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 Nuria Calvet sits on this spectrum.
This scientist: 481 publications — 53rd percentile
53% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Nuria Calvet sits on this spectrum.
This scientist: 116 D-Index — 75th percentile
75% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
Nuria Calvet is affiliated with the University of Michigan-Ann Arbor in the United States. Their work is situated primarily within the field of Physics and Astronomy, contributing extensively to subfields such as Astronomy and Astrophysics, Instrumentation, Spectroscopy, Computational Mechanics, and Aerospace Engineering.
Their research covers a range of topics with a focus on Astrophysics and Star Formation Studies, Stellar, planetary, and galactic studies, Astro and Planetary Science, Astronomy and Astrophysical Research, Molecular Spectroscopy and Structure, Astronomical Observations and Instrumentation, and Atmospheric Ozone and Climate.
Notable recent papers by Nuria Calvet include:
Their frequent co-authors include Thanawuth Thanathibodee, Catherine Espaillat, Caeley V. Pittman, C. Robinson, and Jesús Hernández. This network indicates collaboration across a range of experts in related areas of astrophysics and planetary studies.
Nuria Calvet has contributed to numerous publication venues, with a significant number of papers appearing in:
The scope of their work revolves around observational and theoretical studies in astrophysics, with emphasis on star and planet formation environments, molecular spectroscopy, and related instrumentation techniques. This multidisciplinary approach supports investigations into the physical and chemical processes governing protoplanetary disks and young stellar objects.
Lee Hartmann;Nuria Calvet;Nuria Calvet;Erik Gullbring;Paola D'Alessio
Erik Gullbring;Lee Hartmann;Cesar Briceño;Cesar Briceño;Cesar Briceño;Nuria Calvet;Nuria Calvet
Michael R. Meyer;Nuria Calvet;Lynne A. Hillenbrand
Nuria Calvet;Nuria Calvet;Erik Gullbring
Paola D'Alessio;Jorge Cantö;Nuria Calvet;Nuria Calvet;Susana Lizano
Nuria Calvet;Paola D’Alessio;Lee Hartmann;David Wilner
Paola D’Alessio;Paola D’Alessio;Nuria Calvet;Lee Hartmann
Lee Hartmann;Gregory Herczeg;Nuria Calvet
Paola D’Alessio;Nuria Calvet;Lee Hartmann;Susana Lizano
Jesus Hernandez;L. Hartmann;T. Megeath;R. Gutermuth
K. L. Luhman;P. R. Allen;C. Espaillat;C. Espaillat;L. Hartmann
Lee Hartmann;Robert Hewett;Nuria Calvet
James Muzerolle;James Muzerolle;Nuria Calvet;Nuria Calvet;Lee Hartmann
James Muzerolle;James Muzerolle;James Muzerolle;Lee Hartmann;Lee Hartmann;Nuria Calvet;Nuria Calvet
Jesús Hernández;Jesús Hernández;L. Hartmann;T. Megeath;R. Gutermuth
Lori E. Allen;Nuria Calvet;Paola D’Alessio;Bruno Merin
Nuria Calvet;Nuria Calvet;James Muzerolle;James Muzerolle;César Briceño;César Briceño;Jesus Hernández;Jesus Hernández
James Muzerolle;James Muzerolle;Lynne Hillenbrand;Nuria Calvet;Cesar Briceno;Cesar Briceno
E. Furlan;L. Hartmann;N. Calvet;P. D'Alessio
Erik Gullbring;Nuria Calvet;Nuria Calvet;James Muzerolle;James Muzerolle;Lee Hartmann
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