S. Paltani

19.3k total citations
86 papers, 1.8k citations indexed

About

S. Paltani is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, S. Paltani has authored 86 papers receiving a total of 1.8k indexed citations (citations by other indexed papers that have themselves been cited), including 75 papers in Astronomy and Astrophysics, 29 papers in Nuclear and High Energy Physics and 11 papers in Instrumentation. Recurrent topics in S. Paltani's work include Galaxies: Formation, Evolution, Phenomena (51 papers), Astrophysical Phenomena and Observations (51 papers) and Astrophysics and Cosmic Phenomena (27 papers). S. Paltani is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (51 papers), Astrophysical Phenomena and Observations (51 papers) and Astrophysics and Cosmic Phenomena (27 papers). S. Paltani collaborates with scholars based in Switzerland, France and United States. S. Paltani's co-authors include D. Eckert, S. Molendi, Cláudio Ricci, S. Ettori, T. J.-L. Courvoisier, R. Walter, J. S. Kaastra, Pierre-Olivier Petrucci, M. Mehdipour and G. A. Kriss and has published in prestigious journals such as Nature, Journal of the American Statistical Association and The Astrophysical Journal.

In The Last Decade

S. Paltani

81 papers receiving 1.7k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
S. Paltani Switzerland 24 1.8k 705 295 75 56 86 1.8k
Christopher A. Onken Australia 20 2.8k 1.6× 627 0.9× 619 2.1× 173 2.3× 27 0.5× 56 2.9k
F. J. Carrera Spain 31 2.9k 1.6× 1.0k 1.5× 546 1.9× 71 0.9× 23 0.4× 131 3.0k
G. Trinchieri Italy 30 2.8k 1.6× 880 1.2× 657 2.2× 62 0.8× 21 0.4× 127 2.8k
P. Lira Chile 35 3.2k 1.8× 760 1.1× 808 2.7× 130 1.7× 31 0.6× 99 3.2k
S. C. Gallagher United States 28 2.9k 1.6× 718 1.0× 701 2.4× 64 0.9× 36 0.6× 98 3.0k
Tinggui Wang China 26 2.1k 1.2× 636 0.9× 335 1.1× 36 0.5× 14 0.3× 116 2.1k
Marc Rafelski United States 25 1.7k 1.0× 319 0.5× 613 2.1× 59 0.8× 21 0.4× 91 1.8k
P. Marziani Italy 27 2.7k 1.5× 755 1.1× 645 2.2× 76 1.0× 15 0.3× 156 2.8k
X. Barcons Spain 28 2.5k 1.4× 1.0k 1.5× 375 1.3× 86 1.1× 11 0.2× 119 2.6k
M. G. Watson United Kingdom 23 1.9k 1.1× 606 0.9× 331 1.1× 46 0.6× 15 0.3× 66 2.0k

