activity
20032023
most citedBinary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results

953 citations · 8k across the 76 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.HE2016★ 74 cited

LOSS Revisited - I: Unraveling correlations between supernova rates and galaxy properties, as measured in a reanalysis of the Lick Observatory Supernova Search

Or Graur, Federica B. Bianco, Shan Huang +5

Most types of supernovae (SNe) have yet to be connected with their progenitor stellar systems. Here, we reanalyze the 10-year SN sample collected during 1998-2008 by the Lick Obser…

astro-ph.GA2016★ 65 cited

No evidence for Population III stars or a Direct Collapse Black Hole in the z = 6.6 Lyman- emitter 'CR7'

R. A. A. Bowler, R. J. McLure, J. S. Dunlop +4

The z = 6.6 Lyman- emitter 'CR7' has been claimed to have a Population III-like stellar population, or alternatively, be a candidate Direct Collapse Black Hole (DCBH). In this p…

astro-ph.HE2016★ 49 cited

Diffuse Galactic antimatter from faint thermonuclear supernovae in old stellar populations

Roland M. Crocker, Ashley J. Ruiter, Ivo R. Seitenzahl +10

Our Galaxy hosts the annihilation of a few low-energy positrons every second. Radioactive isotopes capable of supplying such positrons are synthesised in stars, st…

astro-ph.SR2016★ 106 cited

Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries

T. Shenar, R. Hainich, H. Todt +7

Massive WR stars are evolved massive stars characterized by strong mass-loss. Hypothetically, they can form either as single stars or as mass donors in close binaries. About 40% of…

astro-ph.HE2016★ 270 cited

BPASS predictions for Binary Black-Hole Mergers

J. J. Eldridge, E. R. Stanway

Using the Binary Population and Spectral Synthesis code BPASS, we have calculated the rates, timescales and mass distributions for binary black hole mergers as a function of metall…

astro-ph.HE2016★ 5 cited

Progenitor constraints for core-collapse supernovae from Chandra X-ray observations

T. Heikkilä, S. Tsygankov, S. Mattila +3

The progenitors of hydrogen-poor core-collapse supernovae (SNe) of types Ib, Ic and IIb are believed to have shed their outer hydrogen envelopes either by extremely strong stellar…