Astrophysics and Cosmology Research within the JBCA 2017-2020
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 change with time: things which come on and off, often with some kind of regularity. These include Pulsars which are non-standard star time, 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 change with time: things which come on and off, often with some kind of regularity. These include Pulsars which are non-standard star time, 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.
- 230000 Twitter followers
- Stargazing live
- JB Discovery centre with 150000 visitors per year
- Award winning "Live from Jodrell Bank" rock concerts
- Industry contracts for SKA work including CISCO, AASL, NPL, 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.
- 230000 Twitter followers
- Stargazing live
- JB Discovery centre with 150000 visitors per year
- Award winning "Live from Jodrell Bank" rock concerts
- Industry contracts for SKA work including CISCO, AASL, NPL, GEANT
- Newton programme for Radio Astronomy in Africa.
Organisations
Publications
Purser S
(2019)
Erratum: Constraining the nature of DG Tau A's thermal and non-thermal radio emission
in Monthly Notices of the Royal Astronomical Society
Perera B
(2017)
Erratum: Evidence for an intermediate-mass black hole in the globular cluster NGC 6624
in Monthly Notices of the Royal Astronomical Society
Thomas D
(2017)
Estimating the weak-lensing rotation signal in radio cosmic shear surveys
in Monthly Notices of the Royal Astronomical Society
Jin Y
(2019)
Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation
in Monthly Notices of the Royal Astronomical Society
Perera B
(2017)
Evidence for an intermediate-mass black hole in the globular cluster NGC 6624
in Monthly Notices of the Royal Astronomical Society
Ilie C
(2019)
Evidence for magnetospheric effects on the radiation of radio pulsars
in Monthly Notices of the Royal Astronomical Society
Chluba J
(2017)
Evolution of CMB spectral distortion anisotropies and tests of primordial non-Gaussianity
in Monthly Notices of the Royal Astronomical Society
Morgan J
(2019)
Exoplanetary atmosphere target selection in the era of comparative planetology
in Monthly Notices of the Royal Astronomical Society
Remazeilles M
(2018)
Exploring cosmic origins with CORE: B -mode component separation
in Journal of Cosmology and Astroparticle Physics
Melin J
(2018)
Exploring cosmic origins with CORE: Cluster science
in Journal of Cosmology and Astroparticle Physics
Valentino E
(2018)
Exploring cosmic origins with CORE: Cosmological parameters
in Journal of Cosmology and Astroparticle Physics
Burigana C
(2018)
Exploring cosmic origins with CORE: Effects of observer peculiar motion
in Journal of Cosmology and Astroparticle Physics
Zotti G
(2018)
Exploring cosmic origins with CORE: Extragalactic sources in cosmic microwave background maps
in Journal of Cosmology and Astroparticle Physics
Challinor A
(2018)
Exploring cosmic origins with CORE: Gravitational lensing of the CMB
in Journal of Cosmology and Astroparticle Physics
Finelli F
(2018)
Exploring cosmic origins with CORE: Inflation
in Journal of Cosmology and Astroparticle Physics
Natoli P
(2018)
Exploring cosmic origins with CORE: Mitigation of systematic effects
in Journal of Cosmology and Astroparticle Physics
Delabrouille J
(2018)
Exploring cosmic origins with CORE: Survey requirements and mission design
in Journal of Cosmology and Astroparticle Physics
De Bernardis P
(2018)
Exploring cosmic origins with CORE: The instrument
in Journal of Cosmology and Astroparticle Physics
Heesen V
(2018)
Exploring the making of a galactic wind in the starbursting dwarf irregular galaxy IC 10 with LOFAR
in Monthly Notices of the Royal Astronomical Society
Dharmawardena T
(2018)
Extended Dust Emission from Nearby Evolved Stars?
