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 2 per cent distance toz= 0.35 by reconstructing baryon acoustic oscillations – I. Methods and application to the Sloan Digital Sky Survey
2012423 citationsR. Scalzo et al.Monthly Notices of the Royal Astronomical Societyprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of R. Scalzo'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 R. Scalzo with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. Scalzo more than expected).
This network shows the impact of papers produced by R. Scalzo. 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 R. Scalzo. The network helps show where R. Scalzo may publish in the future.
Co-authorship network of co-authors of R. Scalzo
This figure shows the co-authorship network connecting the top 25 collaborators of R. Scalzo.
A scholar is included among the top collaborators of R. Scalzo 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 R. Scalzo. R. Scalzo is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Childress, M., et al.. (2013). SN 2013fs now resembles a SN IIP. ATel. 5527. 1.1 indexed citations
12.
Noguchi, T., P. Schmeer, M. Childress, et al.. (2013). Supernova 2013fs in NGC 7610 = Psn J23194467+1011045. 3671. 1.
13.
Childress, M., R. Scalzo, F. Yuan, B. Schmidt, & B. Tucker. (2013). Spectroscopic Classification of 3 Supernovae with WiFeS. The astronomer's telegram. 5455. 1.
14.
Monard, L. A. G., M. Childress, R. Scalzo, F. Yuan, & B. Schmidt. (2012). Supernova 2012ec in NGC 1084 = Psn J02455988-0734270. 3201. 1.
15.
Morton, Timothy D., A. J. Drake, S. G. Djorgovski, et al.. (2008). Archival light curve for the flaring GLAST blazar PKS 1502+106. ATel. 1661. 1.1 indexed citations
16.
Mahabal, A., A. J. Drake, S. G. Djorgovski, et al.. (2008). Discovery and Confirmation of Supernovae from PQ and CRTS. ATel. 1778. 1.1 indexed citations
17.
Djorgovski, S. G., Timothy D. Morton, A. J. Drake, et al.. (2008). Archival light curves for the gamma-ray bright blazar 3C 454.3. ATel. 1684. 1.3 indexed citations
Zweerink, J., C. E. Covault, P. Fortin, et al.. (2003). Using GHz FADCs to Reject Hadrons from STACEE Data. International Cosmic Ray Conference. 5. 2795.1 indexed citations
20.
Scalzo, R., C. E. Covault, P. Fortin, et al.. (2003). Optimized Pointing Strategies for Solar Tower ACTs. ICRC. 5. 2799.1 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.