Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
A New System of Faint Near-Infrared Standard Stars
1998517 citationsS. E. Persson, D. C. Murphy et al.The Astronomical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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This map shows the geographic impact of D. C. Murphy'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. C. Murphy with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. C. Murphy more than expected).
This network shows the impact of papers produced by D. C. Murphy. 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. C. Murphy. The network helps show where D. C. Murphy may publish in the future.
Co-authorship network of co-authors of D. C. Murphy
This figure shows the co-authorship network connecting the top 25 collaborators of D. C. Murphy.
A scholar is included among the top collaborators of D. C. Murphy 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. C. Murphy. D. C. Murphy is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Martín-Carrillo, A., D. C. Murphy, L. Hanlon, et al.. (2015). Optical monitoring campaign of V404 Cyg with the Watcher Robotic Telescope. ATel. 7718. 1.1 indexed citations
3.
Martín-Carrillo, A., et al.. (2015). Significant colour change of ASASSN-15ni observed with the UCD Watcher telescope. The astronomer's telegram. 7875. 1.
4.
Martín-Carrillo, A., D. C. Murphy, L. Hanlon, et al.. (2015). Significant decrease in the average optical emission from V404 Cyg. ATel. 7729. 1.2 indexed citations
5.
Hanlon, L., D. C. Murphy, Martin Topinka, et al.. (2014). BLAZAR MONITORING WITH THE WATCHER ROBOTIC TELESCOPE. Redalyc (Universidad Autónoma del Estado de México). 45. 71–72.
May, J., et al.. (1993). A deep CO survey of the third galactic quadrant. Astronomy & Astrophysics Supplement Series. 99(1). 105–165.3 indexed citations
15.
Murphy, D. C. & J. May. (1991). Molecular clouds in Vela.. 247(1). 202–214.7 indexed citations
16.
Booth, R. S., R. M. González Delgado, Magnus Hagström, et al.. (1988). The Swedish-ESO Submillimeter Telescope (SEST). NASA STI/Recon Technical Report N. 216. 27605–324.9 indexed citations
17.
May, J., D. C. Murphy, & P. Thaddeus. (1988). A wide latitude CO survey of the third galactic quadrant. Astronomy & Astrophysics Supplement Series. 73(1). 51–83.4 indexed citations
18.
Murphy, D. C., R. S. Cohen, & J. May. (1986). CO observations of dark clouds in Lupus. NASA Technical Reports Server (NASA). 167(2). 234–238.
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.