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Maurilio Pannella

Maurilio Pannella

University of Trieste
Italy

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 77 3234 3075 174 171 179 22027

Maurilio Pannella publications per year

The chart shows the history of publications by Maurilio Pannella between 2002 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Maurilio Pannella published across 24 years, from 2002 to 2025, averaging 7.8 papers a year. Output peaked at 20 publications in 2018. 3 of the 187 publications appeared in the last two years.

No. of publications
5 10 15 20
Bar chart. Horizontal axis: year, 2002 to 2025. Vertical axis: number of publications, 0 to 20. Peak 20 publications in 2018. 2002: 5 publications 2003: 7 publications 2004: 5 publications 2005: 1 publication 2006: 5 publications 2007: 8 publications 2008: 3 publications 2009: 8 publications 2010: 11 publications 2011: 11 publications 2012: 13 publications 2013: 8 publications 2014: 9 publications 2015: 13 publications 2016: 11 publications 2017: 8 publications 2018: 20 publications 2019: 10 publications 2020: 7 publications 2021: 6 publications 2022: 14 publications 2023: 1 publication 2024: 1 publication 2025: 2 publications
2002 2025

187 publications in total across all disciplines

View publications per year as a table
Maurilio Pannella: publications per year, 2002 to 2025
Year Publications
2002 5
2003 7
2004 5
2005 1
2006 5
2007 8
2008 3
2009 8
2010 11
2011 11
2012 13
2013 8
2014 9
2015 13
2016 11
2017 8
2018 20
2019 10
2020 7
2021 6
2022 14
2023 1
2024 1
2025 2
Total 187
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Maurilio Pannella publication distribution in Physics in 2026

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 Maurilio Pannella sits on this spectrum.

No. of scientists
50 100 150
Bar chart with 70 bars. Horizontal axis: publications, 103–122 to 1,469+. Vertical axis: number of scientists, 0 to 162. Most scientists, 162, have 323–342 publications. The last bar groups every scientist with 1,469 publications or more. The highlighted bar, 163–182 publications, is where this scientist sits. 103–122 publications: 7 scientists 123–142 publications: 10 scientists 143–162 publications: 31 scientists 163–182 publications: 35 scientists 183–202 publications: 53 scientists 203–222 publications: 81 scientists 223–242 publications: 85 scientists 243–262 publications: 112 scientists 263–282 publications: 114 scientists 283–302 publications: 126 scientists 303–322 publications: 136 scientists 323–342 publications: 162 scientists 343–362 publications: 155 scientists 363–382 publications: 156 scientists 383–402 publications: 134 scientists 403–422 publications: 145 scientists 423–442 publications: 147 scientists 443–462 publications: 131 scientists 463–482 publications: 131 scientists 483–502 publications: 116 scientists 503–522 publications: 106 scientists 523–542 publications: 103 scientists 543–562 publications: 87 scientists 563–582 publications: 84 scientists 583–602 publications: 94 scientists 603–622 publications: 70 scientists 623–642 publications: 76 scientists 643–662 publications: 60 scientists 663–682 publications: 54 scientists 683–702 publications: 60 scientists 703–722 publications: 48 scientists 723–742 publications: 64 scientists 743–762 publications: 48 scientists 763–782 publications: 37 scientists 783–802 publications: 43 scientists 803–822 publications: 34 scientists 823–842 publications: 36 scientists 843–862 publications: 32 scientists 863–882 publications: 32 scientists 883–902 publications: 31 scientists 903–922 publications: 25 scientists 923–942 publications: 15 scientists 943–962 publications: 24 scientists 963–982 publications: 13 scientists 983–1,002 publications: 21 scientists 1,003–1,022 publications: 21 scientists 1,023–1,042 publications: 16 scientists 1,043–1,062 publications: 9 scientists 1,063–1,082 publications: 19 scientists 1,083–1,102 publications: 11 scientists 1,103–1,122 publications: 17 scientists 1,123–1,142 publications: 11 scientists 1,143–1,162 publications: 7 scientists 1,163–1,182 publications: 4 scientists 1,183–1,202 publications: 10 scientists 1,203–1,222 publications: 8 scientists 1,223–1,242 publications: 16 scientists 1,243–1,262 publications: 4 scientists 1,263–1,282 publications: 10 scientists 1,283–1,302 publications: 5 scientists 1,303–1,322 publications: 7 scientists 1,323–1,342 publications: 4 scientists 1,343–1,362 publications: 8 scientists 1,363–1,382 publications: 6 scientists 1,383–1,402 publications: 7 scientists 1,403–1,422 publications: 3 scientists 1,423–1,442 publications: 4 scientists 1,443–1,462 publications: 4 scientists 1,463–1,468 publications: 3 scientists 1,469+ publications: 100 scientists
103–122 publications 1,469+

