This map shows the geographic impact of M. F. Bode'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 M. F. Bode with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. F. Bode more than expected).
This network shows the impact of papers produced by M. F. Bode. 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 M. F. Bode. The network helps show where M. F. Bode may publish in the future.
Co-authorship network of co-authors of M. F. Bode
This figure shows the co-authorship network connecting the top 25 collaborators of M. F. Bode.
A scholar is included among the top collaborators of M. F. Bode 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 M. F. Bode. M. F. Bode 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.
Darnley, M. J., I. A. Steele, Rowan J. Smith, et al.. (2014). Recurrent Nova M31N 2008-12a: Liverpool Telescope SPRAT Spectrum. ATel. 6540. 1.1 indexed citations
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
4.
Darnley, M. J. & M. F. Bode. (2013). Liverpool Telescope spectral monitoring of Nova Delphini 2013 reveals dramatic changes in the Hydrogen Balmer lines. The astronomer's telegram. 5300. 1.
5.
Shafter, A. W., et al.. (2012). Spectroscopic Observations of the Unusual Transient TCP J00452884+4154095 in M31. The astronomer's telegram. 4503. 1.2 indexed citations
Schwarz, G. J., J. P. Osborne, K. L. Page, et al.. (2011). Swift detection of super soft X-ray emission in Nova V2468 Cygni. The astronomer's telegram. 3754. 1.1 indexed citations
9.
Schaefer, Bradley E., Ashley Pagnotta, M. J. Darnley, et al.. (2010). Discovery of the predicted 2010 eruption and the pre-eruption light curve for recurrent nova U scorpii. Civil War Book Review.16 indexed citations
10.
Schwarz, G. J., J. P. Osborne, K. L. Page, et al.. (2010). Swift super soft X-ray detection in Nova V1213 Centauri. The astronomer's telegram. 2904. 1.2 indexed citations
11.
Schaefer, Bradley E., Ashley Pagnotta, J. P. Osborne, et al.. (2010). Recurrent Nova U Sco Has Sharp Decline in X-ray/UV/Optical/IR. ATel. 2477. 1.3 indexed citations
12.
Bode, M. F., J. P. Osborne, K. L. Page, et al.. (2010). Emergence of a Bright and Highly Variable Super-soft Source Phase in Nova KT Eri (2009). The astronomer's telegram. 2392. 1.1 indexed citations
13.
Shafter, A. W., Robin Ciardullo, M. J. Darnley, M. F. Bode, & K. A. Misselt. (2010). Spectroscopic Observations of a Recent M31 Nova Candidate Near Maximum Light. ATel. 2898. 1.1 indexed citations
Ness, Jan‐Uwe, C. E. Woodward, L. A. Helton, et al.. (2009). The first X-ray detection of the dust-forming C-rich nova V1280 Sco. ATel. 2063. 1.1 indexed citations
16.
Bode, M. F., J. P. Osborne, K. L. Page, et al.. (2009). A 1.19 day UV Photometric Period in Nova LMC 2009. The astronomer's telegram. 2001. 1.1 indexed citations
17.
Osborne, J. P., K. L. Page, A. P. Beardmore, et al.. (2009). Early X-ray detection of Nova Ophiuchi 2009 / V2672 Oph. ATel. 2173. 1.1 indexed citations
18.
Osborne, J. P., K. L. Page, P. A. Evans, et al.. (2008). Nova V2491 Cyg has become a bright super-soft source. ATel. 1542. 1.2 indexed citations
19.
Ness, Jan‐Uwe, et al.. (2008). Nova V1281 Sco now a bright SSS. The astronomer's telegram. 1370. 1.1 indexed citations
20.
Bode, M. F.. (1987). RS Ophiuchi (1985) and the recurrent nova phenomenon : proceedings of the Manchester Conference 16-18 December 1985.2 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
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Rankless may not fully capture the entirety of a scholar's output or impact.