I am the Director for Science at the European Southern Observatory (ESO), on secondment from the Institute for Astronomy (IfA), part of the University of Edinburgh, where I am Professor of Astrophysics. I was previously a PPARC Advanced Fellow (Ernest Rutherford Fellowships nowadays) at the IfA and a lecturer at University College London.
I hold an Advanced Grant, COSMICISM (related publications; philosophical aside), from the European Research Council, which aims to study the formation and evolution of galaxies, mainly via observations at far-infrared, submillimetre and radio wavelengths. I currently lead science projects with the Atacama Large Millimetre/Submillimetre Array (ALMA) in Chile and the National Radio Astronomy Observatory's Jansky Very Large Array (JVLA) near Socorro in New Mexico. My time is split between managing the Directorate of Science at ESO, supervising PhD students, writing proposals to use or build telescopes, analysing data, and writing papers - 36 and 55 refereed papers as first and second author, respectively (all refereed, 1st author refereed; 2nd author refereed; https://orcid.org/0000-0001-5118-1313) - working in a field I perceive to represent the divine intersection of science and art. What I do is esoteric by most standards, but normal in astrophysics. I meddle mainly with faint smudges in far-flung regions of the Universe. The golden rule seems to be that I get interested in things that are ridiculously difficult to study and explain.
THE DARK SIDE OF GALAXY FORMATIONThe submillimetre waveband gives access to redshifted far-infrared emission from very dusty, active galaxies in the distant Universe - UV photons from hot, young stars which have been absorbed by cool dust particles and re-emitted at much longer wavelengths.
The first sensitive submillimetre surveys of the distant Universe were completed in 1997. The first map, taken through the massive lensing cluster, Abell 370, is shown to the left. The map was made with the SCUBA bolometer array on the 15-m JCMT, Hawaii. The bright source at the bottom of the image (`Le Blob' to its friends, or L1/L2) was the first `SCUBA galaxy' - SMM J02399-0136 at z = 2.8.
We know now that these objects can be extremely complex, comprising at least three major components (L1, L1N, L2SW) in the case of SMM J02399-0136: if we look in detail (see the Hubble Space Telescope imaging on the right), we often find that the starburst (L2SW in this case, identified via high-resolution radio imaging) is faint (often invisible) in the UV/optical waveband, even in deep post-SM4 HST imaging, with the optical light dominated by a BAL quasar (labelled L1 here) which isn't responsible for much (if any) of the submillimetre emission. Reddened or reflected starlight sometimes leaks out on the periphery (L2 may be reflected light in this particular case).
The far-infrared luminosity of a galaxy can be used to infer the rate at which it is forming stars (as most of the UV radiation comes from massive stars which don't live very long). The many 1000s of stars formed each year in most of these galaxies - together with the immense quantities of molecular gas that we infer via millimetric observations of carbon monoxide (CO) - indicate that we are probably seeing the formation of massive galaxies. Our surveys in this waveband have demonstrated that roughly half the star formation in the entire history of the Universe has occurred in highly obscured environments, invisible to surveys in the UV/optical. Investigating the detailed properties of this population is a very active field of study.
I'm married to a divine Mackem lass, and we have two adorable/demonic children - one of each (ambiguity intended). I hail from Blackburn, Lancashire, which has a fine history of one-downsmanship (a concept lost on most academics). I'm a fan of Blackburn Rovers, for my sins, though I've made a largely successful effort to get `clean' of football. I attend manic, daily RPM/spinning classes in my local tennis centre, I run (slowly, painfully), play golf (astronomical handicap), potter in my garden and allotment, and spend 72/73rds of the year looking forward to Glastonbury.
Last Modified: 24th July 2017.
ESO, Karl Schwarzschild Strasse 2, D-85748 Garching, Munich, Germany
Tel: +49-89-3200-6669 / Cell: +49-151-185-63-662 / email: rob.ivison [at] eso.org