156 citations · 260 across the 7 of their papers we have counts for
7 papers
Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers
C. Mondal, M. Antonelli, F. Gulminelli +3
Possible strong first-order hadron-quark phase transitions in neutron star interiors leave an imprint on gravitational waves, which could be detected with planned third-generation…
RFI Flagging in Solar and Space Weather Low Frequency Radio Observations
Peijin Zhang, André R. Offringa, Pietro Zucca +2
Radio spectroscopy provides a unique inspection perspective for solar and space weather research, which can reveal the plasma and energetic electron information in the solar corona…
Continuum source catalog for the first APERTIF data release
A. M. Kutkin, T. A. Oosterloo, R. Morganti +25
The first data release of Apertif survey contains 3074 radio continuum images covering a thousand square degrees of the sky. The observations were performed during August 2019 to J…
CompOSE Reference Manual
S. Typel, M. Oertel, T. Klähn +10
CompOSE (CompStar Online Supernovae Equations of State) is an online repository of equations of state (EoS) for use in nuclear physics and astrophysics, e.g., in the description of…
"Zombie" or active? An alternative explanation to the properties of star-forming galaxies at high redshift
Francesco Gabriele Saturni, Mattia Mancini, Edwige Pezzulli +1
Star-forming galaxies at high redshift show anomalous values of infrared excess, which can be described only by extremizing the existing relations between the shape of their ultrav…
Interpreting the evolution of galaxy colours from to
Mattia Mancini, Raffaella Schneider, Luca Graziani +4
We attempt to interpret existing data on the evolution of the UV luminosity function and UV colours, , of galaxies at , to improve our understanding of their du…
The dust mass in z > 6 normal star forming galaxies
Mattia Mancini, Raffaella Schneider, Luca Graziani +5
We interpret recent ALMA observations of z > 6 normal star forming galaxies by means of a semi-numerical method, which couples the output of a cosmological hydrodynamical simulatio…