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Angel R. Lopez-Sanchez
Researcher at Macquarie University
Publications - 250
Citations - 17077
Angel R. Lopez-Sanchez is an academic researcher from Macquarie University. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 68, co-authored 239 publications receiving 15039 citations. Previous affiliations of Angel R. Lopez-Sanchez include Australian Astronomical Observatory & IAC.
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Journal ArticleDOI
Massive Star Formation and Tidal Structures in HCG 31
TL;DR: In this paper, the authors present new broadband optical and near-infrared CCD imaging together with deep optical intermediate-resolution spectroscopy of the Hickson Compact Group 31.
Posted Content
Galaxy And Mass Assembly (GAMA): Trends in galaxy colours, morphology, and stellar populations with large scale structure, group, and pair environments
Mehmet Alpaslan,Mehmet Alpaslan,Simon P. Driver,Simon P. Driver,Aaron S. G. Robotham,Danail Obreschkow,E. Andrae,Michelle E. Cluver,Lee S. Kelvin,Rebecca A. Lange,Matt S. Owers,Matt S. Owers,Edward N. Taylor,Stephen K. Andrews,Steven P. Bamford,Joss Bland-Hawthorn,Sarah Brough,Michael J. I. Brown,Matthew Colless,Luke J. M. Davies,Elizabeth Eardley,Meiert W. Grootes,Andrew M. Hopkins,Rebecca Kennedy,Jochen Liske,Maritza A. Lara-López,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Jon Loveday,Barry F. Madore,Smriti Mahajan,Martin Meyer,Amanda J. Moffett,Peder Norberg,Samantha J. Penny,Kevin A. Pimbblet,Kevin A. Pimbblet,Cristina C. Popescu,Cristina C. Popescu,Mark Seibert,Richard J. Tuffs +40 more
TL;DR: In this paper, the authors explore trends in galaxy properties with Mpc-scale structures using catalogues of environment and large scale structure from the Galaxy And Mass Assembly (GAMA) survey.
Journal ArticleDOI
PISCO: The Pmas/ppak Integral-field Supernova hosts COmpilation
Lluís Galbany,Joseph P. Anderson,Sebastián F. Sánchez,Hanindyo Kuncarayakti,S. Pedraz,Santiago González-Gaitán,Vallery Stanishev,Inma Dominguez,M. E. Moreno-Raya,W. M. Wood-Vasey,A. Mourao,K. A. Ponder,Carles Badenes,Mercedes Mollá,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,F. F. Rosales-Ortega,José M. Vílchez,R. García-Benito,R. A. Marino +19 more
TL;DR: The Pmas/ppak Integral-field Supernova hosts COmpilation (PISCO) as discussed by the authors is the largest collection of SN host galaxies observed with wide-field IFS, totaling 466,347 individual spectra covering a typical spatial resolution of $380 pc.
Journal ArticleDOI
Ionized gas kinematics of galaxies in the CALIFA survey I: Velocity fields, kinematic parameters of the dominant component, and presence of kinematically distinct gaseous systems
Begoña García-Lorenzo,I. Márquez,Jorge K. Barrera-Ballesteros,J. Masegosa,Bernd Husemann,Jesús Falcón-Barroso,Mariya Lyubenova,Sebastián F. Sánchez,J. Walcher,D. Mast,Rubén García-Benito,Jairo Méndez-Abreu,G. van de Ven,Kristine Spekkens,L. Holmes,Ana Monreal-Ibero,A. del Olmo,Bodo L. Ziegler,Joss Bland-Hawthorn,Patricia Sanchez-Blazquez,Jorge Iglesias-Páramo,J. A. L. Aguerri,P. Papaderos,J. M. Gomes,R. A. Marino,R. M. González Delgado,C. Cortijo-Ferrero,Angel R. Lopez-Sanchez,S. Bekeraite,Lutz Wisotzki,Dominik J. Bomans +30 more
TL;DR: In this paper, the authors used the cross-correlation technique to obtain the radial velocity of the dominant gaseous component and derived the main kinematic parameters directly from the radial velocities with no assumptions on the internal motions.
Journal ArticleDOI
Galaxy And Mass Assembly (GAMA): testing galaxy formation models through the most massive galaxies in the Universe
Paola Oliva-Altamirano,Paola Oliva-Altamirano,Sarah Brough,C. Lidman,Warrick J. Couch,Warrick J. Couch,Andrew M. Hopkins,Matthew Colless,Edward N. Taylor,Aaron S. G. Robotham,Madusha Gunawardhana,Madusha Gunawardhana,Madusha Gunawardhana,Trevor J. Ponman,Ivan K. Baldry,Amanda E. Bauer,Jonathan Bland-Hawthorn,Michelle E. Cluver,Michelle E. Cluver,Ewan Cameron,Christopher J. Conselice,Simon P. Driver,A. C. Edge,Alister W. Graham,E. van Kampen,Maritza A. Lara-López,Jochen Liske,Angel R. Lopez-Sanchez,Jonathan Loveday,Smriti Mahajan,John A. Peacock,Steven Phillipps,Kevin A. Pimbblet,Kevin A. Pimbblet,Kevin A. Pimbblet,Rob Sharp +35 more
TL;DR: In this paper, the authors analyzed the growth of BGGs and BCGs over the last 3 billion years using a large sample of 883 galaxies from the Galaxy And Mass Assembly survey and found no significant growth between redshift z = 0.27 and 0.09.