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.
GAS REGULATION OF GALAXIES: THE EVOLUTION OF THE COSMIC SPECIFIC STAR FORMATION RATE, THE METALLICITY-MASS-STAR-FORMATION RATE RELATION, AND THE STELLAR CONTENT OF HALOS
2013523 citationsS. J. Lilly, C. M. Carollo et al.The Astrophysical Journalprofile →
Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang
2015154 citationsSandro Tacchella, C. M. Carollo et al.profile →
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 C. M. Carollo'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 C. M. Carollo with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. M. Carollo more than expected).
This network shows the impact of papers produced by C. M. Carollo. 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 C. M. Carollo. The network helps show where C. M. Carollo may publish in the future.
Co-authorship network of co-authors of C. M. Carollo
This figure shows the co-authorship network connecting the top 25 collaborators of C. M. Carollo.
A scholar is included among the top collaborators of C. M. Carollo 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 C. M. Carollo. C. M. Carollo is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Borisova, Elena, Sebastiano Cantalupo, S. J. Lilly, et al.. (2017). Ubiquitous Giant Lyα Nebulae around the Brightest Quasars at z ∼3.5 Revealed with MUSE. Leiden Repository (Leiden University).96 indexed citations
Carollo, C. M., A. Cibinel, S. J. Lilly, et al.. (2016). ZENS. IV. Similar morphological changes associated with mass quenching and environment quenching and the relative importance of bulge growth versus the fading of disks. Figshare.16 indexed citations
Carollo, C. M., et al.. (2016). The MAD View on the Outskirts of Disks. Proceedings of the International Astronomical Union. 11(S321). 163–171.1 indexed citations
12.
Silverman, J. D., Francesco Miniati, A. Finoguenov, et al.. (2014). The X-Ray Zurich Environmental Study (X-ZENS). I. Chandra and XMM-Newton observations of active galactic nuclei in galaxies in nearby groups. Figshare.4 indexed citations
Bouwens, R. J., G. D. Illingworth, Ivo Labbé, et al.. (2009). Constraints on the First Galaxies: z~10 Galaxy Candidates from HST WFC3/IR. arXiv (Cornell University).1 indexed citations
18.
Hahn, Oliver, C. Porciani, Avishai Dekel, & C. M. Carollo. (2008). The Tidal Origin of the Environment Dependence of Halo Assembly. arXiv (Cornell University).2 indexed citations
19.
Diemand, Juerg, Marcel Zemp, Ben Moore, Joachim Stadel, & C. M. Carollo. (2005). Cusps in CDM halos: The density profile of a billion particle halo. arXiv (Cornell University).8 indexed citations
20.
Baade, D., T. R. Bedding, C. M. Carollo, et al.. (1993). Remote Observing with the NTT and EMMI/SUSI: a First Assessment. The Messenger. 72. 13–14.1 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.