M. Mühlegger

605 total citations
18 papers, 265 citations indexed

About

M. Mühlegger is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, M. Mühlegger has authored 18 papers receiving a total of 265 indexed citations (citations by other indexed papers that have themselves been cited), including 17 papers in Astronomy and Astrophysics, 8 papers in Instrumentation and 4 papers in Nuclear and High Energy Physics. Recurrent topics in M. Mühlegger's work include Astrophysical Phenomena and Observations (14 papers), Galaxies: Formation, Evolution, Phenomena (12 papers) and Astronomy and Astrophysical Research (8 papers). M. Mühlegger is often cited by papers focused on Astrophysical Phenomena and Observations (14 papers), Galaxies: Formation, Evolution, Phenomena (12 papers) and Astronomy and Astrophysical Research (8 papers). M. Mühlegger collaborates with scholars based in Germany, Chile and Spain. M. Mühlegger's co-authors include Joana Santos, A. de Hoon, J. Kohnert, A. Schwope, P. Rosati, R. Fassbender, R. Šuhada, D. Pierini, A. Nastasi and J. J. Mohr and has published in prestigious journals such as The Astrophysical Journal Supplement Series, Astronomy and Astrophysics and New Journal of Physics.

In The Last Decade

M. Mühlegger

17 papers receiving 261 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. Mühlegger Germany 10 253 111 38 25 15 18 265
Davide Decataldo Italy 8 262 1.0× 84 0.8× 23 0.6× 14 0.6× 4 0.3× 10 282
Arnab Sarkar United States 9 211 0.8× 54 0.5× 47 1.2× 19 0.8× 6 0.4× 24 251
Nimisha Kumari United States 12 407 1.6× 143 1.3× 24 0.6× 12 0.5× 9 0.6× 31 445
Mitchell Revalski United States 14 401 1.6× 115 1.0× 71 1.9× 9 0.4× 7 0.5× 35 427
Tim Heckman United States 12 420 1.7× 108 1.0× 91 2.4× 8 0.3× 4 0.3× 15 425
M. G. Pastoriza Brazil 9 465 1.8× 100 0.9× 45 1.2× 22 0.9× 4 0.3× 19 479
M. V. F. Copetti Brazil 12 300 1.2× 73 0.7× 21 0.6× 21 0.8× 3 0.2× 32 322
M. Contini Israel 14 503 2.0× 46 0.4× 77 2.0× 10 0.4× 8 0.5× 61 520
Alessandra Slemer Italy 6 332 1.3× 147 1.3× 19 0.5× 14 0.6× 8 0.5× 16 356
L. Piau France 8 257 1.0× 52 0.5× 49 1.3× 20 0.8× 3 0.2× 11 291

Countries citing papers authored by M. Mühlegger

Since Specialization
Citations

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

Fields of papers citing papers by M. Mühlegger

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of M. Mühlegger. A scholar is included among the top collaborators of M. Mühlegger 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. Mühlegger. M. Mühlegger 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.
Hoon, A. de, G. Lamer, A. Schwope, et al.. (2013). Distant clusters of galaxies in a deep XMM‐Newton observation. Astronomische Nachrichten. 334(4-5). 470–473. 1 indexed citations
2.
Hoon, A. de, G. Lamer, A. Schwope, et al.. (2012). Distant galaxy clusters in a deepXMM-Newtonfield within the CFTHLS D4. Astronomy and Astrophysics. 551. A8–A8. 5 indexed citations
3.
Nastasi, A., R. Fassbender, H. Böhringer, et al.. (2011). Discovery of the X-ray selected galaxy cluster XMMU J0338.8+0021 atz= 1.49. Astronomy and Astrophysics. 532. L6–L6. 11 indexed citations
4.
Šuhada, R., R. Fassbender, A. Nastasi, et al.. (2011). Exploring the galaxy cluster-group transition regime at high redshifts. Astronomy and Astrophysics. 530. A110–A110. 4 indexed citations
5.
Fassbender, R., A. Nastasi, H. Böhringer, et al.. (2011). The X-ray luminous galaxy cluster XMMU J1007.4+1237 atz= 1.56. Astronomy and Astrophysics. 527. L10–L10. 44 indexed citations
6.
Šuhada, R., R. Fassbender, A. Nastasi, et al.. (2011). Exploring the galaxy cluster-group transition regime at high redshifts: Physical properties of two newly detected z > 1 systems. MPG.PuRe (Max Planck Society). 3 indexed citations
7.
Barnes, Peter J., Yoshinori Yonekura, Y. Fukui, et al.. (2011). THE GALACTIC CENSUS OF HIGH- AND MEDIUM-MASS PROTOSTARS. I. CATALOGS AND FIRST RESULTS FROM MOPRA HCO + MAPS. The Astrophysical Journal Supplement Series. 196(1). 12–12. 34 indexed citations
8.
Fassbender, R., A. Nastasi, H. Böhringer, et al.. (2011). The X-ray luminous galaxy cluster XMMU J1007.4+1237 at z=1.56 - The dawn of starburst activity in cluster cores. arXiv (Cornell University). 527. 1–6. 35 indexed citations
9.
Fassbender, R., H. Böhringer, A. Nastasi, et al.. (2011). The x-ray luminous galaxy cluster population at 0.9 <z≲ 1.6 as revealed by the XMM-NewtonDistant Cluster Project. New Journal of Physics. 13(12). 125014–125014. 52 indexed citations
10.
Nastasi, A., R. Fassbender, H. Böhringer, et al.. (2011). Discovery of the X-ray selected galaxy cluster XMMU J0338.8+0021 at z = 1.49 - indications of a young system with a brightest galaxy in formation. Americanae (AECID Library). 532. 1–8. 9 indexed citations
11.
Schwope, A., G. Lamer, A. de Hoon, et al.. (2010). XMMU J100750.5+125818: a strong lensing cluster atz= 1.082. Astronomy and Astrophysics. 513. L10–L10. 16 indexed citations
12.
Fassbender, R., H. Böhringer, Joana Santos, et al.. (2010). A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 atz= 0.975. Astronomy and Astrophysics. 527. A78–A78. 11 indexed citations
13.
Fassbender, R., H. Böhringer, Joana Santos, et al.. (2010). A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 at z=0.975 - Observing the assembly of a massive system. arXiv (Cornell University). 527. 1–26. 11 indexed citations
14.
Schmid, Christian, Michael Martin, J. Wilms, et al.. (2010). Simulations of X-Ray Telescopes for eROSITA and IXO. AIP conference proceedings. 591–592. 2 indexed citations
15.
Mühlegger, M.. (2010). Simulated Observations of Galaxy Clusters for Current and Future X-ray Surveys. mediaTUM – the media and publications repository of the Technical University Munich (Technical University Munich). 1 indexed citations
16.
Freyberg, M. J., Wolfgang Burkert, Péter Friedrich, et al.. (2008). New technology and techniques for x-ray mirror calibration at PANTER. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 5 indexed citations
17.
Friedrich, P., H. Bräuninger, Wolfgang Burkert, et al.. (2008). Design and development of the eROSITA x-ray mirrors. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 7011. 70112T–70112T. 21 indexed citations
18.
Duscha, S., et al.. (2006). GRB060801: optical upper limits in R. Max Planck Institute for Plasma Physics. 5383. 1.

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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