B. Wolff

1.7k total citations
52 papers, 741 citations indexed

About

B. Wolff is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, B. Wolff has authored 52 papers receiving a total of 741 indexed citations (citations by other indexed papers that have themselves been cited), including 32 papers in Astronomy and Astrophysics, 22 papers in Instrumentation and 14 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in B. Wolff's work include Stellar, planetary, and galactic studies (31 papers), Astrophysics and Star Formation Studies (22 papers) and Astronomy and Astrophysical Research (22 papers). B. Wolff is often cited by papers focused on Stellar, planetary, and galactic studies (31 papers), Astrophysics and Star Formation Studies (22 papers) and Astronomy and Astrophysical Research (22 papers). B. Wolff collaborates with scholars based in Germany, United States and Chile. B. Wolff's co-authors include D. Feldmann, K. H. Welge, D. Koester, H. Rottke, S. Hubrig, L. Pasquini, R. Gratton, James Liebert, G. Mathys and V. G. Elkin and has published in prestigious journals such as Physical Review Letters, Monthly Notices of the Royal Astronomical Society and Physics Letters B.

In The Last Decade

B. Wolff

49 papers receiving 712 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
B. Wolff Germany 17 503 195 192 131 80 52 741
D. Péquignot France 13 499 1.0× 156 0.8× 84 0.4× 69 0.5× 66 0.8× 47 604
R. L. Porter United States 15 789 1.6× 129 0.7× 110 0.6× 203 1.5× 48 0.6× 32 917
Kunio Noguchi Japan 13 1.1k 2.1× 103 0.5× 311 1.6× 73 0.6× 67 0.8× 44 1.1k
P. S. Barklem Sweden 11 678 1.3× 76 0.4× 239 1.2× 130 1.0× 59 0.7× 14 769
P. Benvenuti Italy 11 364 0.7× 101 0.5× 60 0.3× 71 0.5× 38 0.5× 57 450
V. Luridiana Spain 19 1.3k 2.6× 77 0.4× 475 2.5× 93 0.7× 69 0.9× 43 1.4k
D. van Buren United States 15 778 1.5× 53 0.3× 87 0.5× 119 0.9× 57 0.7× 45 834
S. Torres‐Peimbert Mexico 21 1.3k 2.7× 112 0.6× 322 1.7× 138 1.1× 89 1.1× 78 1.4k
Liyi Gu Netherlands 14 497 1.0× 153 0.8× 54 0.3× 132 1.0× 23 0.3× 63 595
J. A. Fernley United Kingdom 12 477 0.9× 165 0.8× 191 1.0× 27 0.2× 61 0.8× 39 627

Countries citing papers authored by B. Wolff

Since Specialization
Citations

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

Fields of papers citing papers by B. Wolff

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of B. Wolff

This figure shows the co-authorship network connecting the top 25 collaborators of B. Wolff. A scholar is included among the top collaborators of B. Wolff 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 B. Wolff. B. Wolff 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.
Järvinen, S. P., S. Hubrig, B. Wolff, et al.. (2024). Testing pulsation diagnostics in the rapidly oscillating magnetic Ap star γ Equ using near-infrared CRIRES+ observations. Astronomy and Astrophysics. 683. A66–A66.
2.
Nicholls, C. P., T. Lebzelter, A. Smette, et al.. (2017). CRIRES-POP : a library of high resolution spectra in the near-infrared II. Data reduction and the spectrum of the K giant 10 Leonis. GoeScholar The Publication Server of the Georg-August-Universität Göttingen (Georg-August-Universität Göttingen). 4 indexed citations
3.
Schöller, M., M. A. Pogodin, Н. А. Драке, et al.. (2016). Spectroscopic signatures of magnetospheric accretion in Herbig Ae/Be stars. Springer Link (Chiba Institute of Technology). 12 indexed citations
4.
Nicholls, C. P., T. Lebzelter, A. Smette, et al.. (2016). CRIRES-POP: a library of high resolution spectra in the near-infrared. Astronomy and Astrophysics. 598. A79–A79. 7 indexed citations
5.
Sánchez-Janssen, Rubén, Steffen Mieske, F. Selman, et al.. (2014). Revisiting the impact of atmospheric dispersion and differential refraction on widefield multiobject spectroscopic observations. Springer Link (Chiba Institute of Technology). 2 indexed citations
6.
Cowley, Charles R., S. Hubrig, Francesco Castelli, & B. Wolff. (2012). The narrow, inner CO ring around the magnetic Herbig Ae star HD 101412. Springer Link (Chiba Institute of Technology). 5 indexed citations
7.
Lebzelter, T., Andreas Seifahrt, S. Uttenthaler, et al.. (2012). CRIRES-POP. Astronomy and Astrophysics. 539. A109–A109. 19 indexed citations
8.
Hubrig, S., Francesco Castelli, J. F. González, et al.. (2012). Line identification in high-resolution, near-infrared CRIRES spectra of chemically peculiar and Herbig Ae stars. Astronomy and Astrophysics. 542. A31–A31. 7 indexed citations
9.
Smiljanić, R., P. Bonifacio, Daniele Galli, et al.. (2009). Beryllium abundances and star formation in the halo and in the thick disk. Astronomy and Astrophysics. 499(1). 103–119. 40 indexed citations
10.
Pasquini, L., A. Ecuvillon, P. Bonifacio, & B. Wolff. (2008). Nitrogen abundance in turn-off stars of NGC 6397 and NGC 6752. Astronomy and Astrophysics. 489(1). 315–320. 19 indexed citations
11.
Ávila, Gerardo, A. Kaufer, S. D’Odorico, et al.. (2006). VLT-UVES Long-Slit Spectroscopy. ˜The œMessenger. 123. 17. 2 indexed citations
12.
Wittkowski, M., et al.. (2006). Tests of stellar model atmospheres by optical interferometry. Astronomy and Astrophysics. 460(3). 855–864. 18 indexed citations
13.
Hubrig, S., N. Nesvacil, M. Schöller, et al.. (2005). Detection of an extraordinarily large magnetic field in the unique ultra-cool Ap star HD 154708. Astronomy and Astrophysics. 440(2). L37–L40. 49 indexed citations
14.
Pasquini, L., P. Molaro, P. François, et al.. (2005). Li in NGC 6752 and the formation of globular clusters. Astronomy and Astrophysics. 441(2). 549–553. 82 indexed citations
15.
Modigliani, A., et al.. (2004). The FLAMES-UVES Pipeline. Msngr. 118. 8–10.
16.
Dreizler, S., P. H. Hauschildt, W. Kley, et al.. (2003). OGLE-TR-3: A possible new transiting planet. Astronomy and Astrophysics. 402(2). 791–799. 14 indexed citations
17.
Schuh, Sonja, S. Dreizler, & B. Wolff. (2002). Equilibrium abundances in hot DA white dwarfs as derived from self-consistent diffusion models. Springer Link (Chiba Institute of Technology). 20 indexed citations
18.
Wolff, B., D. Koester, & James Liebert. (2002). Element abundances in cool white dwarfs. Astronomy and Astrophysics. 385(3). 995–1007. 43 indexed citations
19.
Wolff, B., D. Koester, Μ. H. Montgomery, & D. E. Winget. (2002). Is the helium in the variable DB white dwarfs 3He?. Astronomy and Astrophysics. 388(1). 320–325. 8 indexed citations
20.
Koester, D. & B. Wolff. (2001). Spectroscopy of white dwarf candidates from the ESO Imaging Survey(EIS-WIDE). Astronomy and Astrophysics. 379(1). 215–223. 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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