A. Neesemann
About
In The Last Decade
A. Neesemann
40 papers receiving 501 citations
Peers
Comparison fields: 5 of 33
- Astronomy and Astrophysics 503
- Atmospheric Science 207
- Ecology 76
- Aerospace Engineering 50
- Geophysics 48
Countries citing papers authored by A. Neesemann
This map shows the geographic impact of A. Neesemann'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 A. Neesemann with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Neesemann more than expected).
Fields of papers citing papers by A. Neesemann
This network shows the impact of papers produced by A. Neesemann. 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 A. Neesemann. The network helps show where A. Neesemann may publish in the future.
Co-authorship network of co-authors of A. Neesemann
This figure shows the co-authorship network connecting the top 25 collaborators of A. Neesemann. A scholar is included among the top collaborators of A. Neesemann 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 A. Neesemann. A. Neesemann is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 20 | |
| 2 | The Chronostratigraphy of Ceres | 1 |
| 3 | Revisiting the Cerealia and Vinalia Faculae on Ceres | 2 |
| 4 | The HAMO-Based Global Geologic Map and Chronostratigraphy of Ceres | 5 |
| 5 | Faculae on Ceres: Possible Formation Mechanisms | 3 |
| 6 | How the Distribution of Impact Ejecta may explain Surface Features on Ceres and Saturnian Satellites | 0 |
| 7 | The Distribution of Impact Ejecta on Ceres | 8 |
| 8 | Stratigraphy and surface ages of dwarf planet (1) Ceres: results from geologic and topographic mapping in Survey, HAMO and LAMO data of the Dawn Framing Camera images | 1 |
| 9 | Geologic evolution of the dwarf planet (1) Ceres: results from geologic mapping using Dawn FC2 camera imaging data and an update in cratering model ages | 0 |
| 10 | Boulders on Ceres | 2 |
| 11 | Origin and Distribution of Polygonal Craters on (1) Ceres | 4 |
| 12 | Stratigraphy of (1) Ceres from geologic and topographic mapping and crater counts using images of the Dawn FC2 camera | 1 |
| 13 | Polygonal Impact Craters on Ceres: Morphology and Distribution | 2 |
| 14 | Characteristics of Polygonal Craters on (1) Ceres | 1 |
| 15 | Crater Scaling on Weak Targets, from Ceres to Icy Satellites | 0 |
| 16 | Size-Frequency Distributions of km to Sub-km Sized Impact Craters on Ceres | 2 |
| 17 | Geologic Mapping of the Ac-H-7 Kerwan Quadrangle of Ceres from NASA Dawn Mission | 1 |
| 18 | A Preliminary Chronology for Ceres | 0 |
| 19 | Crater Counting on Small Bodies — The Influence of Topography-Related Distortions | 9 |
| 20 | The signature of secondary cratering on 4 Vesta and Tethys | 1 |
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.