Philip A. Pinto

5.2k total citations
62 papers, 2.2k citations indexed

About

Philip A. Pinto is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, Philip A. Pinto has authored 62 papers receiving a total of 2.2k indexed citations (citations by other indexed papers that have themselves been cited), including 46 papers in Astronomy and Astrophysics, 20 papers in Nuclear and High Energy Physics and 12 papers in Instrumentation. Recurrent topics in Philip A. Pinto's work include Gamma-ray bursts and supernovae (33 papers), Astronomy and Astrophysical Research (12 papers) and Stellar, planetary, and galactic studies (11 papers). Philip A. Pinto is often cited by papers focused on Gamma-ray bursts and supernovae (33 papers), Astronomy and Astrophysical Research (12 papers) and Stellar, planetary, and galactic studies (11 papers). Philip A. Pinto collaborates with scholars based in United States, United Kingdom and Canada. Philip A. Pinto's co-authors include Ronald G. Eastman, S. E. Woosley, Daniel J. Eisenstein, T. A. Weaver, M. Hamuy, Lehman H. Garrison, L. Ensman, T. S. Axelrod, B. Leibundgut and D. H. Hartmann and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

Philip A. Pinto

62 papers receiving 2.1k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
Philip A. Pinto United States 26 2.0k 729 268 101 61 62 2.2k
S. Schindler Austria 31 2.6k 1.3× 896 1.2× 837 3.1× 119 1.2× 86 1.4× 100 2.9k
H. M. Antia India 29 2.4k 1.2× 365 0.5× 221 0.8× 121 1.2× 70 1.1× 132 2.7k
N. Vittorio Italy 22 1.9k 0.9× 743 1.0× 87 0.3× 200 2.0× 176 2.9× 95 2.1k
C. M. Gaskell United States 30 3.0k 1.5× 729 1.0× 640 2.4× 139 1.4× 39 0.6× 100 3.1k
S. Bowyer United States 17 1.4k 0.7× 482 0.7× 135 0.5× 108 1.1× 31 0.5× 101 1.7k
R. A. Sunyaev Russia 22 3.1k 1.6× 1.7k 2.3× 290 1.1× 138 1.4× 186 3.0× 73 3.4k
Johannes Büchner Germany 22 2.3k 1.2× 679 0.9× 459 1.7× 91 0.9× 46 0.8× 89 2.6k
Rick Edelson United States 26 3.1k 1.6× 1.6k 2.2× 153 0.6× 186 1.8× 30 0.5× 53 3.3k
D. Q. Lamb United States 23 1.5k 0.8× 790 1.1× 212 0.8× 248 2.5× 60 1.0× 84 2.0k
David Tytler United States 32 3.6k 1.8× 1.5k 2.1× 689 2.6× 141 1.4× 234 3.8× 90 3.9k

Countries citing papers authored by Philip A. Pinto

Since Specialization
Citations

This map shows the geographic impact of Philip A. Pinto's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by Philip A. Pinto with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Philip A. Pinto more than expected).

Fields of papers citing papers by Philip A. Pinto

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Philip A. Pinto. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by Philip A. Pinto. The network helps show where Philip A. Pinto may publish in the future.

