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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 100 1667 1587 878 823 274 30967

Mariska Kriek publications per year

The chart shows the history of publications by Mariska Kriek between 1999 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Mariska Kriek published across 27 years, from 1999 to 2025, averaging 12.3 papers a year. Output peaked at 26 publications in 2020. 48 of the 333 publications appeared in the last two years.

No. of publications
5 10 15 20 25
Bar chart. Horizontal axis: year, 1999 to 2025. Vertical axis: number of publications, 0 to 26. Peak 26 publications in 2020. 1999: 1 publication 2000: 0 publications 2001: 0 publications 2002: 0 publications 2003: 0 publications 2004: 2 publications 2005: 3 publications 2006: 9 publications 2007: 6 publications 2008: 5 publications 2009: 18 publications 2010: 16 publications 2011: 17 publications 2012: 9 publications 2013: 10 publications 2014: 13 publications 2015: 23 publications 2016: 19 publications 2017: 15 publications 2018: 10 publications 2019: 18 publications 2020: 26 publications 2021: 23 publications 2022: 24 publications 2023: 18 publications 2024: 22 publications 2025: 26 publications
1999 2025

333 publications in total across all disciplines

View publications per year as a table
Mariska Kriek: publications per year, 1999 to 2025
Year Publications
1999 1
2000 0
2001 0
2002 0
2003 0
2004 2
2005 3
2006 9
2007 6
2008 5
2009 18
2010 16
2011 17
2012 9
2013 10
2014 13
2015 23
2016 19
2017 15
2018 10
2019 18
2020 26
2021 23
2022 24
2023 18
2024 22
2025 26
Total 333
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Mariska Kriek 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 Mariska Kriek 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, 263–282 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: 274 publications — 13th percentile

13% 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
263–282 114 274
283–302 126
303–322 136
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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Mariska Kriek 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 Mariska Kriek 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, 100–101 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: 100 D-Index — 56th percentile

56% 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
92–93 137
94–95 102
96–97 112
98–99 110
100–101 116 100
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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Research.com Recognitions

  • 2014 - Hellman Fellow

Overview

Mariska Kriek is affiliated with the University of California, Berkeley in the United States. Their research is primarily situated within the field of Physics and Astronomy, with a particular focus on Astronomy and Astrophysics, Instrumentation, Atomic and Molecular Physics and Optics, Spectroscopy, and Computational Mechanics. Their work covers a range of topics including galaxies: formation, evolution, and phenomena; astronomy and astrophysical research; stellar, planetary, and galactic studies; astrophysics and star formation studies; gamma-ray bursts and supernovae; adaptive optics and wavefront sensing; and astrophysical phenomena and observations.

Mariska Kriek has contributed extensively to the scientific literature, with publications appearing predominantly in several key journals. Frequent venues for their work include:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal Letters
  • Astronomy and Astrophysics

Among the recent papers associated with their research network and fields of study are:

  • The JWST UNCOVER Treasury Survey: Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization (2024, The Astrophysical Journal)
  • The UNCOVER Survey: A First-look HST + JWST Catalog of 60,000 Galaxies near A2744 and beyond (2023, The Astrophysical Journal Supplement Series)
  • The MOSDEF-LRIS Survey: The Interplay Between Massive Stars and Ionized Gas in High-Redshift Star-Forming Galaxies (2020, Monthly Notices of the Royal Astronomical Society)
  • The MOSDEF Survey: The First Direct Measurements of the Nebular Dust Attenuation Curve at High Redshift (2020, The Astrophysical Journal)
  • The MOSDEF-LRIS Survey: The connection between massive stars and ionized gas in individual galaxies at z ∼ 2 (2020, Monthly Notices of the Royal Astronomical Society)

Collaboration appears as a significant aspect of their scientific practice, with frequent co-authors including Alice E. Shapley, Sedona H. Price, Naveen A. Reddy, Rachel Bezanson, and Ryan L. Sanders. These repeated collaborations suggest active engagement within research teams contributing to related topics in their field.

Recognition of Mariska Kriek's work includes receiving the Hellman Fellowship in 2014.

Best Publications

  • An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2

    Mariska Kriek;Pieter G. van Dokkum;Ivo Labbé;Marijn Franx

  • The Growth of Massive Galaxies Since z = 2

    Pieter G. van Dokkum;Pieter G. van Dokkum;Katherine E. Whitaker;Katherine E. Whitaker;Gabriel Brammer;Gabriel Brammer;Marijn Franx

  • Confirmation of the Remarkable Compactness of Massive Quiescent Galaxies at z ~ 2.3: Early-Type Galaxies Did not Form in a Simple Monolithic Collapse* **

    Pieter G. van Dokkum;Marijn Franx;Mariska Kriek;Bradford Holden

  • 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses

    Rosalind E. Skelton;Katherine E. Whitaker;Ivelina G. Momcheva;Gabriel B. Brammer

  • The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for $\sim 100,000$ galaxies