This scientist: 179 publications — 2nd percentile

2% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

View publications distribution as a table
Number of Physics scientists by publication count, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
Publications Scientists This scientist
103–122 7
123–142 10
143–162 31
163–182 35 179
183–202 53
203–222 81
223–242 85
243–262 112
263–282 114
283–302 126
303–322 136
323–342 162
343–362 155
363–382 156
383–402 134
403–422 145
423–442 147
443–462 131
463–482 131
483–502 116
503–522 106
523–542 103
543–562 87
563–582 84
583–602 94
603–622 70
623–642 76
643–662 60
663–682 54
683–702 60
703–722 48
723–742 64
743–762 48
763–782 37
783–802 43
803–822 34
823–842 36
843–862 32
863–882 32
883–902 31
903–922 25
923–942 15
943–962 24
963–982 13
983–1,002 21
1,003–1,022 21
1,023–1,042 16
1,043–1,062 9
1,063–1,082 19
1,083–1,102 11
1,103–1,122 17
1,123–1,142 11
1,143–1,162 7
1,163–1,182 4
1,183–1,202 10
1,203–1,222 8
1,223–1,242 16
1,243–1,262 4
1,263–1,282 10
1,283–1,302 5
1,303–1,322 7
1,323–1,342 4
1,343–1,362 8
1,363–1,382 6
1,383–1,402 7
1,403–1,422 3
1,423–1,442 4
1,443–1,462 4
1,463–1,468 3
1,469+ 100
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Maurilio Pannella D-index placement in Physics in 2026

The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Maurilio Pannella sits on this spectrum.

No. of scientists
50 100 150
Bar chart with 59 bars. Horizontal axis: D-Index, 70–71 to 185+. Vertical axis: number of scientists, 0 to 167. Most scientists, 167, have 80–81 D-Index. The last bar groups every scientist with 185 D-Index or more. The highlighted bar, 76–77 D-Index, is where this scientist sits. 70–71 D-Index: 76 scientists 72–73 D-Index: 110 scientists 74–75 D-Index: 143 scientists 76–77 D-Index: 153 scientists 78–79 D-Index: 144 scientists 80–81 D-Index: 167 scientists 82–83 D-Index: 167 scientists 84–85 D-Index: 166 scientists 86–87 D-Index: 132 scientists 88–89 D-Index: 155 scientists 90–91 D-Index: 134 scientists 92–93 D-Index: 137 scientists 94–95 D-Index: 102 scientists 96–97 D-Index: 112 scientists 98–99 D-Index: 110 scientists 100–101 D-Index: 116 scientists 102–103 D-Index: 97 scientists 104–105 D-Index: 103 scientists 106–107 D-Index: 87 scientists 108–109 D-Index: 90 scientists 110–111 D-Index: 67 scientists 112–113 D-Index: 78 scientists 114–115 D-Index: 75 scientists 116–117 D-Index: 67 scientists 118–119 D-Index: 69 scientists 120–121 D-Index: 60 scientists 122–123 D-Index: 59 scientists 124–125 D-Index: 53 scientists 126–127 D-Index: 42 scientists 128–129 D-Index: 41 scientists 130–131 D-Index: 33 scientists 132–133 D-Index: 32 scientists 134–135 D-Index: 45 scientists 136–137 D-Index: 19 scientists 138–139 D-Index: 24 scientists 140–141 D-Index: 28 scientists 142–143 D-Index: 31 scientists 144–145 D-Index: 22 scientists 146–147 D-Index: 20 scientists 148–149 D-Index: 12 scientists 150–151 D-Index: 16 scientists 152–153 D-Index: 24 scientists 154–155 D-Index: 23 scientists 156–157 D-Index: 15 scientists 158–159 D-Index: 15 scientists 160–161 D-Index: 11 scientists 162–163 D-Index: 17 scientists 164–165 D-Index: 12 scientists 166–167 D-Index: 11 scientists 168–169 D-Index: 9 scientists 170–171 D-Index: 9 scientists 172–173 D-Index: 11 scientists 174–175 D-Index: 4 scientists 176–177 D-Index: 8 scientists 178–179 D-Index: 5 scientists 180–181 D-Index: 3 scientists 182–183 D-Index: 4 scientists 184 D-Index: 4 scientists 185+ D-Index: 99 scientists
70–71 D-Index 185+

