V. Burwitz

6.8k total citations · 1 hit paper
192 papers, 2.5k citations indexed

About

V. Burwitz is a scholar working on Astronomy and Astrophysics, Radiation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, V. Burwitz has authored 192 papers receiving a total of 2.5k indexed citations (citations by other indexed papers that have themselves been cited), including 156 papers in Astronomy and Astrophysics, 49 papers in Radiation and 31 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in V. Burwitz's work include Astrophysical Phenomena and Observations (124 papers), Advanced X-ray Imaging Techniques (43 papers) and Adaptive optics and wavefront sensing (28 papers). V. Burwitz is often cited by papers focused on Astrophysical Phenomena and Observations (124 papers), Advanced X-ray Imaging Techniques (43 papers) and Adaptive optics and wavefront sensing (28 papers). V. Burwitz collaborates with scholars based in Germany, United States and Italy. V. Burwitz's co-authors include P. Predehl, J. S. Kaastra, G. Hasinger, Y. Ikebe, S. Komossa, V. E. Zavlin, F. Haberl, Jan‐Uwe Ness, R. Mewe and Gisela Hartner and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

V. Burwitz

183 papers receiving 2.4k citations

Hit Papers

Discovery of a Binary Active Galactic Nucleus in the Ultr... 2002 2026 2010 2018 2002 100 200 300

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
V. Burwitz Germany 24 2.2k 479 299 287 207 192 2.5k
P. Predehl Germany 26 2.3k 1.0× 798 1.7× 301 1.0× 303 1.1× 206 1.0× 164 2.7k
K. Dennerl Germany 23 1.6k 0.7× 436 0.9× 525 1.8× 412 1.4× 172 0.8× 119 2.0k
N. Kawai Japan 26 1.8k 0.8× 838 1.7× 137 0.5× 275 1.0× 202 1.0× 262 2.3k
G. Branduardi‐Raymont United Kingdom 31 3.6k 1.6× 1.1k 2.4× 251 0.8× 247 0.9× 250 1.2× 199 3.8k
M. J. Freyberg Germany 25 2.7k 1.2× 1.1k 2.4× 138 0.5× 197 0.7× 149 0.7× 137 2.9k
R. Willingale United Kingdom 31 2.5k 1.1× 1.1k 2.2× 131 0.4× 230 0.8× 95 0.5× 155 2.8k
F. Paerels United States 32 2.8k 1.3× 874 1.8× 205 0.7× 120 0.4× 285 1.4× 112 3.0k
Yuzuru Tawara Japan 22 1.4k 0.6× 572 1.2× 92 0.3× 197 0.7× 169 0.8× 153 1.6k
C. Erd Netherlands 13 2.1k 1.0× 591 1.2× 213 0.7× 169 0.6× 185 0.9× 54 2.4k
P. J. Serlemitsos United States 27 2.5k 1.1× 1.1k 2.3× 209 0.7× 406 1.4× 254 1.2× 198 2.8k

Countries citing papers authored by V. Burwitz

Since Specialization
Citations

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

Fields of papers citing papers by V. Burwitz

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of V. Burwitz

This figure shows the co-authorship network connecting the top 25 collaborators of V. Burwitz. A scholar is included among the top collaborators of V. Burwitz 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 V. Burwitz. V. Burwitz 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.
Burwitz, V., Gisela Hartner, Thomas Schmidt, et al.. (2023). Einstein probe wide field telescope flight mirror module characterization at PANTER test facility. 38–38. 1 indexed citations
2.
Friedrich, Péter, V. Burwitz, Gisela Hartner, et al.. (2023). Calibration of Einstein Probe FXT-QM and FM at the PANTER X-ray test facility. 120–120. 3 indexed citations
3.
Wolf, J., K. Nandra, M. Salvato, et al.. (2022). X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56. Astronomy and Astrophysics. 669. A127–A127. 6 indexed citations
4.
Heilmann, Ralf K., Alexander R. Bruccoleri, V. Burwitz, et al.. (2022). X-Ray Performance of Critical-angle Transmission Grating Prototypes for the Arcus Mission. The Astrophysical Journal. 934(2). 171–171. 1 indexed citations
5.
Burwitz, V., Gisela Hartner, Carlo Pelliciari, et al.. (2019). Developments in testing x-ray optics at MPE's PANTER facility. 42–42. 8 indexed citations
6.
Beuermann, K., V. Burwitz, & K. Reinsch. (2012). A new soft X-ray spectral model for polars with an application to AM Herculis. Springer Link (Chiba Institute of Technology). 13 indexed citations
7.
Rovilos, E., S. Fotopoulou, M. Salvato, et al.. (2011). Optical and infrared properties of active galactic nuclei in the Lockman Hole. Springer Link (Chiba Institute of Technology). 8 indexed citations
8.
Henze, M., W. Pietsch, F. Haberl, et al.. (2010). X-ray monitoring of classical novae in the central region of M 31. Springer Link (Chiba Institute of Technology). 24 indexed citations
9.
Pietsch, W., M. Henze, V. Burwitz, et al.. (2010). M31N 1963-09c - Fourth recorded outburst of a recurrent nova in M 31 or a foreground U Gem system?. ATel. 3001. 1. 2 indexed citations
10.
Pietsch, W., M. Henze, F. Haberl, & V. Burwitz. (2010). Swift detection of the fast turn-on of the recurrent nova M31N 1963-09c as a supersoft X-ray source. ATel. 3038. 1. 2 indexed citations
11.
Henze, M., W. Pietsch, G. Sala, et al.. (2009). The very short supersoft X-ray state of the classical nova M31N 2007-11a. Springer Link (Chiba Institute of Technology). 4 indexed citations
12.
13.
Meyer, F., et al.. (2008). Low heat conduction in white dwarf boundary layers?. Springer Link (Chiba Institute of Technology). 4 indexed citations
14.
Burwitz, V., K. Reinsch, J. Greiner, et al.. (2008). Variability in the cycle length of the supersoft source \nRX J0513.9-6951. Springer Link (Chiba Institute of Technology). 3 indexed citations
15.
Brinkmann, W., et al.. (2006). XMM-Newton observations of the eastern jet of SS 433. Springer Link (Chiba Institute of Technology). 22 indexed citations
16.
Porquet, D., N. Grosso, V. Burwitz, et al.. (2005). Discovery of a bright X-ray transient in the Galactic Center with XMM-Newton. Springer Link (Chiba Institute of Technology). 17 indexed citations
17.
Haberl, F., V. E. Zavlin, J. Trümper, & V. Burwitz. (2004). A phase-dependent absorption line in the spectrum of the X-ray pulsar RX J0720.4-3125. Springer Link (Chiba Institute of Technology). 45 indexed citations
18.
Burwitz, V., F. Haberl, R. Neuhäuser, et al.. (2003). The thermal radiation of the isolated neutron star RX J1856.5–3754 observed with Chandra and XMM-Newton. Springer Link (Chiba Institute of Technology). 110 indexed citations
19.
Burwitz, V., V. E. Zavlin, R. Neuhäuser, et al.. (2001). The Chandra LETGS high resolution X-ray spectrum of the isolated neutron star RX J1856.5-3754. Springer Link (Chiba Institute of Technology). 55 indexed citations
20.
Predehl, P., et al.. (2000). Chandra measurement of the geometrical distance to Cyg X-3 using its X-ray scattering halo. A&A. 357. 5 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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