P
Philip Rosenfield
Researcher at Harvard University
Publications - 72
Citations - 4985
Philip Rosenfield is an academic researcher from Harvard University. The author has contributed to research in topics: Stars & Galaxy. The author has an hindex of 26, co-authored 72 publications receiving 4268 citations. Previous affiliations of Philip Rosenfield include American Astronomical Society & University of Washington.
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A New Generation of PARSEC-COLIBRI Stellar Isochrones Including the TP-AGB Phase
Paola Marigo,Léo Girardi,Alessandro Bressan,Philip Rosenfield,Bernhard Aringer,Yang Chen,Marco Dussin,Ambra Nanni,Giada Pastorelli,Thaíse S. Rodrigues,Thaíse S. Rodrigues,Michele Trabucchi,Sara Bladh,Julianne J. Dalcanton,Martin Groenewegen,Josefina Montalbán,Peter R. Wood +16 more
TL;DR: In this paper, the authors acknowledge the support from the ERC Consolidator Grant (CRA 1.05.01.94) and Partial Support Agreement (PSA) for the STARKEY project.
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The ACS Nearby Galaxy Survey Treasury. IX. Constraining Asymptotic Giant Branch Evolution with Old Metal-poor Galaxies
Léo Girardi,Benjamin F. Williams,Karoline M. Gilbert,Philip Rosenfield,Julianne J. Dalcanton,Paola Marigo,Martha L. Boyer,Andrew E. Dolphin,Daniel R. Weisz,Jason Melbourne,Knut Olsen,Anil C. Seth,Evan D. Skillman +12 more
TL;DR: In this article, the luminosity functions and number ratios between AGB and red giant branch (RGB) stars from a sample of resolved galaxies from the ACS Nearby Galaxy Survey Treasury were examined.
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New PARSEC evolutionary tracks of massive stars at low metallicity: testing canonical stellar evolution in nearby star-forming dwarf galaxies
Jing Tang,Alessandro Bressan,Philip Rosenfield,Alessandra Slemer,Paola Marigo,Léo Girardi,Luciana Bianchi +6 more
TL;DR: In this paper, the authors extended the library of stellar evolutionary tracks by computing new models of massive stars, from 14 ε to 350 ε, for which the metal poor dwarf irregular star forming galaxies, Sextans A, WLM and NCG6822, provided simple but powerful workbenches.
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The panchromatic hubble andromeda treasury
Julianne J. Dalcanton,Benjamin F. Williams,Dustin Lang,Tod R. Lauer,Jason S. Kalirai,Anil C. Seth,Andrew E. Dolphin,Philip Rosenfield,Daniel R. Weisz,Eric F. Bell,Luciana Bianchi,Martha L. Boyer,Nelson Caldwell,Hui Dong,Claire E. Dorman,Karoline M. Gilbert,Léo Girardi,Stephanie M. Gogarten,Karl D. Gordon,Puragra Guhathakurta,Paul W. Hodge,Jon A. Holtzman,L. Clifton Johnson,Søren S. Larsen,Alexia R. Lewis,Jason Melbourne,Knut Olsen,Hans-Walter Rix,Keith Rosema,Abhijit Saha,Ata Sarajedini,Evan D. Skillman,Krzysztof Z. Stanek +32 more
TL;DR: The Panchromatic Hubble Andromeda Treasury (PHT) as mentioned in this paper is an ongoing Hubble Space Telescope Multi-Cycle Treasury program to image ~1/3 of M31's star-forming disk in six filters, spanning from the ultraviolet (UV) to the near-infrared (NIR).
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Pulsars as Astrophysical Laboratories for Nuclear and Particle Physics
TL;DR: In this article, the authors explore the properties of hadronic matter under extreme conditions of temperature and density, and the determination of the equation of state, the relation between pressure, temperature, and density of such matter.