This scientist: 77 D-Index — 13th percentile

13% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

View D-Index distribution as a table
Number of Physics scientists by D-index, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
D-Index Scientists This scientist
70–71 76
72–73 110
74–75 143
76–77 153 77
78–79 144
80–81 167
82–83 167
84–85 166
86–87 132
88–89 155
90–91 134
92–93 137
94–95 102
96–97 112
98–99 110
100–101 116
102–103 97
104–105 103
106–107 87
108–109 90
110–111 67
112–113 78
114–115 75
116–117 67
118–119 69
120–121 60
122–123 59
124–125 53
126–127 42
128–129 41
130–131 33
132–133 32
134–135 45
136–137 19
138–139 24
140–141 28
142–143 31
144–145 22
146–147 20
148–149 12
150–151 16
152–153 24
154–155 23
156–157 15
158–159 15
160–161 11
162–163 17
164–165 12
166–167 11
168–169 9
170–171 9
172–173 11
174–175 4
176–177 8
178–179 5
180–181 3
182–183 4
184 4
185+ 99
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Overview

Maurilio Pannella is affiliated with the University of Trieste in Italy and has contributed extensively to the field of Physics and Astronomy. Their research primarily focuses on Astronomy and Astrophysics, with significant work in instrumentation and nuclear and high energy physics.

The scientist's work spans several subfields, including:

  • Astronomy and Astrophysics
  • Instrumentation
  • Nuclear and High Energy Physics
  • Statistical and Nonlinear Physics
  • General Health Professions

Their research covers key topics such as:

  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Stellar, planetary, and galactic studies
  • Gamma-ray bursts and supernovae
  • Astrophysics and Cosmic Phenomena
  • Astrophysics and Star Formation Studies
  • Astrophysical Phenomena and Observations

Maurilio Pannella has published multiple papers in well-known venues, with frequent contributions in:

  • Astronomy and Astrophysics
  • arXiv (Cornell University)
  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal
  • Nature

Some recent publications include:

  • "The main sequence of star-forming galaxies across cosmic times," 2022, Monthly Notices of the Royal Astronomical Society
  • "The VANDELS ESO public spectroscopic survey," 2021, Astronomy and Astrophysics
  • "GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies," 2021, arXiv (Cornell University)
  • "Forming intracluster gas in a galaxy protocluster at a redshift of 2.16," 2023, Nature
  • "The 700 ks Chandra Spiderweb Field," 2022, Astronomy and Astrophysics

Frequent co-authors collaborating with Maurilio Pannella include:

  • D. Elbaz
  • S. Juneau
  • Casey Papovich
  • E. Daddi
  • A. Saro

Best Publications

  • GOODS-Herschel: an infrared main sequence for star-forming galaxies

    D.Elbaz;M.Dickinson;H.S.Hwang;T.Diaz-Santos

  • GOODS–Herschel: an infrared main sequence for star-forming galaxies

    D. Elbaz;M. Dickinson;H. S. Hwang;T. Díaz-Santos

  • The star formation history of mass-selected galaxies in the COSMOS field

    Alexander Karim;Eva Schinnerer;Alejo Martinez-Sansigre;Mark T. Sargent

  • The Star Formation History of Mass-selected Galaxies in the COSMOS Field

    A. Karim;A. Karim;E. Schinnerer;A. Martinez-Sansigre;A. Martinez-Sansigre;A. Martinez-Sansigre;M. T. Sargent

  • The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day

    Corentin Schreiber;M. Pannella;D. Elbaz;M. Béthermin

  • The Evolving Interstellar Medium of Star-forming Galaxies since z = 2 as Probed by Their Infrared Spectral Energy Distributions

    Georgios E. Magdis;E. Daddi;M. Béthermin;M. Sargent

  • Star formation and dust obscuration at z~2: galaxies at the dawn of downsizing

    M. Pannella;C.L. Carilli;E. Daddi;H.J. Mc Cracken

  • Star formation and dust obscuration at z≈2: galaxies at the dawn of downsizing

    M. Pannella;C. L. Carilli;E. Daddi;H. J. McCracken

  • The deepest Herschel-PACS far-infrared survey: number counts and infrared luminosity functions from combined PEP/GOODS-H observations

