D. Argast

760 total citations
9 papers, 436 citations indexed

About

D. Argast is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Molecular Biology. According to data from OpenAlex, D. Argast has authored 9 papers receiving a total of 436 indexed citations (citations by other indexed papers that have themselves been cited), including 7 papers in Astronomy and Astrophysics, 3 papers in Nuclear and High Energy Physics and 1 paper in Molecular Biology. Recurrent topics in D. Argast's work include Gamma-ray bursts and supernovae (7 papers), Nuclear physics research studies (3 papers) and Pulsars and Gravitational Waves Research (3 papers). D. Argast is often cited by papers focused on Gamma-ray bursts and supernovae (7 papers), Nuclear physics research studies (3 papers) and Pulsars and Gravitational Waves Research (3 papers). D. Argast collaborates with scholars based in Switzerland, United States and United Kingdom. D. Argast's co-authors include F.‐K. Thielemann, M. Samland, Yong-Zhong Qian, Timothy C. Beers, Enrico Arnone, John E. Norris, Sean G. Ryan, Ortwin Gerhard, F. Brachwitz and Peter Höflich and has published in prestigious journals such as Astronomy and Astrophysics, Nuclear Physics A and Astrophysics and Space Science.

In The Last Decade

D. Argast

9 papers receiving 424 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
D. Argast Switzerland	6	400	140	68	14	12	9	436
Charli M. Sakari United States	15	370 0.9×	73 0.5×	150 2.2×	10 0.7×	12 1.0×	35	404
C. D. Laney South Africa	11	446 1.1×	93 0.7×	108 1.6×	6 0.4×	5 0.4×	21	463
Edmund Hodges‐Kluck United States	14	439 1.1×	158 1.1×	51 0.8×	5 0.4×	5 0.4×	36	460
D. D. Balam Canada	10	563 1.4×	142 1.0×	95 1.4×	10 0.7×	18 1.5×	26	575
Projjwal Banerjee India	10	340 0.8×	202 1.4×	26 0.4×	6 0.4×	4 0.3×	23	385
Doron Kushnir Israel	14	748 1.9×	238 1.7×	36 0.5×	23 1.6×	4 0.3×	35	774
Masa Aki Hashimoto Japan	7	503 1.3×	247 1.8×	65 1.0×	10 0.7×	5 0.4×	7	543
Erika M. Holmbeck United States	11	195 0.5×	84 0.6×	57 0.8×	12 0.9×	9 0.8×	28	243
Z. Barkat Israel	12	553 1.4×	204 1.5×	71 1.0×	32 2.3×	11 0.9×	35	600
J. W. den Hartogh Hungary	11	342 0.9×	76 0.5×	92 1.4×	21 1.5×	2 0.2×	14	364

Countries citing papers authored by D. Argast

Since Specialization

Citations

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

Fields of papers citing papers by D. Argast

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of D. Argast

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

All Works

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9 of 9 papers shown

1.

Argast, D., Des Fitzgerald, H. Holstein, Ronny Stolz, & A. Chwala. (2010). Compensation of the full magnetic tensor gradient signal. ASEG Extended Abstracts. 2010(1). 1–4. 9 indexed citations

2.

Arnone, Enrico, Sean G. Ryan, D. Argast, John E. Norris, & Timothy C. Beers. (2005). Mg abundances in metal-poor halo stars as a tracer of early Galactic mixing. Astronomy and Astrophysics. 430(2). 507–522. 61 indexed citations

3.

Thielemann, F.‐K., D. Argast, F. Brachwitz, et al.. (2005). Nuclear Physics: A Key Ingredient in Astrophysical Modeling. Nuclear Physics A. 751. 301–326. 5 indexed citations

4.

Argast, D., M. Samland, F.‐K. Thielemann, & Yong-Zhong Qian. (2004). Neutron star mergers versus core-collapse supernovae as dominant r-process sites in the early Galaxy. Astronomy and Astrophysics. 416(3). 997–1011. 220 indexed citations

5.

Argast, D. & M. Samland. (2004). Constraints on the Astrophysical Nature of r-Process Nucleosynthesis Sites from Inhomogeneous Chemical Evolution Models. Publications of the Astronomical Society of Australia. 21(2). 161–166. 2 indexed citations

6.

Thielemann, F.‐K., D. Argast, F. Brachwitz, et al.. (2003). Nuclear cross sections, nuclear structure and stellar nucleosynthesis. Nuclear Physics A. 718. 139–146. 75 indexed citations

7.

Argast, D., M. Samland, F.‐K. Thielemann, & Ortwin Gerhard. (2002). Implications of O and Mg abundances in metal-poor halo stars for stellar iron yields. Astronomy and Astrophysics. 388(3). 842–860. 43 indexed citations

8.

Thielemann, F.‐K., D. Argast, F. Brachwitz, et al.. (2002). Nucleosynthesis and Stellar Evolution. Astrophysics and Space Science. 281(1-2). 25–37. 20 indexed citations

9.

Argast, D., M. Samland, Ortwin Gerhard, & F.‐K. Thielemann. (2001). Element Abundance Patterns of Metal-Poor Halo Stars. Astrophysics and Space Science. 277(S1). 193–193. 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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