109 citations · 787 across the 29 of their papers we have counts for
30 papers
Monitoring the radio emission of Proxima Centauri
Miguel Pérez-Torres, José Francisco Gómez, José Luis Ortiz +15
We present results from the most comprehensive radio monitoring campaign towards the closest star to our Sun, Proxima Centauri. We report 1.1 to 3.1 GHz observations with the Austr…
VLBI20-30: a scientific roadmap for the next decade -- The future of the European VLBI Network
Tiziana Venturi, Zsolt Paragi, Michael Lindqvist +77
This white paper describes the science case for Very Long Baseline Interferometry (VLBI) and provides suggestions towards upgrade paths for the European VLBI Network (EVN). The EVN…
Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey
R. Herrero-Illana, G. C. Privon, A. S. Evans +23
We present IRAM-30m Telescope CO and CO observations of a sample of 55 luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) in the local universe. This sam…
Science with an ngVLA: Radio Continuum Emission from Galaxies: An Accounting of Energetic Processes
Eric J. Murphy, James J. Condon, Antxon Alberdi +14
Radio continuum observations have proven to be a workhorse in our understanding of the star formation process (i.e., stellar birth and death) from galaxies both in the nearby unive…
GW170817: implications for the local kilonova rate and for surveys from ground-based facilities
M. Della Valle, D. Guetta, E. Cappellaro +7
We compute the local rate of events similar to GRB 170817A, which has been recently found to be associated with a kilonova (KN) outburst. Our analysis finds an observed rate of suc…
Sub-arcsecond imaging of Arp\,299-A at 150 MHz with LOFAR: Evidence for a starburst-driven outflow
Naím Ramírez-Olivencia, Eskil Varenius, Miguel Pérez-Torres +8
We report on the first sub-arcsecond (0.44 0.41 arcsec) angular resolution image at 150 MHz of the A-nucleus in the Luminous Infrared Galaxy Arp299, from Inter…
No AGN evidence in NGC1614 from deep radio VLBI observations
Rubén Herrero-Illana, Antxon Alberdi, Miguel Ángel Pérez-Torres +3
We present deep dual-band 5.0 and 8.4GHz European VLBI Network (EVN) observations of NGC1614, a local luminous infrared galaxy with a powerful circumnuclear starburst ring, and who…
Star formation and AGN activity in a sample of local Luminous Infrared Galaxies through multi-wavelength characterization
Rubén Herrero-Illana, Miguel Á. Pérez-Torres, Zara Randriamanakoto +8
Nuclear starbursts and AGN activity are the main heating processes in luminous infrared galaxies (LIRGs) and their relationship is fundamental to understand galaxy evolution. In th…
Unveiling the AGN in IC 883: discovery of a parsec-scale radio jet
Cristina Romero-Cañizales, Antxon Alberdi, Claudio Ricci +12
IC883 is a luminous infrared galaxy (LIRG) classified as a starburst-active galactic nucleus (AGN) composite. In a previous study we detected a low-luminosity AGN (LLAGN) radio can…
Radio continuum and X-ray emission from the most extreme FIR-excess galaxy NGC 1377: An extremely obscured AGN revealed
F. Costagliola, R. Herrero-Illana, A. Lohfink +4
Galaxies which strongly deviate from the radio-far IR correlation are of great importance for studies of galaxy evolution as they may be tracing early, short-lived stages of starbu…
Nearby supernova host galaxies from the CALIFA Survey: II. SN environmental metallicity
L. Galbany, V. Stanishev, A. M. Mourão +16
The metallicity of a supernova (SN) progenitor, together with its mass, is one of the main parameters that rules their outcome. We present a metallicity study of 115 nearby SN host…
Discovery of off-axis jet structure of TeV blazar Mrk 501 with mm-VLBI
S. Koyama, M. Kino, M. Giroletti +10
High-resolution millimeter wave very-long-baseline interferometry (mm-VLBI) is an ideal tool for probing the structure at the base of extragalactic jets in detail. The TeV blazar M…
