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.
Submillimeter Galaxies atz∼ 2: Evidence for Major Mergers and Constraints on Lifetimes, IMF, and CO‐H2Conversion Factor
2008369 citationsL. J. Tacconi, R. Genzel et al.The Astrophysical Journalprofile →
An interferometric CO survey of luminous submillimetre galaxies
2005268 citationsT. R. Greve, F. Bertoldi et al.Monthly Notices of the Royal Astronomical Societyprofile →
High‐Resolution Millimeter Imaging of Submillimeter Galaxies
2006261 citationsL. J. Tacconi, R. Neri et al.The Astrophysical Journalprofile →
A survey of molecular gas in luminous sub-millimetre galaxies
2013214 citationsIan Smail, S. C. Chapman et al.Monthly Notices of the Royal Astronomical Societyprofile →
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 A. Omont'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 A. Omont with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Omont more than expected).
This network shows the impact of papers produced by A. Omont. 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 A. Omont. The network helps show where A. Omont may publish in the future.
Co-authorship network of co-authors of A. Omont
This figure shows the co-authorship network connecting the top 25 collaborators of A. Omont.
A scholar is included among the top collaborators of A. Omont 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 A. Omont. A. Omont is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Omont, A., Holger F. Bettinger, & Christina Tönshoff. (2019). Polyacenes and diffuse interstellar bands. Springer Link (Chiba Institute of Technology).30 indexed citations
Greve, T. R., F. Bertoldi, Ian Smail, et al.. (2005). An interferometric CO survey of luminous submillimetre galaxies. Monthly Notices of the Royal Astronomical Society. 359(3). 1165–1183.268 indexed citations breakdown →
Omont, A., P. Cox, S. H. Moseley, et al.. (1995). Mid- and far-infrared emission bands in C-rich proto-planetary nebulae. 73. 413–418.1 indexed citations
16.
Loup, C., T. Forveille, A. Omont, & Jean‐François Paul. (1993). CO and HCN observations of circumstellar envelopes. A catalogue―mass loss rates and distributions. Astronomy & Astrophysics Supplement Series. 99(2). 291–377.20 indexed citations
17.
Walmsley, C. M., et al.. (1990). 1.3 MM continuum emission from circumstellar envelopes.. 248(2). 155–157.4 indexed citations
18.
Mennessier, M. O. & A. Omont. (1990). From Miras to planetary nebulae : which path for stellar evolution ? : Montpellier, France - September 4-7, 1989.15 indexed citations
19.
Omont, A., et al.. (1979). Transitions in LAMBDA -doublets of molecules induced by collisions with ions. II.. Astronomy & Astrophysics Supplement Series. 38. 101–118.1 indexed citations
20.
Omont, A., E. W. Smith, & J. Cooper. (1973). Redistribution of resonance radiation. II - The effect of magnetic fields.. The Astrophysical Journal. 182.1 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.