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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 83 2805 2667 1378 1284 328 18452

Ilaria Pascucci publications per year

The chart shows the history of publications by Ilaria Pascucci between 2001 and 2026, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Ilaria Pascucci published across 26 years, from 2001 to 2026, averaging 15.4 papers a year. Output peaked at 39 publications in 2025. 41 of the 400 publications appeared in the last two years.

No. of publications
10 20 30
Bar chart. Horizontal axis: year, 2001 to 2026. Vertical axis: number of publications, 0 to 39. Peak 39 publications in 2025. 2001: 1 publication 2002: 4 publications 2003: 10 publications 2004: 12 publications 2005: 11 publications 2006: 9 publications 2007: 12 publications 2008: 9 publications 2009: 17 publications 2010: 16 publications 2011: 21 publications 2012: 18 publications 2013: 28 publications 2014: 14 publications 2015: 10 publications 2016: 8 publications 2017: 21 publications 2018: 22 publications 2019: 23 publications 2020: 15 publications 2021: 19 publications 2022: 13 publications 2023: 29 publications 2024: 17 publications 2025: 39 publications 2026: 2 publications
2001 2026

400 publications in total across all disciplines

View publications per year as a table
Ilaria Pascucci: publications per year, 2001 to 2026
Year Publications
2001 1
2002 4
2003 10
2004 12
2005 11
2006 9
2007 12
2008 9
2009 17
2010 16
2011 21
2012 18
2013 28
2014 14
2015 10
2016 8
2017 21
2018 22
2019 23
2020 15
2021 19
2022 13
2023 29
2024 17
2025 39
2026 2
Total 400
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Ilaria Pascucci 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 Ilaria Pascucci 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, 323–342 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: 328 publications — 23rd percentile

23% 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
183–202 53
203–222 81
223–242 85
243–262 112
263–282 114
283–302 126
303–322 136
323–342 162 328
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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Ilaria Pascucci 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 Ilaria Pascucci 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, 82–83 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: 83 D-Index — 26th percentile

26% 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
78–79 144
80–81 167
82–83 167 83
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

Ilaria Pascucci is affiliated with the University of Arizona in the United States. Their research primarily focuses on the field of Physics and Astronomy, with a substantial body of work related to Astronomy and Astrophysics.

Their main areas of study include:

  • Astronomy and Astrophysics
  • Spectroscopy
  • Instrumentation
  • Aerospace Engineering
  • Atmospheric Science

The primary topics covered in Pascucci's research are:

  • Astrophysics and Star Formation Studies
  • Stellar, planetary, and galactic studies
  • Astro and Planetary Science
  • Molecular Spectroscopy and Structure
  • Astronomy and Astrophysical Research
  • Atmospheric Ozone and Climate
  • Spectroscopy and Laser Applications

Pascucci has published extensively, with a significant presence in the following venues:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • The Astronomical Journal
  • Astronomy and Astrophysics
  • The Astrophysical Journal Letters

Among recent publications, notable papers include:

  • "The Evolution of Dust Disk Sizes from a Homogeneous Analysis of 1-10 Myr old Stars" (2020) published in The Astrophysical Journal
  • "X-shooter survey of disk accretion in Upper Scorpius" (2020) published in Astronomy and Astrophysics
  • "JWST Reveals Excess Cool Water near the Snow Line in Compact Disks, Consistent with Pebble Drift" (2023) published in The Astrophysical Journal Letters
  • "The protoplanetary disk population in the ρ-Ophiuchi region L1688 and the time evolution of Class II YSOs" (2022) published in Astronomy and Astrophysics
  • "Pebble-driven planet formation around very low-mass stars and brown dwarfs" (2020) published by Springer Link (Chiba Institute of Technology)

The scientist frequently collaborates with colleagues including:

  • Paola Pinilla
  • Dingshan Deng
  • Gijs D. Mulders
  • Andrea Banzatti
  • Feng Long

Best Publications

  • A Steeper than Linear Disk Mass-Stellar Mass Scaling Relation

    I. Pascucci;L. Testi;G. J. Herczeg;F. Long

  • Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region

    Feng Long;Paola Pinilla;Gregory J. Herczeg;Daniel Harsono

  • A steeper than linear disk mass-stellar mass scaling relation

    Ilaria Pascucci;L. Testi;L. Testi;Gregory J. Herczeg;F. Long

  • The Complete Census of 70-um-Bright Debris Disks within the FEPS (Formation and Evolution of Planetary Systems) Spitzer Legacy Survey of Sun-like Stars

