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Pascale Jablonka

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 72 3596 3420 90 86 290 16231

Pascale Jablonka publications per year

The chart shows the history of publications by Pascale Jablonka between 1990 and 2021, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Pascale Jablonka published across 32 years, from 1990 to 2021, averaging 8.4 papers a year. Output peaked at 31 publications in 2021. 58 of the 269 publications appeared in the last two years.

No. of publications
10 20 30
Bar chart. Horizontal axis: year, 1990 to 2021. Vertical axis: number of publications, 0 to 31. Peak 31 publications in 2021. 1990: 3 publications 1991: 1 publication 1992: 2 publications 1993: 0 publications 1994: 1 publication 1995: 2 publications 1996: 5 publications 1997: 0 publications 1998: 3 publications 1999: 5 publications 2000: 6 publications 2001: 4 publications 2002: 5 publications 2003: 9 publications 2004: 16 publications 2005: 10 publications 2006: 14 publications 2007: 8 publications 2008: 16 publications 2009: 18 publications 2010: 8 publications 2011: 6 publications 2012: 13 publications 2013: 3 publications 2014: 2 publications 2015: 5 publications 2016: 5 publications 2017: 15 publications 2018: 14 publications 2019: 12 publications 2020: 27 publications 2021: 31 publications
1990 2021

269 publications in total across all disciplines

View publications per year as a table
Pascale Jablonka: publications per year, 1990 to 2021
Year Publications
1990 3
1991 1
1992 2
1993 0
1994 1
1995 2
1996 5
1997 0
1998 3
1999 5
2000 6
2001 4
2002 5
2003 9
2004 16
2005 10
2006 14
2007 8
2008 16
2009 18
2010 8
2011 6
2012 13
2013 3
2014 2
2015 5
2016 5
2017 15
2018 14
2019 12
2020 27
2021 31
Total 269
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Pascale Jablonka 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 Pascale Jablonka 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, 283–302 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: 290 publications — 16th percentile

16% 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
283–302 126 290
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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Pascale Jablonka 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 Pascale Jablonka 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, 72–73 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: 72 D-Index — 3rd percentile

3% 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 72
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
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

What is she best known for?

The fields of study she is best known for:

  • Galaxy
  • Milky Way
  • Astronomy

Her scientific interests lie mostly in Astrophysics, Astronomy, Galaxy, Dwarf galaxy and Dwarf spheroidal galaxy. Her work is connected to Milky Way, Galaxy formation and evolution, Metallicity, Galaxy cluster and Globular cluster, as a part of Astrophysics. Stellar population, Elliptical galaxy, Velocity dispersion, Stars and Galaxy group are the subjects of her Astronomy studies.

Her study looks at the relationship between Elliptical galaxy and fields such as Luminous infrared galaxy, as well as how they intersect with chemical problems. Her research in Galaxy is mostly focused on Star formation. In Dwarf galaxy, she works on issues like Spiral galaxy, which are connected to Blue straggler and Galactic halo.

Her most cited work include:

  • Two distinct ancient components in the Sculptor dwarf spheroidal galaxy: First results from the dwarf abundances and radial velocities team (325 citations)
  • The DART Imaging And CaT Survey of the Fornax Dwarf Spheroidal Galaxy (297 citations)
  • The evolution of the star formation activity in galaxies and its dependence on environment (277 citations)

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

Pascale Jablonka mainly focuses on Astrophysics, Galaxy, Astronomy, Metallicity and Stars. Her study in Astrophysics concentrates on Dwarf galaxy, Milky Way, Galaxy cluster, Star formation and Redshift. Her study in Elliptical galaxy, Globular cluster, Lenticular galaxy, Brightest cluster galaxy and Galaxy group is done as part of Astronomy.

While the research belongs to areas of Elliptical galaxy, Pascale Jablonka spends her time largely on the problem of Luminous infrared galaxy, intersecting her research to questions surrounding Radio galaxy. Her Metallicity research is multidisciplinary, incorporating elements of Interstellar medium, Supernova and Dwarf spheroidal galaxy. Her Stars research is multidisciplinary, incorporating perspectives in Spectral line and Galactic halo.

