C
Charles C. Steidel
Researcher at California Institute of Technology
Publications - 502
Citations - 75451
Charles C. Steidel is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 141, co-authored 486 publications receiving 72242 citations. Previous affiliations of Charles C. Steidel include University of California, Berkeley & University of California.
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Journal ArticleDOI
Type Ia supernova discoveries at z > 1 from the Hubble Space Telescope: Evidence for past deceleration and constraints on dark energy evolution
Adam G. Riess,Louis-Gregory Strolger,John L. Tonry,Stefano Casertano,Henry C. Ferguson,Bahram Mobasher,Peter Challis,Alexei V. Filippenko,Saurabh Jha,Weidong Li,Ryan Chornock,Robert P. Kirshner,Bruno Leibundgut,Mark Dickinson,Mario Livio,Mauro Giavalisco,Charles C. Steidel,Txitxo Benítez,Zlatan Tsvetanov +18 more
TL;DR: For a flat universe with a cosmological constant, the transition between the two epochs is constrained to be at z = 0.46 ± 0.13 as mentioned in this paper, and w = -1.02 ± (and w < -0.76 at the 95% confidence level) for an assumed static equation of state of dark energy.
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Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
Adam G. Riess,Louis-Gregory Strolger,John L. Tonry,Stefano Casertano,Henry C. Ferguson,Bahram Mobasher,Peter Challis,Alexei V. Filippenko,Saurabh Jha,Weidong Li,Ryan Chornock,Robert P. Kirshner,Bruno Leibundgut,Mark Dickinson,Mario Livio,Mauro Giavalisco,Charles C. Steidel,Narciso Benítez,Zlatan Tsvetanov +18 more
TL;DR: In this article, the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration was provided by the discovery of 16 Type Ia supernovae with the Hubble Space Telescope (HST).
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High-redshift galaxies in the hubble deep field : colour selection and star formation history to z 4
Piero Madau,Henry C. Ferguson,Mark Dickinson,Mauro Giavalisco,Charles C. Steidel,Andrew S. Fruchter +5 more
TL;DR: In this paper, a sample of star-forming galaxies at 2 ≲z ≲ 4.5 was constructed from the Hubble Deep Field (HDF) images, which is 3 times higher than the local value but still 4 times lower than the rate observed at z ≈ 1.75.
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Lyman Break Galaxies at z>4 and the Evolution of the UV Luminosity Density at High Redshift
TL;DR: In this paper, the authors present an initial results of a survey for star-forming galaxies in the redshift range 3.8 z 4.5 and z 3.23 deg2 to an apparent magnitude of IAB = 25.0.
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Rest-Frame Ultraviolet Spectra of z ∼ 3 Lyman Break Galaxies*
TL;DR: In this article, the authors present the results of a systematic study of the rest-frame UV spectroscopic properties of Lyman break galaxies (LBGs) and isolate some of the major trends in LBG spectra that are least compromised by selection effects.