Countries citing papers authored by S. Paltani

Since Specialization
Citations

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

Fields of papers citing papers by S. Paltani

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of S. Paltani

This figure shows the co-authorship network connecting the top 25 collaborators of S. Paltani. A scholar is included among the top collaborators of S. Paltani 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 S. Paltani. S. Paltani 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.
Mïller, J. M., Ehud Behar, Rozenn Boissay-Malaquin, et al.. (2025). XRISM Spectroscopy of Accretion-driven Wind Feedback in NGC 4151. The Astrophysical Journal Letters. 988(2). L54–L54. 2 indexed citations
2.
Asada, Yoshihisa, G. Desprez, Chris J. Willott, et al.. (2025). Improving Photometric Redshifts of Epoch of Reionization Galaxies: A New Empirical Transmission Curve with Neutral Hydrogen Damping Wing Lyα Absorption. The Astrophysical Journal Letters. 983(1). L2–L2. 7 indexed citations
3.
Ruiz, A., I. Georgantopoulos, Fabio Vito, et al.. (2024). Active galactic nucleus X-ray luminosity function and absorption function in the Early Universe (3 ≤ z ≤ 6). Astronomy and Astrophysics. 685. A97–A97. 12 indexed citations
4.
Bozzo, E., David P. Huenemoerder, M. Falanga, et al.. (2024). Chandra/HETG Doppler velocity measurements in stellar coronal sources. Monthly Notices of the Royal Astronomical Society. 528(3). 4591–4622. 1 indexed citations
5.
Chen, Chien‐Ting, W. N. Brandt, Elias Kammoun, et al.. (2023). NuSTAR Observations of a Heavily X-Ray-obscured AGN in the Dwarf Galaxy J144013+024744. The Astrophysical Journal. 942(2). 82–82. 2 indexed citations
6.
Georgantopoulos, I., A. Ruiz, R. Gilli, et al.. (2021). XXL-HSC: An updated catalogue of high-redshift (z ≥ 3.5) X-ray AGN in the XMM-XXL northern field. Astronomy and Astrophysics. 658. A175–A175. 8 indexed citations
7.
Fotopoulou, S. & S. Paltani. (2018). CPz: Classification-aided photometric-redshift estimation. Springer Link (Chiba Institute of Technology). 26 indexed citations
8.
Lubiński, P., A. A. Zdziarski, R. Walter, et al.. (2017). Extreme flux states of NGC 4151 observed with INTEGRAL. reroDoc Digital Library. 12 indexed citations
9.
Ranalli, P., E. Koulouridis, I. Georgantopoulos, et al.. (2016). The 2–10 keV unabsorbed luminosity function of AGN from the LSS, CDFS, and COSMOS surveys. Springer Link (Chiba Institute of Technology). 15 indexed citations
10.
Masters, Daniel, P. Capak, Daniel Stern, et al.. (2015). MAPPING THE GALAXY COLOR–REDSHIFT RELATION: OPTIMAL PHOTOMETRIC REDSHIFT CALIBRATION STRATEGIES FOR COSMOLOGY SURVEYS. The Astrophysical Journal. 813(1). 53–53. 91 indexed citations
11.
Arav, Nahum, B. Borguet, G. A. Kriss, et al.. (2012). Multiwavelength campaign on Mrk 509. Astronomy and Astrophysics. 544. A33–A33. 20 indexed citations
12.
Ricci, Cláudio, R. Walter, T. J.-L. Courvoisier, & S. Paltani. (2011). Reflection in Seyfert galaxies and the unified model of AGN. Springer Link (Chiba Institute of Technology). 68 indexed citations
13.
Eckert, D., et al.. (2010). Hard X-ray Emission of Intermediate polars. ASEP. 435. 311. 1 indexed citations
14.
Fèvre, O. Le, L. Hill, D. Le Mignant, et al.. (2010). OPTIMOS-DIORAMAS: A Wide-field Imaging and Multi-slit Spectrograph for the E-ELT. Msngr. 140. 34–35. 1 indexed citations
15.
Soldi, S., M. Türler, S. Paltani, et al.. (2008). The multiwavelength variability of 3C 273. Springer Link (Chiba Institute of Technology). 66 indexed citations
16.
Paltani, S., et al.. (2008). A deep INTEGRAL hard X-ray survey of the 3C 273/Coma region. Springer Link (Chiba Institute of Technology). 15 indexed citations
17.
Walter, R., D. Eckert, I. Kreykenbohm, et al.. (2006). IGR J17497-2821: further observations with Swift and INTEGRAL. The astronomer's telegram. 889. 1. 1 indexed citations
18.
Courvoisier, T. J.-L., et al.. (2005). AGN variability time scales and the discrete-event model. Springer Link (Chiba Institute of Technology). 10 indexed citations
19.
Paltani, S. & M. Türler. (2002). Dynamics of the Lyα and Civ emitting gas in 3C 273. 14 indexed citations
20.
Courvoisier, T. J.-L., S. Paltani, & W. Wamsteker. (1992). International Ultraviolet Explorer--Uniform Low Dispersion Archive : active galactic nuclei. 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.

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