H. J. Schober
About
In The Last Decade
H. J. Schober
64 papers receiving 626 citations
Peers
Comparison fields: 5 of 46
- Astronomy and Astrophysics 336
- Civil and Structural Engineering 182
- Mechanical Engineering 145
- Computational Mechanics 112
- Architecture 85
Countries citing papers authored by H. J. Schober
This map shows the geographic impact of H. J. Schober'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 H. J. Schober with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites H. J. Schober more than expected).
Fields of papers citing papers by H. J. Schober
This network shows the impact of papers produced by H. J. Schober. 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 H. J. Schober. The network helps show where H. J. Schober may publish in the future.
Co-authorship network of co-authors of H. J. Schober
This figure shows the co-authorship network connecting the top 25 collaborators of H. J. Schober. A scholar is included among the top collaborators of H. J. Schober 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 H. J. Schober. H. J. Schober 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 | 15 | |
| 3 | 2 | |
| 4 | 9 | |
| 5 | Physical Studies of Asteroids. XXVIII. Lightcurves and photoelectric photometry of asteroids 2, 14, 51, 105, 181, 238, 258, 369, 377, 416, 487, 626, 679, 1048, and 2183 | 8 |
| 6 | Lightcurves and rotation periods for the asteroids 70 Panopaea and 235 Carolina | 1 |
| 7 | The large C-type asteroids 146 Lucina and 410 Chloris, and the small S-type asteroids 152 Atala and 631 Philippina - Rotation periods and lightcurves | 1 |
| 8 | The asteroids 36 Atalante and 48 DORIS - Rotation, UBV-photometry, and lightcurves | 1 |
| 9 | Photoelectric photometry of the asteroids 404 Arsinoe and 628 Christine | 1 |
| 10 | Rotation period and photoelectric lightcurves of asteroids 68 Leto and 563 Suleika | 3 |
| 11 | The asteroids 118 Peitho and 952 CAIA - Rotation periods and lightcurves from photoelectric observations | 3 |
| 12 | 387 Aquitania and 776 Berbericia: two slow spinning asteroids with rotation periods of nearly one day? | 6 |
| 13 | On the light variations of the C-type asteroids 140 Siwa and 790 Pretoria. | 3 |
| 14 | Rotation period of the minor planet 337 Desova: an unusual object with triple extrema in the photoelectric lightcurve. | 1 |
| 15 | UBV photometry of the asteroids 9 Metis, 87 Sylvia and 247 Eukrate during their oppositions in 1978 with respect to lightcurves | 11 |
| 16 | Photoelectric photometry and rotation periods of three large and dark asteroids: 49 Pales, 88 Thisbe and 92 Undina. | 9 |
| 17 | Photometric Variations of the Minor Planets 55 Pandora and 173 Ino during the Opposition in 1977: Light Curves and Rotation Periods | 5 |
| 18 | Photoelectric photometry of the minor planet 32 Pomona: composite light curve and the synodic period of rotation. | 3 |
| 19 | Photoelectric photometry of 1 Ceres during the Ceres-campaign 1975 | 2 |
| 20 | The minor planet 654 Zelinda: rotation period and light curve. | 7 |
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.