T
Theodoros Bitsakis
Researcher at National Autonomous University of Mexico
Publications - 52
Citations - 2475
Theodoros Bitsakis is an academic researcher from National Autonomous University of Mexico. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 21, co-authored 49 publications receiving 2149 citations. Previous affiliations of Theodoros Bitsakis include University of Crete & California Institute of Technology.
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Journal ArticleDOI
Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis
Maria R. Drout,Anthony L. Piro,Benjamin J. Shappee,Charles D. Kilpatrick,J. D. Simon,Carlos Contreras,David A. Coulter,R. J. Foley,Matthew R. Siebert,Nidia Morrell,Konstantina Boutsia,F. Di Mille,Thomas W.-S. Holoien,Daniel Kasen,Daniel Kasen,Juna A. Kollmeier,Barry F. Madore,Andrew J. Monson,Andrew J. Monson,Ariadna Murguia-Berthier,Yen-Chen Pan,Jason X. Prochaska,Enrico Ramirez-Ruiz,Enrico Ramirez-Ruiz,A. Rest,A. Rest,C. Adams,Katherine Alatalo,Katherine Alatalo,Eduardo Bañados,J. Baughman,J. Baughman,Timothy C. Beers,Timothy C. Beers,R. A. Bernstein,Theodoros Bitsakis,Abdo Campillay,Terese T. Hansen,C. R. Higgs,C. R. Higgs,Alexander P. Ji,Grigoris Maravelias,Jennifer L. Marshall,C. Moni Bidin,J. L. Prieto,J. L. Prieto,Kaitlin C. Rasmussen,Kaitlin C. Rasmussen,César Rojas-Bravo,A. L. Strom,N. Ulloa,J. Vargas-González,Z. Wan,Devin D. Whitten,Devin D. Whitten +54 more
TL;DR: In this paper, the authors present ultraviolet, optical, and infrared light curves of SSS17a extending from 10.9 hours to 18 days post-merger, showing that the late-time light curve indicates that SSS 17a produced at least 0.05 solar masses of heavy elements, demonstrating that neutron star mergers play a role in rapid neutron capture (r-process) nucleosynthesis in the universe.
Journal ArticleDOI
Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis
Maria R. Drout,Anthony L. Piro,Benjamin J. Shappee,Charles D. Kilpatrick,J. D. Simon,Carlos Contreras,David A. Coulter,R. J. Foley,Matthew R. Siebert,Nidia Morrell,Konstantina Boutsia,F. Di Mille,Thomas W.-S. Holoien,Daniel Kasen,Daniel Kasen,Juna A. Kollmeier,Barry F. Madore,Andrew J. Monson,Andrew J. Monson,Ariadna Murguia-Berthier,Yen-Chen Pan,Jason X. Prochaska,Enrico Ramirez-Ruiz,Enrico Ramirez-Ruiz,A. Rest,A. Rest,C. Adams,Katherine Alatalo,Katherine Alatalo,Eduardo Bañados,J. Baughman,J. Baughman,Timothy C. Beers,Timothy C. Beers,R. A. Bernstein,Theodoros Bitsakis,Abdo Campillay,Terese T. Hansen,C. R. Higgs,C. R. Higgs,Alexander P. Ji,Grigoris Maravelias,Jennifer L. Marshall,C. Moni Bidin,J. L. Prieto,J. L. Prieto,Kaitlin C. Rasmussen,Kaitlin C. Rasmussen,César Rojas-Bravo,A. L. Strom,N. Ulloa,J. Vargas-González,Z. Wan,Devin D. Whitten,Devin D. Whitten +54 more
TL;DR: The late-time light curve indicates that SSS17a produced at least ~0.05 solar masses of heavy elements, demonstrating that neutron star mergers play a role in rapid neutron capture (r-process) nucleosynthesis in the universe.
Journal ArticleDOI
Early spectra of the gravitational wave source GW170817: Evolution of a neutron star merger.
Benjamin J. Shappee,J. D. Simon,Maria R. Drout,Anthony L. Piro,Nidia Morrell,J. L. Prieto,J. L. Prieto,Daniel Kasen,Daniel Kasen,Thomas W.-S. Holoien,Juna A. Kollmeier,Daniel D. Kelson,David A. Coulter,R. J. Foley,Charles D. Kilpatrick,Matthew R. Siebert,Barry F. Madore,Ariadna Murguia-Berthier,Yen-Chen Pan,Jason X. Prochaska,Enrico Ramirez-Ruiz,Enrico Ramirez-Ruiz,A. Rest,A. Rest,C. Adams,Katherine Alatalo,Katherine Alatalo,Eduardo Bañados,J. Baughman,J. Baughman,R. A. Bernstein,Theodoros Bitsakis,Konstantina Boutsia,J. R. Bravo,F. Di Mille,C. R. Higgs,C. R. Higgs,Alexander P. Ji,Alexander P. Ji,Grigoris Maravelias,Jennifer L. Marshall,Vinicius M. Placco,G. Prieto,Z. Wan +43 more
TL;DR: In this article, the authors reported time-series spectroscopy of SSS17a from 11.75 hours until 8.5 days after the merger, and measured the photosphere cooling from 11, 000 − 900 + 3400 to 9300 − 300 + 300 kelvin and determined a photospheric velocity of roughly 30% of the speed of light.
Journal ArticleDOI
Suppression of star formation in ngc 1266
Katherine Alatalo,Mark Lacy,Lauranne Lanz,Theodoros Bitsakis,Theodoros Bitsakis,Philip N. Appleton,Kristina Nyland,Kristina Nyland,Sabrina Cales,Sabrina Cales,Philip Chang,Timothy A. Davis,Timothy A. Davis,P. T. de Zeeuw,P. T. de Zeeuw,Carol J. Lonsdale,Sergio Martín,David S. Meier,David S. Meier,Patrick Ogle +19 more
TL;DR: In this article, the authors present detailed observations of the gas and dust continuum of NGC 1266 at millimeter wavelengths and show that molecular gas is being driven out of the nuclear region at yr−1, of which the vast majority cannot escape the nucleus.
Journal ArticleDOI
Early Spectra of the Gravitational Wave Source GW170817: Evolution of a Neutron Star Merger
Benjamin J. Shappee,J. D. Simon,Maria R. Drout,Anthony L. Piro,Nidia Morrell,J. L. Prieto,J. L. Prieto,Daniel Kasen,Daniel Kasen,Thomas W.-S. Holoien,Juna A. Kollmeier,Daniel D. Kelson,David A. Coulter,R. J. Foley,Charles D. Kilpatrick,Matthew R. Siebert,Barry F. Madore,Ariadna Murguia-Berthier,Yen-Chen Pan,Jason X. Prochaska,Enrico Ramirez-Ruiz,Enrico Ramirez-Ruiz,A. Rest,A. Rest,C. Adams,Katherine Alatalo,Katherine Alatalo,Eduardo Bañados,J. Baughman,J. Baughman,R. A. Bernstein,Theodoros Bitsakis,Konstantina Boutsia,J. R. Bravo,F. Di Mille,C. R. Higgs,C. R. Higgs,Alexander P. Ji,Alexander P. Ji,Grigoris Maravelias,Jennifer L. Marshall,Vinicius M. Placco,G. Prieto,Z. Wan +43 more
TL;DR: Spectra of a neutron star merger are unlike other astronomical transients and demonstrate rapid evolution of the source and Kilpatrick et al. show how these observations can be explained by an explosion known as a kilonova, which produces large quantities of heavy elements in nuclear reactions.