M. Douspis

89.7k total citations · 1 hit paper
70 papers, 984 citations indexed

About

M. Douspis is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, M. Douspis has authored 70 papers receiving a total of 984 indexed citations (citations by other indexed papers that have themselves been cited), including 67 papers in Astronomy and Astrophysics, 28 papers in Nuclear and High Energy Physics and 12 papers in Instrumentation. Recurrent topics in M. Douspis's work include Galaxies: Formation, Evolution, Phenomena (53 papers), Cosmology and Gravitation Theories (48 papers) and Astrophysics and Cosmic Phenomena (16 papers). M. Douspis is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (53 papers), Cosmology and Gravitation Theories (48 papers) and Astrophysics and Cosmic Phenomena (16 papers). M. Douspis collaborates with scholars based in France, Italy and United States. M. Douspis's co-authors include Nabila Aghanim, L. Salvati, N. Aghanim, M. Langer, S. Ilić, G. Hurier, É. Pointecouteau, H. Tanimura, A. Beelen and Adélie Gorce and has published in prestigious journals such as SHILAP Revista de lepidopterología, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

M. Douspis

67 papers receiving 948 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.

Cosmological parameters derived from the final Planck data release (PR4)

2023 100 citations M. Douspis, S. Ilić et al. Astronomy and Astrophysics profile →

Peers

Countries citing papers authored by M. Douspis

Since Specialization

Citations

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

Fields of papers citing papers by M. Douspis

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by M. Douspis. 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. Douspis. The network helps show where M. Douspis may publish in the future.

Co-authorship network of co-authors of M. Douspis

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

All Works

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20 of 20 papers shown

#	Work	Indexed citations
1	Characterising galaxy clusters’ completeness function in Planck with hydrodynamical simulations 2024 ·Astronomy and Astrophysics ·Salvatore Gallo, M. Douspis, É. Soubrié, L. Salvati	2
2	Self-supervised component separation for the extragalactic submillimetre sky 2024 ·Astronomy and Astrophysics ·(unknown), H. Tanimura, (unknown), (unknown), M. Douspis	2
3	Cosmological constraints from the Planck cluster catalogue with new multi-wavelength mass calibration from Chandra and CFHT 2024 ·Astronomy and Astrophysics ·(unknown), M. Douspis, G. W. Pratt, L. Salvati, É. Soubrié, Felipe Andrade-Santos, W. Forman, C. Jones, N. Aghanim, Ralph Kraft, R. J. van Weeren	1
4	Testing decaying dark matter models as a solution to theS₈tension with the thermal Sunyaev-Zel’dovich effect 2023 ·Astronomy and Astrophysics ·H. Tanimura, M. Douspis, Nabila Aghanim, (unknown)	8
5	Euclid preparation: XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis 2022 ·UCL Discovery (University College London) ·S. Ilić, N. Aghanim, C. Baccigalupi, J. R. Bermejo-Climent, Giulio Fabbian, L. Legrand, D. Paoletti, M. Ballardini, Maria Archidiacono, M. Douspis, F. Finelli⋆, K. Ganga, C. Hernández-Monteagudo, M. Lattanzi, Domenico Marinucci, M. Migliaccio, C. Carbone, Santiago Casas, (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (unknown), (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
6	Constraining hydrostatic mass bias and cosmological parameters with the gas mass fraction in galaxy clusters 2022 ·SHILAP Revista de lepidopterología ·(unknown), M. Douspis, L. Salvati, Nabila Aghanim	4
7	CMB at small scales: Cosmology from tSZ power spectrum 2022 ·SHILAP Revista de lepidopterología ·M. Douspis, L. Salvati, Adélie Gorce, Nabila Aghanim	2
8	Retrieving cosmological information from small-scale CMB foregrounds 2022 ·Astronomy and Astrophysics ·Adélie Gorce, M. Douspis, L. Salvati	18
9	Retrieving cosmological information from small-scale CMB foregrounds 2021 ·Astronomy and Astrophysics ·M. Douspis, (unknown), Adélie Gorce, (unknown)	10
10	Impact of systematics on cosmological parameters from future galaxy cluster surveys 2020 ·Springer Link (Chiba Institute of Technology) ·L. Salvati, M. Douspis, Nabila Aghanim	18
11	First detection of stacked X-ray emission from cosmic web filaments 2020 ·Springer Link (Chiba Institute of Technology) ·H. Tanimura, N. Aghanim, (unknown), M. Douspis, Nicola Malavasi	11
12	Constraints from thermal Sunyaev-Zel’dovich cluster counts and power spectrum combined with CMB 2018 ·Springer Link (Chiba Institute of Technology) ·L. Salvati, M. Douspis, Nabila Aghanim	75
13	X-ray galaxy clusters abundance and mass temperature\n scaling 2015 ·Springer Link (Chiba Institute of Technology) ·S. Ilić, Alain Blanchard, M. Douspis	3
14	Implications of bias evolution on measurements of the integrated Sachs-Wolfe effect: errors and biases in parameter estimation 2009 ·(unknown), M. Douspis, Nabila Aghanim	9
15	Large-scale galaxy correlations as a test for dark energy 2006 ·Springer Link (Chiba Institute of Technology) ·A. Blanchard, M. Douspis, M. Rowan-Robinson, S. Sarkar	11
16	Small scale contributions to the cosmic microwave background: a coherent analysis 2006 ·Springer Link (Chiba Institute of Technology) ·M. Douspis, N. Aghanim, M. Langer	6
17	Bias in matter power spectra? 2001 ·Springer Link (Chiba Institute of Technology) ·M. Douspis, Alain Blanchard, Joseph Silk	2
18	Concerning parameter estimation using the cosmic microwave background 2001 ·Springer Link (Chiba Institute of Technology) ·M. Douspis, J. G. Bartlett, Alain Blanchard, (unknown)	6
19	Cosmology from cosmic microwave background and galaxy clusters 2001 ·Springer Link (Chiba Institute of Technology) ·M. Douspis, Alain Blanchard, R. Sadat, J. G. Bartlett, (unknown)	10
20	Approximating the Likelihood Function of CMB Experiments 2000 ·CERN Bulletin ·J. G. Bartlett, Alain Blanchard, M. Douspis, (unknown)	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.

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