E. E. E. Gall
Max Planck Society
14 Papers
1.4K Citations
E. E. E. Gall is an academic researcher from Max Planck Society. The author has contributed to research in topics: Supernova & Redshift. The author has an hindex of 9, co-authored 14 publications. Previous affiliations of E. E. E. Gall include Queen's University Belfast.
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Papers
The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
Daniel Scolnic,David O. Jones,Armin Rest,Yen-Chen Pan,R. Chornock,Ryan J. Foley,M. E. Huber,Richard Kessler,Gautham Narayan,Adam G. Riess,S. Rodney,Edo Berger,D. J. Brout,Peter Challis,Maria R. Drout,D. P. Finkbeiner,R. Lunnan,R. P. Kirshner,Nathan Edward Sanders,Edward F. Schlafly,S. J. Smartt,Christopher W. Stubbs,John L. Tonry,W. M. Wood-Vasey,Michael Foley,J. Hand,Elizabeth N. Johnson,W. S. Burgett,K. C. Chambers,Peter W. Draper,Klaus W. Hodapp,Nick Kaiser,R. P. Kudritzki,E. A. Magnier,Nigel Metcalfe,F. Bresolin,E. E. E. Gall,Rubina Kotak,M. McCrum,K. W. Smith +39 more
TL;DR: In this paper, the authors present optical light curves, redshifts, and classifications for 365 spectroscopically confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1) Medium Deep Survey.
PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects
Stephen J. Smartt,Stefano Valenti,Morgan Fraser,Cosimo Inserra,David Young,Mark Sullivan,Andrea Pastorello,Stefano Benetti,Avishay Gal-Yam,Cristina Knapic,Marco Molinaro,Riccardo Smareglia,K. W. Smith,S. Taubenberger,O. Yaron,Joseph P. Anderson,Chris Ashall,C. Balland,C. Baltay,C. Barbarino,Franz E. Bauer,S. Baumont,D. Bersier,Nadejda Blagorodnova,S. Bongard,M. T. Botticella,F. Bufano,Mattia Bulla,Enrico Cappellaro,H. Campbell,F. Cellier-Holzem,Ting-Wan Chen,M. J. Childress,Alejandro Clocchiatti,C. Contreras,M. Dall' Ora,John Danziger,T. de Jaeger,A. De Cia,M. Della Valle,Michel Dennefeld,Nancy Elias-Rosa,N. Elman,Ulrich Feindt,M. Fleury,E. E. E. Gall,Santiago González-Gaitán,Lluís Galbany,A. Morales Garoffolo,Laura Greggio,L. Le Guillou,S. Hachinger,E. Hadjiyska,P. E. Hage,Wolfgang Hillebrandt,S. T. Hodgkin,Eric Hsiao,Phil A. James,Anders Jerkstrand,Tuomas Kangas,Erkki Kankare,Rubina Kotak,Markus Kromer,Hanindyo Kuncarayakti,Giorgos Leloudas,Peter Lundqvist,J. D. Lyman,Isobel Hook,Kate Maguire,Ilan Manulis,S. Margheim,Seppo Mattila,Justyn R. Maund,Paolo A. Mazzali,M. McCrum,Ryan McKinnon,M. E. Moreno-Raya,Matt Nicholl,Peter Nugent,R. Pain,M. M. Phillips,Giuliano Pignata,J. Polshaw,Maria Letizia Pumo,David Rabinowitz,E. Reilly,C. Romero-Canizales,Richard Scalzo,Brian P. Schmidt,Steve Schulze,Stuart A. Sim,Jesper Sollerman,Francesco Taddia,Leonardo Tartaglia,Giacomo Terreran,L. Tomasella,Massimo Turatto,E. S. Walker,Nicholas A. Walton,L. Wyrzykowski,Fang Yuan,Luca Zampieri +101 more
TL;DR: In this article, the authors describe the data reduction strategy and data products which are publicly available through the ESO archive as the Spectroscopic Survey Data Release 1 (SSDR1).
Measuring Dark Energy Properties with Photometrically Classified Pan-STARRS Supernovae. II. Cosmological Parameters
David O. Jones,Daniel Scolnic,Adam G. Riess,Adam G. Riess,Armin Rest,Armin Rest,Robert P. Kirshner,Edo Berger,Richard Kessler,Yen-Chen Pan,Ryan J. Foley,Ryan Chornock,C. A. Ortega,Peter Challis,William S. Burgett,K. C. Chambers,Peter W. Draper,H. Flewelling,M. E. Huber,Nick Kaiser,Rolf-Peter Kudritzki,Nigel Metcalfe,John L. Tonry,Richard J. Wainscoat,Christopher Waters,E. E. E. Gall,Rubina Kotak,M. McCrum,Stephen Smartt,K. W. Smith +29 more
TL;DR: In this paper, the authors used 1169 Pan-STARRS supernovae (SNe) and 195 low-z$ ($z < 0.1$) SNe Ia to measure cosmological parameters.
On the nature of hydrogen-rich superluminous supernovae
Cosimo Inserra,Cosimo Inserra,Stephen J. Smartt,E. E. E. Gall,Giorgos Leloudas,T. W. Chen,Steve Schulze,Steve Schulze,Anders Jerkstrand,Matt Nicholl,Joseph P. Anderson,Iair Arcavi,Iair Arcavi,S. Benetti,Régis Cartier,M. Childress,M. Della Valle,Heather Flewelling,Morgan Fraser,Avishay Gal-Yam,Claudia P. Gutiérrez,Griffin Hosseinzadeh,Griffin Hosseinzadeh,D. A. Howell,D. A. Howell,M. E. Huber,Erkki Kankare,Thomas Krühler,Eugene A. Magnier,Kate Maguire,Curtis McCully,Curtis McCully,S. Prajs,N. Primak,Richard Scalzo,Brian P. Schmidt,M. Smith,K. W. Smith,Brad E. Tucker,S. Valenti,M. Wilman,David Young,Fang Yuan +42 more
TL;DR: In this article, two hydrogen-rich superluminous supernovae (SLSNe): SN2103hx and PS15br, were shown to have strong, multicomponent H α emission after 200 d past maximum, which is interpreted as an indication of the interaction of the ejecta with an asymmetric, clumpy circumstellar material.
Interpreting the near-infrared spectra of the 'golden standard' Type Ia supernova 2005cf
E. E. E. Gall,S. Taubenberger,Markus Kromer,Stuart A. Sim,Stefano Benetti,Guillermo A. Blanc,Guillermo A. Blanc,Nancy Elias-Rosa,Nancy Elias-Rosa,Wolfgang Hillebrandt +9 more
TL;DR: In this article, the broad-band spectral energy distribution (SED) of supernova 2005cf is studied in combined ultraviolet (UV), optical and NIR spectra at five epochs between ~ 8 d before and ~ 10 d after maximum light.