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.
[O iii]/[N ii] as an abundance indicator at high redshift
2004985 citationsMax Pettini et al.Monthly Notices of the Royal Astronomical Societyprofile →
Lyman‐Break Galaxies at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z\gtrsim 4$ \end{document} and the Evolution of the Ultraviolet Luminosity Density at High Redshift
1999816 citationsCharles C. Steidel, Kurt L. Adelberger et al.The Astrophysical Journalprofile →
This map shows the geographic impact of Max Pettini'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 Max Pettini with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Max Pettini more than expected).
This network shows the impact of papers produced by Max Pettini. 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 Max Pettini. The network helps show where Max Pettini may publish in the future.
Co-authorship network of co-authors of Max Pettini
This figure shows the co-authorship network connecting the top 25 collaborators of Max Pettini.
A scholar is included among the top collaborators of Max Pettini 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 Max Pettini. Max Pettini is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Díaz, C., et al.. (2016). Tracking the chemical history of the Universe: the density of CIV at z~6. Americanae (AECID Library). 58. 54–56.2 indexed citations
11.
Cooke, Ryan & Max Pettini. (2013). A New, Precise Measurement of the Primordial Abundance of Deuterium. AAS. 221.1 indexed citations
Hamann, Frederick, et al.. (2007). Physical properties of absorbers in high redshift quasars. Redalyc (Universidad Autónoma del Estado de México).3 indexed citations
14.
Nissen, P. E., M. Asplund, D. Fabbian, et al.. (2007). Sulphur Abundances in Metal-Poor Stars First Result from CRIRES Science Verification. The Messenger. 128. 38.1 indexed citations
15.
Pettini, Max. (2006). Deuterium at High Redshifts: Recent Advances and Open Issues. CERN Bulletin. 348. 19.1 indexed citations
16.
Pettini, Max. (2006). Low (and High) Metallicity Galaxies at High Redshift. ASPC. 353. 363.1 indexed citations
Pettini, Max, Charles C. Steidel, Kurt L. Adelberger, et al.. (1998). The Discovery of Primeval Galaxies and the Epoch of Galaxy Formation. CERN Bulletin. 148. 67.1 indexed citations
19.
Cumming, Robert, W. P. S. Meikle, T. R. Geballe, et al.. (1994). Supernova 1994D in NGC 4526. Durham Research Online (Durham University). 5950. 1.
20.
Pettini, Max, et al.. (1990). The Lyman-alpha forest at 6 KM s-1 resolution.. Monthly Notices of the Royal Astronomical Society. 246(4). 545–564.19 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.