She most often published in these fields:

  • Astrophysics (147.63%)
  • Galaxy (106.31%)
  • Astronomy (76.66%)

What were the highlights of her more recent work (between 2018-2021)?

  • Galaxy (106.31%)
  • Astrophysics (147.63%)
  • Dwarf galaxy (46.69%)

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

Her primary areas of investigation include Galaxy, Astrophysics, Dwarf galaxy, Star formation and Stars. The Galaxy study combines topics in areas such as Spectroscopy and Spectral line. Metallicity, Stellar mass, Milky Way, Local Group and Halo are the primary areas of interest in her Astrophysics study.

Her study in Metallicity is interdisciplinary in nature, drawing from both Stellar population and Dwarf spheroidal galaxy. Her study explores the link between Milky Way and topics such as Accretion that cross with problems in Elliptic orbit. Astronomy covers Pascale Jablonka research in Galaxy formation and evolution.

Between 2018 and 2021, her most popular works were:

  • 4MOST: Project overview and information for the First Call for Proposals (74 citations)
  • The Pristine Dwarf-Galaxy survey – II. In-depth observational study of the faint Milky Way satellite Sagittarius II (25 citations)
  • The Pristine Dwarf-Galaxy survey – II. In-depth observational study of the faint Milky Way satellite Sagittarius II (25 citations)

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

  • Galaxy
  • Milky Way
  • Astronomy

Pascale Jablonka mainly investigates Galaxy, Astrophysics, Redshift, Star formation and Galaxy cluster. Her Galaxy study is focused on Astronomy in general. Astrophysics is a component of her Stellar mass, Dwarf galaxy and Velocity dispersion studies.

Her work deals with themes such as Metallicity and Milky Way, which intersect with Dwarf galaxy. Her Metallicity research integrates issues from Dwarf spheroidal galaxy and White dwarf. The various areas that Pascale Jablonka examines in her Redshift study include Universe and Dark matter.

Best Publications

  • Two distinct ancient components in the Sculptor Dwarf Spheroidal Galaxy: First Results from DART

    Eline Tolstoy;M.J. Irwin;A. Helmi;G. Battaglia

  • The evolution of the star formation activity in galaxies and its dependence on environment

    B. M. Poggianti;A. von der Linden;G. De Lucia;V. Desai

  • Two distinct ancient components in the Sculptor dwarf spheroidal galaxy: First results from the dwarf abundances and radial velocities team

    Eline Tolstoy;M. J. Irwin;A. Helmi;G. Battaglia

  • The evolution of the star formation activity in galaxies and its dependence on environment

    Bianca M. Poggianti;Anja von der Linden;Gabriella De Lucia;Vandana Desai

  • The NIR Ca II triplet at low metallicity - Searching for extremely low-metallicity stars in classical dwarf galaxies

    Else Starkenburg;Vanessa Hill;Eline Tolstoy;Jonay I. González Hernández

  • THE KINEMATIC STATUS AND MASS CONTENT OF THE SCULPTOR DWARF SPHEROIDAL GALAXY

    G. Battaglia;Amina Helmi;Eline Tolstoy;M. Irwin

  • The DART Imaging And CaT Survey of the Fornax Dwarf Spheroidal Galaxy

    Giuseppina Battaglia;E. Tolstoy;A. Helmi;M. J. Irwin

  • The build-up of the colour-magnitude relation in galaxy clusters since z ~ 0.8

    Gabriella De Lucia;Bianca M. Poggianti;Alfonso Aragón-Salamanca;Simon D. M. White

  • A new view of the dwarf spheroidal satellites of the Milky Way from VLT flames: Where are the very metal-poor stars?

