World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
99
Citations
25018
World Ranking
1724
National Ranking
910

Dariusz C. Lis 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 Dariusz C. Lis 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: 519 publications — 59th percentile

59% of scientists in this discipline score the same or lower.

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

Dariusz C. Lis 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 Dariusz C. Lis 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: 99 D-Index — 55th percentile

55% of scientists in this discipline score the same or lower.

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

Overview

What is he best known for?

The fields of study he is best known for:

  • Astronomy
  • Astrophysics
  • Optics

His main research concerns Astrophysics, Astronomy, Line, Spectral line and Astrochemistry. Interstellar medium, Molecular cloud, Comet, Protostar and Caltech Submillimeter Observatory are the subjects of his Astrophysics studies. His work on Spectroscopy, Star formation, Galactic Center and Telescope as part of general Astronomy study is frequently connected to Flux, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them.

His research in Line intersects with topics in Stars, Beam, Excited state, Intensity and Mean kinetic temperature. His biological study deals with issues like Absorption spectroscopy, which deal with fields such as Local standard of rest. His Astrochemistry research is multidisciplinary, relying on both Ionization, Cosmic ray and Current.

His most cited work include:

  • Ocean-like water in the Jupiter-family comet 103P/Hartley 2 (338 citations)
  • Detection of the water reservoir in a forming planetary system (261 citations)
  • Deuterated Water in Comet C/1996 B2 (Hyakutake) and Its Implications for the Origin of Comets☆ (248 citations)

What are the main themes of his work throughout his whole career to date?

Dariusz C. Lis focuses on Astrophysics, Astronomy, Molecular cloud, Comet and Line. The study of Astrophysics is intertwined with the study of Spectral line in a number of ways. His Molecular cloud study integrates concerns from other disciplines, such as Line-of-sight and Continuum.

His studies examine the connections between Comet and genetics, as well as such issues in Solar System, with regards to Planet and Protoplanetary disk. Dariusz C. Lis has researched Line in several fields, including Envelope, Stars, Excitation, Mean kinetic temperature and Radiative transfer. His Astrochemistry research incorporates elements of Deuterium, Atomic physics and Spectroscopy.

He most often published in these fields:

  • Astrophysics (83.61%)
  • Astronomy (43.17%)
  • Molecular cloud (20.22%)

What were the highlights of his more recent work (between 2016-2021)?

  • Astrophysics (83.61%)
  • Line (22.04%)
  • Interstellar medium (21.49%)

In recent papers he was focusing on the following fields of study:

Dariusz C. Lis focuses on Astrophysics, Line, Interstellar medium, Star formation and Astronomy. Within one scientific family, Dariusz C. Lis focuses on topics pertaining to Spectral line under Astrophysics, and may sometimes address concerns connected to Submillimeter Array. His work in Line covers topics such as Photoevaporation which are related to areas like Planetary system.

Dariusz C. Lis interconnects Starburst region, Excitation and Emission spectrum in the investigation of issues within Interstellar medium. His Star formation research integrates issues from Telescope, Star, Extreme ultraviolet lithography and Magnetohydrodynamics. In his work, Interstellar cloud, Broadband, Noise and Caltech Submillimeter Observatory is strongly intertwined with Wavelength, which is a subfield of Astronomy.

Between 2016 and 2021, his most popular works were:

  • Survey of Cold Water Lines in Protoplanetary Disks: Indications of Systematic Volatile Depletion (53 citations)
  • Survey of Cold Water Lines in Protoplanetary Disks: Indications of Systematic Volatile Depletion (53 citations)
  • The CARMA-NRO Orion Survey (51 citations)

In his most recent research, the most cited papers focused on:

  • Astronomy
  • Astrophysics
  • Optics

His main research concerns Astrophysics, Line, Spectral line, Astrochemistry and Astronomy. His is doing research in Protostar, Star formation, Interstellar medium, Stars and Submillimeter Array, both of which are found in Astrophysics. His Interstellar medium study integrates concerns from other disciplines, such as Wavelength, Emission spectrum and Caltech Submillimeter Observatory.

His Line research is multidisciplinary, incorporating perspectives in Planetary system, Pluto and Stratopause, Atmosphere, Mesosphere. His research in Astrochemistry intersects with topics in Abundance, Noise, Mass ratio and Photoevaporation. His Astronomy research incorporates elements of Excitation and Broadband.

