The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where Vincenzo Mainieri sits on this spectrum.
This scientist: 486 publications — 54th percentile
54% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Vincenzo Mainieri sits on this spectrum.
This scientist: 136 D-Index — 88th percentile
88% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
Vincenzo Mainieri is affiliated with the European Southern Observatory in Germany and has a significant presence in the field of Physics and Astronomy, contributing extensively to Astronomy and Astrophysics. Their work encompasses an array of topics including galaxies formation, evolution, and phenomena; astrophysical phenomena and observations; astrophysics and star formation studies; and gamma-ray bursts and supernovae.
Mainieri has published scholarly articles primarily in several venues known for astrophysical research. These include:
Their research interests branch into subfields such as instrumentation, nuclear and high energy physics, and atomic and molecular physics alongside the dominant focus in astronomy and astrophysics.
Among recent papers associated with Mainieri's research are:
Their collaborative network features frequent co-authors such as C. M. Harrison, Darshan Kakkad, Chiara Circosta, Nadia L. Zakamska, and A. Marconi, highlighting a pattern of sustained partnerships in the field.
Mainieri's academic contributions are mainly concentrated in research on galaxies and cosmic phenomena, with publications examining the intricacies of AGN feedback, molecular gas content in galaxies, and quasar outflows. These topics reflect a broader engagement with astrophysical phenomena and cosmic star formation processes.
Y. Peng;S. J. Lilly;K. Kovac;M. Bolzonella
Ying-jie Peng;Simon J. Lilly;Katarina Kovač;Micol Bolzonella
S.J. Lilly;O. Le Fevre;A. Renzini;G. Zamorani
O. Ilbert;P. Capak;M. Salvato;H. Aussel
S. J. Lilly;O. Le Fèvre;A. Renzini;G. Zamorani
Joel Vernet;H. Dekker;S. D'Odorico;L. Kaper
P. Rosati;P. Tozzi;R. Giacconi;R. Gilli
Riccardo Giacconi;Riccardo Giacconi;Andrew Zirm;JunXian Wang;Piero Rosati
G. P. Szokoly;J. Bergeron;G. Hasinger;I. Lehmann
Simon J. Lilly;Vincent Le Brun;Christian Maier;Vincenzo Mainieri
Yongquan Xue;Bin Luo;William Nielsen Brandt;Franz E. Bauer;Franz E. Bauer
L. Pozzetti;M. Bolzonella;E. Zucca;G. Zamorani
M. Moresco;A. Cimatti;R. Jimenez;L. Pozzetti
P. Padovani;D. M. Alexander;R. J. Assef;B. De Marco
P. Tozzi;R. Gilli;V. Mainieri;C. Norman
Martin Elvis;Francesca Civano;Cristian Vignali;Simonetta Puccetti
P. Popesso;M. Dickinson;M. Nonino;E. Vanzella;E. Vanzella
C. Gruppioni;F. Pozzi;G. Rodighiero;I. Delvecchio
M. Brusa;F. Civano;A. Comastri;T. Miyaji
F. Fiore;C. Feruglio;F. Shankar;M. Bischetti
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