C. Mancini
INAF
59 Papers
462 Citations
C. Mancini is an academic researcher from INAF. The author has contributed to research in topics: Medicine & Galaxy. The author has an hindex of 13, co-authored 20 publications.
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Papers
THE SINS SURVEY OF z ∼ 2 GALAXY KINEMATICS: PROPERTIES OF THE GIANT STAR-FORMING CLUMPS*
Reinhard Genzel,S. Newman,Therese M. Jones,N. M. Förster Schreiber,Kristen L. Shapiro,Kristen L. Shapiro,Shy Genel,Simon J. Lilly,Alvio Renzini,Linda J. Tacconi,Nicolas Bouché,Andreas Burkert,Giovanni Cresci,P. Buschkamp,C. M. Carollo,Daniel Ceverino,Ric Davies,Avishai Dekel,Frank Eisenhauer,Erin K. S. Hicks,Jaron Kurk,Dieter Lutz,C. Mancini,Thorsten Naab,Yingjie Peng,Amiel Sternberg,Daniela Vergani,G. Zamorani +27 more
TL;DR: In this article, the authors studied the properties of giant star-forming clumps in five z ~ 2 star forming disks with deep SINFONI AO spectroscopy at the ESO VLT.
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The SINS survey of z~2 galaxy kinematics: properties of the giant star forming clumps
Reinhard Genzel,S. Newman,Therese M. Jones,N. M. Förster Schreiber,Kristen L. Shapiro,Kristen L. Shapiro,Shy Genel,Simon J. Lilly,Alvio Renzini,Linda J. Tacconi,Nicolas Bouché,Andreas Burkert,Giovanni Cresci,P. Buschkamp,C. M. Carollo,Daniel Ceverino,Ric Davies,Avishai Dekel,Frank Eisenhauer,Erin K. S. Hicks,Jaron Kurk,Dieter Lutz,C. Mancini,Thorsten Naab,Yingjie Peng,Amiel Sternberg,Daniela Vergani,G. Zamorani +27 more
TL;DR: In this paper, the authors studied the properties of giant star forming clumps in five z~2 star-forming disks with deep SINFONI AO spectroscopy at the ESO VLT.
512
The first Herschel view of the mass-SFR link in high-z galaxies
Giulia Rodighiero,Andrea Cimatti,Carlotta Gruppioni,Paola Popesso,Paola Andreani,Paola Andreani,Bruno Altieri,Herve Aussel,S. Berta,Ángel Bongiovanni,Drew Brisbin,Antonio Cava,J. Cepa,Emanuele Daddi,H. Dominguez-Sanchez,David Elbaz,Adriano Fontana,N. M. Förster Schreiber,Alberto Franceschini,Reinhard Genzel,Andrea Grazian,Dieter Lutz,Georgios E. Magdis,Manuela Magliocchetti,Benjamin Magnelli,Roberto Maiolino,C. Mancini,Raanan Nordon,A. M. Pérez García,Albrecht Poglitsch,Paola Santini,Miguel Sánchez-Portal,Francesca Pozzi,L. Riguccini,Amélie Saintonge,Lijing Shao,E. Sturm,Linda J. Tacconi,Ivan Valtchanov,M. Wetzstein,E. Wieprecht +40 more
TL;DR: In this paper, the authors exploit deep observations of the GOODS-N field taken with PACS onboard of Herschel, as part of the PACS evolutionary probe guaranteed time (PEP), to study the link between star formation and stellar mass in galaxies to z ~ 2.
The first Herschel view of the mass-SFR link in high-z galaxies
Giulia Rodighiero,Andrea Cimatti,Carlotta Gruppioni,Paola Popesso,Paola Andreani,Paola Andreani,Bruno Altieri,Herve Aussel,S. Berta,Ángel Bongiovanni,Drew Brisbin,Antonio Cava,J. Cepa,Emanuele Daddi,H. Dominguez-Sanchez,David Elbaz,Adriano Fontana,N. M. Förster Schreiber,Alberto Franceschini,Reinhard Genzel,Andrea Grazian,Dieter Lutz,Georgios E. Magdis,Manuela Magliocchetti,Benjamin Magnelli,Roberto Maiolino,C. Mancini,Raanan Nordon,A. M. Pérez García,Albrecht Poglitsch,Paola Santini,Miguel Sánchez-Portal,Francesca Pozzi,L. Riguccini,Amélie Saintonge,Lijing Shao,E. Sturm,Linda J. Tacconi,Ivan Valtchanov,M. Wetzstein,E. Wieprecht +40 more
TL;DR: In this article, the authors exploit deep observations of the GOODS-N field taken with PACS, on board of Herschel, as part of the PEP guaranteed time, to study the link between star formation and stellar mass in galaxies to z~2.
279
The SINS/zC-SINF survey of z ∼ 2 galaxy kinematics: Evidence for gravitational quenching
Reinhard Genzel,N. M. Förster Schreiber,Philipp Lang,Sandro Tacchella,Linda J. Tacconi,Stijn Wuyts,K. Bandara,Andreas Burkert,P. Buschkamp,C. M. Carollo,Giovanni Cresci,Ric Davies,Frank Eisenhauer,Erin K. S. Hicks,Jaron Kurk,Simon J. Lilly,Dieter Lutz,C. Mancini,Thorsten Naab,S. Newman,Yingjie Peng,Alvio Renzini,K. Shapiro Griffin,Amiel Sternberg,Daniela Vergani,Emily Wisnioski,Eva Wuyts,G. Zamorani +27 more
TL;DR: In this paper, the radial distributions of Hα surface brightness, stellar mass surface density, and dynamical mass at 2 kpc resolution in 19 z ∼ 2 star-forming disks with deep SINFONI adaptive optics spectroscopy at the ESO Very Large Telescope were derived.
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