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.
PARSEC V2.0: Stellar tracks and isochrones of low- and intermediate-mass stars with rotation
2022111 citationsGuglielmo Costa, L. Girardi et al.Astronomy and Astrophysicsprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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Countries citing papers authored by Paul Goudfrooij
Since
Specialization
Citations
This map shows the geographic impact of Paul Goudfrooij'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 Paul Goudfrooij with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Paul Goudfrooij more than expected).
This network shows the impact of papers produced by Paul Goudfrooij. 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 Paul Goudfrooij. The network helps show where Paul Goudfrooij may publish in the future.
Co-authorship network of co-authors of Paul Goudfrooij
This figure shows the co-authorship network connecting the top 25 collaborators of Paul Goudfrooij.
A scholar is included among the top collaborators of Paul Goudfrooij 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 Paul Goudfrooij. Paul Goudfrooij is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Gómez, Sebastián, P. S. Cowperthwaite, G. Hosseinzadeh, et al.. (2019). LIGO/Virgo S190510g: Spectroscopic Classification of DECam-GROWTH and DES-GW Candidate DG19fqqk/desgw-190510c with Magellan.. GCN. 24511. 1.1 indexed citations
Gorgas, J., P. Jablonka, & Paul Goudfrooij. (2007). Stellar population gradients in bulges along the Hubble sequence - I. The data. Library Open Repository (Universidad Complutense Madrid).5 indexed citations
Goudfrooij, Paul, et al.. (2001). HST CCD Performance in the Second Decade: ChargeTransfer Efficiency. 5.1 indexed citations
14.
Kimble, Randy A., Paul Goudfrooij, & Ronald L. Gilliland. (1999). Radiation Damage Effects on the CCD Detector of the Space Telescope Imaging Spectrograph. American Astronomical Society Meeting Abstracts. 195.1 indexed citations
15.
Walborn, N. R., et al.. (1999). Sensitivity Monitor Report for the STIS First-Order Modes. AAS. 195.1 indexed citations
Lindler, D., I. Busko, Stefi A. Baum, et al.. (1998). Pipeline Calibration for STIS. ASPC. 145. 316.2 indexed citations
18.
McGrath, M. A., Stefi A. Baum, R. C. Bohlin, et al.. (1997). The STScI Pipeline Calibration of STIS Data. American Astronomical Society Meeting Abstracts. 191.1 indexed citations
19.
Goudfrooij, Paul, Stefi A. Baum, & J. R. Walsh. (1997). Fringe Correction for STIS Near-IR Long-Slit Spectra using Contemporaneous Tungsten Flat Fields. AAS. 191. 100.1 indexed citations
20.
Keel, William C., et al.. (1992). Warm IRAS sources. II - Optical spectroscopy of objects from the point source catalog. Astronomy & Astrophysics Supplement Series. 96(2). 389–428.2 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.