H.-S. Zechlin

4.5k citations
15 papers · 298 indexed · h-index 10

H.-S. Zechlin

13 papers receiving 288 citations

Peers

H.-S. Zechlin
Comparison fields: 5 of 20
  • Nuclear and High Energy Physics 285
  • Astronomy and Astrophysics 220
  • Radiological and Ultrasound Technology 4
  • Statistical and Nonlinear Physics 9
  • Instrumentation 1
Replace Tonia M. Venters with:
Tonia M. Venters United States
Silvia Manconi Italy
A. Tohuvavohu United States
I. E. Sleptsov Russia
Denise Boncioli Germany
Thomas Bronzwaer Netherlands
Ronnie Jansson Germany
Warren Essey United States
Bogumiła Świeżewska Poland
H.-S. Zechlin relative to Tonia M. Venters United States Tonia M. Venters's profile →
Citations per field
00.5×5.4×
Tonia M. Venters · 1×
Citations per year

Countries citing papers authored by H.-S. Zechlin

Since Specialization
Citations

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

Fields of papers citing papers by H.-S. Zechlin

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by H.-S. Zechlin. 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 H.-S. Zechlin. The network helps show where H.-S. Zechlin may publish in the future.

Co-authorship network

The 22 scholars most cited alongside H.-S. Zechlin, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with H.-S. Zechlin Line = papers co-authored together H.-S. Zechlin links everyone, so they are left out of the graph.

All Works

15 of 15 papers shown
#Work
1 202013
2 201820
3 201815
4 201712
5 20171
6 20170
7 201625
8 201634
9 201513
10 20138
11 201239
12 201129
13 201083
14
New Constraints on Hidden Photons using Very High Energy Gamma-Rays from the Crab Nebula.
20096
15 20090

About H.-S. Zechlin

H.-S. Zechlin is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics, Radiation, Radiological and Ultrasound Technology and Statistical and Nonlinear Physics, having authored 15 papers that have together received 298 indexed citations. Recurring topics across this work include Astrophysics and Cosmic Phenomena (13 papers), Dark Matter and Cosmic Phenomena (12 papers), Radio Astronomy Observations and Technology (6 papers), Galaxies: Formation, Evolution, Phenomena (2 papers), Radiation Detection and Scintillator Technologies (2 papers), Particle physics theoretical and experimental studies (1 paper), Medical Imaging Techniques and Applications (1 paper) and Cosmology and Gravitation Theories (1 paper). The work is most often cited by research in Nuclear and High Energy Physics (285 citations), Astronomy and Astrophysics (220 citations), Radiological and Ultrasound Technology (4 citations), Statistical and Nonlinear Physics (9 citations) and Instrumentation (1 citation). H.-S. Zechlin has collaborated with scholars based in Germany, Italy and Netherlands. Frequent co-authors include D. Horns, M. Meyer, Fiorenza Donato, N. Fornengo, A. Cuoco, Silvia Manconi, Marco Regis, Andrea Vittino, Dominik Elsässer and M. V. Fernandes. Their work appears in journals such as Physical review. D, The Astrophysical Journal Supplement Series, The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

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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