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.
Strange stars
1986834 citationsC. Alcock et al.The Astrophysical Journalprofile →
An evolution free test for non-zero cosmological constant
This map shows the geographic impact of C. Alcock'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. Alcock with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. Alcock more than expected).
This network shows the impact of papers produced by C. Alcock. 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. Alcock. The network helps show where C. Alcock may publish in the future.
Co-authorship network of co-authors of C. Alcock
This figure shows the co-authorship network connecting the top 25 collaborators of C. Alcock.
A scholar is included among the top collaborators of C. Alcock 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. Alcock. C. Alcock is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Emami, Razieh, Shy Genel, Lars Hernquist, et al.. (2021). Morphological Types of DM Halos in Milky Way-like Galaxies in the TNG50 Simulation: Simple, Twisted, or Stretched. DSpace@MIT (Massachusetts Institute of Technology).3 indexed citations
3.
Kim, Dae‐Won, et al.. (2011). Automatic QSO Selection Algorithm Using Time Series Analysis and Machine Learning. 217.1 indexed citations
4.
Bianco, Federica, B. A. McLeod, & C. Alcock. (2007). Sub-second, High Precision Photometry with the MMT/Megacam System to Probe the Kuiper Belt Population. AAS. 211.1 indexed citations
Stubbs, C. W., Kem H. Cook, Suzanne L. Hawley, et al.. (2001). A Next Generation Microlensing Survey of the LMC. 37.1 indexed citations
8.
Alcock, C., D. Ciarlo, Jian Ge, et al.. (1999). Adaptive optics high resolution spectroscopy: present status and future direction. University of North Texas Digital Library (University of North Texas). 195. 568.
Bennett, D. P., C. Alcock, R. A. Allsman, et al.. (1993). The MACHO Project II: Data Reduction and Analysis of 6 Million Lightcurves. AAS. 183.1 indexed citations
Frieman, J., Angela V. Olinto, Marcelo Gleiser, & C. Alcock. (1989). Cosmic evolution of nontopological solitons. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields. 40(10). 3241–3251.47 indexed citations
Alcock, C., A. S. Chisholm, M. Tyndel, & P. C. M. Yock. (1973). Search For Massive and/or Fractionally Charged Particles. ICRC. 3(36/4). 2106–2111.1 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.