H. Otí-Floranes

681 total citations
10 papers, 230 citations indexed

About

H. Otí-Floranes is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, H. Otí-Floranes has authored 10 papers receiving a total of 230 indexed citations (citations by other indexed papers that have themselves been cited), including 10 papers in Astronomy and Astrophysics, 3 papers in Nuclear and High Energy Physics and 2 papers in Instrumentation. Recurrent topics in H. Otí-Floranes's work include Galaxies: Formation, Evolution, Phenomena (5 papers), Astrophysical Phenomena and Observations (5 papers) and Astrophysics and Star Formation Studies (4 papers). H. Otí-Floranes is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (5 papers), Astrophysical Phenomena and Observations (5 papers) and Astrophysics and Star Formation Studies (4 papers). H. Otí-Floranes collaborates with scholars based in Spain, Mexico and United States. H. Otí-Floranes's co-authors include J. M. Más-Hesse, Matthew Hayes, D. Schaerer, M. Cerviño, Angela Adamo, Hakim Atek, Andreas Sandberg, John M. Cannon, Peter Laursen and L. Guaita and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

H. Otí-Floranes

9 papers receiving 225 citations

Peers

H. Otí-Floranes

NHEP

INSTR

GEOPH

AMPO

Iu. Babyk Ukraine

Aleksandra Olejak Poland

Bülent Kızıltan United States

U. M. Noebauer Germany

David R. Aguilera-Dena Germany

D. Volpi Belgium

Marzena Śniegowska Poland

Aleksey Generozov United States

M. A. Tucker United States

V. N. Komarova Russia

Iu. Babyk Ukraine

H. Otí-Floranes

320 ×1.5

108 ×1.5

NHEP

61 ×1.1

INSTR

8 ×0.4

GEOPH

6 ×0.6

AMPO

Citations per year, relative to H. Otí-Floranes H. Otí-Floranes (= 1×) peers Iu. Babyk

Countries citing papers authored by H. Otí-Floranes

Since Specialization

Citations

This map shows the geographic impact of H. Otí-Floranes'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. Otí-Floranes with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites H. Otí-Floranes more than expected).

Fields of papers citing papers by H. Otí-Floranes

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by H. Otí-Floranes. 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. Otí-Floranes. The network helps show where H. Otí-Floranes may publish in the future.

Co-authorship network of co-authors of H. Otí-Floranes

This figure shows the co-authorship network connecting the top 25 collaborators of H. Otí-Floranes. A scholar is included among the top collaborators of H. Otí-Floranes 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. Otí-Floranes. H. Otí-Floranes is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

Sort: Min cites: Since: Top N: Style:

10 of 10 papers shown

Oskinova, L. M., Arjan Bik, J. M. Más-Hesse, et al.. (2019). ULX contribution to stellar feedback: an intermediate-mass black hole candidate and the population of ULXs in the low-metallicity starburst galaxy ESO 338-4. Springer Link (Chiba Institute of Technology). 7 indexed citations

Paggi, A., D. Milisavljević, N. Masetti, et al.. (2014). OPTICAL SPECTROSCOPIC OBSERVATIONS OF γ-RAY BLAZAR CANDIDATES. I. PRELIMINARY RESULTS. The Astronomical Journal. 147(5). 112–112. 39 indexed citations

Hayes, Matthew, Göran Östlin, Florent Duval, et al.. (2014). THE LYMAN ALPHA REFERENCE SAMPLE. II.HUBBLE SPACE TELESCOPEIMAGING RESULTS, INTEGRATED PROPERTIES, AND TRENDS. The Astrophysical Journal. 782(1). 6–6. 70 indexed citations

Zelati, F. Coti, M. C. Baglio, S. Campana, et al.. (2014). Engulfing a radio pulsar: the case of PSR J1023+0038. Monthly Notices of the Royal Astronomical Society. 444(2). 1783–1792. 38 indexed citations

Pardy, Stephen, John M. Cannon, Göran Östlin, et al.. (2014). THE LYMAN ALPHA REFERENCE SAMPLE. III. PROPERTIES OF THE NEUTRAL ISM FROM GBT AND VLA OBSERVATIONS. The Astrophysical Journal. 794(2). 101–101. 21 indexed citations

Paggi, A., R. D’Abrusco, F. Massaro, et al.. (2014). Multi-wavelength selection and identification of gamma-ray blazar candidates. Proceedings of the International Astronomical Union. 10(S313). 58–63.

Miralles-Caballero, D., F. F. Rosales-Ortega, Á. I. Díaz, et al.. (2014). Ionizing stellar population in the disc of NGC 3310 – II. The Wolf–Rayet population★. Monthly Notices of the Royal Astronomical Society. 445(4). 3803–3822. 6 indexed citations

Otí-Floranes, H., J. M. Más-Hesse, E. Jiménez‐Bailón, et al.. (2012). Multiwavelength analysis of the Lyman-αemitting galaxy Haro 2: relation between the diffuse Lyman-αand soft X-ray emissions. Astronomy and Astrophysics. 546. A65–A65. 16 indexed citations

Otí-Floranes, H. & J. M. Más-Hesse. (2009). Calibration of star formation rate tracers for short- and long-lived star formation episodes. Astronomy and Astrophysics. 511. A61–A61. 15 indexed citations

10.

Más-Hesse, J. M., H. Otí-Floranes, & M. Cerviño. (2008). Soft X-ray to far infrared luminosities ratio in star-forminggalaxies: predictions from synthesis models. Astronomy and Astrophysics. 483(1). 71–78. 18 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.

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