P. Hoêflich

2.6k total citations
50 papers, 557 citations indexed

About

P. Hoêflich is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, P. Hoêflich has authored 50 papers receiving a total of 557 indexed citations (citations by other indexed papers that have themselves been cited), including 47 papers in Astronomy and Astrophysics, 17 papers in Nuclear and High Energy Physics and 9 papers in Instrumentation. Recurrent topics in P. Hoêflich's work include Gamma-ray bursts and supernovae (43 papers), Stellar, planetary, and galactic studies (12 papers) and Astrophysics and Cosmic Phenomena (12 papers). P. Hoêflich is often cited by papers focused on Gamma-ray bursts and supernovae (43 papers), Stellar, planetary, and galactic studies (12 papers) and Astrophysics and Cosmic Phenomena (12 papers). P. Hoêflich collaborates with scholars based in United States, Germany and Chile. P. Hoêflich's co-authors include A. M. Khokhlov, Eva-Maria Mueller, E. Y. Hsiao, M. Stritzinger, M. M. Phillips, C. R. Burns, N. Morrell, N. B. Suntzeff, C. Ashall and E. Baron and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

P. Hoêflich

43 papers receiving 531 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
P. Hoêflich United States	11	551	191	43	14	8	50	557
M. Jarvis Germany	9	457 0.8×	183 1.0×	35 0.8×	13 0.9×	6 0.8×	13	467
F. Ciaraldi-Schoolmann Germany	10	609 1.1×	181 0.9×	46 1.1×	13 0.9×	21 2.6×	11	626
Aaron Sokasian United States	7	459 0.8×	214 1.1×	53 1.2×	10 0.7×	5 0.6×	7	471
Melina C. Bersten Japan	16	759 1.4×	248 1.3×	77 1.8×	4 0.3×	5 0.6×	31	769
S. E. G. Hales United Kingdom	9	367 0.7×	282 1.5×	38 0.9×	13 0.9×	8 1.0×	10	381
Conrad Chan Australia	8	430 0.8×	162 0.8×	59 1.4×	3 0.2×	5 0.6×	9	457
Nicolas Vasset France	4	302 0.5×	172 0.9×	21 0.5×	12 0.9×	8 1.0×	5	347
В. П. Утробин Russia	15	566 1.0×	224 1.2×	37 0.9×	16 1.1×	6 0.8×	48	576
V. Cracco Italy	12	443 0.8×	256 1.3×	80 1.9×	5 0.4×	9 1.1×	26	452
S. Dichiara United States	15	455 0.8×	194 1.0×	23 0.5×	4 0.3×	8 1.0×	43	465

Countries citing papers authored by P. Hoêflich

Since Specialization

Citations

This map shows the geographic impact of P. Hoêflich'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 P. Hoêflich with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites P. Hoêflich more than expected).

Fields of papers citing papers by P. Hoêflich

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by P. Hoêflich. 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 P. Hoêflich. The network helps show where P. Hoêflich may publish in the future.

Co-authorship network of co-authors of P. Hoêflich

This figure shows the co-authorship network connecting the top 25 collaborators of P. Hoêflich. A scholar is included among the top collaborators of P. Hoêflich 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 P. Hoêflich. P. Hoêflich is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

Hirai, Ryosuke, et al.. (2025). Supernova-induced Binary-interaction-powered Supernovae: A Model for SN2022jli. The Astrophysical Journal. 995(1). 55–55. 1 indexed citations

Ashall, C., Melissa Shahbandeh, E. Y. Hsiao, et al.. (2025). Using Nebular Near-infrared Spectroscopy to Measure Asymmetric Chemical Distributions in 2003fg-like Thermonuclear Supernovae. The Astrophysical Journal. 984(1). 34–34. 4 indexed citations

Ashall, C., Melissa Shahbandeh, James M. DerKacy, et al.. (2025). The Hawaii Infrared Supernova Study (HISS): Spectroscopic Data Release 1. The Astrophysical Journal Supplement Series. 281(2). 28–28.

