M. R. Calabretta

38 papers receiving 1.9k citations

Hit Papers

HI4PI: a full-sky H i survey based on EBHIS and GASS20162026201920222016250500750

Peers

M. R. Calabretta
Comparison fields: 5 of 61
  • Astronomy and Astrophysics 1.8k
  • Nuclear and High Energy Physics 581
  • Instrumentation 244
  • Computational Mechanics 98
  • Atomic and Molecular Physics, and Optics 62
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S. Bowyer United States
J. L. Donley United States
V. Kashyap United States
M. Haverkorn Netherlands
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T. L. Landecker Canada
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R. W. Argyle France
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M. R. Calabretta relative to S. Bowyer United States S. Bowyer's profile →
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Countries citing papers authored by M. R. Calabretta

Since Specialization
Citations

This map shows the geographic impact of M. R. Calabretta'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 M. R. Calabretta with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. R. Calabretta more than expected).

Fields of papers citing papers by M. R. Calabretta

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by M. R. Calabretta. 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 M. R. Calabretta. The network helps show where M. R. Calabretta may publish in the future.

Co-authorship network of co-authors of M. R. Calabretta

This figure shows the co-authorship network connecting the top 25 collaborators of M. R. Calabretta. A scholar is included among the top collaborators of M. R. Calabretta 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 M. R. Calabretta. M. R. Calabretta is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
#WorkIndexed citations
1 13
2
HI4PI: a full-sky H i survey based on EBHIS and GASSbreakdown →
853
3 45
4
Representations of Time Coordinates in FITS Time and Relative Dimension in Space
4
5 6
6
Wcslib and Pgsbox
2
7 3
8 104
9 1
10 25
11 24
12
Implementation of -TAB coordinates in WCSLIB
1
13 48
14 2
15 10
16 10
17 96
18 203
19
Representations of World Coordinates in FITS
0
20
Representations of Celestial Coordinates in FITS
3

About M. R. Calabretta

M. R. Calabretta is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 40 papers that have together received 2.0k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (15 papers), Astrophysics and Star Formation Studies (10 papers) and Astrophysics and Cosmic Phenomena (9 papers). The work is most often cited by research in Astronomy and Astrophysics (1.8k citations), Instrumentation (244 citations) and Nuclear and High Energy Physics (581 citations). M. R. Calabretta has collaborated with scholars based in Australia, United States and Germany. Frequent co-authors include E. W. Greisen, L. Staveley‐Smith, H. Alyson Ford, P. M. W. Kalberla, D. J. Pisano, N. M. McClure‐Griffiths, Tara Murphy, H. Nakanishi, L. Dedes and B. K. Gibson. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

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.

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