M. Hernanz
About
In The Last Decade
M. Hernanz
143 papers receiving 3.0k citations
Peers
Comparison fields: 5 of 60
- Astronomy and Astrophysics 2.6k
- Nuclear and High Energy Physics 1.2k
- Instrumentation 431
- Atomic and Molecular Physics, and Optics 288
- Radiation 271
Countries citing papers authored by M. Hernanz
This map shows the geographic impact of M. Hernanz'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. Hernanz with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Hernanz more than expected).
Fields of papers citing papers by M. Hernanz
This network shows the impact of papers produced by M. Hernanz. 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. Hernanz. The network helps show where M. Hernanz may publish in the future.
Co-authorship network of co-authors of M. Hernanz
This figure shows the co-authorship network connecting the top 25 collaborators of M. Hernanz. A scholar is included among the top collaborators of M. Hernanz 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. Hernanz. M. Hernanz is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | UVES observations of Nova Reticuli 2020 during Minimal Science Operations show it is entering the nebular phase | 1 |
| 2 | A Wide Field Monitor (WFM) for the new generation X-ray missions eXTP (China) and STROBE-X (NASA) | 0 |
| 3 | Confirmation of PNV J00430400+4117079 as another eruption of the recurrent nova M31N 1990-10a and additional constraints on the eruption date | 1 |
| 4 | 24 | |
| 5 | 27 | |
| 6 | 2 | |
| 7 | Novae in γ-rays | 2 |
| 8 | The X-ray Nebula around the Recurrent Nova T Pyxidis | 3 |
| 9 | Bounds to the gamma--ray flux emitted by SN 2011fe before the maximum of light as obtained by INTEGRAL/SPI | 1 |
| 10 | 24 | |
| 11 | Broad UV and probable X-ray eclipses in nova U Sco | 1 |
| 12 | 4 | |
| 13 | Testing the Relationship between the Masses of White Dwarfs and those of their Progenitors | 1 |
| 14 | 28 | |
| 15 | Long Distance Test of the CLAIRE Gamma-Ray Lens | 2 |
| 16 | 44 | |
| 17 | 1 | |
| 18 | Gamma-Ray Emission of Classical Novae and its Detectability by Integral | 2 |
| 19 | Possibility of the Detection of Classical Novae with the Shield of the Integral Spectrometer SPI | 2 |
| 20 | 6 |
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.