Domı́nguez, I., Almadena Chtchelkanova, P. Hoêflich, et al.. (2025). Three-dimensional Structure of Incomplete Carbon–Oxygen Detonations in Type Ia Supernovae. The Astrophysical Journal. 982(2). 204–204. 1 indexed citations

Baron, E., C. R. Burns, E. Y. Hsiao, et al.. (2024). Extrapolation of Type Ia Supernova Spectra into the Near-infrared Using Principal Component Analysis. The Astrophysical Journal. 967(1). 55–55. 1 indexed citations

Gall, C., J. Hjorth, L. Christensen, et al.. (2024). Origin of the Strong Sodium Absorption of the Lensed Supernova 2016geu at z = 0.4. The Astrophysical Journal. 972(1). 114–114.

Hoêflich, P., E. Y. Hsiao, M. M. Phillips, et al.. (2024). Type Ia Supernova Progenitor Properties and their Host Galaxies. The Astrophysical Journal. 969(2). 80–80. 3 indexed citations

Vasylyev, Sergiy S., Yi Yang, Kishore C. Patra, et al.. (2023). Spectropolarimetry of the Type IIP supernova 2021yja: an unusually high continuum polarization during the photospheric phase. Monthly Notices of the Royal Astronomical Society. 527(2). 3106–3121. 2 indexed citations

Anderson, J. P., Melina C. Bersten, M. Hamuy, et al.. (2022). Type II supernovae from the Carnegie Supernova Project-I. Astronomy and Astrophysics. 660. A42–A42. 20 indexed citations

10.

Graham, M. L., Sahana Kumar, David J. Sand, et al.. (2022). Nebular-phase spectra of Type Ia supernovae from the Las Cumbres Observatory Global Supernova Project. Monthly Notices of the Royal Astronomical Society. 511(3). 3682–3707. 5 indexed citations

11.

Rho, Jeonghee, A. Evans, T. R. Geballe, et al.. (2021). Near-infrared and Optical Observations of Type Ic SN 2020oi and Broad-lined Type Ic SN 2020bvc: Carbon Monoxide, Dust, and High-velocity Supernova Ejecta. Repository of the Academy's Library (Library of the Hungarian Academy of Sciences). 1 indexed citations

12.

Baron, E., C. Ashall, C. R. Burns, et al.. (2020). Carnegie supernova project: classification of type Ia supernovae. Conicet. 8 indexed citations

13.

Ashall, C., E. Y. Hsiao, P. Hoêflich, et al.. (2019). Carnegie Supernova Project-II: Using Near-infrared Spectroscopy to Determine the Location of the Outer ⁵⁶Ni in Type Ia Supernovae^∗. The Astrophysical Journal Letters. 875(2). L14–L14. 7 indexed citations

14.

Patat, F., S. Taubenberger, D. Baade, et al.. (2014). Spectropolarimetry of SN2014J in M82: another low R(V) event. ATel. 5830. 1. 1 indexed citations

15.

Quimby, R., D. B. Fox, P. Hoêflich, B. Roman, & J. C. Wheeler. (2005). GRB 051109: HET optical spectrum and absorption redshift.. GCN. 4221. 1. 3 indexed citations

16.

Quimby, R., et al.. (2005). Texas Supernova Search: A Wide Field Search for Nearby SNe. American Astronomical Society Meeting Abstracts. 207. 1 indexed citations

17.

Avrett, E. H., P. Hoêflich, H. Uitenbroek, & P. Ulmschneider. (1996). Temporal Variations in Solar Chromospheric Modeling.. 109. 105. 1 indexed citations

18.

Wheeler, J. C., et al.. (1996). Maximum Brightness and Post-Maximum Decline of Light Curves of SN Ia: A Comparison of Theory and Observations. AAS. 189(4). 1332. 1 indexed citations

19.

Hoêflich, P., A. M. Khokhlov, & E. Müeller. (1994). Gamma-ray light curves and spectra of models for Type IA supernovae. The Astrophysical Journal Supplement Series. 92. 501–501. 10 indexed citations

20.

Mueller, Eva-Maria & P. Hoêflich. (1992). A comparison of calculated and observed monochromatic Type Ia supernova light curves. STIN. 281(1). 17629–65. 3 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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