Stargazing live, Pulsar Hunters, Science Programmes presented by Danielle George
- JB Discovery centre with 190000 visitors per year
- Award winning Bluedot Festivals
- Industry contracts for SKA work including CISCO, AASL, NPL, AEON, Critical Software, MMI, GEANT
- Newton programme for Radio Astronomy in Africa.
Organisations
Publications
Shim H
(2022)
Multiwavelength properties of 850-µm selected sources from the North Ecliptic Pole SCUBA-2 survey
in Monthly Notices of the Royal Astronomical Society
Shimajiri Y
(2020)
The accretion history of high-mass stars: an ArTéMiS pilot study of infrared dark clouds
in Monthly Notices of the Royal Astronomical Society
Shimwell T
(2022)
The LOFAR Two-metre Sky Survey V. Second data release
in Astronomy & Astrophysics
Simpson C
(2023)
How cosmic rays mediate the evolution of the interstellar medium
in Monthly Notices of the Royal Astronomical Society
Singh S
(2022)
The GMRT High Resolution Southern Sky Survey for Pulsars and Transients. III. Searching for Long-period Pulsars
in The Astrophysical Journal
Singh S
(2023)
The GMRT High Resolution Southern Sky Survey for Pulsars and Transients. IV. Discovery of Four New Pulsars with an FFA Search
in The Astrophysical Journal
Singha J
(2021)
A real-time automated glitch detection pipeline at Ooty Radio Telescope
in Monthly Notices of the Royal Astronomical Society
Skipper C
(2022)
A GPU-based Imager with Polarised Primary-beam Correction
Skipper C
(2022)
A GPU-based Imager with Polarised Primary-beam Correction
Slijepcevic I
(2022)
Radio Galaxy Zoo: using semi-supervised learning to leverage large unlabelled data sets for radio galaxy classification under data set shift
in Monthly Notices of the Royal Astronomical Society
Smarra C
(2023)
Second Data Release from the European Pulsar Timing Array: Challenging the Ultralight Dark Matter Paradigm
in Physical Review Letters
Smith C
(2022)
Pulsations of microwave emission from a solar flare in a twisted loop caused by intrinsic magnetohydrodynamic oscillations
in Monthly Notices of the Royal Astronomical Society
Sobey C
(2022)
Searching for pulsars associated with polarised point sources using LOFAR: Initial discoveries from the TULIPP project
in Astronomy & Astrophysics
Sobey C
(2021)
A polarization census of bright pulsars using the ultrawideband receiver on the Parkes radio telescope
in Monthly Notices of the Royal Astronomical Society
Soler J
(2022)
The Galactic dynamics revealed by the filamentary structure in atomic hydrogen emission
in Astronomy & Astrophysics
Soler J
(2020)
The history of dynamics and stellar feedback revealed by the H I filamentary structure in the disk of the Milky Way
in Astronomy & Astrophysics
Song X
(2021)
The Thousand-Pulsar-Array programme on MeerKAT - II. Observing strategy for pulsar monitoring with subarrays
in Monthly Notices of the Royal Astronomical Society
Sormani M
(2020)
Simulations of the Milky Way's Central Molecular Zone - II. Star formation
in Monthly Notices of the Royal Astronomical Society
Specht D
(2023)
Kepler K2 Campaign 9 - II. First space-based discovery of an exoplanet using microlensing
in Monthly Notices of the Royal Astronomical Society
Specht D
(2020)
MaBµlS-2: high-precision microlensing modelling for the large-scale survey era
in Monthly Notices of the Royal Astronomical Society
Spencer R
(2022)
Major and minor flares on Cygnus X-3 revisited
in Monthly Notices of the Royal Astronomical Society
Spiewak R
(2022)
The MeerTime Pulsar Timing Array: A census of emission properties and timing potential
in Publications of the Astronomical Society of Australia
Spinelli M
(2022)
SKAO H i intensity mapping: blind foreground subtraction challenge
