K. Schenker

441 total citations
11 papers, 292 citations indexed

About

K. Schenker is a scholar working on Astronomy and Astrophysics, Ocean Engineering and Electrical and Electronic Engineering. According to data from OpenAlex, K. Schenker has authored 11 papers receiving a total of 292 indexed citations (citations by other indexed papers that have themselves been cited), including 9 papers in Astronomy and Astrophysics, 2 papers in Ocean Engineering and 2 papers in Electrical and Electronic Engineering. Recurrent topics in K. Schenker's work include Astrophysical Phenomena and Observations (8 papers), Pulsars and Gravitational Waves Research (6 papers) and Gamma-ray bursts and supernovae (5 papers). K. Schenker is often cited by papers focused on Astrophysical Phenomena and Observations (8 papers), Pulsars and Gravitational Waves Research (6 papers) and Gamma-ray bursts and supernovae (5 papers). K. Schenker collaborates with scholars based in United Kingdom, Switzerland and Germany. K. Schenker's co-authors include A. R. King, U. Kolb, J. M. Hameury, Z. Zhang, G. A. Wynn, C. A. Haswell, R. I. Hynes, H. G. Ritter, Jost Kaufmann and Daniel J. Rolfe and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Magnetic Resonance Imaging.

In The Last Decade

K. Schenker

11 papers receiving 280 citations

Peers

K. Schenker

AA

NHEP

GEOPH

CM

BE

R. M. Bandyopadhyay United States

Chin‐Ping Hu Taiwan

Д. В. Бисикало Russia

F. E. Marshall United States

J. J. M. in’t Zand Netherlands

B. Paul India

S. Kiyota Japan

D. G. Koch

I. A. Mereminskiy Russia

R. M. Bandyopadhyay United States

K. Schenker

259 ×1.0

AA

85 ×1.9

NHEP

24 ×0.7

GEOPH

25 ×1.3

CM

25 ×1.3

BE

Citations per year, relative to K. Schenker K. Schenker (= 1×) peers R. M. Bandyopadhyay

Countries citing papers authored by K. Schenker

Since Specialization

Citations

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

Fields of papers citing papers by K. Schenker

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

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

All Works

Sort: Min cites: Since: Top N: Style:

11 of 11 papers shown

1.

King, A. R., Daniel J. Rolfe, & K. Schenker. (2003). A new evolutionary channel for Type Ia supernovae. Monthly Notices of the Royal Astronomical Society. 341(4). L35–L38. 23 indexed citations

2.

King, A. R., K. Schenker, & J. M. Hameury. (2002). Blunting the spike: the cataclysmic variable minimum period. Monthly Notices of the Royal Astronomical Society. 335(3). 513–516. 56 indexed citations

3.

Haswell, C. A., R. I. Hynes, A. R. King, & K. Schenker. (2002). The ultraviolet line spectrum of the soft X-ray transient XTE J1118+480: a CNO-processed core exposed. Monthly Notices of the Royal Astronomical Society. 332(4). 928–932. 48 indexed citations

4.

Schenker, K., A. R. King, U. Kolb, G. A. Wynn, & Z. Zhang. (2002). AE Aquarii: how cataclysmic variables descend from supersoft binaries. Monthly Notices of the Royal Astronomical Society. 337(3). 1105–1112. 80 indexed citations

5.

King, A. R., J. P. Osborne, & K. Schenker. (2002). The short period supersoft source in M31. Monthly Notices of the Royal Astronomical Society. 329(2). L43–L46. 13 indexed citations

6.

Kolb, U., S. Rappaport, K. Schenker, & Steve B. Howell. (2001). Nova‐induced Mass Transfer Variations. The Astrophysical Journal. 563(2). 958–970. 14 indexed citations

7.

Burleigh, M. R., M. A. Barstow, K. Schenker, et al.. (2001). The low-mass white dwarf companion to ss Crateris. Monthly Notices of the Royal Astronomical Society. 327(4). 1158–1164. 3 indexed citations

8.

Schenker, K., U. Kolb, & H. G. Ritter. (1998). Properties of discontinuous and nova-amplified mass transfer in cataclysmic variables. Monthly Notices of the Royal Astronomical Society. 297(2). 633–647. 25 indexed citations

9.

Kaufmann, Jost, et al.. (1997). Study of water suction of concrete with magnetic resonance imaging methods. Magazine of Concrete Research. 49(180). 157–165. 17 indexed citations

10.

Schenker, K., U. Kolb, & H. G. Ritter. (1996). Nova Outbursts and the Secular Evolution of Cataclysmic Variables. International Astronomical Union Colloquium. 158. 447–448. 1 indexed citations

11.

Kaufmann, Jost, et al.. (1994). Water transport in concrete. Magnetic Resonance Imaging. 12(2). 203–205. 12 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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