    Lynne A. Hillenbrand;John M. Carpenter;Jinyoung Serena Kim;Michael R. Meyer

  • The dispersal of planet-forming discs: theory confronts observations

    Barbara Ercolano;Ilaria Pascucci

  • Formation and Evolution of Planetary Systems (FEPS): Properties of Debris Dust around Solar-type Stars

    John M. Carpenter;Jeroen Bouwman;Eric E. Mamajek;Michael R. Meyer

  • A STELLAR-MASS-DEPENDENT DROP IN PLANET OCCURRENCE RATES

    Gijs D. Mulders;Ilaria Pascucci;Dániel Apai

  • The complete census of 70 μm-bright debris disks within "the formation and evolution of planetary systems" Spitzer legacy survey of sun-like stars

    Lynne A. Hillenbrand;John M. Carpenter;Jinyoung Serena Kim;Michael R. Meyer

  • AN INCREASE in the MASS of PLANETARY SYSTEMS AROUND LOWER-MASS STARS

    Gijs D. Mulders;Ilaria Pascucci;Dániel Apai

  • The Onset of Planet Formation in Brown Dwarf Disks

    Dániel Apai;Dániel Apai;Ilaria Pascucci;Jeroen Bouwman;Antonella Natta

  • The Formation and Evolution of Planetary Systems: Grain Growth and Chemical Processing of Dust in T Tauri Systems

    J. Bouwman;Th. Henning;L. A. Hillenbrand;M. R. Meyer

  • Compact Disks in a High-resolution ALMA Survey of Dust Structures in the Taurus Molecular Cloud

    Feng Long;Gregory J. Herczeg;Daniel Harsono;Paola Pinilla;Paola Pinilla

  • Tracing Slow Winds from T Tauri Stars via Low Velocity Forbidden Line Emission

    M. N. Simon;I. Pascucci;Suzan Edwards;W. Feng

  • FORMATION AND EVOLUTION OF PLANETARY SYSTEMS: PROPERTIES OF DEBRIS DUST AROUND SOLAR-TYPE STARS

    John M. Carpenter;Jeroen Bouwman;Eric E. Mamajek;Michael R. Meyer

  • Emission Lines from the Gas Disk around TW Hydra and the Origin of the Inner Hole

    U. Gorti;U. Gorti;D. Hollenbach;J. Najita;I. Pascucci

  • DISK IMAGING SURVEY OF CHEMISTRY WITH SMA. II. SOUTHERN SKY PROTOPLANETARY DISK DATA AND FULL SAMPLE STATISTICS

    Karin I. Öberg;Chunhua Qi;Jeffrey K. J. Fogel;Edwin A. Bergin

  • THE DIFFERENT EVOLUTION OF GAS AND DUST IN DISKS AROUND SUN-LIKE AND COOL STARS

    I. Pascucci;D. Apai;K. Luhman;Th. Henning

  • Formation and Evolution of Planetary Systems: Upper Limits to the Gas Mass in Disks around Sun-like Stars

    I. Pascucci;U. Gorti;D. Hollenbach;J. Najita

  • THE DISK IMAGING SURVEY OF CHEMISTRY WITH SMA. I. TAURUS PROTOPLANETARY DISK DATA

    Karin I. Öberg;Chunhua Qi;Jeffrey K. J. Fogel;Edwin A. Bergin

  • Protoplanetary Disk Properties in the Orion Nebula Cluster: Initial Results from Deep, High-resolution ALMA Observations

    J. A. Eisner;H. G. Arce;N. P. Ballering;J. Bally

Frequent Co-Authors

Daniel Apai
Daniel Apai University of Arizona
Gregory J. Herczeg
Gregory J. Herczeg Peking University
Jeroen Bouwman
Jeroen Bouwman Max Planck Society
Michael Meyer
Michael Meyer University of Michigan–Ann Arbor
Sean M. Andrews
Sean M. Andrews Harvard University
Lynne A. Hillenbrand
Lynne A. Hillenbrand California Institute of Technology
Sebastian Wolf
Sebastian Wolf Kiel University
John M. Carpenter
John M. Carpenter California Institute of Technology
Th. Henning
Th. Henning Max Planck Society
Giuseppe Lodato
Giuseppe Lodato University of Milan

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