M. R. Siebert

7.4k total citations
18 papers, 232 citations indexed

About

M. R. Siebert is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, M. R. Siebert has authored 18 papers receiving a total of 232 indexed citations (citations by other indexed papers that have themselves been cited), including 15 papers in Astronomy and Astrophysics, 5 papers in Nuclear and High Energy Physics and 3 papers in Instrumentation. Recurrent topics in M. R. Siebert's work include Gamma-ray bursts and supernovae (13 papers), Stellar, planetary, and galactic studies (7 papers) and Astrophysical Phenomena and Observations (5 papers). M. R. Siebert is often cited by papers focused on Gamma-ray bursts and supernovae (13 papers), Stellar, planetary, and galactic studies (7 papers) and Astrophysical Phenomena and Observations (5 papers). M. R. Siebert collaborates with scholars based in United States, Taiwan and France. M. R. Siebert's co-authors include R. J. Foley, D. O. Jones, C. D. Kilpatrick, Y. C. Pan, Saurabh W. Jha, K. Dettman, D. Scolnic, Adam G. Riess, D. A. Coulter and A. Rest and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Foot & Ankle Orthopaedics.

In The Last Decade

M. R. Siebert

16 papers receiving 216 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
M. R. Siebert United States 7 225 84 50 7 3 18 232
C. Rojas-Bravo United States 8 226 1.0× 85 1.0× 38 0.8× 4 0.6× 6 2.0× 15 244
Yuu Niino Japan 7 205 0.9× 114 1.4× 55 1.1× 8 1.1× 4 1.3× 18 228
F. Savini Italy 8 227 1.0× 159 1.9× 24 0.5× 5 0.7× 2 0.7× 10 232
A. Wilber Netherlands 8 240 1.1× 166 2.0× 25 0.5× 5 0.7× 2 0.7× 13 245
B. Mobasher United States 3 186 0.8× 59 0.7× 68 1.4× 10 1.4× 4 1.3× 3 187
R. Morganti United Kingdom 4 208 0.9× 78 0.9× 37 0.7× 5 0.7× 6 2.0× 4 212
Christopher H. Greer United States 8 185 0.8× 57 0.7× 45 0.9× 4 0.6× 4 1.3× 11 189
Bade Uzgil United States 5 142 0.6× 53 0.6× 37 0.7× 8 1.1× 5 1.7× 10 153
Konstantinos Kolokythas United States 10 187 0.8× 68 0.8× 59 1.2× 5 0.7× 3 1.0× 19 196
V. Smolčić Germany 5 242 1.1× 93 1.1× 80 1.6× 3 0.4× 4 1.3× 5 244

Countries citing papers authored by M. R. Siebert

Since Specialization
Citations

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

Fields of papers citing papers by M. R. Siebert

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by M. R. Siebert. 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 M. R. Siebert. The network helps show where M. R. Siebert may publish in the future.

Co-authorship network of co-authors of M. R. Siebert

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

All Works

18 of 18 papers shown
1.
Dhawan, Suhail, Justin Pierel, Minfeng Gu, et al.. (2024). Spectroscopic analysis of the strongly lensed SN Encore: constraints on cosmic evolution of Type Ia supernovae. Monthly Notices of the Royal Astronomical Society. 535(4). 2939–2947. 4 indexed citations
2.
Chen, Y., M. R. Drout, Anthony L. Piro, et al.. (2023). Late-time Hubble Space Telescope Observations of AT 2018cow. I. Further Constraints on the Fading Prompt Emission and Thermal Properties 50–60 days Post-discovery. The Astrophysical Journal. 955(1). 42–42. 4 indexed citations
3.
Siebert, M. R., R. J. Foley, Yossef Zenati, et al.. (2023). An Asymmetric Double-degenerate Type Ia Supernova Explosion with a Surviving Companion Star. The Astrophysical Journal. 958(2). 173–173. 6 indexed citations
4.
Jones, D. O., W. D. Kenworthy, Mi Dai, et al.. (2023). A Spectroscopic Model of the Type Ia Supernova–Host-galaxy Mass Correlation from SALT3. The Astrophysical Journal. 951(1). 22–22. 5 indexed citations
5.
Kilpatrick, C. D., D. A. Coulter, R. J. Foley, et al.. (2022). Updated Photometry of the Yellow Supergiant Progenitor and Late-time Observations of the Type IIb Supernova SN 2016gkg. The Astrophysical Journal. 936(2). 111–111. 11 indexed citations
6.
Siebert, M. R., et al.. (2022). Sesamoid View X-ray vs Weightbearing Computed Tomography in the Measurement of Metatarsal Pronation Angle. Foot & Ankle Orthopaedics. 7(4). 1 indexed citations
7.
Kenworthy, W. D., D. O. Jones, Mi Dai, et al.. (2021). SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances. The Astrophysical Journal. 923(2). 265–265. 56 indexed citations
8.
Dettman, K., Saurabh W. Jha, Mi Dai, et al.. (2021). The Foundation Supernova Survey: Photospheric Velocity Correlations in Type Ia Supernovae. The Astrophysical Journal. 923(2). 267–267. 10 indexed citations
9.
Siebert, M. R., et al.. (2020). Constraining the Asymmetry of Type Ia Supernovae Using Late-Time Spectra. 235.
10.
Siebert, M. R., C. D. Kilpatrick, R. J. Foley, & R. Cartier. (2020). Spectroscopic Classification of 2020oi with SOAR/Goodman. ATel. 13393. 1. 1 indexed citations
11.
Foley, R. J., G. Dimitriadis, David Jones, et al.. (2020). Measuring the Effect of Progenitor Metallicity on Type Ia Supernova Distance Estimates. 16238. 1 indexed citations
12.
Siebert, M. R., R. J. Foley, D. O. Jones, & Kyle W. Davis. (2020). A possible distance bias for type Ia supernovae with different ejecta velocities. Monthly Notices of the Royal Astronomical Society. 493(4). 5713–5725. 12 indexed citations
13.
Kilpatrick, C. D., D. A. Coulter, C. Rojas-Bravo, et al.. (2019). LIGO/Virgo S190425z: Swope follow-up observations.. GRB Coordinates Network. 24212. 1.
14.
Siebert, M. R., R. J. Foley, D. O. Jones, et al.. (2019). Investigating the diversity of Type Ia supernova spectra with the open-source relational data base kaepora. Monthly Notices of the Royal Astronomical Society. 486(4). 5785–5808. 18 indexed citations
15.
Jones, D. O., Adam G. Riess, D. Scolnic, et al.. (2018). Should Type Ia Supernova Distances Be Corrected for Their Local Environments?. The Astrophysical Journal. 867(2). 108–108. 65 indexed citations
16.
Coulter, D. A., C. D. Kilpatrick, M. R. Siebert, et al.. (2017). LIGO/Virgo G298048: Potential optical counterpart discovered by Swope telescope. GRB Coordinates Network. 21529. 1. 6 indexed citations
17.
Drout, M. R., Joshua D. Simon, B. J. Shappee, et al.. (2017). LIGO/VIRGO G298048: Magellan Optical Spectrum of the Potential Optical Counterpart Associated with NGC 4993. GRB Coordinates Network. 21547. 1. 1 indexed citations
18.
Kilpatrick, C. D., R. J. Foley, Louis E. Abramson, et al.. (2016). On the progenitor of the Type IIb supernova 2016gkg. Monthly Notices of the Royal Astronomical Society. 465(4). 4650–4657. 31 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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