in Monthly Notices of the Royal Astronomical Society
Srinivasan S
(2021)
Cosmological gravity on all scales. Part II. Model independent modified gravity N-body simulations
in Journal of Cosmology and Astroparticle Physics
Stanford S
(2021)
Euclid Preparation. XIV. The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Data Release 3
in The Astrophysical Journal Supplement Series
Stankowiak G
(2020)
Detection chain and electronic readout of the QUBIC instrument
Stappers B
(2020)
Study of spider pulsar binary eclipses and discovery of an eclipse mechanism transition
in Monthly Notices of the Royal Astronomical Society
Steeghs D
(2022)
The Gravitational-wave Optical Transient Observer (GOTO): prototype performance and prospects for transient science
in Monthly Notices of the Royal Astronomical Society
Stewart J
(2022)
Oscillatory reconnection and waves driven by merging magnetic flux ropes in solar flares
in Monthly Notices of the Royal Astronomical Society
Stockmann M
(2021)
The Fundamental Plane of Massive Quiescent Galaxies at z ~ 2
in The Astrophysical Journal
Suphapolthaworn S
(2022)
Earth through the looking glass: how frequently are we detected by other civilizations through photometric microlensing?
in Monthly Notices of the Royal Astronomical Society
Susobhanan A
(2021)
pinta : The uGMRT data processing pipeline for the Indian Pulsar Timing Array
in Publications of the Astronomical Society of Australia
Sweetnam T
(2022)
Simulating the behaviour of travelling wave superconducting parametric amplifiers using a commercial circuit simulator
in Superconductor Science and Technology
Sweijen F
(2022)
Deep sub-arcsecond wide-field imaging of the Lockman Hole field at 144 MHz
in Nature Astronomy
Sweijen F
(2022)
High-resolution international LOFAR observations of 4C 43.15 Spectral ages and injection indices in a high-z radio galaxy
in Astronomy & Astrophysics
Swiggum J
(2023)
The Green Bank North Celestial Cap Survey. VII. 12 New Pulsar Timing Solutions
in The Astrophysical Journal
Szary A
(2022)
MeerKAT Observations of the Reversing Drifting Subpulses in PSR J1750-3503
in The Astrophysical Journal
Szary A
(2020)
Single-pulse Modeling and the Bi-drifting Subpulses of Radio Pulsar B1839-04
in The Astrophysical Journal
Tahani M
(2023)
JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334
in The Astrophysical Journal
Tan C
(2023)
X-ray non-detection of PSR J0250 + 5854
in Monthly Notices of the Royal Astronomical Society
Tan S
(2023)
Morphologies and Central Stars of Planetary Nebulae in the Galactic bulge from VLT, HST and Pan-STARRS imaging
in Monthly Notices of the Royal Astronomical Society
Tan S
(2023)
When the Stars Align: A 5s Concordance of Planetary Nebulae Major Axes in the Center of Our Galaxy
in The Astrophysical Journal Letters
Tan S
(2024)
A catalogue of planetary nebulae chemical abundances in the Galactic bulge
in Monthly Notices of the Royal Astronomical Society
Tang H
(2022)
Radio Galaxy Zoo: giant radio galaxy classification using multidomain deep learning
in Monthly Notices of the Royal Astronomical Society
Tasse C
(2021)
The LOFAR Two-meter Sky Survey: Deep Fields Data Release 1 I. Direction-dependent calibration and imaging
in Astronomy & Astrophysics
Tatematsu K
(2022)
Nobeyama Survey of Inward Motions toward Cores in Orion Identified by SCUBA-2
in The Astrophysical Journal
Tatematsu K
(2020)
ALMA ACA and Nobeyama Observations of Two Orion Cores in Deuterated Molecular Lines
in The Astrophysical Journal
Tatematsu K
(2021)
Molecular Cloud Cores with High Deuterium Fractions: Nobeyama Mapping Survey
in The Astrophysical Journal Supplement Series