Twenty-Three High-Redshift Supernovae from the Institute for Astronomy Deep Survey: Doubling the Supernova Sample at z > 0.7

By B. Barris, J. Tonry, S. Blondin, P. Challis, Ryan Chornock, A. Clocchiatti, A. Filippenko, P. Garnavich, S. Holland, S. Jha and 22 more. 2004

350 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/b4389e76777b475ce13209cb3d00a4020041fd3e

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Citations in the corpus

Is there supernova evidence for dark energy metamorphosis (2003, methodology): “…the techniques developed in Saini et al. (2000), Sahni et al. (2003) to a new data set consisting of 172 SNe from Tonry et al. (2003) and an additional 22 SNe from Barris et al. (2004) we show that the DE equation of state which best fits the data evolves from w 0 at z 1 to −1.2 w −1 today.”
Cosmological parameters from supernova observations: A critical comparison of three data sets (2003, methodology): “For completeness, we describe the data sets in detail: (i) TONRY: In this data set we start with the 230 data points listed in Tonry et al. (2003) alongwith the 23 points from Barris et al. (2004).”
New Hubble Space Telescope Discoveries of Type Ia Supernovae at z ≥ 1: Narrowing Constraints on the Early Behavior of Dark Energy (2006, background): “Increasingly incisive samples of SNe Ia at z < 1 have reinforced the significance of this result (Tonry et al. 2003; Knop et al. 2003; Barris et al. 2004; Conley et al. 2006; Astier et al. 2006).”
f(R) Theories Of Gravity (2008, background): “…on f(R) models derives from the need to explain the present acceleration of the universe discovered with supernovae of type Ia (Astier et al., 2006; Barris et al., 2004; Filippenko and Riess, 1998; Knop et al., 2003; Perlmutter et al., 1998; Riess et al., 1998, 1999, 2004; Schmidt et al., 1998;…”
The ESSENCE Supernova Survey: Survey Optimization, Observations, and Supernova Photometry (2007, background): “The observation of acceleration from SNe Ia is the unique clue that indicates that this component must have negative pressure (Riess et al. 1998, 2001, 2004, 2007; Perlmutter et al. 1999; Tonry et al. 2003; Knop et al. 2003; Barris et al. 2004; Clocchiatti et al. 2006; Astier et al. 2006).”
Hubble Space Telescope and Ground-based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications (2005, methodology): “Considering only the SNe in Riess et al. (1998b), Tonry et al. (2003), and Barris et al. (2004), the mean distance modulus is 42:39 0:08 (1 uncertainty), for a weighted mean redshift of, again, 0.48.”
SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 < z < 1.12 AND THE UNION2 COMPILATION (2010, methodology): “…has successfully been used for high-precision optical and infrared follow-up of SNe discovered from the ground (Knop et al. 2003; Tonry et al. 2003; Barris et al. 2004; Nobili et al. 2009), and, by using the Advanced Camera for Surveys (ACS), to carry out both search and follow-up from space…”
UBVRI Light Curves of 44 Type Ia Supernovae (2005, background): “…with applications of these exquisite distance idicators ranging from our galactic neighbors to establish the Hubble constant, to halfway across the observable Universe to uncover cosmic deceleration and acceleration (Riess et al. 2004; Barris et al. 2004; Knopet al. 2003 and references therein).”
Type Ia Supernovae Are Good Standard Candles in the Near Infrared: Evidence from PAIRITEL (2007, background): “The history of cosmic expansion has been traced out to redshift z 1 (Tonry et al. 2003; Knop et al. 2003; Barris et al. 2004).”