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Physics

D-Index
81
Citations
23637
World Ranking
2934
National Ranking
6

Paola D'Alessio 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 Paola D'Alessio sits on this spectrum.

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 publications 1,469+

This scientist: 204 publications — 4th percentile

4% of scientists in this discipline score the same or lower.

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

Paola D'Alessio 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 Paola D'Alessio sits on this spectrum.

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 D-Index 185+

This scientist: 81 D-Index — 22nd percentile

22% of scientists in this discipline score the same or lower.

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

Overview

Paola D'Alessio was affiliated with the National Autonomous University of Mexico in Mexico. Their research contributions spanned the fields of Physics and Astronomy as well as Chemistry, with a focus on subfields including Astronomy and Astrophysics and Spectroscopy.

The main topics covered by D'Alessio's work included:

  • Astrophysics and Star Formation Studies
  • Stellar, planetary, and galactic studies
  • Molecular Spectroscopy and Structure

One of the documented research papers authored in collaboration featured the title "Testing the Potential for Radio Variability in Disks around T Tauri Stars with Observations and Chemical Modeling." This paper was published in 2022 in The Astrophysical Journal and had been cited by other researchers multiple times.

D'Alessio frequently worked with several co-authors, including:

  • Catherine Espaillat
  • Enrique Macías
  • John Wendeborn
  • R. Franco-Hernández
  • Nuria Calvet

Their work was published primarily in The Astrophysical Journal, highlighting a consistent contribution to that venue.

Best Publications

  • Accretion and the Evolution of T Tauri Disks

    Lee Hartmann;Nuria Calvet;Nuria Calvet;Erik Gullbring;Paola D'Alessio

  • Accretion Disks around Young Objects. I. The Detailed Vertical Structure

    Paola D'Alessio;Jorge Cantö;Nuria Calvet;Nuria Calvet;Susana Lizano

  • Evidence for a Developing Gap in a 10 Myr Old Protoplanetary Disk

    Nuria Calvet;Paola D’Alessio;Lee Hartmann;David Wilner

  • ACCRETION DISKS AROUND YOUNG OBJECTS. III. GRAIN GROWTH

    Paola D’Alessio;Paola D’Alessio;Nuria Calvet;Lee Hartmann

  • Accretion Disks around Young Objects. II. Tests of Well-mixed Models with ISM Dust

    Paola D’Alessio;Nuria Calvet;Lee Hartmann;Susana Lizano

  • Infrared Array Camera (IRAC) Colors of Young Stellar Objects

    Lori E. Allen;Nuria Calvet;Paola D’Alessio;Bruno Merin

  • A Survey and Analysis of Spitzer Infrared Spectrograph Spectra of T Tauri Stars in Taurus

    E. Furlan;L. Hartmann;N. Calvet;P. D'Alessio

  • Disks in Transition in the Taurus Population: Spitzer IRS Spectra of GM Aurigae and DM Tauri

    N. Calvet;P. D'Alessio;D. M. Watson;R. Franco-Hernández

  • Effects of dust growth and settling in t tauri disks

    Paola D’Alessio;Nuria Calvet;Lee Hartmann;Ramiro Franco-Hernández;Ramiro Franco-Hernández

  • On the Diversity of the Taurus Transitional Disks: UX Tau A & Lk Ca 15

    C. Espaillat;N. Calvet;P. D'Alessio;J. Hernandez

  • CSI 2264: SIMULTANEOUS OPTICAL AND INFRARED LIGHT CURVES OF YOUNG DISK-BEARING STARS IN NGC 2264 WITH CoRoT and SPITZER—EVIDENCE FOR MULTIPLE ORIGINS OF VARIABILITY*

    Ann Marie Cody;John Stauffer;Annie Baglin;Giuseppina Micela

  • Unveiling the Inner Disk Structure of T Tauri Stars

    James Muzerolle;Nuria Calvet;Lee Hartmann;Paola D'Alessio

  • IRAC OBSERVATIONS OF TAURUS PRE-MAIN-SEQUENCE STARS

    Lee Hartmann;S. T. Megeath;Lori Allen;Kevin Luhman

  • Imaging of the CO Snow Line in a Solar Nebula Analog

    Chunhua Qi;Karin I. Öberg;David J. Wilner;Paola D’Alessio

  • Irradiation of Accretion Disks around Young Objects. I. Near-Infrared CO Bands

    Nuria Calvet;Alberto Patino;Gladis C. Magris;Paola D'Alessio

  • Magnetospheres and Disk Accretion in Herbig Ae/Be Stars

    James Muzerolle;James Muzerolle;Paola D’Alessio;Nuria Calvet;Lee Hartmann

  • On the Diversity of the Taurus Transitional Disks: UX Tauri A and LkCa 15

    C. Espaillat;N. Calvet;P. D'Alessio;J. Hernández;J. Hernández

  • A ∼ 0.2-solar-mass protostar with a Keplerian disk in the very young L1527 IRS system

    John J. Tobin;Lee Hartmann;Hsin-Fang Chiang;Hsin-Fang Chiang;David J. Wilner

  • Disk evolution in Cep OB2: Results from the Spitzer space telescope

    Aurora Sicilia-Aguilar;Lee Hartmann;Nuria Calvet;S. T. Megeath

  • The Truncated Disk of CoKu Tau/4

    Paola D'Alessio;Lee Hartmann;Nuria Calvet;Ramiro Franco-Hernández

Frequent Co-Authors

Nuria Calvet
Nuria Calvet University of Michigan–Ann Arbor
Lee Hartmann
Lee Hartmann University of Michigan–Ann Arbor
Dan M. Watson
Dan M. Watson University of Rochester
Kevin Luhman
Kevin Luhman Pennsylvania State University
David J. Wilner
David J. Wilner Harvard University
Chunhua Qi
Chunhua Qi Harvard University
James Muzerolle
James Muzerolle Space Telescope Science Institute
Sean M. Andrews
Sean M. Andrews Harvard University
Paul T. P. Ho
Paul T. P. Ho Institute of Astronomy and Astrophysics, Academia Sinica
Bernhard R. Brandl
Bernhard R. Brandl Leiden University

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