    Amina Helmi;M. J. Irwin;E. Tolstoy;G. Battaglia

  • A Database for Galaxy Evolution Modeling

    C Leitherer;D Alloin;U FritzVonAlvensleben;JS Gallagher

  • The build-up of the red-sequence in galaxy clusters since z~0.8

    G. De Lucia;B. M. Poggianti;A. Aragon-Salamanca;D. Clowe

  • A high-resolution VLT/FLAMES study of individual stars in the centre of the Fornax dwarf spheroidal galaxy

    B. Letarte;V. Hill;V. Hill;Eline Tolstoy;P. Jablonka;P. Jablonka

  • The NIR Ca II triplet at low metallicity: Searching for extremely low-metallicity stars in classical dwarf galaxies

    E. Starkenburg;V. Hill;Eline Tolstoy;J.I. Gonzalez Hernandez;J.I. Gonzalez Hernandez

  • The Morphological Content of Ten EDisCS Clusters at 0.5 < z < 0.8

    V. Desai;J. J. Dalcanton;A. Aragon-Salamanca;P. Jablonka

  • Mayall II = G1 in M31: Giant Globular Cluster or Core of a Dwarf Elliptical Galaxy?

    G. Meylan;G. Meylan;G. Meylan;A. Sarajedini;P. Jablonka;S. G. Djorgovski

  • Analysis and calibration of CaII triplet spectroscopy of red giant branch stars from VLT/FLAMES observations

    G. Battaglia;M. Irwin;Eline Tolstoy;V. Hill

  • The Pristine survey - I. Mining the Galaxy for the most metal-poor stars

    Else Starkenburg;Nicolas Martin;Nicolas Martin;Kris Youakim;David S. Aguado;David S. Aguado

  • The Buildup of the red sequence in galaxy clusters since z ∼ 0.8

    G. De Lucia;B. M. Poggianti;A. Aragón-Salamanca;D. Clowe

  • The dynamical and chemical evolution of dwarf spheroidal galaxies

    Y. Revaz;P. Jablonka;P. Jablonka;T. Sawala;V. Hill

  • The morphological content of 10 EDisCS clusters at 0.5 < z < 0.8

    V. Desai;V. Desai;J. J. Dalcanton;A. Aragón-Salamanca;P. Jablonka

Frequent Co-Authors

Dennis Zaritsky
Dennis Zaritsky University of Arizona
Alfonso Aragón-Salamanca
Alfonso Aragón-Salamanca University of Nottingham
Eline Tolstoy
Eline Tolstoy University of Groningen
Bo Milvang-Jensen
Bo Milvang-Jensen University of Copenhagen
Roberto P. Saglia
Roberto P. Saglia Max Planck Society
Bianca M. Poggianti
Bianca M. Poggianti National Institute for Astrophysics
Amina Helmi
Amina Helmi University of Groningen
Matthew Shetrone
Matthew Shetrone The University of Texas at Austin
Nobuo Arimoto
Nobuo Arimoto Seoul National University
Georges Meylan
Georges Meylan École Polytechnique Fédérale de Lausanne

External Links

Personal website of Pascale Jablonka

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Best Scientists Citing Pascale Jablonka

Anna Frebel

Anna Frebel

MIT

Publications: 91

Eva K. Grebel

Eva K. Grebel

Heidelberg University

Publications: 80

Puragra Guhathakurta

Puragra Guhathakurta

University of California, Santa Cruz

Publications: 69

Eline Tolstoy

Eline Tolstoy

University of Groningen

Publications: 64

Rodrigo A. Ibata

Rodrigo A. Ibata

University of Strasbourg

Publications: 61

Eric F. Bell

Eric F. Bell

University of Michigan–Ann Arbor

Publications: 57

Alexis Finoguenov

Alexis Finoguenov

University of Helsinki

Publications: 53

Jacopo Fritz

Jacopo Fritz

National Autonomous University of Mexico

Publications: 53

Timothy C. Beers

Timothy C. Beers

University of Notre Dame

Publications: 52

Warrick J. Couch

Warrick J. Couch

Swinburne University of Technology

Publications: 49

Geraint F. Lewis

Geraint F. Lewis

University of Sydney

Publications: 49

Julio F. Navarro

Julio F. Navarro

University of Victoria

Publications: 49

Bianca M. Poggianti

Bianca M. Poggianti

National Institute for Astrophysics

Publications: 46

Simona Mei

Simona Mei

Université Paris Cité

Publications: 44

Francesca Matteucci

Francesca Matteucci

University of Trieste

Publications: 43

Antonio Aparicio

Antonio Aparicio

University of La Laguna

Publications: 43

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