M. Polletta

9.2k total citations
41 papers, 1.5k citations indexed

About

M. Polletta is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, M. Polletta has authored 41 papers receiving a total of 1.5k indexed citations (citations by other indexed papers that have themselves been cited), including 40 papers in Astronomy and Astrophysics, 22 papers in Instrumentation and 5 papers in Nuclear and High Energy Physics. Recurrent topics in M. Polletta's work include Galaxies: Formation, Evolution, Phenomena (35 papers), Astronomy and Astrophysical Research (22 papers) and Astrophysics and Star Formation Studies (16 papers). M. Polletta is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (35 papers), Astronomy and Astrophysical Research (22 papers) and Astrophysics and Star Formation Studies (16 papers). M. Polletta collaborates with scholars based in United States, Italy and France. M. Polletta's co-authors include Carol J. Lonsdale, H. E. Smith, D. Farrah, S. F. Hönig, D. L. Shupe, J. Surace, Seb Oliver, M. Rowan-Robinson, P. Gandhi and A. Smette and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

M. Polletta

37 papers receiving 1.4k 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. Polletta United States 22 1.4k 535 281 48 29 41 1.5k
K. E. K. Coppin United Kingdom 24 1.5k 1.1× 708 1.3× 256 0.9× 21 0.4× 43 1.5× 44 1.6k
Elena Malanushenko United States 16 1.6k 1.1× 558 1.0× 314 1.1× 25 0.5× 41 1.4× 17 1.6k
N. Bourne United Kingdom 21 1.0k 0.7× 432 0.8× 203 0.7× 22 0.5× 41 1.4× 31 1.1k
B. Magnelli Germany 21 1.3k 0.9× 560 1.0× 243 0.9× 18 0.4× 29 1.0× 50 1.3k
S. Berta Italy 27 1.8k 1.3× 835 1.6× 329 1.2× 44 0.9× 44 1.5× 52 1.8k
Y. Roehlly France 12 1.2k 0.8× 540 1.0× 156 0.6× 43 0.9× 47 1.6× 17 1.2k
F. Durret France 22 1.4k 1.0× 575 1.1× 236 0.8× 66 1.4× 37 1.3× 85 1.4k
R. J. Tuffs Germany 19 1.0k 0.7× 290 0.5× 231 0.8× 43 0.9× 21 0.7× 36 1.1k
Marc S. Seigar United States 17 974 0.7× 465 0.9× 108 0.4× 53 1.1× 38 1.3× 37 1000
R. K. Cochrane United Kingdom 17 1.0k 0.7× 505 0.9× 210 0.7× 41 0.9× 17 0.6× 40 1.1k

