activity
20112025
most citedConstraining the properties of AGN host galaxies with Spectral Energy Distribution modeling

251 citations · 876 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.IM2025

PRIMA survey of the Virgo cluster

Jacopo Fritz, Maarten Baes, Diego Alejandro Vasquez Torres +11

Clusters of galaxies are unique laboratories for investigating the dependence of galaxy evolution on their environment. The Herschel Virgo Cluster Survey (HeViCS) mapped the centra…

astro-ph.SR2018★ 64 cited

The Near-Ultraviolet Continuum Radiation in the Impulsive Phase of HF/GF-Type dMe Flares I: Data

Adam F. Kowalski, John P. Wisniewski, Suzanne L. Hawley +8

We present NUV flare spectra from the Hubble Space Telescope/Cosmic Origins Spectrograph during two moderate-amplitude U-band flares on the dM4e star GJ 1243. These spectra are som…

astro-ph.GA2018★ 30 cited

Spatially resolving the dust properties and submillimetre excess in M 33

M. Relaño, I. De Looze, R. C. Kennicutt +9

The relative abundance of the dust grain types in the interstellar medium (ISM) is directly linked to physical quantities that trace the evolution of galaxies. We study the dust pr…

astro-ph.GA2017★ 126 cited

DustPedia: Multiwavelength Photometry and Imagery of 875 Nearby Galaxies in 42 Ultraviolet--Microwave Bands

Christopher J. R. Clark, S. Verstocken, S. Bianchi +16

The DustPedia project is capitalising on the legacy of the Herschel Space Observatory, using cutting-edge modelling techniques to study dust in the 875 DustPedia galaxies - represe…

astro-ph.GA2017★ 102 cited

From molecules to Young Stellar Clusters: the star formation cycle across the M33 disk

Edvige Corbelli, Jonathan Brain, Rino Bandiera +8

To shed light on the time evolution of local star formation episodes in M33, we study the association between 566 Giant Molecular Clouds (GMCs), identified through the CO (J=2-1) I…

astro-ph.GA2016★ 138 cited

DustPedia - A Definitive Study of Cosmic Dust in the Local Universe

J. I. Davies, M. Baes, S. Bianchi +20

The European Space Agency has invested heavily in two cornerstones missions; Herschel and Planck. The legacy data from these missions provides us with an unprecedented opportunity…

astro-ph.GA2016★ 20 cited

Dust Properties in HII Regions in M33

M. Relano, R. Kennicutt, U. Lisenfeld +11

The conversion of the IR emission into star formation rate can be strongly dependent on the physical properties of the dust, which are affected by the environmental conditions wher…

astro-ph.EP2015★ 5 cited

NELIOTA: ESA's new NEO lunar impact monitoring project with the 1.2m telescope at the National Observatory of Athens

A. Z. Bonanos, M. Xilouris, P. Boumis +7

NELIOTA is a new ESA activity launched at the National Observatory of Athens in February 2015 aiming to determine the distribution and frequency of small near-earth objects (NEOs)…

astro-ph.GA2015★ 56 cited

Measuring star formation with resolved observations: the test case of M33

M. Boquien, D. Calzetti, S. Aalto +15

Context. Measuring star formation at a local scale is important to constrain star formation laws. Yet, it is not clear whether and how the measure of star formation is affected by…

astro-ph.GA2015★ 251 cited

Constraining the properties of AGN host galaxies with Spectral Energy Distribution modeling

L. Ciesla, V. Charmandaris, A. Georgakakis +8

[abridged] We use the latest release of CIGALE, a galaxy SED fitting model relying on energy balance, to study the influence of an AGN in estimating both the SFR and stellar mass i…

astro-ph.GA2014★ 28 cited

The Heating of Mid-Infrared Dust in the Nearby Galaxy M33: A Testbed for Tracing Galaxy Evolution

M. Calapa, D. Calzetti, B. T. Draine +10

Because the 8 μm polycyclic aromatic hydrocarbon (PAH) emission has been found to correlate with other well-known star formation tracers, it has widely been used as a star formatio…

astro-ph.GA2012★ 1 cited

The molecular gas in Luminous Infrared Galaxies: a new emergent picture

Padelis P. Papadopoulos, Zhi-Yu Zhang, Axel Weiss +5

Results from a large, multi-J CO, {13}CO, and HCN line survey of Luminous Infrared Galaxies (L_{IR}>=10^{10} L_{\odot}) in the local Universe (z<=0.1), complemented by CO J=4--3 up…

astro-ph.CO2012★ 47 cited

Herschel/SPIRE Observations of the Dusty Disk of NGC 4244

B. W. Holwerda, S. Bianchi, T. Böker +7

We present Herschel/SPIRE images at 250, 350, and 500 μm of NGC 4244, a typical low-mass, disk-only and edge-on spiral galaxy. The dust disk is clumpy and shows signs of truncation…

astro-ph.CO2011★ 3 cited

Variation in the dust spectral index across M33

F. S. Tabatabaei, J. Braine, C. Kramer +9

Using the Herschel PACS and SPIRE FIR/submm data, we investigate variations in the dust spectral index in the nearby spiral galaxy M33 at a linear resolution of 160 pc. We use…

astro-ph.CO2011★ 5 cited

New HErschel Multi-wavelength Extragalactic Survey of Edge-on Spirals (NHEMESES)

B. W. Holwerda, S. Bianchi, M. Baes +5

Edge-on spiral galaxies offer a unique perspective on the vertical structure of spiral disks, both stars and the iconic dark dustlanes. The thickness of these dustlanes can now be…