2009 - Dannie Heineman Prize for Astrophysics, American Astronomical Society
2004 - Fellow of the Royal Society, United Kingdom
1988 - Fellow of American Physical Society (APS) Citation For incisive theoretical studies of the interstellar medium and intergalactic medium
1983 - Fellow of Alfred P. Sloan Foundation
His primary areas of investigation include Astrophysics, Redshift, Astronomy, Galaxy and Star formation. His research links Spectral line with Astrophysics. Lennox L. Cowie has researched Redshift in several fields, including Wavelength, Luminosity and Galaxy formation and evolution.
His Galaxy research includes themes of Telescope and Spectrograph. The Star formation study combines topics in areas such as Sky, Extragalactic background light and Solar mass. His work on Hubble Ultra-Deep Field as part of general Hubble Deep Field research is often related to Flux, thus linking different fields of science.
The scientist’s investigation covers issues in Astrophysics, Galaxy, Redshift, Astronomy and Star formation. Hubble Deep Field, Luminous infrared galaxy, Luminosity, Active galactic nucleus and Galaxy formation and evolution are the subjects of his Astrophysics studies. In the field of Hubble Deep Field, his study on Hubble Ultra-Deep Field overlaps with subjects such as Field.
He interconnects Stars and Emission spectrum in the investigation of issues within Galaxy. His Redshift research integrates issues from Spectral line, Equivalent width and Quasar. His work in Star formation is not limited to one particular discipline; it also encompasses Solar mass.
Lennox L. Cowie mainly focuses on Astrophysics, Galaxy, Redshift, Astronomy and Active galactic nucleus. His Galaxy formation and evolution, Luminous infrared galaxy and Extragalactic background light study, which is part of a larger body of work in Astrophysics, is frequently linked to Flux, bridging the gap between disciplines. His Galaxy formation and evolution study deals with Equivalent width intersecting with Extinction.
His Redshift research is multidisciplinary, incorporating elements of Line, Metallicity, Universe and Continuum. His research integrates issues of Stars and Very-long-baseline interferometry in his study of Active galactic nucleus. His Star formation study incorporates themes from Quasar and Sigma.
His scientific interests lie mostly in Astrophysics, Galaxy, Redshift, Astronomy and Submillimeter Array. His study involves Active galactic nucleus, Luminous infrared galaxy, Stars, Extragalactic background light and Luminosity, a branch of Astrophysics. His study in Luminosity is interdisciplinary in nature, drawing from both Extinction and Equivalent width.
A large part of his Galaxy studies is devoted to James Clerk Maxwell Telescope. His Redshift research includes elements of Star formation, Dark energy and Dark matter. His studies deal with areas such as Photometric redshift and Interferometry as well as Submillimeter Array.
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.
New Insight on Galaxy Formation and Evolution From Keck Spectroscopy of the Hawaii Deep Fields
Lennox L. Cowie;Antoinette Songaila;Esther M. Hu;J. G. Cohen.
The Astronomical Journal (1996)
The Chandra Deep Field North Survey. XIII. 2 Ms Point-Source Catalogs
D. M. Alexander;F. E. Bauer;W. N. Brandt;D. P. Schneider.
The Astronomical Journal (2003)
Dusty star forming galaxies at high redshift
A. J. Barger;L. L. Cowie;D. B. Sanders;E. Fulton.
arXiv: Astrophysics (1998)
Resolving the extragalactic hard X-ray background
R. F. Mushotzky;L. L. Cowie;A. J. Barger;K. A. Arnaud;K. A. Arnaud.
Nature (2000)
The Cosmic evolution of hard x-ray selected active galactic nuclei
A. J. Barger;A. J. Barger;L. L. Cowie;R. F. Mushotzky;Y. Yang;Y. Yang.
The Astronomical Journal (2005)
Caltech Faint Galaxy Redshift Survey. X. A Redshift Survey in the Region of the Hubble Deep Field North
Judith G. Cohen;David W. Hogg;David W. Hogg;Roger Blandford;Lennox L. Cowie.
The Astrophysical Journal (2000)
Deuterium abundance and background radiation temperature in high-redshift primordial clouds
A. Songaila;A. Songaila;L. L. Cowie;L. L. Cowie;C. J Hogan;M. Rugers.
Nature (1994)
Optical and Infrared Properties of the 2 Ms Chandra Deep Field North X-Ray Sources
A. J. Barger;A. J. Barger;L. L. Cowie;P. Capak;D. M. Alexander.
The Astronomical Journal (2003)
The Density of Lyman-alpha Emitters at Very High Redshift
Esther M. Hu;Lennox L. Cowie;Richard G. McMahon.
arXiv: Astrophysics (1998)
HIGH-Z LYALPHA EMITTERS. I. A BLANK-FIELD SEARCH FOR OBJECTS NEAR REDSHIFT Z = 3.4 IN AND AROUND THE HUBBLE DEEP FIELD AND THE HAWAII DEEP FIELD SSA 22
Lennox L. Cowie;Lennox L. Cowie;Lennox L. Cowie;Esther M. Hu;Esther M. Hu.
The Astronomical Journal (1998)
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