activity
20032022
most citedThe Low-Redshift Lyman Continuum Survey I: New, Diverse Local Lyman-Continuum Emitters

180 citations · 625 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2022★ 164 cited

The Low-Redshift Lyman Continuum Survey II: New Insights into LyC Diagnostics

Sophia R. Flury, Anne E. Jaskot, Harry C. Ferguson +44

The Lyman continuum (LyC) cannot be observed at the epoch of reionization (z {\gtrsim} 6) due to intergalactic H I absorption. To identify Lyman continuum emitters (LCEs) and infer…

astro-ph.GA2022★ 180 cited

The Low-Redshift Lyman Continuum Survey I: New, Diverse Local Lyman-Continuum Emitters

Sophia R. Flury, Anne E. Jaskot, Harry C. Ferguson +44

The origins of Lyman continuum (LyC) photons responsible for the reionization of the universe are as of yet unknown and highly contested. Detecting LyC photons from the epoch of re…

astro-ph.GA2020★ 5 cited

Low-redshift quasars in the SDSS Stripe 82 II: associated companion galaxies and signature of star formation

Maria Babakhanyan Stone, Daniela Bettoni, Renato Falomo +4

We present optical spectroscopy of the close companions of 22 low redshift (z<0.5) quasars (QSO) selected from a larger sample of QSO in the SDSS Stripe82 region for which both the…

astro-ph.HE2017★ 26 cited

AX J1910.7+0917: the slowest X-ray pulsar

L. Sidoli, G. L. Israel, P. Esposito +2

Pulsations from the high mass X-ray binary AXJ1910.7+0917 were discovered during Chandra observations performed in 2011 (Israel et al. 2016). We report here more details on this di…

astro-ph.HE2009★ 5 cited

The Behavior of Matter under Extreme Conditions

F. Paerels, M. Mendez, M. Agueros +29

The cores of neutron stars harbor the highest matter densities known to occur in nature, up to several times the densities in atomic nuclei. Similarly, magnetic field strengths can…

astro-ph2007★ 27 cited

The red and blue galaxy populations in the GOODS field: evidence for an excess of red dwarfs

S. Salimbeni, E. Giallongo, N. Menci +8

We study the evolution of the galaxy population up to z\sim3 as a function of its colour properties. In particular, luminosity functions and luminosity densities have been derived…