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.
THE MASS-METALLICITY RELATION WITH THE DIRECT METHOD ON STACKED SPECTRA OF SDSS GALAXIES
2013332 citationsPaul Martini et al.The Astrophysical 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 Paul Martini'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 Paul Martini with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Paul Martini more than expected).
This network shows the impact of papers produced by Paul Martini. 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 Paul Martini. The network helps show where Paul Martini may publish in the future.
Co-authorship network of co-authors of Paul Martini
This figure shows the co-authorship network connecting the top 25 collaborators of Paul Martini.
A scholar is included among the top collaborators of Paul Martini 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 Paul Martini. Paul Martini is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Bolatto, Alberto D., L. Armus, Sylvain Veilleux, et al.. (2019). Cold Gas Outflows, Feedback, and the Shaping of Galaxies. CaltechAUTHORS (California Institute of Technology).1 indexed citations
6.
Montero-Camacho, Paulo, Christopher M. Hirata, Paul Martini, & K. Honscheid. (2019). Impact of inhomogeneous reionization on the Lyman-α forest. Monthly Notices of the Royal Astronomical Society. 487(1). 1047–1056.17 indexed citations
Prieto, J. L., Matthew D. Kistler, T. A. Thompson, et al.. (2008). Discovery of the Dust-Enshrouded Progenitor of the Type IIn SN 2008S with Spitzer. arXiv (Cornell University).
10.
Martini, Paul, S. E. Persson, D. C. Murphy, et al.. (2004). PANIC: A Near-infrared Camera for the Magellan Telescopes.45 indexed citations
11.
Stanek, K. Z., Paul Martini, & P. Garnavich. (2003). GRB 030329, optical photometry.. GRB Coordinates Network. 2018. 1.1 indexed citations
12.
Martini, Paul, P. Garnavich, & K. Z. Stanek. (2003). GRB 030328, optical spectroscopy.. GRB Coordinates Network. 1980. 1.1 indexed citations
Chen, Hsiao‐Wen, Ronald O. Marzke, Patrick J. McCarthy, et al.. (2002). The Las Campanas Infrared Survey. IV. The Photometric Redshift Survey and the Rest-frame R-band Galaxy Luminosity Function at 0.5 ≤ z ≤ 1.5.51 indexed citations
16.
Martini, Paul, John S. Mulchaey, Richard W. Pogge, & Michael W. Regan. (2001). Nuclear bars and nuclear spirals in nearby normal and active galaxies. AAS. 198.1 indexed citations
Atwood, Bruce, Paul L. Byard, D. L. DePoy, et al.. (1998). Ohio State University Imaging Sciences Laboratory (ISL). Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 3354. 777–777.1 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.