L
Luke A. Barnes
Researcher at University of Sydney
Publications - 90
Citations - 7048
Luke A. Barnes is an academic researcher from University of Sydney. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 26, co-authored 80 publications receiving 6333 citations. Previous affiliations of Luke A. Barnes include University of Cambridge & Liverpool John Moores University.
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Journal ArticleDOI
Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
Yingjie Peng,Simon J. Lilly,Katarina Kovac,Micol Bolzonella,Lucia Pozzetti,Alvio Renzini,G. Zamorani,Olivier Ilbert,C. Knobel,A. Iovino,Christian Maier,Olga Cucciati,Lidia Tasca,C. Marcella Carollo,John D. Silverman,P. Kampczyk,Loic de Ravel,David B. Sanders,Nick Scoville,Thierry Contini,Vincenzo Mainieri,Marco Scodeggio,Jean-Paul Kneib,Olivier Le Fevre,S. Bardelli,Angela Bongiorno,Karina Caputi,Graziano Coppa,Sylvain de la Torre,P. Franzetti,Bianca Garilli,F. Lamareille,Jean-Francois Le Borgne,Vincent Le Brun,M. Mignoli,Enrique Perez Montero,R. Pello,E. Ricciardelli,Masayuki Tanaka,Laurence Tresse,Daniela Vergani,Niraj Welikala,E. Zucca,Pascal Oesch,U. Abbas,Luke A. Barnes,Rongmon Bordoloi,D. Bottini,A. Cappi,Paolo Cassata,Andrea Cimatti,M. Fumana,Günther Hasinger,Anton M. Koekemoer,A. Leauthaud,D. Maccagni,Christian Marinoni,H. J. McCracken,P. Memeo,B. Meneux,Preethi Nair,Cristiano Porciani,V. Presotto,Roberto Scaramella +63 more
TL;DR: In this paper, the authors explore the simple interrelationships between mass, star formation rate, and environment in the SDSS, zCOSMOS, and other deep surveys.
Journal ArticleDOI
Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
Yingjie Peng,Simon J. Lilly,Katarina Kovac,M. Bolzonella,Lucia Pozzetti,Alvio Renzini,G. Zamorani,Olivier Ilbert,C. Knobel,A. Iovino,Christian Maier,Olga Cucciati,L. A. M. Tasca,C. M. Carollo,John D. Silverman,P. Kampczyk,L. de Ravel,David B. Sanders,Nick Scoville,T. Contini,Vincenzo Mainieri,Marco Scodeggio,Jean-Paul Kneib,O. Le Fevre,S. Bardelli,Angela Bongiorno,Karina Caputi,Graziano Coppa,S. de la Torre,P. Franzetti,B. Garilli,F. Lamareille,J. F. Le Borgne,V. Le Brun,M. Mignoli,E. Perez Montero,R. Pello,E. Ricciardelli,Masaomi Tanaka,L. Tresse,D. Vergani,Niraj Welikala,E. Zucca,Pascal Oesch,U. Abbas,Luke A. Barnes,Rongmon Bordoloi,D. Bottini,A. Cappi,Paolo Cassata,A. Cimatti,M. Fumana,G. Hasinger,Anton M. Koekemoer,A. Leauthaud,D. Maccagni,Christian Marinoni,H. J. McCracken,P. Memeo,B. Meneux,P. Nair,Cristiano Porciani,V. Presotto,Roberto Scaramella +63 more
TL;DR: In this paper, the authors explore the interrelationships between mass, star-formation rate and environment in the SDSS, zCOSMOS and other surveys, and show that the mass quenching of galaxies around and above M * must be proportional to their star formation rates at all z < 2.
Journal ArticleDOI
Improved constraints on the expansion rate of the Universe up to z ∼ 1.1 from the spectroscopic evolution of cosmic chronometers
Michele Moresco,Andrea Cimatti,Raul Jimenez,Lucia Pozzetti,G. Zamorani,Micol Bolzonella,James Dunlop,F. Lamareille,F. Lamareille,M. Mignoli,H. J. Pearce,Piero Rosati,Daniel Stern,Licia Verde,E. Zucca,C. M. Carollo,Thierry Contini,Thierry Contini,Jean-Paul Kneib,O. Le Fèvre,S. Lilly,Vincenzo Mainieri,Alvio Renzini,Marco Scodeggio,Italo Balestra,Italo Balestra,Raphael Gobat,Ross J. McLure,S. Bardelli,Angela Bongiorno,Karina Caputi,Olga Cucciati,S. de la Torre,L. de Ravel,P. Franzetti,Bianca Garilli,A. Iovino,P. Kampczyk,C. Knobel,K. Kovac,K. Kovac,J. F. Le Borgne,J. F. Le Borgne,V. Le Brun,Christian Maier,Christian Maier,R. Pello,R. Pello,Yingjie Peng,Enrique Pérez-Montero,V. Presotto,V. Presotto,John D. Silverman,Masayuki Tanaka,Lidia Tasca,Laurence Tresse,Daniela Vergani,Omar Almaini,Luke A. Barnes,Rongmon Bordoloi,E. J. Bradshaw,A. Cappi,Robert Chuter,Michele Cirasuolo,Graziano Coppa,Graziano Coppa,C. Diener,S. Foucaud,William G. Hartley,Marc Kamionkowski,Anton M. Koekemoer,C. López-Sanjuan,H. J. McCracken,Preethi Nair,Pascal Oesch,Pascal Oesch,Adam Stanford,Adam Stanford,Niraj Welikala +78 more
TL;DR: In this paper, the authors presented new improved constraints on the Hubble parameter H(z) in the redshift range 0.15 -1.1, obtained from the differential spectroscopic evolution of early-type galaxies as a function of redshift.
