M. Santos‐Lleó

5.2k total citations
73 papers, 2.1k citations indexed

About

M. Santos‐Lleó is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, M. Santos‐Lleó has authored 73 papers receiving a total of 2.1k indexed citations (citations by other indexed papers that have themselves been cited), including 66 papers in Astronomy and Astrophysics, 27 papers in Nuclear and High Energy Physics and 6 papers in Instrumentation. Recurrent topics in M. Santos‐Lleó's work include Astrophysical Phenomena and Observations (62 papers), Galaxies: Formation, Evolution, Phenomena (43 papers) and Astrophysics and Cosmic Phenomena (26 papers). M. Santos‐Lleó is often cited by papers focused on Astrophysical Phenomena and Observations (62 papers), Galaxies: Formation, Evolution, Phenomena (43 papers) and Astrophysics and Cosmic Phenomena (26 papers). M. Santos‐Lleó collaborates with scholars based in Spain, United States and United Kingdom. M. Santos‐Lleó's co-authors include N. Schartel, M. Guainazzi, E. Jiménez‐Bailón, P. M. Rodriguez‐Pascual, E. Piconcelli, S. Komossa, A. L. Longinotti, D. Grupe, J. Clavel and M. L. Parker and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

M. Santos‐Lleó

70 papers receiving 2.1k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
M. Santos‐Lleó Spain 24 2.0k 879 117 98 90 73 2.1k
K. C. Steenbrugge United States 25 1.8k 0.9× 696 0.8× 124 1.1× 39 0.4× 188 2.1× 64 1.8k
A. J. Blustin United Kingdom 16 1.3k 0.6× 521 0.6× 73 0.6× 78 0.8× 71 0.8× 38 1.3k
E. Nardini Italy 28 2.5k 1.2× 899 1.0× 251 2.1× 112 1.1× 84 0.9× 88 2.5k
Yoshitaka Ishisaki Japan 21 1.1k 0.5× 491 0.6× 86 0.7× 31 0.3× 77 0.9× 75 1.2k
Karen M. Leighly United States 26 2.2k 1.1× 842 1.0× 259 2.2× 44 0.4× 65 0.7× 66 2.3k
K. A. Pounds United Kingdom 22 1.7k 0.8× 713 0.8× 87 0.7× 52 0.5× 70 0.8× 65 1.7k
Pierre-Olivier Petrucci France 28 2.4k 1.2× 1.1k 1.3× 92 0.8× 214 2.2× 129 1.4× 125 2.5k
P. Arévalo Chile 24 1.9k 0.9× 706 0.8× 147 1.3× 66 0.7× 97 1.1× 69 2.0k
T. Yaqoob United States 26 3.5k 1.7× 1.5k 1.7× 124 1.1× 208 2.1× 154 1.7× 73 3.6k
Fumio Takahara Japan 22 1.7k 0.8× 1.1k 1.3× 103 0.9× 120 1.2× 55 0.6× 107 1.8k