in Monthly Notices of the Royal Astronomical Society
Remazeilles M
(2018)
Extracting foreground-obscured µ-distortion anisotropies to constrain primordial non-Gaussianity
in Monthly Notices of the Royal Astronomical Society
Rattenbury N
(2017)
Faint-source-star planetary microlensing: the discovery of the cold gas-giant planet OGLE-2014-BLG-0676Lb
in Monthly Notices of the Royal Astronomical Society
McCallum N
(2022)
Fast map-based simulations of systematics in CMB surveys including effects of the scanning strategy
in Monthly Notices of the Royal Astronomical Society
| Description | The consolidated grant supported a wide range of activities in astrophysics and cosmology at the JBCA. This was based around three areas: cosmology - the study of the Universe as a single entity, pulsars - spinning neutron stars which emit pulse of radio waves at regular intervals, astrophysical processes - the study of galaxy and star formation in the universe. Progress was made in all these areas. |
| Exploitation Route | The wide range of work produce by the grant has been published in journals. These papers have received significant citations indicating that all the areas have had an impact within the academic research community. |
| Sectors | Digital/Communication/Information Technologies (including Software) Education Other |
| Description | The research has been used extensively in the outreach program of the Jodrell Bank Discovery Centre, which attracts 160,000 visitors per annum and focusses on hard-to-reach audiences. |
| First Year Of Impact | 2020 |
| Sector | Education |
| Impact Types | Cultural Societal |
| Title | MKT J170456.2-482100: the first transient discovered byMeerKAT |
| Description | These are the data files required to make Figures 2, 4, 5, 6, 8, 10, 11, and 12 of the manuscript: https://doi.org/10.1093/mnras/stz3027 or Open-Access on ArXiv: https://arxiv.org/abs/1911.07713 The code that uses these files to make the plots can be found here (DOI). Please make sure to cite these data correctly! The required citations for these data are: ASAS_data.tsv is ASAS data from their catalogue and therefore are not covered by our licence. If you make use of these data please cite ASAS appropriately according to their guidelines. KELT_S36_lc_027056_V01_west_tfa.dat and KELT_S36_lc_027057_V01_east_tfa.dat are data sets from KELT and therefore are not covered by our licence. If you make use of these data please cite KELT by citing Pepper et al. 2007. ASASSN.csv is ASAS-SN data from their catalogue and therefore are not covered by our licence. If you make use of these data please cite ASAS-SN appropriately according to their guidelines (when using ASAS-SN light curves in publications cite: Shappee et al. (2014) and Kochanek et al. (2017)). TYC_optical_semesters.npy, TYC_optical_binned.npy, and TYC_optical_binned_noOutliers.npy also make use of the above ASAS, KELT, and ASAS-SN. If you use these data please cite ASAS, KELT, and ASAS-SN as above, as well as our work. TYC_MeerKAT_fluxes.npy and TYC_local_RMS.npy are the data as presented in Table A1 in our manuscript. Therefore, please cite our work if you make use of these data. TYC_SED_datapoints.txt and TYC_SED_model.txt are the data and model used to make the SED of TYC 8332-2529-1. Please cite our work and the references therein for the datapoints, and our work and McDonald et al. 2012 and McDonald et al. 2017 if you make use of the model. TYC_MeerKAT_ScaledFlux.npy is presented in Figures 2 and 10 of our manuscript, please cite our work if you make use of these data SALT_radial_velocities.npy and LCO_radial_velocities.npy are presented in Table 2 of our manuscript, please cite our work if you make use of these data TYC_LS_periods.npy and TYC_LS_periodErrors.npy are the results of the Lomb-Scargle analysis of the optical observations and are presented in Figure 4 of our manuscript, please cite our work if you make use of these data More information about the format of these data and how to use them can be found in the GitHub repo (DOI). |
| Type Of Material | Database/Collection of data |
| Year Produced | 2019 |
| Provided To Others? | Yes |
| URL | https://zenodo.org/record/3548868 |
| Title | MKT J170456.2-482100: the first transient discovered byMeerKAT |
| Description | These are the data files required to make Figures 2, 4, 5, 6, 8, 10, 11, and 12 of the manuscript: https://doi.org/10.1093/mnras/stz3027 or Open-Access on ArXiv: https://arxiv.org/abs/1911.07713 The code that uses these files to make the plots can be found here (DOI). Please make sure to cite these data correctly! The required citations for these data are: ASAS_data.tsv is ASAS data from their catalogue and therefore are not covered by our licence. If you make use of these data please cite ASAS appropriately according to their guidelines. KELT_S36_lc_027056_V01_west_tfa.dat and KELT_S36_lc_027057_V01_east_tfa.dat are data sets from KELT and therefore are not covered by our licence. If you make use of these data please cite KELT by citing Pepper et al. 2007. ASASSN.csv is ASAS-SN data from their catalogue and therefore are not covered by our licence. If you make use of these data please cite ASAS-SN appropriately according to their guidelines (when using ASAS-SN light curves in publications cite: Shappee et al. (2014) and Kochanek et al. (2017)). TYC_optical_semesters.npy, TYC_optical_binned.npy, and TYC_optical_binned_noOutliers.npy also make use of the above ASAS, KELT, and ASAS-SN. If you use these data please cite ASAS, KELT, and ASAS-SN as above, as well as our work. TYC_MeerKAT_fluxes.npy and TYC_local_RMS.npy are the data as presented in Table A1 in our manuscript. Therefore, please cite our work if you make use of these data. TYC_SED_datapoints.txt and TYC_SED_model.txt are the data and model used to make the SED of TYC 8332-2529-1. Please cite our work and the references therein for the datapoints, and our work and McDonald et al. 2012 and McDonald et al. 2017 if you make use of the model. TYC_MeerKAT_ScaledFlux.npy is presented in Figures 2 and 10 of our manuscript, please cite our work if you make use of these data SALT_radial_velocities.npy and LCO_radial_velocities.npy are presented in Table 2 of our manuscript, please cite our work if you make use of these data TYC_LS_periods.npy and TYC_LS_periodErrors.npy are the results of the Lomb-Scargle analysis of the optical observations and are presented in Figure 4 of our manuscript, please cite our work if you make use of these data More information about the format of these data and how to use them can be found in the GitHub repo (DOI). |
| Type Of Material | Database/Collection of data |
| Year Produced | 2019 |
| Provided To Others? | Yes |
| URL | https://zenodo.org/record/3548867 |
