F. Atrio‐Barandela

21.3k citations

56 papers · 1.8k indexed · 1 hit paper · h-index 19

Astronomy and Astrophysics top 1%
Nuclear and High Energy Physics top 2%
Statistical and Nonlinear Physics top 5%
Instrumentation top 5%
Oceanography

Co-authors: Diego Pavón Germán Olivares A. Kashlinsky P. A. R. Ade Dale D. Kocevski H. Ebeling N. Aghanim M. Arnaud
Topics: Cosmology and Gravitation Theories (40 papers)Galaxies: Formation, Evolution, Phenomena (38 papers)Dark Matter and Cosmic Phenomena (18 papers)
Cited by: Astronomy and Astrophysics Nuclear and High Energy Physics Instrumentation
Journals: Reviews of Modern Physics The Astrophysical Journal Monthly Notices of the Royal Astronomical Society
Partner nations: Spain Germany United States

In The Last Decade

F. Atrio‐Barandela

54 papers receiving 1.7k citations

Hit Papers

align trajectories

What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

Planck 2013 results - VII. HFI time response and beams

2014 491 citations P. A. R. Ade, N. Aghanim et al. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) profile →

Peers

Countries citing papers authored by F. Atrio‐Barandela

Since Specialization

Citations

This map shows the geographic impact of F. Atrio‐Barandela'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 F. Atrio‐Barandela with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites F. Atrio‐Barandela more than expected).

Fields of papers citing papers by F. Atrio‐Barandela

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by F. Atrio‐Barandela. 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 F. Atrio‐Barandela. The network helps show where F. Atrio‐Barandela may publish in the future.

Co-authorship network of co-authors of F. Atrio‐Barandela

This figure shows the co-authorship network connecting the top 25 collaborators of F. Atrio‐Barandela. A scholar is included among the top collaborators of F. Atrio‐Barandela 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 F. Atrio‐Barandela. F. Atrio‐Barandela 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:

