M. Juda

2.1k total citations
56 papers, 1.1k citations indexed

About

M. Juda is a scholar working on Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics and Radiation. According to data from OpenAlex, M. Juda has authored 56 papers receiving a total of 1.1k indexed citations (citations by other indexed papers that have themselves been cited), including 33 papers in Astronomy and Astrophysics, 17 papers in Atomic and Molecular Physics, and Optics and 15 papers in Radiation. Recurrent topics in M. Juda's work include Superconducting and THz Device Technology (12 papers), Adaptive optics and wavefront sensing (11 papers) and Astrophysical Phenomena and Observations (11 papers). M. Juda is often cited by papers focused on Superconducting and THz Device Technology (12 papers), Adaptive optics and wavefront sensing (11 papers) and Astrophysical Phenomena and Observations (11 papers). M. Juda collaborates with scholars based in United States, Germany and Netherlands. M. Juda's co-authors include D. McCammon, Bradford J. Wargelin, Richard L. Kelley, S. H. Moseley, Wei Cui, Andrew E. Szymkowiak, J. Zhang, J. J. Drake, Maxim Markevitch and Herman L. Marshall and has published in prestigious journals such as Physical review. B, Condensed matter, The Astrophysical Journal and Sensors.

In The Last Decade

M. Juda

49 papers receiving 1.1k 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. Juda United States 18 934 447 154 122 95 56 1.1k
N. Nakajima Japan 28 1.6k 1.8× 2.3k 5.2× 157 1.0× 220 1.8× 56 0.6× 194 2.5k
M. Ottaviani France 24 1.0k 1.1× 1.4k 3.1× 105 0.7× 129 1.1× 9 0.1× 58 1.5k
E. Figueroa‐Feliciano United States 21 1.3k 1.4× 1.1k 2.5× 284 1.8× 265 2.2× 84 0.9× 120 2.0k
G. Vlad Italy 22 1.5k 1.6× 1.9k 4.2× 278 1.8× 88 0.7× 47 0.5× 77 2.0k
V. Igochine Germany 25 998 1.1× 1.6k 3.5× 121 0.8× 111 0.9× 81 0.9× 111 1.7k
S. Briguglio Italy 23 1.4k 1.5× 1.8k 4.1× 301 2.0× 83 0.7× 50 0.5× 68 2.0k
D. Farina Italy 20 321 0.3× 1.0k 2.3× 507 3.3× 165 1.4× 39 0.4× 89 1.2k
L. Sugiyama United States 17 806 0.9× 1.1k 2.4× 101 0.7× 102 0.8× 16 0.2× 52 1.2k
J.C. Vallet France 18 278 0.3× 739 1.7× 65 0.4× 104 0.9× 103 1.1× 43 909
M. F. F. Nave United Kingdom 25 1.3k 1.4× 2.2k 4.9× 130 0.8× 136 1.1× 27 0.3× 84 2.3k

Countries citing papers authored by M. Juda

Since Specialization
Citations

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

Fields of papers citing papers by M. Juda

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of M. Juda. A scholar is included among the top collaborators of M. Juda 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. Juda. M. Juda 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.
2.
Elvis, M., Roger Brissenden, G. Fabbiano, et al.. (2014). Active X-ray Optics for Generation-X, the Next High Resolution X-ray Observatory.
3.
Juda, M. & Margarita Karovska. (2010). Chandra's Ultimate Angular Resolution: Studies of the HRC-I Point Spread Function. 1 indexed citations
4.
Wargelin, Bradford J., Jonathan D. Slavin, I. P. Robertson, & M. Juda. (2009). Solar Wind Charge Exchange in the Chandra Deep Field-South During Solar Max and Min. 205. 1 indexed citations
5.
Markwardt, C. B., M. Juda, & J. H. Swank. (2003). XTE J1807-294 - precise position and orbit determination. The astronomer's telegram. 127. 1.
6.
Juda, M., Rich Donnelly, A. Kenter, et al.. (2003). Characteristics of the on-orbit background of the Chandra x-ray observatory high-resolution camera. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 4851. 112–112. 2 indexed citations
7.
Drake, J. J., Herman L. Marshall, Stefan Dreizler, et al.. (2002). Is RX J1856.5−3754 a Quark Star?. The Astrophysical Journal. 572(2). 996–1001. 132 indexed citations
8.
Marshall, Herman L., D. E. Harris, John Grimes, et al.. (2001). Structure of the X-Ray Emission from the Jet of 3C 273. The Astrophysical Journal. 549(2). L167–L171. 88 indexed citations
9.
Marshall, Herman L., Daniel Dewey, Kathryn A. Flanagan, et al.. (1997). <title>Toward the calibration of the HETGS line response function</title>. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 3113. 160–171. 2 indexed citations
10.
Dewey, Daniel, Kathryn A. Flanagan, Herman L. Marshall, et al.. (1997). <title>Toward the calibration of the HETGS effective area</title>. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 3113. 144–159. 2 indexed citations
11.
Juda, M.. (1996). Subassembly Calibration: LETG. 4. 9. 2 indexed citations
12.
Flanagan, Kathryn A., Taotao Fang, John E. Davis, et al.. (1996). <title>Modeling the diffraction efficiencies of the AXAF high-energy transmission gratings: II</title>. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 2808. 650–676. 4 indexed citations
13.
Stahle, C. K., Richard L. Kelley, S. H. Moseley, et al.. (1994). Delayed thermalization of X-rays absorbed in tin films far below the superconducting transition temperature. Physica B Condensed Matter. 194-196. 127–128. 3 indexed citations
14.
Burbine, T. H., William Podgorski, M. Juda, et al.. (1994). <title>Molecular contamination study of iridium-coated x-ray mirrors</title>. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 2279. 12–26. 4 indexed citations
15.
Stahle, C. K., S. H. Moseley, Andrew E. Szymkowiak, et al.. (1993). Thermalization of X-rays in evaporated tin and bismuth films used as the absorbing materials in X-ray calorimeters. Journal of Low Temperature Physics. 93(3-4). 257–262. 5 indexed citations
16.
Moseley, S. H., M. Juda, Richard L. Kelley, et al.. (1992). X ray microcalorimeters: Principles and performance. 356. 13–19.
17.
Juda, M., J. J. Bloch, B. C. Edwards, et al.. (1991). Limits on the density of neutral gas within 100 parsecs from observations of the soft X-ray background. The Astrophysical Journal. 367. 182–182. 19 indexed citations
18.
McCammon, D., B. Edwards, M. Juda, et al.. (1990). Thermal detection of X-rays. NASA Technical Reports Server (NASA). 213–225. 1 indexed citations
19.
Szymkowiak, Andrew E., R. L. Kelley, G. M. Madejski, et al.. (1989). High resolution microcalorimeters as detectors for inelastic scattering (invited). Review of Scientific Instruments. 60(7). 1557–1560. 1 indexed citations
20.
Sanders, W. T., S. L. Snowden, J. J. Bloch, et al.. (1984). Ultrasoft X-Ray Background Observations of the Local Interstellar Medium. International Astronomical Union Colloquium. 81. 222–225. 1 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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