S. Tacchella on Muck Rack

S. Tacchella

As seen in: El País, Nature
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Articles

Cuando todo en el universo cambió

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By Elizabeth Quill, B. Johnson, S. Tacchella, P. Cargile
| El País
El revolucionario telescopio espacial ‘James Webb’ y los radiotelescopios de nueva generación están sondeando lo que se conoce como la época de la reionización. En ella se encuentran pistas sobre las primeras estrellas y galaxias, y quizás sobre la naturaleza de la materia oscura Elizabeth Quill KNOWABLE EN ESPAÑOL Durante los millones de años que siguieron al Big Bang, después de que se enfriara la sopa de partículas del universo, el cosmos era un lugar oscuro y aburrido.
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Identification and properties of intense star-forming galaxies at redshifts z > 10 - Nature Astronomy

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By B. Robertson, S. Tacchella, B. Johnson, S. Arribas, A. J. Cameron, S. Carniani, C. Willott, Z. Jeffrey Chen, A. A. De Graaff, N. Kumari, J. Lyu, E. A. Nelson, A. Saxena, L. Whitler, D. J. Eisenstein, E. Egami, R. Hausen, C. C. Williams, A. Bunker, S. Charlot, M. Curti, E. Curtis-Lake, F. D’Eugenio, P. Jakobsen, T. J. Looser, M. V. Maseda, T. Rawle, H.-W. Rix, R. Smit, J. Witstok, R. Bhatawdekar, K. Boyett, R. E. Hviding, L. Sandles, K. A. Suess
| Nature
Author notes These authors contributed equally: B. E. Robertson, S. Tacchella. Authors and Affiliations Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA, USA B. E. Robertson & K. A. Suess Kavli Institute for Cosmology, University of Cambridge, Cambridge, UK S. Tacchella, M. Curti, F. D’Eugenio, T. J. Looser, R. Maiolino, H. Übler, J. Witstok & L. Sandles Cavendish Laboratory, University of Cambridge, Cambridge, UK S. Tacchella, M. Curti, F. D’Eugenio, T. J. Looser, R. Maiolino, H.
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Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang

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By S. Tacchella, C. M. Carollo, A. Renzini
| Science Magazine
Most galaxies exceeding 100 billion solar masses are dense spheroids that exhibit no star-forming activity in the present day. Nevertheless, galaxies of the same size were actively forming stars when the universe was only a few billion years old. Tacchella et al. used integral-field spectroscopy and high-resolution imaging to map the distributions of star formation rates and stellar mass densities within ancient galaxies.
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