Zobrazeno 1 - 10
of 81
pro vyhledávání: '"Viaene, Sébastien"'
This paper addresses a long-standing problem in the field of accounting: mapping company-specific ledger accounts to a standardized chart of accounts. We propose a novel solution, TopoLedgerBERT, a unique sentence embedding method devised specificall
Externí odkaz:
http://arxiv.org/abs/2407.05175
Publikováno v:
The Astrophysical Journal, 2024, Vol 966, 193
Deep interferometric observations of CO and dust continuum emission are obtained with the Sub-Millimeter Array (SMA) at 230 GHz to investigate the physical nature of the giant molecular cloud (GMC) population in the Andromeda galaxy (M31). We use J =
Externí odkaz:
http://arxiv.org/abs/2403.19746
Autor:
Pappalardo, Ciro, Bendo, George J., Boquien, Mederic, Baes, Maarten, Viaene, Sebastien, Bianchi, Simone, Fritz, Jacopo
Publikováno v:
A&A 655, A104 (2021)
In recent years, significant growth in the amount of data available to astronomers has opened up the possibility to uncover fundamental correlations, linking the dust component of a galaxy to its star formation rate (SFR). In this paper, we re-examin
Externí odkaz:
http://arxiv.org/abs/2110.00022
VALES VIII: Weak ionized gas outflows in star-forming galaxies at $z \sim 0.15$ traced with VLT/MUSE
Autor:
Couto, Guilherme S., Hughes, Thomas M., Boquien, Médéric, Ibar, Eduardo, Viaene, Sébastien, Leiton, Roger, Xue, Yongquan
Publikováno v:
A&A 654, A128 (2021)
We characterize the ionized gas outflows in 15 low-redshift star-forming galaxies, a Valpara\'iso ALMA Line Emission Survey (VALES) subsample, using MUSE integral field spectroscopy and GAMA photometric broadband data. We measure the emission-line sp
Externí odkaz:
http://arxiv.org/abs/2108.02334
We present simultaneous measurements of emission from dust continuum at 230 GHz and the J=2-1 $^{12}$CO, $^{13}$CO and C$^{18}$O isotopologues at $\sim$ 15 pc resolution from individual Giant Molecular Clouds (GMCs) in the Andromeda galaxy (M31). The
Externí odkaz:
http://arxiv.org/abs/2102.07129
Autor:
Nersesian, Angelos, Viaene, Sebastien, De Looze, Ilse, Baes, Maarten, Xilouris, Emmanuel M., Smith, Matthew W. L., Bianchi, Simone, Casasola, Viviana, Cassara, Letizia P., Clark, Christopher J. R., Dobbels, Wouter, Fritz, Jacopo, Galliano, Frederic, Madden, Suzanne C., Mosenkov, Aleksandr V., Trcka, Ana
Publikováno v:
A&A 643, A90 (2020)
Investigating the dust heating mechanisms in galaxies provides a deeper understanding of how the internal energy balance drives their evolution. Over the last decade, radiative transfer simulations based on the Monte Carlo method have underlined the
Externí odkaz:
http://arxiv.org/abs/2009.07280
Autor:
Baes, Maarten, Nersesian, Angelos, Casasola, Viviana, Bianchi, Simone, Cassarà, Letizia P., Clark, Christopher J. R., De Looze, Ilse, Dobbels, Wouter, Fritz, Jacopo, Galametz, Maud, Galliano, Frédéric, Madden, Suzanne C., Mosenkov, Aleksandr V., Viaene, Sébastien, Trčka, Ana, Xilouris, Emmanuel M.
Publikováno v:
A&A 641, A119 (2020)
We present the first nonparametric morphological analysis of a set of spiral galaxies from UV to submm wavelengths. Our study is based on high-quality multi-wavelength imaging for nine well-resolved spiral galaxies from the DustPedia database, combin
Externí odkaz:
http://arxiv.org/abs/2007.02012
Autor:
Zabel, Nikki, Davis, Timothy A., Sarzi, Marc, Nedelchev, Boris, Chevance, Mélanie, Kruijssen, J. M. Diederik, Iodice, Enrichetta, Baes, Maarten, Bendo, George J., Corsini, Enrico Maria, De Looze, Ilse, de Zeeuw, P. Tim, Gadotti, Dimitri A., Grossi, Marco, Peletier, Reynier, Pinna, Francesca, Serra, Paolo, van de Voort, Freeke, Venhola, Aku, Viaene, Sébastien, Vlahakis, Catherine
We combine data from ALMA and MUSE to study the resolved (~300 pc scale) star formation relation (star formation rate vs. molecular gas surface density) in cluster galaxies. Our sample consists of 9 Fornax cluster galaxies, including spirals, ellipti
Externí odkaz:
http://arxiv.org/abs/2005.13454
Autor:
Verstocken, Sam, Nersesian, Angelos, Baes, Maarten, Viaene, Sébastien, Bianchi, Simone, Casasola, Viviana, Clark, Christopher J. R., Davies, Jonathan I., De Looze, Ilse, De Vis, Pieter, Dobbels, Wouter, Galliano, FrédÉric, Jones, Anthony P., Madden, Suzanne C., Mosenkov, Aleksandr V., Trčka, Ana, Xilouris, Emmanuel M.
Publikováno v:
A&A 637, A24 (2020)
Interstellar dust absorbs stellar light very efficiently and thus shapes the energetic output of galaxies. Studying the impact of different stellar populations on the dust heating remains hard because it requires decoupling the relative geometry of s
Externí odkaz:
http://arxiv.org/abs/2004.03615
Autor:
Nersesian, Angelos, Verstocken, Sam, Viaene, Sebastien, Baes, Maarten, Xilouris, Emmanuel M., Bianchi, Simone, Casasola, Viviana, Clark, Christopher J. R., Davies, Jonathan I., De Looze, Ilse, De Vis, Pieter, Dobbels, Wouter, Fritz, Jacopo, Galametz, Maud, Galliano, Frederic, Jones, Anthony P., Madden, Suzanne C., Mosenkov, Aleksandr V., Trcka, Ana, Ysard, Nathalie
Context: Dust in late-type galaxies in the local Universe is responsible for absorbing approximately one third of the energy emitted by stars. It is often assumed that dust heating is mainly attributable to the absorption of UV and optical photons em
Externí odkaz:
http://arxiv.org/abs/2004.03616