New Constraints on ΩM, ΩΛ, and w from an Independent Set of 11 High-Redshift Supernovae Observed with the Hubble Space Telescope

2003

368 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/c9751956f8ee59a6e9c87914c89eb0a053283c84

Citations in the corpus

• Scrutinizing Exotic Cosmological Models Using ESSENCE Supernova Data Combined with Other Cosmological Probes (2007, positive): “MODELS Hithertho, all measurements ofw have been consistent with a cosmological constant,w = −1 (e.g., Garnavich et al. 1998; Tonry et al. 2003; Knop et al. 2003; Hannestad & Mörtsell 2004; Eisenstein et al. 2005; Astier et al. 2006; Spergel et al. 2006; Riess et al. 2007; Wood-Vasey et al. 2007).”
• Is there supernova evidence for dark energy metamorphosis (2003, positive): “…values for the equation of state (w −1) of phantom.6 Caldwell’s results have since been confirmed by larger and betterquality SNe data sets – for instance Knop et al. (2003) find that, in the absence of priors being placed on 0m, the DE equation of state has a 99 per cent confidence limit of being…”
• The ESSENCE Supernova Survey: Survey Optimization, Observations, and Supernova Photometry (2007, neutral): “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).”
• Safety in Numbers: Gravitational Lensing Degradation of the Luminosity Distance-Redshift Relation (2004, positive): “Indeed, observations of supernovae play a major role in our confidence that the current expansion of the Universe is accelerating (Riess et al. 1998; Perlmutter et al. 1999; Tonry et al. 2003; Knop et al. 2003; Riess et al. 2004).”
• Using Gravitational-Wave Standard Sirens (2005, positive): “One of the major challenges to cosmology for the foreseeable future is to understand ‘‘dark energy,’’ the mysterious component responsible for the apparent accelerating expansion of our universe (Riess et al. 1998; Perlmutter et al. 1999; Tonry et al. 2003; Knop et al. 2003).”
• Cosmological parameters from supernova observations: A critical comparison of three data sets (2003, neutral): “…& Choudhury 2003; Visser 2004; Caresia, Matarrese, & Moscardini 2004; Alcaniz 2004; Wang & Mukherjee 2004; Novello, Perez Bergliaffa, & Salim 2003; Knop et al. 2003; Zhu & Fujimoto 2003; Dev, Jain, & Alcaniz 2004; Gong, Chen, & Duan 2004; Gong & Chen 2004; Gong & Duan 2004; Gong 2004; Bertolami…”
• Improved Distances to Type Ia Supernovae with Multicolor Light-Curve Shapes: MLCS2k2 (2006, positive): “This method has been presented in detail for the B band (Goldhaber et al. 2001) and can be extended straightforwardly to U and V (with R and I posing more difficulty; Nugent et al. 2002; Knop et al. 2003; Nobili et al. 2005; Jha et al. 2006).”
• Determining the Type, Redshift, and Age of a Supernova Spectrum (2006, positive): “1 (Tonry et al. 2003; Knop et al. 2003; Barris et al. 2004), but also at higher redshifts where the universal expansion is in a decelerating phase (Riess et al. 2004).”