activity
20002025
most citedMultidimensional supernova simulations with approximative neutrino transport. II. Convection and the advective-acoustic cycle in the supernova core

196 citations · 545 across the 26 of their papers we have counts for

collaborators

28 papers

astro-ph.IM2025

Euclid preparation: The NISP spectroscopy channel, on ground performance and calibration

Euclid Collaboration, W. Gillard, T. Maciaszek +356

ESA's Euclid cosmology mission relies on the very sensitive and accurately calibrated spectroscopy channel of the Near-Infrared Spectrometer and Photometer (NISP). With three opera…

astro-ph.GA2022★ 9 cited

Mid-infrared imaging of Supernova 1987A

Mikako Matsuura, Roger Wesson, Richard G. Arendt +9

At a distance of 50 kpc, Supernova 1987A is an ideal target to study how a young supernova (SN) evolves in time. Its equatorial ring, filled with material expelled from the progeni…

astro-ph.GA2022★ 21 cited

The Black Hole-Galaxy Connection: Interplay between Feedback, Obscuration, and Host Galaxy Substructure

Stéphanie Juneau, Andy D. Goulding, Julie Banfield +20

There is growing evidence for physical influence between supermassive black holes and their host galaxies. We present a case study of nearby galaxy NGC 7582, for which we find evid…

astro-ph.GA2018★ 30 cited

The integrated properties of the CALIFA galaxies: Model-derived galaxy parameters and quenching of star formation

T. Bitsakis, S. F. Sanchez, L. Ciesla +6

We present a study of the integrated properties of the 835 galaxies in the CALIFA survey. To derive the main physical parameters of the galaxies we have fitted their UV-to-IR spect…

astro-ph.HE2017★ 17 cited

Microquasars as heating sources of the intergalactic medium during reionisation of the Universe

Vanesa M. Douna, Leonardo J. Pellizza, Philippe Laurent +1

The effect of the primeval sources of radiation and particles on the thermodynamical state of the intergalactic medium during the Epoch of Reionisation is still unclear. In this wo…

astro-ph.HE2011

Revealing the nature of high-mass X-ray binaries through multi-wavelength and statistical analyses

Arash Bodaghee, John A. Tomsick, Jerome Rodriguez

We summarize the results of our long-running campaign to help understand the nature of high-mass X-ray binaries (HMXBs), emphasizing recent Suzaku observations of IGR J16207-5129 a…