M. Wolf

3.4k total citations
151 papers, 1.6k citations indexed

About

M. Wolf is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, M. Wolf has authored 151 papers receiving a total of 1.6k indexed citations (citations by other indexed papers that have themselves been cited), including 146 papers in Astronomy and Astrophysics, 71 papers in Instrumentation and 26 papers in Computational Mechanics. Recurrent topics in M. Wolf's work include Stellar, planetary, and galactic studies (122 papers), Astronomy and Astrophysical Research (71 papers) and Astrophysics and Star Formation Studies (66 papers). M. Wolf is often cited by papers focused on Stellar, planetary, and galactic studies (122 papers), Astronomy and Astrophysical Research (71 papers) and Astrophysics and Star Formation Studies (66 papers). M. Wolf collaborates with scholars based in Czechia, Slovakia and United States. M. Wolf's co-authors include P. Zasche, L. Šarounová, Petr Pravec, Miloslav Zejda, James B. Pollack, C. E. Carlston, D. S. Colburn, June Hunter, Ralph A. Kahn and P. Harmanec and has published in prestigious journals such as Science, SHILAP Revista de lepidopterología and Journal of Geophysical Research Atmospheres.

In The Last Decade

M. Wolf

142 papers receiving 1.5k citations

Author Peers

Peers are selected by citation overlap in the author's most active subfields. citations · hero ref

Author						Papers	Cites
M. Wolf	1.6k	433	103	100	96	151	1.6k
S. P. Ewald	1.8k 1.1×	191 0.4×	349 3.4×	87 0.9×	31 0.3×	60	1.9k
W. A. Baum	1.6k 1.0×	412 1.0×	145 1.4×	92 0.9×	21 0.2×	91	1.7k
A. L. Whipple	1000 0.6×	244 0.6×	76 0.7×	13 0.1×	52 0.5×	55	1.2k
P. J. Shelus	1.2k 0.7×	254 0.6×	70 0.7×	13 0.1×	55 0.6×	74	1.4k
R. Molinaro	798 0.5×	343 0.8×	47 0.5×	52 0.5×	38 0.4×	49	885
L. F. A. Teodoro	1000 0.6×	182 0.4×	68 0.7×	22 0.2×	17 0.2×	51	1.1k
A. García Muñoz	1.1k 0.7×	168 0.4×	319 3.1×	94 0.9×	21 0.2×	80	1.2k
Barbara M. Middlehurst	952 0.6×	55 0.1×	122 1.2×	41 0.4×	53 0.6×	21	1.1k
Gordon I. Ogilvie	3.6k 2.2×	167 0.4×	64 0.6×	46 0.5×	226 2.4×	111	3.7k
D. Hatzidimitriou	1.5k 0.9×	457 1.1×	266 2.6×	316 3.2×	87 0.9×	78	1.8k

Countries citing papers authored by M. Wolf

Since Specialization

Citations

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

Fields of papers citing papers by M. Wolf

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. Wolf

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

All Works

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20 of 20 papers shown

Hornoch, K., A. W. Shafter, H. Kučáková, et al.. (2024). Exploring the Maximum Magnitude versus Rate of Decline Relation for Novae in M31. The Astrophysical Journal Supplement Series. 272(2). 28–28. 2 indexed citations

Zharikov, S. V., et al.. (2023). The Z Camelopardalis-type Star AY Piscium: Stellar and Accretion Disk Parameters. The Astrophysical Journal. 950(1). 47–47. 2 indexed citations

Shafter, A. W., K. Hornoch, H. Kučáková, et al.. (2022). M31N 1926-07c: A Recurrent Nova in M31 with a 2.8 yr Recurrence Time. Research Notes of the AAS. 6(10). 214–214. 3 indexed citations

Wolf, M., Miloslav Zejda, M. Mašek, et al.. (2021). The two eccentric eclipsing binaries in multiple systems: V539 Arae and V335 Serpentis. New Astronomy. 92. 101708–101708. 2 indexed citations

Zasche, P., M. Wolf, H. Kučáková, et al.. (2020). First apsidal motion and light curve analysis of 162 eccentric eclipsing binaries from LMC. Springer Link (Chiba Institute of Technology). 4 indexed citations

Zasche, P., H. Lehmann, Joshua Pepper, et al.. (2020). CzeV1731: The unique doubly eclipsing quadruple system. Springer Link (Chiba Institute of Technology). 4 indexed citations

Zharikov, S. V., G. Tovmassian, V. Neustroev, et al.. (2020). Structure of accretion flows in the nova-like cataclysmic variable RW Tri. Monthly Notices of the Royal Astronomical Society. 497(2). 1475–1487. 13 indexed citations

Zasche, P., David Vokrouhlický, M. Wolf, et al.. (2019). Doubly eclipsing systems. Springer Link (Chiba Institute of Technology). 21 indexed citations

Zasche, P., M. Wolf, R. Uhlář, et al.. (2018). The first study of 54 new eccentric eclipsing binaries in our Galaxy. Springer Link (Chiba Institute of Technology). 6 indexed citations

10.

Skopal, A., S. Yu. Shugarov, M. Wolf, et al.. (2017). New outburst of the symbiotic nova AG Pegasi after 165 yr. Springer Link (Chiba Institute of Technology). 16 indexed citations

11.

Torres, Guillermo, Claud H. Sandberg Lacy, Francis C. Fekel, M. Wolf, & Matthew W. Muterspaugh. (2017). The Quadruple-lined, Doubly Eclipsing System V482 Persei. The Astrophysical Journal. 846(2). 115–115. 10 indexed citations

12.

Zasche, P., et al.. (2016). The first study of the light-travel time effect in massive LMC eclipsing binaries. Springer Link (Chiba Institute of Technology). 12 indexed citations

13.

Zasche, P., M. Wolf, J. Vraštil, et al.. (2014). Apsidal motion and a light curve solution for eighteen SMC eccentric eclipsing binaries. Springer Link (Chiba Institute of Technology). 33 indexed citations

14.

Harmanec, P., M. Wolf, H. Božić, et al.. (2014). Revised physical elements of the astrophysically important O9.5+O9.5V eclipsing binary system Y Cygni. Springer Link (Chiba Institute of Technology). 8 indexed citations

15.

Wolf, M.. (2014). Light-time effect as a valuable tool in stellar astrophysics. Contributions of the Astronomical Observatory Skalnaté Pleso. 43. 493. 2 indexed citations

16.

Zasche, P. & M. Wolf. (2013). Apsidal motion and absolute parameters for five LMC eccentric eclipsing binaries. Springer Link (Chiba Institute of Technology). 12 indexed citations

17.

Zasche, P. & M. Wolf. (2011). V456 Ophiuchi and V490 Cygni: Systems with the shortest apsidal-motion periods. Springer Link (Chiba Institute of Technology). 3 indexed citations

18.

Harmanec, P., H. Božić, P. Mayer, et al.. (2011). V2368 Ophiuchi: an eclipsing and double-lined spectroscopic binary used as a photometric comparison star for U Ophiuchi. Springer Link (Chiba Institute of Technology). 1 indexed citations

19.

Hornoch, K., et al.. (2010). Apparent Nova in M31: M31N 2010-10e. 2573. 1. 1 indexed citations

20.

Holmgren, D. & M. Wolf. (1996). Apsidal motion in the eclipsing binary IT Cassiopeiae. Observatory. 116. 307–312. 4 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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