K. Pottschmidt

8.9k total citations
210 papers, 4.4k citations indexed

About

K. Pottschmidt is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Geophysics. According to data from OpenAlex, K. Pottschmidt has authored 210 papers receiving a total of 4.4k indexed citations (citations by other indexed papers that have themselves been cited), including 207 papers in Astronomy and Astrophysics, 84 papers in Nuclear and High Energy Physics and 45 papers in Geophysics. Recurrent topics in K. Pottschmidt's work include Astrophysical Phenomena and Observations (190 papers), Pulsars and Gravitational Waves Research (117 papers) and Astrophysics and Cosmic Phenomena (74 papers). K. Pottschmidt is often cited by papers focused on Astrophysical Phenomena and Observations (190 papers), Pulsars and Gravitational Waves Research (117 papers) and Astrophysics and Cosmic Phenomena (74 papers). K. Pottschmidt collaborates with scholars based in United States, Germany and Spain. K. Pottschmidt's co-authors include J. Wilms, Michael A. Nowak, R. E. Rothschild, Felix Fürst, G. G. Pooley, R. Staubert, I. Kreykenbohm, John A. Tomsick, P. Kretschmar and V. Grinberg and has published in prestigious journals such as Science, SHILAP Revista de lepidopterología and The Astrophysical Journal.

In The Last Decade

K. Pottschmidt

191 papers receiving 4.3k citations

Author Peers

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

Author Last Decade Papers Cites
K. Pottschmidt 4.3k 1.7k 1.0k 463 261 210 4.4k
S. Campana 5.1k 1.2× 1.3k 0.8× 1.1k 1.0× 272 0.6× 181 0.7× 310 5.3k
E. Kuulkers 4.7k 1.1× 1.2k 0.7× 1.3k 1.2× 564 1.2× 226 0.9× 299 4.8k
John A. Tomsick 4.7k 1.1× 2.0k 1.2× 660 0.6× 670 1.4× 183 0.7× 272 4.8k
P. Kaaret 4.1k 1.0× 1.8k 1.1× 512 0.5× 462 1.0× 117 0.4× 205 4.3k
Mariano Méndez 5.1k 1.2× 1.5k 0.9× 1.5k 1.4× 740 1.6× 152 0.6× 216 5.2k
A. N. Parmar 3.0k 0.7× 811 0.5× 695 0.7× 423 0.9× 206 0.8× 186 3.2k
J. Homan 6.5k 1.5× 2.2k 1.4× 1.4k 1.3× 1.2k 2.5× 168 0.6× 210 6.6k
M. Gilfanov 5.0k 1.2× 2.0k 1.2× 381 0.4× 276 0.6× 212 0.8× 275 5.1k
J. H. Swank 5.5k 1.3× 1.3k 0.8× 1.6k 1.6× 541 1.2× 249 1.0× 247 5.7k
Tadayasu Dotani 3.6k 0.8× 1.2k 0.7× 618 0.6× 525 1.1× 115 0.4× 175 3.8k

