Martin White
About
In The Last Decade
Martin White
215 papers receiving 12.1k citations
Hit Papers
Peers
Comparison fields: 5 of 82
- Astronomy and Astrophysics 11.9k
- Nuclear and High Energy Physics 4.5k
- Instrumentation 3.3k
- Statistical and Nonlinear Physics 922
- Atomic and Molecular Physics, and Optics 386
Countries citing papers authored by Martin White
This map shows the geographic impact of Martin White'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 Martin White with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Martin White more than expected).
Fields of papers citing papers by Martin White
This network shows the impact of papers produced by Martin White. 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 Martin White. The network helps show where Martin White may publish in the future.
Co-authorship network of co-authors of Martin White
This figure shows the co-authorship network connecting the top 25 collaborators of Martin White. A scholar is included among the top collaborators of Martin White 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 Martin White. Martin White is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 8 | |
| 3 | 24 | |
| 4 | 18 | |
| 5 | 36 | |
| 6 | Synergies between radio, optical and microwave observations at high\n redshift | 15 |
| 7 | Modeling CMB lensing cross correlations with CLEFT | 27 |
| 8 | 11 | |
| 9 | The Gaussian streaming model and convolution Lagrangian effective field theory | 74 |
| 10 | ZeldovichRecon: Halo correlation function using the Zeldovich approximation | 1 |
| 11 | The Dark Energy Spectroscopic Instrument (DESI): Tiling and Fiber Assignment | 1 |
| 12 | 29 | |
| 13 | 88 | |
| 14 | 123 | |
| 15 | The Baryon Oscillation Spectroscopic Survey: Precision measurements of the absolute cosmic distance scale | 3 |
| 16 | Precision Determination Of The Nonlinear Matter Power Spectrum | 1 |
| 17 | SDSS-III: The Baryon Oscillation Spectroscopic Survey (BOSS) | 7 |
| 18 | Cosmic variance of weak lensing surveys in the non-linear regime | 3 |
| 19 | 71 | |
| 20 | 19 |
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.