Best Publications

  • New molecules found in comet C/1995 O1 (Hale-Bopp) Investigating the link between cometary and interstellar material

    D. Bockelée-Morvan;D. C. Lis;J. E. Wink;D. Despois

  • Ocean-like water in the Jupiter-family comet 103P/Hartley 2

    Paul Hartogh;Dariusz C. Lis;Dominique Bockelée-Morvan;Miguel de Val-Borro

  • Deuterated Water in Comet C/1996 B2 (Hyakutake) and Its Implications for the Origin of Comets☆

    D. Bockelee-Morvan;D. Gautier;D. C. Lis;K. Young

  • Detection of the water reservoir in a forming planetary system

    Michiel R. Hogerheijde;Edwin A. Bergin;Christian Brinch;L. Ilsedore Cleeves

  • Water in star-forming regions with the Herschel Space Observatory (WISH). I. Overview of key program and first results

    E. F. van Dishoeck;L. E. Kristensen;A. O. Benz;E. A. Bergin

  • A Line Survey of Orion-KL from 607 to 725 GHz

    P. Schilke;P. Schilke;P. Schilke;D. J. Benford;T. R. Hunter;D. C. Lis

  • Herschel Survey of Galactic OH+, H2O+, and H3O+: Probing the Molecular Hydrogen Fraction and Cosmic-Ray Ionization Rate

    N. Indriolo;D.A. Neufeld;M. Gerin;P. Schilke

  • Astrochemistry: Recent successes and current challenges

    Dariusz C. Lis;Geoffrey A. Blake;Eric Herbst

  • The composition of ices in comet C/1995 O1 (Hale-Bopp) from radio spectroscopy - Further results and upper limits on undetected species

    J. Crovisier;D. Bockelée-Morvan;P. Colom;N. Biver

  • DETECTION OF TRIPLY DEUTERATED AMMONIA IN THE BARNARD 1 CLOUD

    D. C. Lis;E. Roueff;M. Gerin;T. G. Phillips

  • SHARC II: a Caltech Submillimeter Observatory facility camera with 384 pixels

    Charles Darren Dowell;Christine A. Allen;R. Sachidananda Babu;Minoru M. Freund

  • Long-term Evolution of the Outgassing of Comet Hale-Bopp From Radio Observations

    N. Biver;D. Bockelée-Morvan;P. Colom;J. Crovisier

  • Interstellar OH+, H2O+ and H3O+ along the sight-line to G10.6–0.4

    M. Gerin;M. De Luca;J. Black;J. R. Goicoechea

  • 350 Micron Continuum Imaging of the Orion A Molecular Cloud with the Submillimeter High Angular Resolution Camera

    D. C. Lis;E. Serabyn;Jocelyn Keene;C. D. Dowell

  • Triply deuterated ammonia in NGC 1333

    F. F. S. van der Tak;P. Schilke;H. S. P. Müller;D. C. Lis

  • Triply deuterated ammonia in NGC 1333

    F.F.S. van der Tak;P. Schilke;H.S.P. M"uller;D.C. Lis

  • Herschel observations of EXtra-Ordinary Sources: Analysis of the HIFI 1.2 THz Wide Spectral Survey Toward Orion KL I. Methods

    Nathan R. Crockett;Edwin A. Bergin;Justin L. Neill;Cécile Favre

  • Ubiquitous argonium (ArH + ) in the diffuse interstellar medium: A molecular tracer of almost purely atomic gas

    P. Schilke;D. A. Neufeld;H. S. P. Müller;C. Comito

  • Herschel/HIFI observations of interstellar OH+ and H2O+ towards W49N: a probe of diffuse clouds with a small molecular fraction

    D. A. Neufeld;J. R. Goicoechea;P. Sonnentrucker;J. H. Black

  • The physical and chemical structure of Sagittarius B2 - I. Three-dimensional thermal dust and free-free continuum modeling on 100 au to 45 pc scales

    A. Schmiedeke;P. Schilke;Th. Möller;Á. Sánchez-Monge

Frequent Co-Authors

Thomas G. Phillips
Thomas G. Phillips California Institute of Technology
Peter Schilke
Peter Schilke University of Cologne
David A. Neufeld
David A. Neufeld Johns Hopkins University
José Cernicharo
José Cernicharo Spanish National Research Council
Paul F. Goldsmith
Paul F. Goldsmith California Institute of Technology
Geoffrey A. Blake
Geoffrey A. Blake California Institute of Technology
Maryvonne Gerin
Maryvonne Gerin École Normale Supérieure
Emmanuel Caux
Emmanuel Caux Federal University of Toulouse Midi-Pyrénées
Edwin A. Bergin
Edwin A. Bergin University of Michigan–Ann Arbor
F. F. S. van der Tak
F. F. S. van der Tak Netherlands Institute for Space Research

If you think any of the details on this page are incorrect, let us know.

Report an issue

We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below:

Best Scientists Citing Dariusz C. Lis

Trending Scientists