activity
19932026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 27.5k across the 205 of their papers we have counts for

collaborators

205 papers

astro-ph.GA2026

Calibrating Mid-Infrared Emission Features As Diagnostics of Star Formation in Infrared-Luminous Galaxies via Radiative Transfer Modeling

L. Robinson, D. Farrah, A. Efstathiou +13

Luminous infrared galaxies are key sites of obscured stellar mass assembly at z > 0.5. Their star formation rates (SFRs) are often estimated using the luminosities of the 6.2 micro…

astro-ph.GA2025

Modelling JWST mid-infrared counts II: Extension to 5.6 μm, optical, radio and X-rays

Michael Rowan-Robinson

In Paper I (Rowan-Robinson 2024), models derived in 2009 to fit mid-infrared (8-24 micron) source counts from the IRAS, ISO and Spitzer missions, were found to provide an excellent…

astro-ph.GA2023

Modelling JWST mid-infrared counts: excellent consistency with models derived for IRAS, ISO and Spitzer

Michael Rowan-Robinson

Models derived in 2009 to fit mid-infrared (8-24 micron) source counts from the IRAS, ISO and Spitzer missions, provide an excellent fit to deep counts with JWST, demonstrating tha…

astro-ph.GA2022★ 32 cited

Stellar and black hole assembly in z<0.3 infrared-luminous mergers: intermittent starbursts vs. super-Eddington accretion

Duncan Farrah, Andreas Efstathiou, Jose Afonso +20

We study stellar and black hole mass assembly in a sample of 42 infrared-luminous galaxy mergers at z<0.3 by combining results from radiative transfer modelling with archival measu…

astro-ph.EP2021★ 8 cited

A search for Planet 9 in the IRAS data

Michael Rowan-Robinson

I have carried out a search for Planet 9 in the IRAS data. At the distance range proposed for Planet 9, the signature would be a 60 micron unidentified IRAS point source with an as…

astro-ph.GA2018★ 3 cited

AKARI and IRAS: From Beam Corrections to SEDs

David L. Clements, Michael Rowan-Robinson, Chris Pearson +6

There is significant scientific value to be gained from combining AKARI fluxes with data at other far-IR wavelengths from the IRAS and Herschel missions. To be able to do this we m…