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.
GAIA: Composition, formation and evolution of the Galaxy
2001623 citationsM. A. C. Perryman, K. S. de Boer et al.Astronomy and Astrophysicsprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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This map shows the geographic impact of O. Pace'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 O. Pace with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites O. Pace more than expected).
This network shows the impact of papers produced by O. Pace. 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 O. Pace. The network helps show where O. Pace may publish in the future.
Co-authorship network of co-authors of O. Pace
This figure shows the co-authorship network connecting the top 25 collaborators of O. Pace.
A scholar is included among the top collaborators of O. Pace 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 O. Pace. O. Pace is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
18 of 18 papers shown
1.
Rougier, Gilles, et al.. (2004). A 1.3 giga pixels focal plane for GAIA. ESASP. 554. 767–773.1 indexed citations
2.
Pace, O.. (2003). GAIA: the satellite and payload. ESASP. 298. 13.3 indexed citations
Perryman, M. A. C., K. S. de Boer, G. Gilmore, et al.. (2001). GAIA: Composition, formation and evolution of the Galaxy. Astronomy and Astrophysics. 369(1). 339–363.623 indexed citations breakdown →
Pace, O.. (1997). Lagrangian L2 or geostationary orbit: A system level trade-off for the GAIA mission.. 402. 807–809.
11.
Bersanelli, M., N. Mandolesi, C. J. Césarsky, et al.. (1996). COBRAS/SAMBA: the European space mission to map the CBR anisotropy. ORCA Online Research @Cardiff. 33. 19–24.
12.
Bersanelli, M., F. R. Bouchet, G. Efstathiou, et al.. (1996). COBRAS/SAMBA: report on the Phase A study.22 indexed citations
13.
Catala, C., F. Favata, M. Fridlund, et al.. (1996). STARS: Seismic Telescope for Astrophysical Research from Space. 4. 1.3 indexed citations
14.
Bersanelli, M., F. R. Bouchet, G. Efstathiou, et al.. (1996). COBRAS/SAMBA. A mission dedicated to imaging the anisotropies of the cosmic microwave background. Report on the phase A study.. OpenGrey (Institut de l'Information Scientifique et Technique).4 indexed citations
Tauber, J. A., O. Pace, & S. Volonté. (1994). COBRAS/SAMBA - a mission dedicated to the measurement of cosmic background anisotropies.. 18(3). 239–246.1 indexed citations
18.
Pace, O., et al.. (1994). Integral: Mission and satellite. The Astrophysical Journal Supplement Series. 92. 339–339.2 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.