A. Nastasi

3.2k total citations
16 papers, 265 citations indexed

About

A. Nastasi is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, A. Nastasi has authored 16 papers receiving a total of 265 indexed citations (citations by other indexed papers that have themselves been cited), including 16 papers in Astronomy and Astrophysics, 9 papers in Instrumentation and 3 papers in Nuclear and High Energy Physics. Recurrent topics in A. Nastasi's work include Galaxies: Formation, Evolution, Phenomena (16 papers), Astrophysical Phenomena and Observations (14 papers) and Astronomy and Astrophysical Research (9 papers). A. Nastasi is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (16 papers), Astrophysical Phenomena and Observations (14 papers) and Astronomy and Astrophysical Research (9 papers). A. Nastasi collaborates with scholars based in Germany, Chile and Spain. A. Nastasi's co-authors include R. Fassbender, Joana Santos, P. Rosati, A. de Hoon, A. Schwope, R. Šuhada, H. Böhringer, D. Pierini, J. Kohnert and M. Mühlegger and has published in prestigious journals such as The Astrophysical Journal, Astronomy and Astrophysics and New Journal of Physics.

In The Last Decade

A. Nastasi

16 papers receiving 262 citations

Peers

Countries citing papers authored by A. Nastasi

Since Specialization

Citations

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

Fields of papers citing papers by A. Nastasi

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of A. Nastasi

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

All Works

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16 of 16 papers shown

#	Work	Indexed citations
1	CHANDRADEEP OBSERVATION OF XDCP J0044.0-2033, A MASSIVE GALAXY CLUSTER ATz> 1.5 2015 ·The Astrophysical Journal ·P. Tozzi, Joana Santos, M. James Jee, R. Fassbender, P. Rosati, A. Nastasi, W. Forman, B. Sartoris, S. Borgani, H. Boehringer, B. Altieri, G. W. Pratt, M. Nonino, C. Jones	25
2	Kinematic analysis of a sample of X-ray luminous distant galaxy clusters 2014 ·Astronomy and Astrophysics ·A. Nastasi, H. Böhringer, R. Fassbender, A. de Hoon, G. Lamer, J. J. Mohr, Nelson Padilla, G. W. Pratt, H. Quintana, P. Rosati, Joana Santos, A. Schwope, R. Šuhada, M. Verdugo	8
3	The reversal of the SF–density relation in a massive, X-ray-selected galaxy cluster at z = 1.58: results from Herschel 2014 ·Monthly Notices of the Royal Astronomical Society Letters ·Joana Santos, B. Altieri, I. Valtchanov, A. Nastasi, H. Böhringer, G. Cresci, D. Elbaz, R. Fassbender, P. Rosati, P. Tozzi, M. Verdugo	41
4	F-VIPGI: a new adapted version of VIPGI for FORS2 spectroscopy. Application to a sample of 16 X-ray selected galaxy clusters at 0.6 < z < 1.2 2013 ·arXiv (Cornell University) ·A. Nastasi, M. Scodeggio, R. Fassbender, H. Böhringer, D. Pierini, M. Verdugo, B. Garilli, P. Franzetti	2
5	Distant clusters of galaxies in a deep XMM‐Newton observation 2013 ·Astronomische Nachrichten ·A. de Hoon, G. Lamer, A. Schwope, M. Mühlegger, R. Fassbender, H. Böhringer, M. Lerchster, A. Nastasi, R. Šuhada, P. Rosati, D. Pierini, Joana Santos, H. Quintana	1
6	F-VIPGI: a new adapted version of VIPGI for FORS2 spectroscopy 2012 ·Astronomy and Astrophysics ·A. Nastasi, M. Scodeggio, R. Fassbender, H. Böhringer, D. Pierini, M. Verdugo, B. Garilli, P. Franzetti	3