    Ivelina G. Momcheva;Gabriel B. Brammer;Pieter G. van Dokkum;Rosalind E. Skelton

  • 3D-HST: a wide-field grism spectroscopic survey with the Hubble Space Telescope

    Gabriel B. Brammer;Pieter G. Van Dokkum;Marijn Franx;Mattia Fumagalli

  • The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-frame Optical Spectroscopy for ~1500 H-selected Galaxies at 1.37 ? z ? 3.8

    Mariska Kriek;Alice E. Shapley;Naveen A. Reddy;Brian Siana

  • The number density and mass density of star-forming and quiescent galaxies at 0.4 < z < 2.2

    Gabriel B. Brammer;Katherine E. Whitaker;Pieter G. van Dokkum;Danilo Marchesini

  • THE RELATION BETWEEN COMPACT, QUIESCENT HIGH-REDSHIFT GALAXIES AND MASSIVE NEARBY ELLIPTICAL GALAXIES: EVIDENCE FOR HIERARCHICAL, INSIDE-OUT GROWTH

    Rachel Bezanson;Pieter G. van Dokkum;Tomer Tal;Danilo Marchesini

  • THE 3D-HST SURVEY: HUBBLE SPACE TELESCOPE WFC3/G141 GRISM SPECTRA, REDSHIFTS, AND EMISSION LINE MEASUREMENTS FOR ∼100,000 GALAXIES

    Ivelina G. Momcheva;Gabriel B. Brammer;Pieter G. Van Dokkum;Rosalind E. Skelton

  • THE DUST ATTENUATION LAW IN DISTANT GALAXIES: EVIDENCE FOR VARIATION WITH SPECTRAL TYPE

    Mariska Kriek;Charlie Conroy

  • The Stellar Mass Density and Specific Star Formation Rate of the Universe at z ~ 7

    Valentino González;Ivo Labbé;Rychard J. Bouwens;Rychard J. Bouwens;Garth Illingworth

  • THE NEWFIRM MEDIUM-BAND SURVEY: PHOTOMETRIC CATALOGS, REDSHIFTS, AND THE BIMODAL COLOR DISTRIBUTION OF GALAXIES OUT TO z ∼ 3

    Katherine E. Whitaker;Katherine E. Whitaker;Ivo Labbé;Ivo Labbé;Pieter G. van Dokkum;Pieter G. van Dokkum;Gabriel Brammer;Gabriel Brammer;Gabriel Brammer

  • THE MOSDEF SURVEY: MEASUREMENTS OF BALMER DECREMENTS AND THE DUST ATTENUATION CURVE AT REDSHIFTS z ∼ 1.4–2.6*

    Naveen A. Reddy;Mariska Kriek;Alice E. Shapley;William R. Freeman

  • Hubble space telescope and Spitzer imaging of red and blue galaxies at z 2.5: a correlation between size and star formation activity from compact quiescent galaxies to extended star-forming galaxies

    S. Toft;S. Toft;P. van Dokkum;M. Franx;I. Labbe

  • EVOLUTION OF GALAXY STELLAR MASS FUNCTIONS, MASS DENSITIES, AND MASS-TO-LIGHT RATIOS FROM z ∼ 7 TO z ∼ 4

    Valentino González;Ivo Labbé;Rychard J. Bouwens;Garth Illingworth

  • THE NUMBER DENSITY AND MASS DENSITY OF STAR-FORMING AND QUIESCENT GALAXIES AT 0.4 ⩽ z ⩽ 2.2

    Gabriel B. Brammer;Gabriel B. Brammer;Gabriel B. Brammer;K. E. Whitaker;P. G. van Dokkum;D. Marchesini

  • HST and Spitzer imaging of red and blue galaxies at z~2.5: A correlation between size and star formation activity from compact quiescent galaxies to extended star forming galaxies

    S. Toft;P. van Dokkum;M. Franx;I. Labbe

  • Forming Compact Massive Galaxies

    Pieter G van Dokkum;Erica June Nelson;Marijn Franx;Pascal Oesch

  • Evidence for Wide-Spread AGN Driven Outflows in the Most Massive z~1-2 Star Forming Galaxies

    R. Genzel;N. M. Förster Schreiber;D. Rosario;P. Lang

Frequent Co-Authors

Pieter G. van Dokkum
Pieter G. van Dokkum Yale University
Gabriel B. Brammer
Gabriel B. Brammer University of Copenhagen
Danilo Marchesini
Danilo Marchesini Tufts University
Brian Siana
Brian Siana University of California, Riverside
Naveen A. Reddy
Naveen A. Reddy University of California, Riverside
Marijn Franx
Marijn Franx Leiden University
Alison L. Coil
Alison L. Coil University of California, San Diego
Bahram Mobasher
Bahram Mobasher University of California, Riverside
Garth D. Illingworth
Garth D. Illingworth University of California, Santa Cruz
Ivo Labbe
Ivo Labbe Swinburne University of Technology

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