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D-Index & Metrics

Physics

D-Index
106
Citations
52137
World Ranking
1318
National Ranking
689

Houjun Mo 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 Houjun Mo 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: 356 publications — 29th percentile

29% of scientists in this discipline score the same or lower.

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

Houjun Mo 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 Houjun Mo 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: 106 D-Index — 65th percentile

65% of scientists in this discipline score the same or lower.

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

Overview

Houjun Mo is affiliated with the University of Massachusetts Amherst in the United States. Their research primarily focuses on engineering, with a specialization in electrical and electronic engineering. Additional work includes fields related to building and construction as well as ecological modeling.

The scientist has contributed to several topics within their research domain, with particular emphasis on:

  • Energy Load and Power Forecasting
  • Traffic Prediction and Management Techniques
  • Evaluation Methods in Various Fields

Houjun Mo's recent publications include the following papers:

  • Quarter-Hourly Power Load Forecasting Based on a Hybrid CNN-BiLSTM-Attention Model with CEEMDAN, K-Means, and VMD, 2025, published in Energies
  • Correction: Liu et al. Quarter-Hourly Power Load Forecasting Based on a Hybrid CNN-BiLSTM-Attention Model with CEEMDAN, K-Means, and VMD. Energies 2025, 18, 2675, published in Energies, 2025

The venues in which Mo frequently publishes include:

  • Energies

Frequent co-authors collaborating with Houjun Mo are:

  • Xiaoyu Liu
  • Jiangfeng Song
  • Hai Tao
  • Wenjie Du
  • Peng Wang

Best Publications

  • Sloan Digital Sky Survey: Early data release

    C. Stoughton;R. H. Lupton;M. Bernardi;M. R. Blanton

  • Sloan digital sky survey: Early data release

    Chris Stoughton;Robert H. Lupton;Mariangela Bernardi;Michael R. Blanton;Michael R. Blanton

  • The Formation of Galactic Disks

    H. J. Mo;Shude Mao;Simon D. M. White

  • The formation of galactic discs

    H. J. Mo;Shude Mao;Simon D. M. White

  • Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes

    Ravi K. Sheth;H. J. Mo;Giuseppe Tormen

  • An analytic model for the spatial clustering of dark matter haloes

    H.J. Mo;H.J. Mo;Simon D.M. White;Simon D.M. White

  • The size distribution of galaxies in the Sloan Digital Sky Survey

    Shiyin Shen;H. J. Mo;Simon D. M. White;Michael R. Blanton

  • Galaxy Formation and Evolution

    Houjun Mo;Frank van den Bosch;Simon White

  • Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties

    Xiaohu Yang;H.J. Mo;Frank C. van den Bosch;Anna Pasquali

  • Galaxy Groups in the SDSS DR4. I. The Catalog and Basic Properties

    Xiaohu Yang;H. J. Mo;Frank C. van den Bosch;Anna Pasquali

  • Properties of Galaxy Groups in the SDSS: I.-- The Dependence of Colour, Star Formation, and Morphology on Halo Mass

    Simone M. Weinmann;Frank C. van den Bosch;Xiaohu Yang;H. J. Mo

  • Galaxy Clustering in Early SDSS Redshift Data

    Idit Zehavi;Michael R. Blanton;Joshua A. Frieman

  • Properties of galaxy groups in the Sloan Digital Sky Survey – I. The dependence of colour, star formation and morphology on halo mass

    Simone M. Weinmann;Simone M. Weinmann;Frank C. van den Bosch;Frank C. van den Bosch;Xiaohu Yang;H. J. Mo

  • Constraining galaxy formation and cosmology with the conditional luminosity function of galaxies

    Xiaohu Yang;H. J. Mo;Frank C. van den Bosch

  • Accurate universal models for the mass accretion histories and concentrations of dark matter halos

    D. H. Zhao;Y. P. Jing;H. J. Mo;G. Boerner

  • Spatial correlation function and pairwise velocity dispersion of galaxies: CDM models versus the Las Campanas Survey

    Y.P. Jing;H.J. Mo;G. Boerner

  • ACCURATE UNIVERSAL MODELS FOR THE MASS ACCRETION HISTORIES AND CONCENTRATIONS OF DARK MATTER HALOS

    D. H. Zhao;Y. P. Jing;H. J. Mo;G. Börner

  • Spatial Correlation Function and Pairwise Velocity Dispersion of Galaxies: Cold Dark Matter Models versus the Las Campanas Survey

    Y. P. Jing;Y. P. Jing;H. J. Mo;G. Börner

  • The Growth and Structure of Dark Matter Haloes

    Donghai Zhao;Houjun Mo;Yipeng Jing;Gerhard Boerner

  • The Correlation function of clusters of galaxies and the amplitude of mass fluctuations in the Universe

    H. J. Mo;Y. P. Jing;S. D. M. White

Frequent Co-Authors

Frank C. van den Bosch
Frank C. van den Bosch Yale University
Xiaohu Yang
Xiaohu Yang Shanghai Jiao Tong University
Simon D. M. White
Simon D. M. White Max Planck Institute for Astrophysics
Shude Mao
Shude Mao Tsinghua University
Neal Katz
Neal Katz University of Massachusetts Amherst
Ravi K. Sheth
Ravi K. Sheth University of Pennsylvania
Daniel H. McIntosh
Daniel H. McIntosh University of Missouri–Kansas City
Wolfgang Voges
Wolfgang Voges Max Planck Society
Michael R. Blanton
Michael R. Blanton New York University
István Csabai
István Csabai Eötvös Loránd University

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