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).
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
20 of 20 papers shown
1.
Sanchez, J. L. Gálvez, et al.. (2019). A Wide Field Monitor (WFM) for the new generation X-ray missions eXTP (China) and STROBE-X (NASA). 560–567.
2.
Henze, M., G. Sala, A. Ederoclite, et al.. (2017). Additional Photometry for nova M31N 2016-12e and classification as a recurrent nova (= M31N 2007-11f). The astronomer's telegram. 10001. 1.1 indexed citations
3.
Henze, M., S. C. Williams, M. J. Darnley, et al.. (2016). Confirmation of PNV J00430400+4117079 as another eruption of the recurrent nova M31N 1990-10a and additional constraints on the eruption date. ATel. 9276. 1.1 indexed citations
4.
Feroci, M., J. W. den Herder, E. Bozzo, et al.. (2014). View.24 indexed citations
Hernanz, M.. (2012). Novae in γ-rays. 40. 377.2 indexed citations
8.
Balman, Ş., S. Starrfield, J. J. Drake, et al.. (2012). The X-ray Nebula around the Recurrent Nova T Pyxidis. ATel. 3915. 1.3 indexed citations
9.
Isern, J., P. Jean, Eduardo Bravo, et al.. (2011). Bounds to the gamma--ray flux emitted by SN 2011fe before the maximum of light as obtained by INTEGRAL/SPI. ATel. 3683. 1.1 indexed citations
Osborne, J. P., K. L. Page, G. A. Wynn, et al.. (2010). Broad UV and probable X-ray eclipses in nova U Sco. The astronomer's telegram. 2442. 1.1 indexed citations
Hernanz, M. & J. José. (2002). Classical nova explosions: international conference on classical nova explosions, Sitges, Spain, 20-24 May 2002. American Institute of Physics eBooks.2 indexed citations
19.
Hernanz, M., et al.. (1999). Gamma-Ray Emission of Classical Novae and its Detectability by Integral. HAL (Le Centre pour la Communication Scientifique Directe). 38. 407.2 indexed citations
20.
Mochkovitch, R., et al.. (1995). Gamma-ray bursts from relativistic beams in neutron star mergers.. A&A. 293. 803–809.1 indexed citations
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.