Journal ArticleDOI
The SAMI Galaxy Survey: Instrument specification and target selection
Julia J. Bryant,Julia J. Bryant,Matt S. Owers,Aaron S. G. Robotham,Scott M. Croom,Simon P. Driver,Simon P. Driver,Michael J. Drinkwater,Nuria P. F. Lorente,Luca Cortese,Nicholas Scott,Matthew Colless,Adam L. Schaefer,Adam L. Schaefer,Edward N. Taylor,I. S. Konstantopoulos,I. S. Konstantopoulos,J. T. Allen,Ivan K. Baldry,Luke A. Barnes,Amanda E. Bauer,Joss Bland-Hawthorn,J. V. Bloom,Alyson Brooks,Sarah Brough,Gerald Cecil,Gerald Cecil,Warrick J. Couch,Darren J. Croton,R. I. Davies,Simon Ellis,L. M. R. Fogarty,Caroline Foster,Karl Glazebrook,Michael Goodwin,Andrew W. Green,Madusha Gunawardhana,Elise Hampton,I-Ting Ho,Andrew M. Hopkins,Lisa J. Kewley,Jon Lawrence,Sergio G. Leon-Saval,Sarah K. Leslie,Rebecca McElroy,Geraint F. Lewis,Jochen Liske,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Smriti Mahajan,Smriti Mahajan,Anne M. Medling,Nigel Metcalfe,Martin Meyer,Jeremy Mould,Danail Obreschkow,Simon J. O'Toole,Michael Pracy,Samuel N. Richards,Samuel N. Richards,Tom Shanks,Rob Sharp,Rob Sharp,Sarah M. Sweet,Sarah M. Sweet,A. D. Thomas,C. Tonini,C. J. Walcher +67 more
TL;DR: The SAMI Galaxy Survey as discussed by the authors is a 3-year survey of 3400 galaxies with the Sydney-AAO Multi-Object Integral Field Spectrograph (SAMI) on the Anglo-Australian Telescope (AAT).
Journal ArticleDOI
The radial and azimuthal profiles of Mg II absorption around 0,5 <z <0,9 zCosmos galaxies of different colors, masses, and environments
Rongmon Bordoloi,Simon J. Lilly,C. Knobel,M. Bolzonella,P. Kampczyk,C. M. Carollo,A. Iovino,E. Zucca,Thierry Contini,Thierry Contini,Jean-Paul Kneib,O. Le Fèvre,V. Mainieri,Alvio Renzini,M. Scodeggio,G. Zamorani,Italo Balestra,S. Bardelli,Angela Bongiorno,Karina Caputi,Olga Cucciati,S. de la Torre,L. de Ravel,Bianca Garilli,Bianca Garilli,K. Kovac,F. Lamareille,F. Lamareille,J. F. Le Borgne,J. F. Le Borgne,V. Le Brun,Christian Maier,M. Mignoli,R. Pello,R. Pello,Yingjie Peng,E. Perez Montero,E. Perez Montero,E. Perez Montero,V. Presotto,Claudia Scarlata,John D. Silverman,Masayuki Tanaka,Lidia Tasca,Laurence Tresse,Daniela Vergani,Luke A. Barnes,A. Cappi,Andrea Cimatti,Graziano Coppa,C. Diener,P. Franzetti,Anton M. Koekemoer,C. López-Sanjuan,H. J. McCracken,Michele Moresco,Preethi Nair,Pascal Oesch,Pascal Oesch,Lucia Pozzetti,Niraj Welikala +60 more
TL;DR: In this article, the radial and azimuthal distribution of Mg II gas within 200 kpc (physical) of ~ 4000 galaxies at redshifts 0.5 1.