Weak-Lensing Results from the 75 Square Degree Cerro Tololo Inter-American Observatory Survey

By M. Jarvis, G. Bernstein, P. Fischer, D. Smith, B. Jain, J. Tyson, D. Wittman. 2003

145 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/6cec262e350c8610b33287a86fd40564ef3051d6

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Citations in the corpus

Very weak lensing in the CFHTLS Wide: Cosmology from cosmic shear in the linear regime (2007, result): “It is also interesting to notice that our results are in excellent agreement with the CTIO survey (Jarvis et al. 2003, 2006).”
Detection of large-scale intrinsic ellipticity—density correlation from the Sloan Digital Sky Survey and implications for weak lensing surveys (2005, background): “…1999; Bartelmann & Schneider 2001; Refregier 2003a) following detection of the two-point function of the lensing-induced shear by several groups (Bacon et al. 2000; Van Waerbeke et al. 2000; Rhodes et al. 2001; Hoekstra et al. 2002; Van Waerbeke et al. 2002; Brown et al. 2003; Jarvis et al. 2003).”
The Galaxy-Mass Correlation Function Measured from Weak Lensing in the Sloan Digital Sky Survey (2003, methodology): “…& Gaztañaga 1999; Szapudi et al. 2002; Verde et al. 2002), from the cosmic shear weak lensing power spectrum (Hoekstra, Yee, & Gladders 2002b; Jarvis et al. 2003), and from comparison of the 2dF galaxy power spectrum (Percival et al. 2001) with the WMAP cosmic microwave background (CMB)…”
Cosmological constraints from the 100-deg2 weak-lensing survey (2007, background): “…competitive constraints on cosmological parameters (Hoekstra, Yee & Gladders 2002b; Bacon et al. 2003; Brown et al. 2003; Hamana et al. 2003; Jarvis et al. 2003; Rhodes et al. 2004; Massey et al. 2005; Heymans et al. 2005; Van Waerbeke, Mellier & Hoekstra 2005; Hoekstra et al. 2006;…”
The Dark Side of the Halo Occupation Distribution (2003, methodology): “This normalization is suggested by several recent measurements (e.g., Borgani et al. 2001; Pierpaoli et al. 2001; Lahav et al. 2002; Schuecker et al. 2003; Jarvis et al. 2003).”
Evidence of the accelerated expansion of the Universe from weak lensing tomography with COSMOS (2009, background): “Larger surveys have significantly reduced statistical uncertainties (e.g. Hoekstra et al. 2002; Brown et al. 2003; Jarvis et al. 2003; Massey et al. 2005; Van Waerbeke et al. 2005; Hoekstra et al. 2006; Semboloni et al. 2006; Hetterscheidt et al. 2007; Fu et al. 2008), while tests on simulated data…”
COSMOS: Three-dimensional Weak Lensing and the Growth of Structure (2007, background): “…measured the projected two-dimensional power spectrum of the large-scale mass distribution and drawn competitive constraints on cosmological parameters (Brown et al. 2003; Bacon et al. 2003; Hamana et al. 2003; Jarvis et al. 2003; VanWaerbeke et al. 2005; Massey et al. 2005; Hoekstra et al. 2006).”
Systematic errors in future weak-lensing surveys: requirements and prospects for self-calibration (2005, background): “…imposes strong constraints on the matter density relative to critical ΩM and the amplitude of mass fluctuations σ8 (Hoekstra, Yee & Gladders 2002, Jarvis et al. 2003, Rhodes et al. 2004, Heymans et al. 2004; for a review see Refregier 2003), as well as the first interesting constraints on the…”
Halo Substructure and the Power Spectrum (2002, methodology): “…rms fluctuation amplitude on a length scale of 8 h−1 Mpc ), numerous recent studies relying on similar techniques, advocate rather “low” values of σ8 ∼ 0.7 − 0.8 (Jarvis et al. 2003; Bahcall et al. 2003; Schuecker et al 2003; Pierpaoli et al. 2003; Viana et al. 2002; Brown et al. 2002; Allen et…”
The DES Science Verification weak lensing shear catalogues (2015, result): “Most of our null tests were similar to ones that have been performed in previous analyses (cf. e.g. Jarvis et al. 2003; Schrabback et al. 2010; Velander et al. 2011; Heymans et al. 2012b; Jee et al. 2013; Kuijken et al. 2015).”
Cosmological parameters from lensing power spectrum and bispectrum tomography (2003, methodology): “…along the line of sight by measuring the correlated distortion of images of distant galaxies (see Mellier 1999;Bartelmann & Schneider 2001 for review; and also see, e.g., Hamana et al. 2003, Jarvis et al. 2003, Van Waerbeke & Mellier 2003 and references th rein for the state of observations).”
The Shear Testing Programme – I. Weak lensing analysis of simulated ground-based observations (2005, background): “This approach, taken by Jarvis et al. (2003), demands that a source is detected in at least two of the four exposures taken of each field.”
Observational probes of cosmic acceleration (2012, methodology): “The first wide-shallow surveys were also carried out from the ground: the 53 deg2 Red-Sequence Cluster Survey (Hoekstra et al., 2002) and the 75 deg2 CTIO survey (Jarvis et al., 2003).”
The shear power spectrum from the COMBO-17 survey (2002, background): “Since this paper was submitted, two other groups have presented cosmic shear results yielding somewhat lower valuesof σ8 – Jarvis et al. 2003 measure the shear signal from the 75 sq. degree CTIO survey and find a power spectrum normalisation of σ8 = 0.71 while Hamana et al. 2002 have used the…”