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| Funder | Science and Technology Facilities Council |
|---|---|
| Recipient Organization | The University of Manchester |
| Country | United Kingdom |
| Start Date | Sep 30, 2021 |
| End Date | Mar 30, 2025 |
| Duration | 1,277 days |
| Number of Grantees | 2 |
| Roles | Student; Supervisor |
| Data Source | UKRI Gateway to Research |
| Grant ID | 2627016 |
LIRGI includes 42 local (D < 260 Mpc) galaxies of the most luminous infra-red galaxies selected from the IRAS revised Bright Galaxy Sample in the Northern Hemisphere, with L= log(Lir/Lsol) >11.4.
The galaxies of the sample have properties of area star formation densities, gas and radiation densities similar to star-forming galaxies a high redshift.
LIRGI will provide a much needed high-spatial resolution radio complement to the legacy observations made with the NASA Great Observatories (GOALS).
The e-MERLIN LIRGI project has observed at C- and L-band (both in continuum and spectra line mode), as well as EVN for the whole sample, and access to LOFAR data for a sub-sample of LIRGI. In addition, there is ancillary JVLA data for the whole sample.
This project exploits the combined dataset of e-MERLIN/LOFAR/JVLA, to trace the nature of the ISM in LIRGs (clumpy vs. uniform media), as well as for unveiling nuclear outflows.
The University of Manchester
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