7	Distant galaxy clusters in a deepXMM-Newtonfield within the CFTHLS D4 2012 ·Astronomy and Astrophysics ·A. de Hoon, G. Lamer, A. Schwope, M. Mühlegger, R. Fassbender, H. Böhringer, M. Lerchster, A. Nastasi, R. Šuhada, M. Verdugo, J. P. Dietrich, F. Brimioulle, P. Rosati, D. Pierini, Joana Santos, H. Quintana, (unknown), A. Takey	5
8	Discovery of the X-ray selected galaxy cluster XMMU J0338.8+0021 atz= 1.49 2011 ·Astronomy and Astrophysics ·A. Nastasi, R. Fassbender, H. Böhringer, R. Šuhada, P. Rosati, D. Pierini, M. Verdugo, Joana Santos, A. Schwope, A. de Hoon, J. Kohnert, G. Lamer, M. Mühlegger, H. Quintana	11
9	Exploring the galaxy cluster-group transition regime at high redshifts 2011 ·Astronomy and Astrophysics ·R. Šuhada, R. Fassbender, A. Nastasi, H. Böhringer, A. de Hoon, D. Pierini, Joana Santos, P. Rosati, M. Mühlegger, H. Quintana, A. Schwope, G. Lamer, J. Kohnert, G. W. Pratt	4
10	The X-ray luminous galaxy cluster XMMU J1007.4+1237 atz= 1.56 2011 ·Astronomy and Astrophysics ·R. Fassbender, A. Nastasi, H. Böhringer, R. Šuhada, Joana Santos, P. Rosati, D. Pierini, M. Mühlegger, H. Quintana, A. Schwope, G. Lamer, A. de Hoon, J. Kohnert, G. W. Pratt, J. J. Mohr	44
11	Exploring the galaxy cluster-group transition regime at high redshifts: Physical properties of two newly detected z > 1 systems 2011 ·MPG.PuRe (Max Planck Society) ·R. Šuhada, R. Fassbender, A. Nastasi, H. Böhringer, A. de Hoon, D. Pierini, Joana Santos, P. Rosati, M. Mühlegger, H. Quintana, A. Schwope, G. Lamer, J. Kohnert, G. W. Pratt	3
12	The X-ray luminous galaxy cluster XMMU J1007.4+1237 at z=1.56 - The dawn of starburst activity in cluster cores 2011 ·arXiv (Cornell University) ·R. Fassbender, A. Nastasi, H. Böhringer, R. Šuhada, Joana Santos, P. Rosati, D. Pierini, M. Mühlegger, H. Quintana, A. Schwope, G. Lamer, A. de Hoon, J. Kohnert, G. W. Pratt, J. J. Mohr	35
13	The x-ray luminous galaxy cluster population at 0.9 <z≲ 1.6 as revealed by the XMM-NewtonDistant Cluster Project 2011 ·New Journal of Physics ·R. Fassbender, H. Böhringer, A. Nastasi, R. Šuhada, M. Mühlegger, A. de Hoon, J. Kohnert, G. Lamer, J. J. Mohr, D. Pierini, G. W. Pratt, H. Quintana, P. Rosati, Joana Santos, A. Schwope	52
14	Discovery of the X-ray selected galaxy cluster XMMU J0338.8+0021 at z = 1.49 - indications of a young system with a brightest galaxy in formation 2011 ·Americanae (AECID Library) ·A. Nastasi, R. Fassbender, H. Böhringer, R. Šuhada, P. Rosati, D. Pierini, M. Verdugo, Joana Santos, A. Schwope, A. de Hoon, J. Kohnert, G. Lamer, M. Mühlegger, H. Quintana	9
15	A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 atz= 0.975 2010 ·Astronomy and Astrophysics ·R. Fassbender, H. Böhringer, Joana Santos, G. W. Pratt, R. Šuhada, J. Kohnert, M. Lerchster, E. Rovilos, D. Pierini, G. Chon, A. Schwope, G. Lamer, M. Mühlegger, P. Rosati, H. Quintana, A. Nastasi, A. de Hoon, S. Seitz, J. J. Mohr	11
16	A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 at z=0.975 - Observing the assembly of a massive system 2010 ·arXiv (Cornell University) ·R. Fassbender, H. Böhringer, Joana Santos, G. W. Pratt, R. Šuhada, J. Kohnert, M. Lerchster, E. Rovilos, D. Pierini, G. Chon, A. Schwope, G. Lamer, M. Mühlegger, P. Rosati, H. Quintana, A. Nastasi, A. de Hoon, S. Seitz, J. J. Mohr	11

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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