R
R. Carraro
Researcher at Valparaiso University
Publications - 24
Citations - 546
R. Carraro is an academic researcher from Valparaiso University. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 11, co-authored 19 publications receiving 348 citations. Previous affiliations of R. Carraro include University of Padua.
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Journal ArticleDOI
The ALPINE-ALMA [CII] survey: Star-formation-driven outflows and circumgalactic enrichment in the early Universe
Michele Ginolfi,G. C. Jones,M. Bethermin,Y. Fudamoto,F. Loiacono,Seiji Fujimoto,O. Le Fevre,Andreas L. Faisst,Daniel Schaerer,Paolo Cassata,John D. Silverman,Lin Yan,Peter Capak,S. Bardelli,Médéric Boquien,R. Carraro,Miroslava Dessauges-Zavadsky,M. Giavalisco,Carlotta Gruppioni,E. Ibar,Y. Khusanova,Brian Lemaux,Roberto Maiolino,D. Narayanan,Pascal Oesch,Francesca Pozzi,G. Rodighiero,Margherita Talia,S. Toft,Livia Vallini,D. Vergani,G. Zamorani +31 more
TL;DR: In this paper, the authors study the efficiency of galactic feedback in the early Universe by stacking the [C II] 158 um emission in a large sample of normal star-forming galaxies at 4 4.
Journal ArticleDOI
The ALPINE-ALMA [C II] survey: Star-formation-driven outflows and circumgalactic enrichment in the early Universe
Michele Ginolfi,G. C. Jones,Matthieu Béthermin,Y. Fudamoto,F. Loiacono,Seiji Fujimoto,O. Le Fevre,Andreas L. Faisst,Daniel Schaerer,Paolo Cassata,John D. Silverman,John D. Silverman,Lin Yan,Peter Capak,S. Bardelli,Médéric Boquien,R. Carraro,Miroslava Dessauges-Zavadsky,Mauro Giavalisco,Carlotta Gruppioni,Edo Ibar,Y. Khusanova,Brian C. Lemaux,Roberto Maiolino,Desika Narayanan,Pascal Oesch,Francesca Pozzi,G. Rodighiero,Margherita Talia,Sune Toft,Livia Vallini,D. Vergani,G. Zamorani +32 more
TL;DR: In this paper, the authors study the efficiency of galactic feedback in the early Universe by stacking the [C II] 158 μ m emission in a large sample of normal star-forming galaxies at 4' |≲500 km s−1, and find that the combined core emission (|v | ) of the higher-SFR galaxies is extended on physical sizes of ∼30 kpc (diameter scale).
Journal ArticleDOI
The ALPINE-ALMA [CII] survey - The nature, luminosity function, and star formation history of dusty galaxies up to z ≃ 6
Carlotta Gruppioni,Matthieu Béthermin,F. Loiacono,O. Le Fèvre,Peter Capak,Paolo Cassata,Andreas L. Faisst,Daniel Schaerer,John D. Silverman,Lin Yan,S. Bardelli,Médéric Boquien,R. Carraro,Andrea Cimatti,Andrea Cimatti,Miroslava Dessauges-Zavadsky,Michele Ginolfi,Seiji Fujimoto,Nimish P. Hathi,G. C. Jones,Y. Khusanova,Anton M. Koekemoer,Guilaine Lagache,Brian C. Lemaux,Pascal Oesch,Francesca Pozzi,Dominik A. Riechers,Dominik A. Riechers,Giulia Rodighiero,M. Romano,Margherita Talia,Livia Vallini,Daniela Vergani,G. Zamorani,E. Zucca +34 more
TL;DR: In this article, a sample of 56 sources serendipitously detected in ALMA band 7 as part of the ALMA Large Program to Investigate CII at Early Times (ALPINE) has been used to derive the total infrared luminosity function (LF) and to estimate the cosmic star formation rate density (SFRD) up to z ǫ ≥ 6.
Journal ArticleDOI
The infrared-radio correlation of star-forming galaxies is strongly M$_{\star}$-dependent but nearly redshift-invariant since z$\sim$4
I. Delvecchio,E. Daddi,M. T. Sargent,Matt J. Jarvis,D. Elbaz,Shuowen Jin,Daizhong Liu,I. H. Whittam,H. S. B. Algera,R. Carraro,C. D'Eugenio,J. Delhaize,Boris S. Kalita,Sarah K. Leslie,D. Cs. Molnár,Mario Novak,Isabella Prandoni,V. Smolcic,Yiping Ao,Manuel Aravena,F. Bournaud,Jordan D. Collier,S. M. Randriamampandry,Z. Randriamanakoto,G. Rodighiero,J. Schober,Sarah V. White,G. Zamorani +27 more
TL;DR: In this paper, the spectral energy distributions of star-forming galaxies in the COSMOS field were used to calibrate radio emission as a star formation rate (SFR) indicator, showing that the lower IR/radio ratios seen in more massive galaxies are well described by their observed SFR surface densities.
Journal ArticleDOI
Probing black hole accretion tracks, scaling relations and radiative efficiencies from stacked X-ray active galactic nuclei
Francesco Shankar,David H. Weinberg,Christopher Marsden,Philip J. Grylls,Mariangela Bernardi,Guang Yang,Benjamin P. Moster,Hao Fu,R. Carraro,David M. Alexander,Viola Allevato,Tonima Tasnim Ananna,Angela Bongiorno,Giorgio Calderone,Francesca Civano,Emanuele Daddi,Ivan Delvecchio,Ivan Delvecchio,F. Duras,Fabio La Franca,Andrea Lapi,Youjun Lu,Nicola Menci,Mar Mezcua,Federica Ricci,Giulia Rodighiero,Ravi K. Sheth,Hyewon Suh,Carolin Villforth,Lorenzo Zanisi +29 more
TL;DR: In this paper, the authors combine X-ray measurements of the mean black hole accretion luminosity as a function of stellar mass and redshift with empirical models of galaxy stellar mass growth, integrating over time to predict the evolving Mbh-Mstar relation.