J
Joss Bland-Hawthorn
Researcher at University of Sydney
Publications - 1157
Citations - 84957
Joss Bland-Hawthorn is an academic researcher from University of Sydney. The author has contributed to research in topics: Galaxy & Stars. The author has an hindex of 136, co-authored 1114 publications receiving 77593 citations. Previous affiliations of Joss Bland-Hawthorn include Macquarie University & Australian National University.
Papers
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Journal ArticleDOI
Suppression of the near-infrared OH night sky lines with fibre Bragg gratings - first results
Simon Ellis,Joss Bland-Hawthorn,Jon Lawrence,Anthony Horton,Christopher Q. Trinh,Sergio G. Leon-Saval,K. Shortridge,Julia J. Bryant,Scott W. Case,Matthew Colless,W. J. Couch,Kenneth C. Freeman,Luke Gers,Karl Glazebrook,Roger Haynes,Steve Lee,H. Loehmannsroeben,J. O.Byrne,Stan Miziarski,M. Roth,Brian P. Schmidt,C. G. Tinney,Jessica R. Zheng +22 more
TL;DR: The GNOSIS as mentioned in this paper is a low-resolution spectrograph for low-resolved spectroscopy with fiber Bragg gratings, which has a resolving power of approximately 10,000.
Journal ArticleDOI
CALIFA, the Calar Alto Legacy Integral Field Area survey: IV. Third Public data release
Sebastián F. Sánchez,Rubén García-Benito,Stefano Zibetti,C. J. Walcher,B. Husemann,M. A. Mendoza,Lluís Galbany,Jesús Falcón-Barroso,D. Mast,Jesús Aceituno,J. A. L. Aguerri,J. Alves,A. L. Amorim,Yago Ascasibar,D. Barrado-Navascues,Jorge K. Barrera-Ballesteros,S. Bekeraite,Joss Bland-Hawthorn,M. Cano Díaz,R. Cid Fernandes,Oscar Cavichia,C. Cortijo,Helmut Dannerbauer,Markus Demleitner,Angeles I. Díaz,R. J. Dettmar,A. de Lorenzo-Cáceres,A. del Olmo,Anna Gallazzi,Begoña García-Lorenzo,A. Gil de Paz,R. M. González Delgado,L. Holmes,Jorge Iglesias-Páramo,C. Kehrig,Andreas Kelz,Robert C. Kennicutt,B. Kleemann,E. A. D. Lacerda,R. López Fernández,A. R. López Sánchez,Mariya Lyubenova,R. A. Marino,Isabel Márquez,Jairo Méndez-Abreu,Mercedes Mollá,Ana Monreal-Ibero,R. Ortega Minakata,Juan Pablo Torres-Papaqui,Enrique Pérez,F. F. Rosales-Ortega,Markus Roth,Patricia Sanchez-Blazquez,U. Schilling,Kristine Spekkens,N. Vale Asari,R. C. E. van den Bosch,G. van de Ven,José M. Vílchez,Vivienne Wild,Lutz Wisotzki,Akın Yıldırım,Bodo L. Ziegler +62 more
TL;DR: The third public data release (DR3) of the Calar Alto Legacy Integral Field Area (CALIFA) survey as mentioned in this paper contains 1576 datacubes, including ~1.5 million independent spectra.
Journal ArticleDOI
The interstellar disk-halo connection in the spiral galaxy NGC 3079
TL;DR: In this paper, the authors used the Hawaii Imaging Fabry-Perot Interferometer (HIFI) to map 150,000 H-alpha + (N II) lambda lambda 6548, 6583 emission-line profiles across the entire disk, with resolution 70 km/s at subarcsecond steps, down to a flux level of approximately 10(exp −17) ergs/s/sq cm (EM approximately equal to 4 cm(exp -6) pc).
Journal ArticleDOI
A Kinematic Link between Boxy Bulges, Stellar Bars, and Nuclear Activity in NGC 3079 & NGC 4388
TL;DR: In this paper, the authors presented direct kinematic evidence for bar streaming motions in two active galaxies with boxy stellar bulges, and used the Hawaii Imaging Fabry-Perot Interferometer to derive the two-dimensional velocity field of the line-emitting gas in the disks of the Sc galaxy NGC 3079 and the Sb galaxy nGC 4388.
Journal ArticleDOI
The dependence of oxygen and nitrogen abundances on stellar mass from the CALIFA survey
Enrique Pérez-Montero,Rubén García-Benito,José M. Vílchez,Sebastián F. Sánchez,Sebastián F. Sánchez,C. Kehrig,Bernd Husemann,S. Duarte Puertas,Jorge Iglesias-Páramo,Lluís Galbany,Lluís Galbany,Mercedes Mollá,C. J. Walcher,Yago Ascasibar,R. M. González Delgado,R. A. Marino,R. A. Marino,Josefa Masegosa,Enrique Pérez,F. F. Rosales-Ortega,Patricia Sanchez-Blazquez,Patricia Sanchez-Blazquez,Joss Bland-Hawthorn,Dominik J. Bomans,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Bodo L. Ziegler +26 more
TL;DR: In this paper, the authors analyzed the optical spectra of individual selected H II regions extracted from a sample of 350 spiral galaxies of the CALIFA survey and performed linear fitting to the abundances as a function of the de-projected galactocentric distances.