Countries citing papers authored by K. Pottschmidt

Since Specialization
Citations

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

Fields of papers citing papers by K. Pottschmidt

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of K. Pottschmidt

This figure shows the co-authorship network connecting the top 25 collaborators of K. Pottschmidt. A scholar is included among the top collaborators of K. Pottschmidt 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 K. Pottschmidt. K. Pottschmidt 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.
Mizumoto, Misaki, Yoshiaki Kanemaru, S. Yamada, et al.. (2025). High-count-rate effects in event processing for the XRISM/Resolve X-ray microcalorimeter. II. Energy scale and resolution in orbit. Publications of the Astronomical Society of Japan. 77(Supplement_1). S39–S49.
2.
Uttley, P., Matteo Bachetti, Arash Bahramian, et al.. (2025). Long-term variability of Cygnus X−1. IX. A spectral-timing comparison of Cygnus X−1 and MAXI J1820+070 in the hard state. Monthly Notices of the Royal Astronomical Society. 542(2). 982–997.
3.
Sokolova-Lapa, E., Jakob Stierhof, Ralf Ballhausen, et al.. (2024). An in-depth analysis of the variable cyclotron lines in GX 301−2. Astronomy and Astrophysics. 686. A95–A95. 2 indexed citations
4.
Corbet, R. H. D., et al.. (2023). Investigating the Superorbital Modulations in 4U 1909 + 07, IGR J16418-4532, and IGR J16479-4514 with Swift XRT, BAT, and NuSTAR Observations. The Astrophysical Journal. 948(1). 45–45. 2 indexed citations
5.
Zhou, Menglei, V. Grinberg, Qingcui Bu, et al.. (2022). The spectral-timing analysis of Cygnus X-1 with Insight-HXMT. Astronomy and Astrophysics. 666. A172–A172. 6 indexed citations
6.
Yukita, Mihoko, A. Ptak, A. E. Hornschemeier, et al.. (2017). Identification of the Hard X-Ray Source Dominating the E > 25 keV Emission of the Nearby Galaxy M31. The Astrophysical Journal. 838(1). 47–47. 5 indexed citations
7.
Rothschild, R. E., M. Bissinger, K. Pottschmidt, et al.. (2017). Discovery and modelling of a flattening of the positive cyclotron line/luminosity relation in GX 304−1 with RXTE. arXiv (Cornell University). 466(3). 2752–2779. 16 indexed citations
8.
Klochkov, D., К. А. Постнов, E. Sokolova-Lapa, et al.. (2017). Luminosity-dependent changes of the cyclotron line energy and spectral hardness in Cepheus X-4. Astronomy and Astrophysics. 601. A126–A126. 35 indexed citations
9.
Schönherr, G., Sebastian Falkner, K. Pottschmidt, et al.. (2016). Cyclotron resonant scattering feature simulations. Astronomy and Astrophysics. 597. A3–A3. 31 indexed citations
10.
Dauser, Thomas, V. Grinberg, Juan Rodríguez, et al.. (2016). Revealing the broad iron Kαline in Cygnus X-1 through simultaneousXMM-Newton, RXTE, and INTEGRAL observations. Astronomy and Astrophysics. 589. A14–A14. 23 indexed citations
11.
Bozzo, E., E. Kuulkers, A. Bazzano, et al.. (2015). INTEGRAL observations of SAX J1808.4-3658 currently in outburst. The astronomer's telegram. 7380. 1–1.
12.
Pearlman, Aaron B., R. H. D. Corbet, & K. Pottschmidt. (2013). Superorbital Modulation and Orbital Parameters of the Eclipsing High-Mass X-ray Pulsar IGR J16493-4348. 221. 2 indexed citations
13.
Ferrigno, C., R. Farinelli, E. Bozzo, et al.. (2013). RX J0440.9 + 4431: a persistent Be/X-ray binary in outburst. Astronomy and Astrophysics. 553. A103–A103. 30 indexed citations
14.
Fürst, Felix, I. Kreykenbohm, S. Suchy, et al.. (2010). 4U 1909+07: a well-hidden pearl. Astronomy and Astrophysics. 525. A73–A73. 12 indexed citations
15.
Kreykenbohm, I., K. Pottschmidt, J. Wilms, et al.. (2010). X-ray variation statistics and wind clumping in Vela X-1. Astronomy and Astrophysics. 519. A37–A37. 48 indexed citations
16.
Pottschmidt, K.. (2009). Monitoring the black hole binary GRS 1758-258 with INTEGRAL and RXTE. NASA STI Repository (National Aeronautics and Space Administration). 98–98. 1 indexed citations
17.
McBride, V. A., J. Wilms, I. Kreykenbohm, et al.. (2007). On the cyclotron line in Cepheus X-4. Astronomy and Astrophysics. 470(3). 1065–1070. 17 indexed citations
18.
Wilms, J., et al.. (2006). Long term variability of Cygnus X-1. Astronomy and Astrophysics. 447(1). 245–261. 88 indexed citations
19.
Pottschmidt, K., M. Chernyakova, A. A. Zdziarski, et al.. (2006). INTEGRALandRXTEmonitoring of GRS 1758-258 in 2003 and 2004. Astronomy and Astrophysics. 452(1). 285–294. 20 indexed citations
20.
Gleissner, T., J. Wilms, G. G. Pooley, et al.. (2004). Long term variability of Cygnus X-1. Astronomy and Astrophysics. 425(3). 1061–1068. 39 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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