D-Index & Metrics Best Publications
D. Stern

D. Stern

California Institute of Technology
United States

Overview

What is he best known for?

The fields of study he is best known for:

  • Astronomy
  • Galaxy
  • Astrophysics

The scientist’s investigation covers issues in Astrophysics, Redshift, Galaxy, Luminosity and Quasar. His research brings together the fields of Spectroscopy and Astrophysics. His work deals with themes such as Stellar population and Extinction, which intersect with Redshift.

He has researched Galaxy in several fields, including Equivalent width, Emission spectrum, Continuum, Infrared and Spitzer Space Telescope. D. Stern interconnects Intergalactic travel and Spectral line in the investigation of issues within Luminosity. His work on Advanced Camera for Surveys as part of general Star formation study is frequently linked to Excitation, bridging the gap between disciplines.

His most cited work include:

  • Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources (480 citations)
  • The Rest-Frame UV Luminosity Density of Star-Forming Galaxies at Redshifts z>3.5 (410 citations)
  • The unusual afterglow of GRB 980326: evidence for the gamma-ray burst/supernova connection (403 citations)

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

D. Stern focuses on Astrophysics, Astronomy, Redshift, Galaxy and Quasar. His Astrophysics research is multidisciplinary, incorporating perspectives in Spectral line and X-ray. His work on Infrared, Luminous infrared galaxy, Pulsar and Hubble Deep Field as part of general Astronomy research is frequently linked to Field, bridging the gap between disciplines.

The concepts of his Redshift study are interwoven with issues in Star formation, Advanced Camera for Surveys, Spectroscopy and Radio galaxy. His Galaxy study combines topics in areas such as Stars and Emission spectrum. His study in Quasar is interdisciplinary in nature, drawing from both Supermassive black hole and Blazar.

He most often published in these fields:

  • Astrophysics (75.91%)
  • Astronomy (32.85%)
  • Redshift (30.66%)

What were the highlights of his more recent work (between 2015-2020)?

  • Astrophysics (75.91%)
  • Redshift (30.66%)
  • Astronomy (32.85%)

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

His primary scientific interests are in Astrophysics, Redshift, Astronomy, Galaxy and Quasar. His Astrophysics research is multidisciplinary, relying on both Spectral line and X-ray. His Redshift study integrates concerns from other disciplines, such as Cosmology, Infrared, Galaxy cluster and Photometry.

His Planck and Galactic plane study, which is part of a larger body of work in Astronomy, is frequently linked to Field, bridging the gap between disciplines. The various areas that D. Stern examines in his Galaxy study include Line-of-sight, Spectrograph and Emission spectrum. D. Stern combines subjects such as Accretion, Astrometry, Telescope and Gravitational lens with his study of Quasar.

Between 2015 and 2020, his most popular works were:

  • Physical properties of 15 quasars at $z\gtrsim 6.5$ (159 citations)
  • A New Population of Compton-Thick AGN Identified Using the Spectral Curvature Above 10 keV (88 citations)
  • NuSTAR and Swift observations of the very high state in GX 339-4: Weighing the black hole with X-rays (71 citations)

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

  • Astronomy
  • Astrophysics
  • Galaxy

The scientist’s investigation covers issues in Astrophysics, Redshift, Spectral line, Galaxy and X-ray. His Astrophysics research includes themes of Astronomy and Photon. His research integrates issues of Gravitation and Accretion in his study of Spectral line.

His Hydrostatic equilibrium research extends to the thematically linked field of Galaxy. In his work, Absorption, Rest frame and Active galactic nucleus is strongly intertwined with Luminosity, which is a subfield of X-ray. His biological study spans a wide range of topics, including Accretion, Plasma and Emission spectrum.

This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.

Best Publications

Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report

D. Spergel;N. Gehrels;C. Baltay;D. Bennett.
arXiv: Instrumentation and Methods for Astrophysics (2015)

1137 Citations

The Rest-Frame UV Luminosity Density of Star-Forming Galaxies at Redshifts z>3.5

M. Giavalisco;M. Dickinson;H. C. Ferguson;S. Ravindranath.
arXiv: Astrophysics (2003)

669 Citations

The unusual afterglow of GRB 980326: evidence for the gamma-ray burst/supernova connection

J. S. Bloom;S. R. Kulkarni;S. G. Djorgovski;A. C. Eichelberger.
arXiv: Astrophysics (1999)

642 Citations

Two bright submillimeter galaxies in a z=4.05 proto-cluster in GOODS-North, and accurate radio-infrared photometric redshifts

E. Daddi;H. Dannerbauer;D. Stern;M. Dickinson.
arXiv: Astrophysics (2008)

562 Citations

Planck 2013 results - XXXII. The updated Planck catalogue of Sunyaev-Zeldovich sources

P. A.R. Ade;N. Aghanim;M. Arnaud;M. Ashdown.
Astronomy and Astrophysics (2015)

462 Citations

Using the Bright Ultra-Hard XMM-Newton Survey to define an IR selection of luminous AGN based on WISE colours

S. Mateos;A. Alonso-Herrero;F. J. Carrera;A. Blain.
arXiv: Cosmology and Nongalactic Astrophysics (2012)

423 Citations

The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models

L.-G. Strolger;A. G. Riess;T. Dahlen;M. Livio.
arXiv: Astrophysics (2004)

413 Citations

Spectroscopic Observations of Lyman-Break Galaxies at Redshift ~ 4, 5 and 6 in the GOODS-South Field

E. Vanzella;M. Giavalisco;M. Dickinson;S. Cristiani.
arXiv: Cosmology and Nongalactic Astrophysics (2009)

351 Citations

LOW-RESOLUTION SPECTRAL TEMPLATES FOR ACTIVE GALACTIC NUCLEI AND GALAXIES FROM 0.03 TO 30 μm

R. J. Assef;C. S. Kochanek;M. Brodwin;R. Cool.
The Astrophysical Journal (2010)

327 Citations

Galaxy Clusters around radio-loud AGN at 1.3 < z < 3.2 as seen by Spitzer

D. Wylezalek;A. Galametz;D. Stern;J. Vernet.
arXiv: Cosmology and Nongalactic Astrophysics (2013)

289 Citations

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