Discovery of TeV gamma-ray emission from the pulsar wind nebula 3C 58 by MAGIC
R. López-Coto, E. Carmona, W. Bednarek +6
The pulsar wind nebula (PWN) 3C 58 has been proposed as a good candidate for detection at VHE (VHE; E>100 GeV) for many years. It is powered by one of the highest spin-down power p…
Excitation Mechanisms for HCN (1-0) and HCO+ (1-0) in Galaxies from the Great Observatories All-sky LIRG Survey
G. C. Privon, R. Herrero-Illana, A. S. Evans +18
We present new IRAM 30m spectroscopic observations of the GHz band, including emission from the CCH (n=1-0) multiplet, HCN (1-0), HCO+ (1-0), and HNC (1-0), for a sample o…
Star Formation in the Local Universe from the CALIFA sample. I. Calibrating the SFR using IFS data
C. Catalán-Torrecilla, A. Gil de Paz, A. Castillo-Morales +24
The Star Formation Rate (SFR) is one of the main parameters used to analyze the evolution of galaxies through time. The need for recovering the light reprocessed by dust commonly r…
The off-axis jet structure in Mrk 501 at mm-wavelengths
Shoko Koyama, Motoki Kino, Marcello Giroletti +10
We present results from 43 GHz (VLBA, six epochs from 2012.2 to 2013.2) and 86 GHz (GMVA, one epoch in 2012.4) observations toward the basis of the jet in the TeV Blazar Mrk 501. T…
Discovery of TeV gamma-ray emission from the Pulsar Wind Nebula 3C 58 by MAGIC
O. Blanch Bigas, R. Lopez, E. Carmona +2
The Pulsar Wind Nebula (PWN) 3C 58 is energized by one of the highest spin-down power pulsars known (5% of Crab pulsar) and it has been compared to the Crab Nebula due to their mor…
Very Long Baseline Interferometry with the SKA
Zsolt Paragi, Leith Godfrey, Cormac Reynolds +79
Adding VLBI capability to the SKA arrays will greatly broaden the science of the SKA, and is feasible within the current specifications. SKA-VLBI can be initially implemented by pr…
Nearby supernova host galaxies from the CALIFA Survey: I. Sample, data analysis, and correlation to star-forming regions
L. Galbany, V. Stanishev, A. M. Mourão +25
[Abridged] We use optical IFS of nearby SN host galaxies provided by the CALIFA Survey with the goal of finding correlations in the environmental parameters at the location of diff…
Core-collapse and Type Ia supernovae with the SKA
M. A. Pérez-Torres, A. Alberdi, R. J. Beswick +10
Core-collapse SNe (CCSNe): Systematic searches of radio emission from CCSNe are still lacking, and only targeted searches of radio emission from just some of the optically discover…
MAGIC search for VHE -ray emission from AE Aquarii in a multiwavelength context
J. Aleksić, S. Ansoldi, L. A. Antonelli +152
It has been claimed that the nova-like cataclysmic variable (CV) AE Aquarii (AE Aqr) is a very-high-energy (VHE, 100 GeV) source both on observational and theoretical grounds.…
A multi-wavelength view of the central kiloparsec region in the Luminous Infrared Galaxy NGC1614
Rubén Herrero-Illana, Miguel Á. Pérez-Torres, Almudena Alonso-Herrero +9
The Luminous Infrared Galaxy NGC1614 hosts a prominent circumnuclear ring of star formation. However, the nature of the dominant emitting mechanism in its central ~100 pc is still…
The nature of supernovae 2010O and 2010P in Arp 299 - II. Radio emission
C. Romero-Cañizales, R. Herrero-Illana, M. A. Pérez-Torres +8
We report radio observations of two stripped-envelope supernovae (SNe), 2010O and 2010P, which exploded within a few days of each other in the luminous infrared galaxy Arp 299. Whi…
The nature of supernovae 2010O and 2010P in Arp 299 - I. Near-infrared and optical evolution
E. Kankare, S. Mattila, S. Ryder +10
We present near-infrared and optical photometry, plus optical spectroscopy of two stripped-envelope supernovae (SNe) 2010O and 2010P that exploded in two different components of an…