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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 90 2236 2128 91 89 315 29451

Ph. André publications per year

The chart shows the history of publications by Ph. André between 1985 and 2024, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Ph. André published across 40 years, from 1985 to 2024, averaging 8.1 papers a year. Output peaked at 32 publications in 2010. 6 of the 323 publications appeared in the last two years.

No. of publications
10 20 30
Bar chart. Horizontal axis: year, 1985 to 2024. Vertical axis: number of publications, 0 to 32. Peak 32 publications in 2010. 1985: 2 publications 1986: 1 publication 1987: 4 publications 1988: 4 publications 1989: 1 publication 1990: 2 publications 1991: 3 publications 1992: 1 publication 1993: 3 publications 1994: 5 publications 1995: 5 publications 1996: 4 publications 1997: 2 publications 1998: 3 publications 1999: 0 publications 2000: 1 publication 2001: 3 publications 2002: 7 publications 2003: 3 publications 2004: 4 publications 2005: 5 publications 2006: 11 publications 2007: 3 publications 2008: 6 publications 2009: 9 publications 2010: 32 publications 2011: 11 publications 2012: 21 publications 2013: 25 publications 2014: 22 publications 2015: 26 publications 2016: 15 publications 2017: 19 publications 2018: 13 publications 2019: 9 publications 2020: 23 publications 2021: 8 publications 2022: 1 publication 2023: 4 publications 2024: 2 publications
1985 2024

323 publications in total across all disciplines

View publications per year as a table
Ph. André: publications per year, 1985 to 2024
Year Publications
1985 2
1986 1
1987 4
1988 4
1989 1
1990 2
1991 3
1992 1
1993 3
1994 5
1995 5
1996 4
1997 2
1998 3
1999 0
2000 1
2001 3
2002 7
2003 3
2004 4
2005 5
2006 11
2007 3
2008 6
2009 9
2010 32
2011 11
2012 21
2013 25
2014 22
2015 26
2016 15
2017 19
2018 13
2019 9
2020 23
2021 8
2022 1
2023 4
2024 2
Total 323
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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.

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, 303–322 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: 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.

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
303–322 136 315
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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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.

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, 90–91 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: 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.

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
84–85 166
86–87 132
88–89 155
90–91 134 90
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

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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