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

Autor: Anthony P. Jones, Christopher J. R. Clark, Jonathan Ivor Davies, Sébastien Viaene, M. Xilouris, Nathalie Ysard, Suzanne C. Madden, G. Wagle, M. Vika, Aleksandr V. Mosenkov, Sophia Lianou, Maud Galametz, Matthew Smith, Viviana Casasola, M. Bocchio, S. Verstocken, Letizia P. Cassarà, I. De Looze, Frédéric Galliano, Maarten Baes, Simone Bianchi, Jacopo Fritz, Richard Evans

Publikováno v: Publications of the Astronomical Society of the Pacific
Publications of the Astronomical Society of the Pacific, 2017, 129 (974), pp.044102. ⟨10.1088/1538-3873/129/974/044102⟩
Publications of the Astronomical Society of the Pacific, Astronomical Society of the Pacific, 2017, ⟨10.1088/1538-3873/129/974/044102⟩
Publ.Astron.Soc.Pac.
Publ.Astron.Soc.Pac., 2017, 129, pp.044102. 〈10.1088/1538-3873/129/974/044102〉
Publ.Astron.Soc.Pac., 2017, 129 (974), pp.044102. ⟨10.1088/1538-3873/129/974/044102⟩
Publications of the Astronomical Society of the Pacific, Astronomical Society of the Pacific, 2017, 129 (974), pp.044102. ⟨10.1088/1538-3873/129/974/044102⟩

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 to study cosmic dust in galaxies so that we can answer fundamental que

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aed61a647504af9e8f6444b6b191f434
https://hal.science/hal-02137562

Convolution kernels for multi-wavelength imaging

Autor: Alain Abergel, François Orieux, Alexandre Boucaud, M. Bocchio, H. Dole, Mohamed Amine Hadj-Youcef

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 596, pp.A63. ⟨10.1051/0004-6361/201629080⟩
Astronomy and Astrophysics-A&A, 2016, 596, pp.A63. ⟨10.1051/0004-6361/201629080⟩

Astrophysical images issued from different instruments and/or spectral bands often require to be processed together, either for fitting or comparison purposes. However each image is affected by an instrumental response, also known as PSF, that depend

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::845a7f4de28417053a5b63640c5b829f
https://hal.sorbonne-universite.fr/hal-01465825

The metal and dust yields of the first massive stars

Autor: Stefania Marassi, Simone Bianchi, Raffaella Schneider, Alessandro Chieffi, M. Bocchio, Marco Limongi

We quantify the role of Population (Pop) III core-collapse supernovae (SNe) as the first cosmic dust polluters. Starting from a homogeneous set of stellar progenitors with masses in the range [13 - 80] Msun, we find that the mass and composition of n

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f353560f019bc156820c723820fdcecf

The Herschel Fornax Cluster Survey II : FIR properties of optically selected Fornax cluster galaxies

Autor: M. S. Clemens, Jonathan Ivor Davies, I. De Looze, Alessandro Boselli, Robbie Richard Auld, Simone Bianchi, P. Serra, M. Bocchio, Maarten Baes, M. Grossi, Matthew Smith, Thomas M. Hughes, Timothy A. Davis, Sébastien Viaene, Crispian Fuller, S. di Serego Alighieri

Publikováno v: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 440 (2), pp.1571--1589. ⟨10.1093/mnras/stu369⟩
Monthly Notices of the Royal Astronomical Society, 2014, 440 (2), pp.1571--1589. ⟨10.1093/mnras/stu369⟩

The $Herschel$ Fornax Cluster Survey (HeFoCS) is a deep, far-infrared (FIR) survey of the Fornax cluster. The survey is in 5 $Herschel$ bands (100 - 500 $\mu$m) and covers an area of 16 deg$^2$ centred on NGC1399. This paper presents photometry, dete

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4972d20783976000cd76576278d77c35
https://biblio.ugent.be/publication/5921303/file/5921737

Gas-to-Dust mass ratios in local galaxies over a 2 dex metallicity range

Autor: Svitlana Zhukovska, Maarten Baes, Thomas M. Hughes, Frédéric Galliano, I. Delooze, S. C. Madden, Ryosuke Asano, M. Bocchio, Tsutomu T. Takeuchi, L. Spinoglio, A. Rémy-Ruyer, D. Cormier, O. Ł. Karczewski, Médéric Boquien, Vianney Lebouteiller, V. Doublier-Pritchard, George J. Bendo, Anthony P. Jones, Alessandro Boselli, Maud Galametz

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 563, pp.A31. ⟨10.1051/0004-6361/201322803⟩
Astronomy and Astrophysics-A&A, 2014, 563, pp.A31. ⟨10.1051/0004-6361/201322803⟩
ASTRONOMY & ASTROPHYSICS

This paper analyses the behaviour of the gas-to-dust mass ratio (G/D) of local Universe galaxies over a large metallicity range. We combine three samples: the Dwarf Galaxy Survey, the KINGFISH survey and a subsample from Galametz et al. (2011) totall

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a6553411b22079db491c6186e2379b67
http://arxiv.org/abs/1312.3442