20 of 20 papers shown

#	Work	Indexed citations
1	Probing the Dipole of the Diffuse Gamma-Ray Background 2024 ·The Astrophysical Journal Letters ·A. Kashlinsky,F. Atrio‐Barandela,(unknown)	1
2	Further understanding the interaction between dark energy and dark matter: current status and future directions 2024 ·Reports on Progress in Physics ·Bin Wang,Élcio Abdalla,F. Atrio‐Barandela,Diego Pavón	41
3	2015 ·MURAL - Maynooth University Research Archive Library (National University of Ireland, Maynooth) ·(unknown),F. Atrio‐Barandela,(unknown),C. Baccigalupi,(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown)	9
4	Planck 2013 results - X. HFI energetic particle effects: characterization, removal, and simulation 2014 ·LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) ·P. A. R. Ade,N. Aghanim,(unknown),M. Arnaud,M. Ashdown,F. Atrio‐Barandela,J. Aumont,C. Baccigalupi,A. J. Banday,(unknown),(unknown),I. D. Novikov,H. U. Nørgaard-Nielsen,(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown)	1
5	Planck 2013 results - XII. Diffuse component separation 2014 ·LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) ·P. A. R. Ade,N. Aghanim,C. Armitage-Caplan,M. Arnaud,(unknown),F. Atrio‐Barandela,J. Aumont,(unknown),(unknown),(unknown),(unknown),I. D. Novikov,H. U. Nørgaard-Nielsen,(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown)	5
6	Planck 2013 results - XVI. Cosmological parameters 2014 ·LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) ·P. A. R. Ade,N. Aghanim,C. Armitage-Caplan,M. Arnaud,M. Ashdown,F. Atrio‐Barandela,(unknown),(unknown),(unknown),I. D. Novikov,H. U. Nørgaard-Nielsen,(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown)	6
7	Planck 2013 results - VII. HFI time response and beamsbreakdown → 2014 ·LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) ·P. A. R. Ade,N. Aghanim,C. Armitage-Caplan,M. Arnaud,M. Ashdown,F. Atrio‐Barandela,J. Aumont,C. Baccigalupi,A. J. Banday	491
8	Constraining f(R) gravity with Planck data on galaxy cluster profiles 2014 ·Monthly Notices of the Royal Astronomical Society ·Ivan De Martino,Mariafelicia De Laurentis,F. Atrio‐Barandela,Salvatore Capozzıello	30
9	Planck 2013 results - V. LFI calibration 2014 ·LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) ·N. Aghanim,C. Armitage-Caplan,M. Arnaud,M. Ashdown,F. Atrio‐Barandela,J. Aumont,C. Baccigalupi,A. J. Banday,R. B. Barreiro,E. Battaner,K. Benabed	17
10	Planck intermediate results VIII : Filaments between interacting clusters 2013 ·MURAL - Maynooth University Research Archive Library (National University of Ireland, Maynooth) ·P. A. R. Ade,M. Juvela,M. Arnaud,M. Ashdown,F. Atrio‐Barandela,(unknown)	42
11	Planck intermediate results - X. Physics of the hot gas in the Coma cluster 2013 ·HAL (Le Centre pour la Communication Scientifique Directe) ·P. A. R. Ade,N. Aghanim,M. Arnaud,M. Ashdown,F. Atrio‐Barandela,J. Aumont	49
12	Planck 2013 results. XXI. Cosmology with the all-sky Planck Compton parameter y-map 2013 ·Research at the University of Copenhagen (University of Copenhagen) ·P. A. R. Ade,N. Aghanim,(unknown),M. Arnaud,M. Ashdown,F. Atrio‐Barandela,(unknown),(unknown),Pavel Naselsky,I. D. Novikov,H. U. Nørgaard-Nielsen	1
13	Planck 2013 Results. XXIV. Constraints on primordial non-Gaussianity 2013 ·MURAL - Maynooth University Research Archive Library (National University of Ireland, Maynooth) ·P. A. R. Ade,N. Aghanim,(unknown),M. Arnaud,M. Ashdown,F. Atrio‐Barandela,J. Aumont,(unknown),A. J. Banday,(unknown),(unknown),I. D. Novikov,H. U. Nørgaard-Nielsen,(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown),(unknown)	4
14	Planck Intermediate Results. XI. The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies 2013 ·MURAL - Maynooth University Research Archive Library (National University of Ireland, Maynooth) ·P. A. R. Ade,N. Aghanim,M. Arnaud,M. Ashdown,F. Atrio‐Barandela	74
15	Bulk flows in inflation and in Lemaître-Tolman-Bondi models 2010 ·Journal of Physics Conference Series ·F. Atrio‐Barandela,A. Kashlinsky,H. Ebeling,Dale D. Kocevski	2
16	A Measurement of Large-Scale Peculiar Velocities of Clusters of Galaxies: Results and Cosmological Implications 2008 ·The Astrophysical Journal ·A. Kashlinsky,F. Atrio‐Barandela,Dale D. Kocevski,H. Ebeling	187
17	Using peak distribution of the cosmic microwave background for WMAP and Planck data analysis: Formalism and simulations 2004 ·Astronomy and Astrophysics ·(unknown),A. Kashlinsky,F. Atrio‐Barandela	5
18	Temperature Anisotropies and Distortions Induced by Hot Intracluster Gas on the Cosmic Microwave Background. 1998 ·F. Atrio‐Barandela	30
19	The Power Spectrum of Microwave Background Temperature Anisotropies Measured by the Tenerife Experiment 1997 ·The Astrophysical Journal ·F. Atrio‐Barandela,Stefan Gottlöber,(unknown)	9
20	Interacting hot dark matter 1997 ·Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields ·F. Atrio‐Barandela,Sacha Davidson	19

About F. Atrio‐Barandela

F. Atrio‐Barandela is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation, having authored 56 papers that have together received 1.8k indexed citations. Recurring topics across this work include Cosmology and Gravitation Theories (40 papers), Galaxies: Formation, Evolution, Phenomena (38 papers) and Dark Matter and Cosmic Phenomena (18 papers). The work is most often cited by research in Astronomy and Astrophysics (1.7k citations), Nuclear and High Energy Physics (1.1k citations) and Instrumentation (104 citations). F. Atrio‐Barandela has collaborated with scholars based in Spain, Germany and United States. Frequent co-authors include Diego Pavón, Germán Olivares, A. Kashlinsky, P. A. R. Ade, Dale D. Kocevski, H. Ebeling, N. Aghanim, M. Arnaud, M. Ashdown and J. Aumont. Their work appears in journals such as Reviews of Modern Physics, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

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.

Explore authors with similar magnitude of impact