    B. Magnelli;P. Popesso;S. Berta;F. Pozzi

  • GOODS-Herschel: The far-infrared view of star formation in AGN host galaxies since z~3

    J. R. Mullaney;M. Pannella;E. Daddi;D. M. Alexander

  • The hidden "AGN main sequence": Evidence for a universal black hole accretion to star formation rate ratio since z~2 producing a M_BH-M* relation

    J. R. Mullaney;E. Daddi;M. Béthermin;D. Elbaz

  • GOODS-HERSCHEL: star formation, dust attenuation and the FIR-radio correlation on the Main Sequence of star-forming galaxies up to z~4

    Maurilio Pannella;David Elbaz;Emanuele Daddi;Mark E. Dickinson

  • Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation

    Matthieu Béthermin;Emanuele Daddi;Georgios Magdis;Claudia Lagos

  • The stellar mass function of galaxies to z ~ 5 in the Fors Deep and GOODS-S fields

    N. Drory;M. Salvato;A. Gabasch;R. Bender

  • A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies

    Matthieu Béthermin;Emanuele Daddi;Georgios Magdis;Mark T Sargent

  • GOODS-Herschel: The far-infrared view of star formation in active galactic nucleus host galaxies since z ≈ 3

    J. R. Mullaney;M. Pannella;Emanuele Daddi;D. M. Alexander

  • Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation

    Matthieu Béthermin;Emanuele Daddi;Georgios Magdis;Claudia Lagos

  • The Stellar Mass Function of Galaxies to z ~ 5 in the FORS Deep and GOODS-South Fields

    N. Drory;M. Salvato;A. Gabasch;R. Bender

  • THE HIDDEN “AGN MAIN SEQUENCE”: EVIDENCE FOR A UNIVERSAL BLACK HOLE ACCRETION TO STAR FORMATION RATE RATIO SINCE z ∼ 2 PRODUCING AN M BH-M * RELATION

    J. R. Mullaney;Emanuele Daddi;M. Béthermin;D. Elbaz

  • GOODS-Herschel~: Gas-to-dust mass ratios and CO-to-H_2 conversion factors in normal and starbursting galaxies at high-z

    Georgios E. Magdis;E. Daddi;E. Elbaz;M. Sargent

Frequent Co-Authors

Emanuele Daddi
Emanuele Daddi University of Paris-Saclay
David Elbaz
David Elbaz CEA Saclay
Vassilis Charmandaris
Vassilis Charmandaris University of Crete
Rob Ivison
Rob Ivison European Southern Observatory
Mark Dickinson
Mark Dickinson National Optical Astronomy Observatory
Douglas Scott
Douglas Scott University of British Columbia
Herve Aussel
Herve Aussel University of Paris-Saclay
Anton M. Koekemoer
Anton M. Koekemoer Space Telescope Science Institute
David M. Alexander
David M. Alexander Durham University
Henry C. Ferguson
Henry C. Ferguson Space Telescope Science Institute

External Links

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Best Scientists Citing Maurilio Pannella

Rob Ivison

Rob Ivison

European Southern Observatory

Publications: 325

Emanuele Daddi

Emanuele Daddi

University of Paris-Saclay

Publications: 219

Ian Smail

Ian Smail

Durham University

Publications: 182

Franz E. Bauer

Franz E. Bauer

Pontificia Universidad Católica de Chile

Publications: 178

Anton M. Koekemoer

Anton M. Koekemoer

Space Telescope Science Institute

Publications: 173

Peter Capak

Peter Capak

California Institute of Technology

Publications: 157

Fabian Walter

Fabian Walter

Max Planck Society

Publications: 152

Mara Salvato

Mara Salvato

Max Planck Society

Publications: 143

Dieter Lutz

Dieter Lutz

Max Planck Society

Publications: 137

Douglas Scott

Douglas Scott

University of British Columbia

Publications: 135

Duncan Farrah

Duncan Farrah

University of Hawaii at Manoa

Publications: 127

Alvio Renzini

Alvio Renzini

National Institute for Astrophysics

Publications: 127

Scott Chapman

Scott Chapman

Dalhousie University

Publications: 126

Asantha Cooray

Asantha Cooray

University of California, Irvine

Publications: 120

Mattia Vaccari

Mattia Vaccari

University of Cape Town

Publications: 117

Andrea Cimatti

Andrea Cimatti

University of Bologna

Publications: 114

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