Citations per year, relative to A. W. Shafter A. W. Shafter (= 1×)
peers
M. F. Bode
Countries citing papers authored by A. W. Shafter
Since
Specialization
Citations
This map shows the geographic impact of A. W. Shafter'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 A. W. Shafter with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. W. Shafter more than expected).
This network shows the impact of papers produced by A. W. Shafter. 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 A. W. Shafter. The network helps show where A. W. Shafter may publish in the future.
Co-authorship network of co-authors of A. W. Shafter
This figure shows the co-authorship network connecting the top 25 collaborators of A. W. Shafter.
A scholar is included among the top collaborators of A. W. Shafter 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 A. W. Shafter. A. W. Shafter is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Hornoch, K., et al.. (2019). A fourth observed outburst of a Galactic flare star in the field of M31. The astronomer's telegram. 12513. 1.1 indexed citations
7.
Boyd, D., K. Hornoch, M. Henze, et al.. (2017). Recurrent Nova M31N 2008-12a: discovery of the 2017 eruption. ATel. 11116. 1.1 indexed citations
8.
Henze, M., S. C. Williams, M. J. Darnley, et al.. (2016). Confirmation of PNV J00430400+4117079 as another eruption of the recurrent nova M31N 1990-10a and additional constraints on the eruption date. ATel. 9276. 1.1 indexed citations
9.
Hornoch, K., M. Henze, M. J. Darnley, A. W. Shafter, & Mariko Kato. (2015). Optical Photometry of M31N 2008-12a After Maximum Light of the 2015 Eruption. ATel. 7969. 1.
10.
Hornoch, K., H. Kučáková, R. Quimby, et al.. (2015). Late-time Optical Photometry of the 2015 Eruption of M31N 2008-12a. ATel. 7976. 1.
11.
Tomov, T., S. Fabrika, E. A. Barsukova, et al.. (2015). M31N 2015-01a - A Luminous Red Nova. ATel. 7150. 1.
12.
Darnley, M. J., M. F. Bode, A. W. Shafter, et al.. (2014). Recurrent Nova M31N 2008-12a: Additional observations, pre-detection limit, and erratum to ATel #6527. ATel. 6535. 1.1 indexed citations
13.
Noguchi, T., A. Pearce, U. Munari, et al.. (2014). Nova Scorpii 2014 = Tcp J17154683-3128303. 3841. 1.2 indexed citations
14.
Williams, S. C., M. F. Bode, M. J. Darnley, et al.. (2013). Rapid dust formation in novae : the speed-class formation timescale correlation eplained. Lancaster EPrints (Lancaster University).5 indexed citations
15.
Page, K. L., F. M. Walter, G. J. Schwarz, et al.. (2012). Swift detection of UV and super-soft X-ray emission in Nova LMC 2012. The astronomer's telegram. 4043. 1.1 indexed citations
16.
Shafter, A. W.. (2007). Spectroscopic Classes of Galactic Novae. American Astronomical Society Meeting Abstracts. 211.1 indexed citations
17.
Shafter, A. W., et al.. (2007). Modeling the Eclipses of the Classical Nova QU Vulpeculae and the Novalike Variable LX Serpentis. American Astronomical Society Meeting Abstracts. 211.
18.
Shafter, A. W.. (1994). Interacting binary stars : a symposium held in conjunction with the 105th Meeting of the Astronomical Society of the Pacific, San Diego State University, 13-15 July 1993. Astronomical Society of the Pacific eBooks.3 indexed citations
19.
Shafter, A. W. & R. Campbell. (1990). Time-Resolved CCD Photometry of Classical Novae. Bulletin of the American Astronomical Society. 22. 1211.3 indexed citations
20.
Shafter, A. W. & F. V. Hessman. (1984). Time Resolved Spectroscopy and Photometry of a New Eclipsing Cataclysmic Variable, PG1030+590. Bulletin of the American Astronomical Society. 16. 505.
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.