World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
90
Citations
29451
World Ranking
2236
National Ranking
91

Ph. André 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 Ph. André 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: 315 publications — 20th percentile

20% of scientists in this discipline score the same or lower.

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

Ph. André 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 Ph. André 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: 90 D-Index — 40th percentile

40% of scientists in this discipline score the same or lower.

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

Overview

Ph. André is affiliated with the International Astronomical Union in France and has contributed extensively to the field of Physics and Astronomy. Their work primarily focuses on Astronomy and Astrophysics, with significant research output spanning a range of related subfields including Spectroscopy, Atmospheric Science, Instrumentation, and Computational Mechanics.

The scientist's main topics of research encompass:

  • Astrophysics and Star Formation Studies
  • Stellar, planetary, and galactic studies
  • Molecular Spectroscopy and Structure
  • Atmospheric Ozone and Climate
  • Astro and Planetary Science
  • Solar and Space Plasma Dynamics
  • Astronomy and Astrophysical Research

Ph. André has published research in several frequently cited venues, including:

  • Astronomy and Astrophysics
  • Monthly Notices of the Royal Astronomical Society
  • arXiv (Cornell University)
  • Springer Link (Chiba Institute of Technology)
  • EPJ Web of Conferences

Among recent notable papers are:

  • "Questioning the spatial origin of complex organic molecules in young protostars with the CALYPSO survey," 2020, Astronomy and Astrophysics
  • "The role of Galactic H II regions in the formation of filaments," 2020, Astronomy and Astrophysics
  • "The accretion history of high-mass stars: an ArTéMiS pilot study of infrared dark clouds," 2020, Monthly Notices of the Royal Astronomical Society
  • "The census of dense cores in the Serpens region from the Herschel Gould Belt Survey," 2020, Monthly Notices of the Royal Astronomical Society
  • "Compressed magnetized shells of atomic gas and the formation of the Corona Australis molecular cloud," 2020, Springer Link (Chiba Institute of Technology)

Ph. André often collaborates with several frequent co-authors, including:

  • D. Arzoumanian
  • Yoshito Shimajiri
  • V. Könyves
  • P. Palmeirim
  • S. Bontemps

Best Publications

  • Submillimeter Continuum Observations of rho Ophiuchi A: The Candidate Protostar VLA 1623 and Prestellar Clumps

    Philippe Andre;Derek Ward-Thompson;Mary Barsony

  • From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

    Ph. André;A. Men'shchikov;S. Bontemps;V. Könyves

  • Characterizing interstellar filaments with Herschel in IC5146

    D. Arzoumanian;Ph. André;P. Didelon;V. Konyves

  • Clouds, filaments, and protostars: The Herschel Hi-GAL Milky Way

    S. Molinari;B. Swinyard;J. Bally;M. Barlow

  • Characterizing interstellar filaments with Herschel in IC 5146

    D. Arzoumanian;Ph. André;P. Didelon;V. Könyves

  • Herschel view of the Taurus B211/3 filament and striations: Evidence of filamentary growth?

    P. Palmeirim;Ph. André;J. Kirk;D. Ward-Thompson

  • The circumstellar environment of low-mass protostars: A millimeter continuum mapping survey ?

    F. Motte;F. Motte;P. André

  • Herschel view of the Taurus B211/3 filament and striations: evidence of filamentary growth?

    P. Palmeirim;Ph. André;Jason Matthew Kirk;Derek Ward-Thompson

  • Further Mid-Infrared Study of the rho Ophiuchi Cloud Young Stellar Population: Luminosities and Masses of Pre--Main-Sequence Stars

    Thomas P. Greene;Bruce A. Wilking;Philippe Andre;Erick T. Young

  • A submillimetre continuum survey of pre-protostellar cores

    D. Ward-Thompson;P. F. Scott;R. E. Hills;P. André

  • Cluster-formation in the Rosette molecular cloud at the junctions of filaments

    N. Schneider;T. Csengeri;M. Hennemann;F. Motte

  • A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey

    V. Könyves;V. Könyves;Ph. André;A. Men'shchikov;P. Palmeirim

  • ISOCAM observations of the rho Ophiuchi cloud: Luminosity and mass functions of the pre-main sequence embedded cluster

    Sylvain Bontemps;P. Andre;A. A. Kaas;L. Nordh

  • Hi-GAL, the Herschel infrared Galactic Plane Survey: photometric maps and compact source catalogues. First data release for Inner Milky Way: +68{\deg}> l > -70{\deg}

    S. Molinari;E. Schisano;D. Elia;M. Pestalozzi

  • The Aquila prestellar core population revealed by Herschel

    V. Könyves;Ph. André;A. Men'shchikov;N. Schneider

  • Filamentary structures and compact objects in the Aquila and Polaris clouds observed by Herschel

    A. Men'shchikov;Ph. André;P. Didelon;V. Könyves

  • Global collapse of molecular clouds as a formation mechanism for the most massive stars

    N. Peretto;G. A. Fuller;A. Duarte-Cabral;A. Avison

  • What Determines the Density Structure of Molecular Clouds? A Case Study of Orion B with Herschel

    N Schneider;N Schneider;Ph Andre;Vera Konyves;Vera Konyves;S Bontemps

  • Molecular line study of the very young protostar IRAM 04191 in Taurus: infall, rotation, and outflow

    A. Belloche;P. André;D. Despois;S. Blinder;S. Blinder

  • A multi-scale, multi-wavelength source extraction method: getsources

    A. Men’shchikov;Ph. André;P. Didelon;F. Motte

Frequent Co-Authors

Nicola Schneider
Nicola Schneider University of Cologne
Frédérique Motte
Frédérique Motte Grenoble Alpes University
Glenn J. White
Glenn J. White The Open University
Derek Ward-Thompson
Derek Ward-Thompson University of Central Lancashire
Sergio Molinari
Sergio Molinari National Institute for Astrophysics
Peter A. R. Ade
Peter A. R. Ade Cardiff University
Philip Daniel Mauskopf
Philip Daniel Mauskopf Arizona State University
Carole Tucker
Carole Tucker Cardiff University
Alain Benoit
Alain Benoit Grenoble Alpes University
Matthew Joseph Griffin
Matthew Joseph Griffin Cardiff University

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