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 survey of interstellar H I from L-alpha absorption measurements. II
19781.5k citationsR. C. Bohlin, Blair D. Savage et al.The Astrophysical Journalprofile →
INTERSTELLAR ABUNDANCES FROM ABSORPTION-LINE OBSERVATIONS WITH THE HUBBLE SPACE TELESCOPE
1996792 citationsBlair D. Savage, Kenneth R. SembachAnnual Review of Astronomy and Astrophysicsprofile →
Observed Properties of Interstellar Dust
1979751 citationsBlair D. Savage et al.Annual Review of Astronomy and Astrophysicsprofile →
The analysis of apparent optical depth profiles for interstellar absorption lines
1991466 citationsBlair D. Savage, Kenneth R. SembachThe Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
Countries citing papers authored by Blair D. Savage
Since
Specialization
Citations
This map shows the geographic impact of Blair D. Savage'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 Blair D. Savage with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Blair D. Savage more than expected).
This network shows the impact of papers produced by Blair D. Savage. 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 Blair D. Savage. The network helps show where Blair D. Savage may publish in the future.
Co-authorship network of co-authors of Blair D. Savage
This figure shows the co-authorship network connecting the top 25 collaborators of Blair D. Savage.
A scholar is included among the top collaborators of Blair D. Savage 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 Blair D. Savage. Blair D. Savage is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Savage, Blair D. & Kenneth R. Sembach. (1996). INTERSTELLAR ABUNDANCES FROM ABSORPTION-LINE OBSERVATIONS WITH THE HUBBLE SPACE TELESCOPE. Annual Review of Astronomy and Astrophysics. 34(1). 279–329.792 indexed citations breakdown →
14.
Diplas, A. & Blair D. Savage. (1993). An IUE Survey of Interstellar H I LY alpha Absorption. ASPC. 35. 289.1 indexed citations
15.
Cardelli, Jason A., et al.. (1992). Abundance of Interstellar Carbon Toward ζ Ophiuchi. American Astronomical Society Meeting Abstracts. 181.1 indexed citations
16.
Cardelli, Jason A., Blair D. Savage, & U. J. Sofia. (1991). Interstellar Gas Phase Abundance of Carbon, Oxygen, Nitrogen, Copper, Gallium, Germanium, and Krypton Toward ζ Ophiuchi. Bulletin of the American Astronomical Society. 23. 1365.1 indexed citations
17.
Diplas, A. & Blair D. Savage. (1991). Neutral Hydrogen in the Outer Galaxy. Bulletin of the American Astronomical Society. 23. 889.1 indexed citations
Savage, Blair D. & R. C. Bohlin. (1978). Measurements of Interstellar Extinction in the Orion Nebula from the International Ultraviolet Explorer.. Bulletin of the American Astronomical Society. 10. 445.1 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.