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.
Mid‐Infrared Selection of Active Galaxies
2005545 citationsDaniel Stern, M. A. Pahre et al.The Astrophysical Journalprofile →
A REMARKABLY LUMINOUS GALAXY AT Z = 11.1 MEASURED WITH HUBBLE SPACE TELESCOPE GRISM SPECTROSCOPY
2016257 citationsM. L. N. Ashby, G. G. Fazio et al.The Astrophysical Journalprofile →
Author Peers
Peers are selected by citation overlap in the author's most active subfields.
citations ·
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This map shows the geographic impact of S. P. Willner'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 S. P. Willner with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. P. Willner more than expected).
This network shows the impact of papers produced by S. P. Willner. 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 S. P. Willner. The network helps show where S. P. Willner may publish in the future.
Co-authorship network of co-authors of S. P. Willner
This figure shows the co-authorship network connecting the top 25 collaborators of S. P. Willner.
A scholar is included among the top collaborators of S. P. Willner 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 S. P. Willner. S. P. Willner is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Falco, E., S. P. Willner, P. Challis, et al.. (2015). Spectroscopic Classification of ASASSN-15hg. ATel. 7420. 1.
13.
Carey, S., James G. Ingalls, W. Glaccum, et al.. (2011). Improvements to Warm IRAC/Spitzer Space Telescope Operations. AAS. 218.1 indexed citations
14.
Fazio, G. G., M. L. N. Ashby, M. L. N. Ashby, et al.. (2008). The Spitzer/IRAC Star Formation Reference Survey. 50128.1 indexed citations
15.
Polomski, Elisha, R. D. Gehrz, C. E. Woodward, et al.. (2006). Multi-Epoch Imaging and Spectroscopy of M33. ASPC. 357. 196.1 indexed citations
16.
Willner, S. P., et al.. (2004). M33 Mapping and Spectroscopy. 5.1 indexed citations
17.
Molnár, L., et al.. (1988). Multicolor Infrared Photometry of Cygnus X-3. Bulletin of the American Astronomical Society. 20. 736.1 indexed citations
18.
Fazio, G. G., David Koch, Gary J. Melnick, et al.. (1984). A Wide Field and Diffraction Limited Array Camera for the Space Infrared Telescope Facility (SIRTF). Bulletin of the American Astronomical Society. 16. 906.
19.
Puetter, R. C., R. W. Russell, B. T. Soifer, & S. P. Willner. (1977). Infrared Spectra of Protostars.. Bulletin of the American Astronomical Society. 9. 571.3 indexed citations
20.
Forrest, W. J., F. C. Gillett, J. R. Houck, et al.. (1976). Spectrophotometry of OH 26. 5+0. 6.. Bulletin of the American Astronomical Society. 8. 32.1 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.