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.
New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit
2015853 citationsI. Baraffe, D. Homeier et al.Springer Link (Chiba Institute of Technology)profile →
Low‐Temperature Opacities
2005801 citationsJason W. Ferguson, D. R. Alexander et al.profile →
The NextGen Model Atmosphere Grid for \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 $3000\leq T_{\mathrm{eff}\,}\leq \mathrm{10,000}\,$ \end{document} K
1999667 citationsP. H. Hauschildt, F. Allard et al.profile →
Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458
2003649 citationsTravis Barman, F. Allard et al.Springer Link (Chiba Institute of Technology)profile →
The Limiting Effects of Dust in Brown Dwarf Model Atmospheres
2001580 citationsF. Allard, D. R. Alexander et al.profile →
Models of very-low-mass stars, brown dwarfs and exoplanets
2012459 citationsF. Allard, D. Homeier et al.profile →
VOSA: virtual observatory SED analyzer
2008340 citationsA. Bayo, C. Rodrigo et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of F. Allard'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 F. Allard with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites F. Allard more than expected).
This network shows the impact of papers produced by F. Allard. 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 F. Allard. The network helps show where F. Allard may publish in the future.
Co-authorship network of co-authors of F. Allard
This figure shows the co-authorship network connecting the top 25 collaborators of F. Allard.
A scholar is included among the top collaborators of F. Allard 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 F. Allard. F. Allard is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Baraffe, I., D. Homeier, F. Allard, & G. Chabrier. (2015). New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit. Springer Link (Chiba Institute of Technology).853 indexed citations breakdown →
Bayo, A., C. Rodrigo, D. Barrado, & F. Allard. (2014). Physical parameter determinations of young Ms. Taking advantage of the Virtual Observatory to compare methodologies. MmSAI. 85. 773.1 indexed citations
Freytag, B., F. Allard, H.‐G. Ludwig, D. Homeier, & M. Steffen. (2011). Radiation-Hydrodynamics Simulations of Cool Stellar and Substellar Atmospheres. ASPC. 448. 855.1 indexed citations
Homeier, D., N. F. Allard, F. Allard, Luka Č. Popović, & M. S. Dimitrijević. (2007). Alkali Line Profiles in Degenerate Dwarfs. AIP conference proceedings. 938. 170–175.1 indexed citations
Hauschildt, P. H., F. Allard, E. Baron, J. P. Aufdenberg, & A. Schweitzer. (2003). Stellar atmospheres and synthetic spectra for GAIA. ASPC. 298. 179.1 indexed citations
Barman, Travis, P. H. Hauschildt, & F. Allard. (2002). Irradiation of CV secondaries. 261. 49.
19.
Allard, F., P. H. Hauschildt, D. R. Alexander, Jason W. Ferguson, & Akemi Tamanai. (2000). Model Atmospheres and Spectra of Brown Dwarfs to Giant Planets. ASPC. 212. 127.1 indexed citations
20.
Hauschildt, P. H., et al.. (1994). Novae at Maximum Light: They can be Cool!. ASPC. 64. 705.1 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.