Countries citing papers authored by M. Santos‐Lleó

Since Specialization
Citations

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

Fields of papers citing papers by M. Santos‐Lleó

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. Santos‐Lleó

This figure shows the co-authorship network connecting the top 25 collaborators of M. Santos‐Lleó. A scholar is included among the top collaborators of M. Santos‐Lleó 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. Santos‐Lleó. M. Santos‐Lleó 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.
Matzeu, G. A., E. Nardini, M. L. Parker, et al.. (2020). The first broad-band X-ray view of the narrow-line Seyfert 1 Ton S180. Monthly Notices of the Royal Astronomical Society. 497(2). 2352–2370. 19 indexed citations
2.
Kollatschny, W., D. Grupe, M. L. Parker, et al.. (2020). Optical and X-ray discovery of the changing-look AGN IRAS 23226-3843 showing extremely broad and double-peaked Balmer profiles. Springer Link (Chiba Institute of Technology). 16 indexed citations
3.
Mao, Junjie, J. S. Kaastra, M. Guainazzi, et al.. (2019). CIELO-RGS: a catalog of soft X-ray ionized emission lines. Springer Link (Chiba Institute of Technology). 3 indexed citations
4.
Giroletti, M., F. Panessa, A. L. Longinotti, et al.. (2017). Coexistence of a non-thermal jet and a complex ultra-fast X-ray outflow in a moderately luminous AGN. Springer Link (Chiba Institute of Technology). 19 indexed citations
5.
Kollatschny, W., N. Schartel, M. Zetzl, et al.. (2015). The peculiar optical-UV X-ray spectra of the X-ray weak quasar PG 0043+039. Springer Link (Chiba Institute of Technology). 2 indexed citations
6.
Pereira-Santaella, M., A. Alonso‐Herrero, M. Santos‐Lleó, et al.. (2011). The X-ray emission of local luminous infrared galaxies. Springer Link (Chiba Institute of Technology). 60 indexed citations
7.
Fabian, A. C., Abderahmen Zoghbi, Dan Wilkins, et al.. (2011). 1H 0707−495 in 2011: an X-ray source within a gravitational radius of the event horizon. Monthly Notices of the Royal Astronomical Society. 419(1). 116–123. 94 indexed citations
8.
Schartel, N., P. M. Rodriguez‐Pascual, M. Santos‐Lleó, et al.. (2010). A long hard look at the minimum state of PG 2112+059 with XMM-Newton. Springer Link (Chiba Institute of Technology). 11 indexed citations
9.
Cardaci, M. V., M. Santos‐Lleó, Y. Krongold, et al.. (2009). Characterization of the emitting and absorbing media around the nucleus of the active galaxy UGC 11763 using XMM-Newton data. Springer Link (Chiba Institute of Technology). 11 indexed citations
10.
Santos‐Lleó, M., N. Schartel, H. Tananbaum, W. H. Tucker, & Martin C. Weisskopf. (2009). The first decade of science with Chandra and XMM-Newton. Nature. 462(7276). 997–1004. 15 indexed citations
11.
Jiménez‐Bailón, E., N. Loiseau, M. Guainazzi, et al.. (2007). XMM-Newton view of galaxy pairs: activation of quiescent black holes?. Springer Link (Chiba Institute of Technology). 5 indexed citations
12.
Jiménez‐Bailón, E., M. Guainazzi, G. Matt, et al.. (2007). X-ray properties of a sample of polar-scattered Seyfert galaxies. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas). 32(2). 131–133. 2 indexed citations
13.
Jiménez‐Bailón, E., M. Santos‐Lleó, Marcus S. Dahlem, et al.. (2005). X-ray emission from NGC 1808: more than a complex\nstarburst. Springer Link (Chiba Institute of Technology). 16 indexed citations
14.
Santos‐Lleó, M., et al.. (2003). GRB 031203 XMM-newton observation.. GCN. 2464. 1. 1 indexed citations
15.
Rodriguez‐Pascual, P. M., M. Santos‐Lleó, R. González-Riestra, N. Schartel, & B. Altieri. (2003). XMM-newton observation of GRB031203.. GRB Coordinates Network. 2474. 1. 1 indexed citations
16.
González‐Riestra, R., et al.. (2003). XTE J1720-318. IAUC. 8080. 1. 2 indexed citations
17.
Zand, J. J. M. in ’t, C. B. Markwardt, A. Bazzano, et al.. (2002). The nature of the X-ray transient SAX J1711.6-3808. Springer Link (Chiba Institute of Technology). 12 indexed citations
18.
Page, K. L., K. O. Mason, F. J. Carrera, et al.. (2001). The variable XMM-Newton spectrum of Markarian 766. Springer Link (Chiba Institute of Technology). 24 indexed citations
19.
Santos‐Lleó, M., N. Schartel, M. Guainazzi, et al.. (2001). The life cycle of XMM-Newton's "Targets of Opportunity". 107. 54–62. 3 indexed citations
20.
Clavel, J., A. Boksenberg, G. E. Bromage, et al.. (1990). The ultra-compact broad emission line region in NGC 4151. Monthly Notices of the Royal Astronomical Society. 246(4). 668–677. 22 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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