The Microwave Anisotropy Probe (MAP) Mission

By C. Bennett, M. Bay, Mark Halpern, Gary F. Hinshaw, C. Jackson, N. Jarosik, Alan Kogut, M. Limon, S. Meyer, L. Page and 5 more. 2002

198 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/f730c230578c8413360a9533c0330dae703ce903

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Citations in the corpus

• SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: POWER SPECTRA AND WMAP-DERIVED PARAMETERS (2010, methodology): “The Wilkinson Microwave Anisotropy Probe (WMAP Bennett et al. 2003b,a) is a Medium-Class Explorer (MIDEX) satellite aimed at understanding cosmology through full-sky observations of the cosmic microwave background (CMB).”
• STAR FORMATION IN MASSIVE CLUSTERS VIA THE WILKINSON MICROWAVE ANISOTROPY PROBE AND THE SPITZER GLIMPSE SURVEY (2009, methodology): “The antenna temperature was converted into flux density using the conversion: Fν = 2kBν2 c2 ∆TA (1) whereν is the frequency of the WMAP band,kB is Boltzman’s constant,c is the speed of light, and∆TA is the antenna temperature (Bennett et al. 2003b).”
• Cosmological constraints from a combination of galaxy clustering and lensing – I. Theoretical framework (2012, background): “Various experiments that probe fluctuations in the cosmic microwave background (CMB), most notably the Wilkinson Microwave Anisotropy Probe (WMAP; Bennett et al. 2003) have yielded constraints on various cosmological parameters at the few percent level (Spergel et al. 2003, ⋆ E-mail:…”
• SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: SKY MAPS, SYSTEMATIC ERRORS, AND BASIC RESULTS (2010, background): “An overall description of the mission including instrument nomenclature is contained in Bennett et al. (2003b) and Limon et al. (2010), while details of the optical system and radiometers can be found in Page et al. (2003b) and Jarosik et al. (2003).”
• THE ATACAMA COSMOLOGY TELESCOPE: COSMOLOGICAL PARAMETERS FROM THE 2008 POWER SPECTRUM (2010, methodology): “This is commonly done in CMB analyses for subtracting Galactic components (e.g., Bennett et al. 2003), and has also been used for subtracting the IR point sources (Hall et al. 2010; Lueker et al. 2009).”
• SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP ) OBSERVATIONS: ARE THERE COSMIC MICROWAVE BACKGROUND ANOMALIES? (2010, methodology): “When WMAP data were first released in 2003, an image of the full sky was presented in Galactic coordinates, centered on the Galactic center (Bennett et al. 2003b).”
• NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: FINAL MAPS AND RESULTS (2012, methodology): “We have used the “KpX” series of Galactic masks, described by Bennett et al. (2003c) as a graduated set of sky cuts.”
• SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: PLANETS AND CELESTIAL CALIBRATION SOURCES (2010, background): “The primary goal of the Wilkinson Microwave Anisotropy Probe (WMAP) mission (Bennett et al. 2003b) is to study the cosmic microwave background (CMB) anisotropy, an undertaking that requires detailed knowledge of the instrumental angular response and noise, low systematic errors, and absolute…”
• Radio and millimeter continuum surveys and their astrophysical implications (2009, methodology): “A high quality all-sky CMB temperature map has been provided by the WMAP satellite (Bennett et al. 2003; Hinshaw et al. 2007; Hinshaw & Naeye 2008).”
• The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package (2022, methodology): “For reproducibility, this cosmology may be set to old defaults, such as the Wilkinson Microwave Anisotropy Probe (WMAP) Three Year values.”