J. Zsargó

636 total citations
28 papers, 443 citations indexed

About

J. Zsargó is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, J. Zsargó has authored 28 papers receiving a total of 443 indexed citations (citations by other indexed papers that have themselves been cited), including 23 papers in Astronomy and Astrophysics, 6 papers in Instrumentation and 5 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in J. Zsargó's work include Astrophysics and Star Formation Studies (21 papers), Stellar, planetary, and galactic studies (19 papers) and Astronomy and Astrophysical Research (6 papers). J. Zsargó is often cited by papers focused on Astrophysics and Star Formation Studies (21 papers), Stellar, planetary, and galactic studies (19 papers) and Astronomy and Astrophysical Research (6 papers). J. Zsargó collaborates with scholars based in United States, Mexico and Spain. J. Zsargó's co-authors include S. R. Federman, D. J. Hillier, Maurice A. Leutenegger, David H. Cohen, S. P. Owocki, Emma E. Wollman, Л. Георгиев, Jason A. Cardelli, Kenneth R. Sembach and A. W. Fullerton and has published in prestigious journals such as SHILAP Revista de lepidopterología, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

J. Zsargó

28 papers receiving 430 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
J. Zsargó United States 12 409 72 69 67 40 28 443
Tomer Holczer Israel 10 410 1.0× 80 1.1× 117 1.7× 24 0.4× 15 0.4× 14 479
P. A. Aannestad United States 10 282 0.7× 45 0.6× 40 0.6× 35 0.5× 34 0.8× 21 314
Adam G. Jensen United States 13 393 1.0× 66 0.9× 69 1.0× 68 1.0× 65 1.6× 21 442
C. Sneden United States 8 262 0.6× 41 0.6× 104 1.5× 17 0.3× 23 0.6× 13 300
T. Khouri Sweden 17 621 1.5× 62 0.9× 128 1.9× 95 1.4× 108 2.7× 42 679
C. Sneden United States 8 569 1.4× 43 0.6× 225 3.3× 28 0.4× 26 0.7× 8 610
A. Mesa‐Delgado Spain 13 546 1.3× 43 0.6× 124 1.8× 22 0.3× 48 1.2× 22 570
P. R. Wesselius Netherlands 10 702 1.7× 51 0.7× 106 1.5× 58 0.9× 78 1.9× 43 734
Y. Osorio Spain 10 291 0.7× 41 0.6× 116 1.7× 25 0.4× 7 0.2× 16 322
M. Bryce United Kingdom 16 812 2.0× 55 0.8× 176 2.6× 28 0.4× 49 1.2× 50 835

Countries citing papers authored by J. Zsargó

Since Specialization
Citations

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

Fields of papers citing papers by J. Zsargó

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of J. Zsargó

This figure shows the co-authorship network connecting the top 25 collaborators of J. Zsargó. A scholar is included among the top collaborators of J. Zsargó 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 J. Zsargó. J. Zsargó 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.
Sigalotti, Leonardo Di G., et al.. (2022). The impact of the initial core temperature on protostellar disc fragmentation. Monthly Notices of the Royal Astronomical Society. 519(2). 2578–2589. 2 indexed citations
2.
Zsargó, J., et al.. (2020). Creating and using large grids of precalculated model atmospheres for a rapid analysis of stellar spectra. Astronomy and Astrophysics. 643. A88–A88. 7 indexed citations
3.
Carciofi, A. C., et al.. (2016). HDUST3 — A chemically realistic, 3-D, NLTE radiative transfer code. Proceedings of the International Astronomical Union. 12(S329). 390–390. 1 indexed citations
4.
Cohen, David H., Emma E. Wollman, Maurice A. Leutenegger, et al.. (2014). Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive. Monthly Notices of the Royal Astronomical Society. 439(1). 908–923. 58 indexed citations
5.
Мирошниченко, А. С., N. Manset, S. V. Zharikov, et al.. (2014). Confirmation of the Luminous Blue Variable Status of MWC 930. Advances in Astronomy. 2014. 1–9. 3 indexed citations
6.
Barranco-Jiménez, M. A., et al.. (2012). An Endoreversible Thermodynamic Model Applied to the Convective Zone of the Sun. SHILAP Revista de lepidopterología. 2012. 1–7. 1 indexed citations
7.
Cohen, David H., Maurice A. Leutenegger, Emma E. Wollman, et al.. (2010). A mass-loss rate determination for ζ Puppis from the quantitative analysis of X-ray emission-line profiles. Monthly Notices of the Royal Astronomical Society. no–no. 45 indexed citations
8.
Leutenegger, Maurice A., David H. Cohen, J. Zsargó, et al.. (2010). MODELING BROADBAND X-RAY ABSORPTION OF MASSIVE STAR WINDS. The Astrophysical Journal. 719(2). 1767–1774. 25 indexed citations
9.
Zsargó, J., D. J. Hillier, J.‐C. Bouret, et al.. (2008). On the Importance of the Interclump Medium for Superionization: O vi Formation in the Wind of ζ Puppis. The Astrophysical Journal. 685(2). L149–L152. 34 indexed citations
10.
Zsargó, J., D. J. Hillier, & Л. Георгиев. (2007). Axi-symmetric models of B[e] supergiants. Astronomy and Astrophysics. 478(2). 543–551. 10 indexed citations
11.
12.
Георгиев, Л., D. J. Hillier, & J. Zsargó. (2006). 2D non-LTE modeling for axisymmetric winds. Astronomy and Astrophysics. 458(2). 597–608. 10 indexed citations
13.
Zsargó, J., D. J. Hillier, & Л. Георгиев. (2005). 2D non-LTE Modeling for Axi-symmetric Winds. II. A Short Characteristic Solution for Radiative Transfer in Rotating Winds. ArXiv.org. 9 indexed citations
14.
Zsargó, J., et al.. (2003). A search for OVI in the winds of B-type stars. Springer Link (Chiba Institute of Technology). 3 indexed citations
15.
Zsargó, J., Kenneth R. Sembach, J. Christopher Howk, & Blair D. Savage. (2003). Highly Ionized Gas in the Galactic Halo: AFUSESurvey of OviAbsorption toward 22 Halo Stars. The Astrophysical Journal. 586(2). 1019–1049. 37 indexed citations
16.
Federman, S. R. & J. Zsargó. (2001). Atomic Physics with the Goddard High Resolution Spectrograph on theHubble Space Telescope. V. Oscillator Strengths for Neutral Carbon Lines below 1200 A. The Astrophysical Journal. 555(2). 1020–1026. 8 indexed citations
17.
Petrovay, K. & J. Zsargó. (1998). On the validity of quasi-linear kinematic mean-field electrodynamics in astrophysical flows. Monthly Notices of the Royal Astronomical Society. 296(2). 245–252. 3 indexed citations
18.
Lawler, J. E., et al.. (1998). Absolute Vacuum Ultraviolet Oscillator Strengths in Coiiand the Interstellar Cobalt Abundance. The Astrophysical Journal. 500(2). 1064–1068. 21 indexed citations
19.
Zsargó, J., S. R. Federman, & Jason A. Cardelli. (1997). Atomic Physics with the Goddard High Resolution Spectrograph on the Hubble Space Telescope. The Astrophysical Journal. 484(2). 2 indexed citations
20.
Zsargó, J., S. R. Federman, & Jason A. Cardelli. (1997). Atomic Physics with the Goddard High Resolution Spectrograph on theHubble Space Telescope. III. Oscillator Strengths for Neutral Carbon. The Astrophysical Journal. 484(2). 820–827. 17 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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