Co-authorship network of co-authors of Philip A. Pinto

This figure shows the co-authorship network connecting the top 25 collaborators of Philip A. Pinto. A scholar is included among the top collaborators of Philip A. Pinto based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with Philip A. Pinto. Philip A. Pinto is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Pinto, Philip A., Amy B. Mullens, Dagmar Bruenig, et al.. (2025). A Pilot Epigenome-Wide Study of Posttraumatic Growth: Identifying Novel Candidates for Future Research. Epigenomes. 9(4). 39–39. 1 indexed citations
2.
Wibking, Benjamin D., et al.. (2019). Cosmology with stacked cluster weak lensing and cluster–galaxy cross-correlations. Monthly Notices of the Royal Astronomical Society. 491(3). 3061–3081. 20 indexed citations
3.
Mehta, Kushal, et al.. (2011). Galaxy Bias and its Effects on the Baryon Acoustic Oscillations Measurements. arXiv (Cornell University). 218. 1 indexed citations
4.
Krabbendam, Victor L., Srinivasan Chandrasekharan, K. H. Cook, et al.. (2010). LSST Operations Simulator. 215. 1 indexed citations
5.
Cook, Kem H., Philip A. Pinto, Francisco Delgado, et al.. (2009). LSST: Cadence Design and Simulation. AAS. 213. 2 indexed citations
6.
Pinto, Philip A., K. H. Cook, Francisco Delgado, et al.. (2007). LSST: Cadence Design and Simulation. American Astronomical Society Meeting Abstracts. 211. 2 indexed citations
7.
Ivezić, Željko, D. G. Monet, Nicholas A. Bond, et al.. (2007). Astrometry with digital sky surveys: from SDSS to LSST. Proceedings of the International Astronomical Union. 3(S248). 537–543. 4 indexed citations
8.
Pinto, Philip A., K. H. Cook, Francisco Delgado, et al.. (2006). LSST Survey Strategy: Cadence Design and Simulation. American Astronomical Society Meeting Abstracts. 209. 1 indexed citations
9.
Cook, K. H., et al.. (2004). LSST Operational Cadence Simulation and Design. AAS. 205. 1 indexed citations
10.
Chambers, D. M., Philip A. Pinto, J. Hawreliak, et al.. (2002). K-shell spectroscopy of an independently diagnosed uniaxially expanding laser-produced aluminum plasma. Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics. 66(2). 26410–26410. 20 indexed citations
11.
Hamuy, M. & Philip A. Pinto. (2002). Type II Supernovae as Standardized Candles. The Astrophysical Journal. 566(2). L63–L65. 107 indexed citations
12.
Pinto, Philip A., Ronald G. Eastman, & T. M. Rogers. (2001). A Test for the Nature of the Type Ia Supernova Explosion Mechanism. The Astrophysical Journal. 551(1). 231–243. 3 indexed citations
13.
Burrows, Adam, T. Young, Philip A. Pinto, R. G. Eastman, & Todd A. Thompson. (1999). Supernova Neutrinos and a New Algorithm for Neutrino Transport. arXiv (Cornell University). 1 indexed citations
14.
Fryer, Chris L., Stirling A. Colgate, & Philip A. Pinto. (1999). Iron Opacity and the Pulsar of SN 1987A. The Astrophysical Journal. 511(2). 885–895. 25 indexed citations
15.
Meikle, W. P. S., T. R. Geballe, N. A. Walton, et al.. (1997). Infrared and optical spectroscopy of Type Ia supernovae in the nebular phase. Monthly Notices of the Royal Astronomical Society. 290(4). 663–679. 40 indexed citations
16.
Woosley, S. E., F. X. Timmes, R. D. Hoffman, et al.. (1995). Radioactivities Made in Supernovae. Annals of the New York Academy of Sciences. 759(1). 388–391. 1 indexed citations
17.
Pinto, Philip A., Ronald E. Taam, & J. M. Laming. (1991). A New Model for X-Ray Burst Absorption Lines. Bulletin of the American Astronomical Society. 23(4). 1320. 1 indexed citations
18.
Pinto, Philip A. & S. E. Woosley. (1987). X-and γ-ray Spectra from Supernova 1987a. Bulletin of the American Astronomical Society. 19. 1050. 1 indexed citations
19.
Robertis, M. M. De & Philip A. Pinto. (1985). Spectrophotometry of the supernova 1983u in NGC 3227. The Astrophysical Journal. 293. L77–L77. 2 indexed citations
20.
Mallama, Anthony, et al.. (1975). Minima of Eclipsing Variables. Information Bulletin on Variable Stars. 1249. 1. 1 indexed citations

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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