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.
Flores, H., F. Hammer, F.–X. Désert, et al.. (1999). Deep Galaxy survey at 6.75µm with the ISO satellite. ORCA Online Research @Cardiff (Cardiff University). 343(2). 389–398.2 indexed citations
6.
Fuente, A., J. Cernicharo, & A. Omont. (1998). INFERRING ACETYLENE ABUNDANCES FROM C2H : THE C2H2/HCN ABUNDANCE RATIO. A&A. 330(1). 232–242.2 indexed citations
7.
Josselin, E., C. Loup, A. Omont, C. Barnbaum, & L.-Å. Nyman. (1996). INFRARED GIANTS VS. SUPERGIANTS. I. FAR INFRARED-TO-CO(1-0) INTENSITY RATIO. 315(1).2 indexed citations
8.
Barnbaum, C., A. Omont, & M. Morris. (1996). The unusual circumstellar environment of the evolved star, U Equulei.. 310(1). 259–270.2 indexed citations
9.
Omont, A., R. G. McMahon, P. Cox, et al.. (1996). Continuum millimetre observations of high-redshift radio-quiet QSOs II. Five new detections at z>4.. 315(1). 1–10.3 indexed citations
10.
Omont, A., et al.. (1995). The distribution of dust around Asymptotic Giant Branch stars. 295. 445–458.3 indexed citations
11.
Little-Marenin, I. R., R. Sahai, P. G. Wannier, et al.. (1994). A search for SiO, OH, CO and HCN radio emission from silicate-carbon stars.. NASA Technical Reports Server (NASA). 281(2). 451–459.1 indexed citations
12.
Rouan, Daniel, A. Léger, A. Omont, & M. Giard. (1992). Physics of the rotation of a PAH molecule in interstellar environments. 253(2). 498–514.10 indexed citations
13.
Vallée, J. P., S. Guilloteau, T. Forveille, & A. Omont. (1990). NGC 7027 at Millimeter Wavelengths - Microturbulences in the Ionized Shell. 230(2). 457–462.1 indexed citations
14.
Lucas, Ray A., et al.. (1988). New HCN masers in stars.. 194. 230–236.2 indexed citations
Lucas, Ray A., A. Omont, & R. Stora. (1985). Birth and infancy of stars.49 indexed citations
17.
Morris, M., R. Lucas, & A. Omont. (1985). Molecular emission from expanding circumstellar envelopes : polarization and profile asymmetries.. 142(1). 107–116.2 indexed citations
18.
Lucas, R., et al.. (1982). Molecular abundances in IRC +10216.. 106. 201–213.14 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.