output
20082022
most citedThe Herschel-ATLAS Data Release 1 Paper I: Maps, Catalogues and Number Counts

202 citations

36 papers

math.OA2022★ 2 cited

Étale categories, restriction semigroups, and their operator algebras

Natã Machado, Gilles G. de Castro

We define the full and reduced non-self-adjoint operator algebras associated with étale categories and restriction semigroups, answering a question posed by Kudryavtseva and Lawson…

astro-ph.GA2017★ 20 cited

Dynamical equivalence, the origin of the Galactic field stellar and binary population, and the initial radius--mass relation of embedded clusters

Diogo Belloni, Pavel Kroupa, Helio J. Rocha-Pinto +1

In order to allow a better understanding of the origin of Galactic field populations, dynamical equivalence of stellar-dynamical systems has been postulated by Kroupa and Belloni e…

astro-ph.GA2017★ 59 cited

The Herschel Bright Sources (HerBS): Sample definition and SCUBA-2 observations

Tom J. L. C. Bakx, S. A. Eales, M. Negrello +20

We present the Herschel Bright Sources (HerBS) sample, a sample of bright, high-redshift Herschel sources detected in the 616.4 square degree H-ATLAS survey. The HerBS sample conta…

astro-ph.GA2017★ 29 cited

On the relation between the mass of Compact Massive Objects and their host galaxies

R. Capuzzo-Dolcetta, I. Tosta e Melo

Supermassive black holes and/or very dense stellar clusters are found in the central regions of galaxies. Nuclear star clusters are present mainly in faint galaxies while upermassi…

astro-ph.GA2017★ 97 cited

The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation

F. Stanley, D. M. Alexander, C. M. Harrison +15

We investigate the mean star formation rates (SFRs) in the host galaxies of ~3000 optically selected QSOs from the SDSS survey within the Herschel-ATLAS fields, and a radio-luminou…

astro-ph.GA2017★ 65 cited

On the initial binary population for star cluster simulations

Diogo Belloni, Abbas Askar, Mirek Giersz +2

Colour-magnitude diagrams (CMDs) are powerful tools that might be used to infer stellar properties in globular clusters (GCs), for example, the binary fraction and their mass ratio…