J. Isern
About
In The Last Decade
J. Isern
167 papers receiving 4.6k citations
Peers
Comparison fields: 5 of 66
- Astronomy and Astrophysics 4.4k
- Nuclear and High Energy Physics 1.3k
- Instrumentation 1.2k
- Atomic and Molecular Physics, and Optics 357
- Geophysics 245
Countries citing papers authored by J. Isern
This map shows the geographic impact of J. Isern'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 J. Isern with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites J. Isern more than expected).
Fields of papers citing papers by J. Isern
This network shows the impact of papers produced by J. Isern. 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 J. Isern. The network helps show where J. Isern may publish in the future.
Co-authorship network of co-authors of J. Isern
This figure shows the co-authorship network connecting the top 25 collaborators of J. Isern. A scholar is included among the top collaborators of J. Isern 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 J. Isern. J. Isern is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | The effect of <SUP>22</SUP>Ne diffusion in the evolution and pulsational properties of white dwarfs with solar metallicity progenitors | 52 |
| 2 | 20 | |
| 3 | 24 | |
| 4 | Revisiting the axion bounds from the Galactic white dwarf luminosity function | 123 |
| 5 | 9 | |
| 6 | 11 | |
| 7 | 48 | |
| 8 | Bounds to the gamma--ray flux emitted by SN 2011fe before the maximum of light as obtained by INTEGRAL/SPI | 1 |
| 9 | White Dwarfs as Physics Laboratories: The Axion Case | 4 |
| 10 | 8 | |
| 11 | 4 | |
| 12 | Testing the Relationship between the Masses of White Dwarfs and those of their Progenitors | 1 |
| 13 | The science of gamma-ray spectroscopy | 1 |
| 14 | What Are White Dwarfs Telling Us About the Galactic Disk and Halo | 1 |
| 15 | Gamma-Ray Emission of Classical Novae and its Detectability by Integral | 2 |
| 16 | Possibility of the Detection of Classical Novae with the Shield of the Integral Spectrometer SPI | 2 |
| 17 | 6 | |
| 18 | Gamma-ray bursts from relativistic beams in neutron star mergers. | 1 |
| 19 | 3 | |
| 20 | On the contribution of Ne-22 to the synthesis of Fe-54 and Ni-58 in thermonuclear supernovae | 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.