Countries citing papers authored by M. Polletta

Since Specialization
Citations

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

Fields of papers citing papers by M. Polletta

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of M. Polletta. A scholar is included among the top collaborators of M. Polletta 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. Polletta. M. Polletta 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.
Li, Qiong, Christopher J. Conselice, Florian Sarron, et al.. (2025). EPOCHS paper – X. Environmental effects on Galaxy formation and protocluster Galaxy candidates at 4.5 < z < 10 from JWST observations. Monthly Notices of the Royal Astronomical Society. 539(2). 1796–1819. 3 indexed citations
2.
Hill, Ryley, M. Polletta, M. Béthermin, et al.. (2025). An ALMA spectroscopic survey of the Planck high-redshift object PLCK G073.4−57.5 confirms two protoclusters. Astronomy and Astrophysics. 698. A204–A204.
3.
Demarco, R., et al.. (2023). The AGN fraction in high-redshift protocluster candidates selected by Planck and Herschel. Monthly Notices of the Royal Astronomical Society. 527(2). 3006–3017. 4 indexed citations
4.
Polletta, M., et al.. (2022). Molecular gas properties of Planck-selected protocluster candidates at z ≃ 1.3–3. Astronomy and Astrophysics. 662. A85–A85. 6 indexed citations
5.
Aghanim, N., et al.. (2022). Questioning Planck-selected star-forming high-redshift galaxy protoclusters and their fate. Astronomy and Astrophysics. 664. A155–A155. 7 indexed citations
6.
Vietri, G., B. Garilli, M. Polletta, et al.. (2021). The Type II AGN-host galaxy connection. Astronomy and Astrophysics. 659. A129–A129. 18 indexed citations
7.
Polletta, M., G. Soucail, H. Dole, et al.. (2021). Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z = 2.16 in the Cosmos field. Astronomy and Astrophysics. 654. A121–A121. 29 indexed citations
8.
Rettura, A., H. Dole, M. D. Lehnert, et al.. (2018). Spitzer Planck Herschel Infrared Cluster (SPHerIC) survey: Candidate galaxy clusters at 1.3 < z < 3 selected by high star-formation rate. Astronomy and Astrophysics. 620. A198–A198. 18 indexed citations
9.
Polletta, M., N. P. H. Nesvadba, R. Neri, et al.. (2011). Disk, merger, or outflow? Molecular gas kinematics in two powerful obscured QSOs atz ≥ 3.4. Astronomy and Astrophysics. 533. A20–A20. 25 indexed citations
10.
Fiolet, N., A. Omont, G. Lagache, et al.. (2010). Mid-infrared spectroscopy ofSpitzer-selected ultra-luminous starbursts atz  ~ 2. Astronomy and Astrophysics. 524. A33–A33. 17 indexed citations
11.
Oliver, Seb, D. Farrah, E. González-Solares, et al.. (2010). Specific star formation and the relation to stellar mass from 0 <z< 2 as seen in the far-infrared at 70 and 160μm. Monthly Notices of the Royal Astronomical Society. 71 indexed citations
12.
Hönig, S. F., P. Gandhi, A. Smette, et al.. (2010). The dusty heart of nearby active galaxies. Astronomy and Astrophysics. 515. A23–A23. 104 indexed citations
13.
Polletta, M., A. Omont, S. Berta, et al.. (2008). Obscured and powerful AGN and starburst activities atz ~ 3.5. Astronomy and Astrophysics. 492(1). 81–92. 17 indexed citations
14.
Siana, Brian, M. Polletta, H. E. Smith, et al.. (2008). High‐Redshift QSOs in the SWIRE Survey and thez∼3 QSO Luminosity Function. The Astrophysical Journal. 675(1). 49–70. 44 indexed citations
15.
Berta, S., Carol J. Lonsdale, Brian Siana, et al.. (2007). Keck spectroscopy ofz= 1–3 ULIRGs from the Spitzer SWIRE survey. Astronomy and Astrophysics. 467(2). 565–584. 13 indexed citations
16.
Tajer, M., M. Polletta, L. Chiappetti, et al.. (2007). Obscured and unobscured AGN populations in a hard-X-ray selected sample of the XMDS survey. Astronomy and Astrophysics. 467(1). 73–91. 25 indexed citations
17.
Pozzi, F., M. Polletta, A. Afonso-Luis, et al.. (2006). Optical and infrared diagnostics of SDSS galaxies in the SWIRE survey. Sussex Research Online (University of Sussex). 16 indexed citations
18.
Polletta, M., B. J. Wilkes, Brian Siana, et al.. (2006). The Most Obscured AGN in the Chandra/SWIRE Survey in the Lockman Hole. ESASP. 604. 807.
19.
Farrah, D., Carol J. Lonsdale, Colin Borys, et al.. (2006). The Spatial Clustering of Ultraluminous Infrared Galaxies over 1.5 < z < 3. The Astrophysical Journal. 641(1). L17–L20. 47 indexed citations
20.
Polletta, M., Carol J. Lonsdale, C. K. Xu, & B. J. Wilkes. (2003). X‐Ray counts and contribution to the X‐ray background of an IR population of starburst and active galaxies. Astronomische Nachrichten. 324(1-2). 170–170.

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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