Question: Which survey in 2010 recommended the The Wide Field Infrared Survey Telescope as the top priority for astronomy?
Context: The Astronomy and Astrophysics Decadal Survey is a review of astronomy and astrophysics literature produced approximately every ten years by the National Research Council of the National Academy of Sciences in the United States.  The report surveys the current state of the field, identifies research priorities, and makes recommendations for the coming decade.  The editing committee is informed by topical panels and subcommittees, dedicated conferences, and direct community input in the form of white papers summarizing the state of the art in each subdiscipline.  The most recent report, Astro2010, is currently available in prepublication form, with the final version set for release before the end of 2010. The Wide Field Infrared Explorer (WIRE) was a satellite launched on March 5, 1999, on the Pegasus XL rocket into polar orbit between 409 and above the Earth's surface.  WIRE was intended to be a four-month infrared survey of the entire sky at 21-27 micrometres and 9-15 micrometres, specifically focusing on starburst galaxies and luminous protogalaxies. Tod R. Lauer (born 1957) is an American astronomer on the research staff of the National Optical Astronomy Observatory.  He was a member of the Hubble Space Telescope Wide Field and Planetary Camera team, and is a founding member of the Nuker Team.  His research interests includes observational searches for massive black holes in the centers of galaxies, the structure of elliptical galaxies, stellar populations, large-scale structure of the universe, and astronomical image processing.  He was the Principal Investigator of the Destiny JDEM concept study, one of the precursors to the Wide Field Infrared Survey Telescope mission.  Asteroid 3135 Lauer is named for him.  He appears in an episode of the documentary series Naked Science.  He joined the New Horizons Pluto team in order to apply his extensive experience with deep space imaging to the New Horizons data, yielding significantly clearer and mathematically accurate images of Pluto and Charon. The VISTA (Visible and Infrared Survey Telescope for Astronomy) is a wide-field reflecting telescope with a 4.1 metre mirror, located at the Paranal Observatory in Chile.  It is operated by the European Southern Observatory and started science operations in December 2009.  VISTA is a survey telescope working at infrared wavelengths, and is by far the largest telescope in the world dedicated to surveying the sky at near-infrared wavelengths.  The telescope has only one instrument: VIRCAM, the Vista InfraRed CAMera.  This is a 3-tonne camera containing 16 special detectors sensitive to infrared light, with a combined total of 67 million pixels. The Infrared Science Archive (IRSA) curates the science products of NASA's infrared and submillimeter projects, such as the Spitzer Space Telescope, the Wide-field Infrared Survey Explorer (WISE), the Infrared Astronomical Satellite (IRAS), and the Two Micron All-Sky Survey (2MASS).  IRSA also serves data from infrared and submillimeter European Space Agency missions with NASA participation, including the Infrared Space Observatory (ISO), Planck, and the Herschel Space Observatory.  s of 2014 , IRSA provides access to more than 20 billion astronomical measurements, including all-sky coverage in 20 bands, spanning wavelengths from 1 micron to 10 millimeters.  Approximately 10% of all refereed astronomical journal articles cite data sets curated by IRSA. The Wide Field Infrared Survey Telescope (WFIRST) is a future infrared space observatory that was recommended in 2010 by United States National Research Council Decadal Survey committee as the top priority for the next decade of astronomy.  On February 17, 2016, WFIRST was formally designated as a mission by NASA. The Kunlun Dark Universe Survey Telescope, also known as KDUST, is a planned large survey telescope to be installed at the Chinese Antarctic Kunlun Station located at Dome A ice plateau in Antarctica in the second half of the 2010s.  It is intended to take advantage of the exceptional observation conditions due to low temperature, clean air quality and low disturbances which reduce background noises for infrared observations. The UKIRT Infrared Deep Sky Survey or UKIDSS is an astronomical survey conducted using the WFCAM wide field camera on the United Kingdom Infrared Telescope on Mauna Kea in Hawaii.  Survey observations were commenced in 2005. The VLT Survey Telescope (VST) is the latest telescope to be added to ESO’s Paranal Observatory in the Atacama Desert of northern Chile.  It is housed in an enclosure immediately adjacent to the four Very Large Telescope (VLT) Unit Telescopes on the summit of Cerro Paranal.  The VST is a wide-field survey telescope with a field of view twice as broad as the full Moon.  It is the largest telescope in the world designed to exclusively survey the sky in visible light. David Nathaniel Spergel (born March 25, 1961), is an American theoretical astrophysicist and Princeton University professor known for his work on the WMAP (Wilkinson Microwave Anisotropy Probe) mission.  Spergel is a MacArthur Fellow.  He is a member of the NASA Advisory Council and is chair of the Space Studies Board.  He was once the W.M. Keck distinguished visiting professor at the Institute for Advanced Study in Princeton, New Jersey.  He was part of the team that originated the WMAP mission and designed the spacecraft, and has worked on deciphering the data that it beams back from space.  Spergel is playing a leading role in developing the WFIRST(Wide Field Infrared Space Telescope), a multibillion-dollar space mission planned for launch in the mid-2020s.  Spergel is the Charles A Young Professor of Astronomy and a member of the National Academy of Sciences.  Spergel is the Founding Director of the Center for Computational Astrophysics.  He
Answer: Astronomy and Astrophysics Decadal Survey