Not listed MOTIVATION TO DETECT PROTOPLANETS: THOUSANDS OF GAS-RICH EXOPLANETS ARE KNOWN TODAY. YET UNTIL RECENTLY NONE OF THESE WERE YOUNG FORMING/ACCRETING "PROTOPLANETS". MULTI WAVELENGTH OBSERVATIONS (AO AND JWST) OF SUCH PROTOPLANETS ARE THE BEST APPROACH TO UNRAVELING THE MYSTERY OF PLANET FORMATION. TECHNICAL BACKGROUND OF THE MAGAO INSTRUMENT: THE PI AND HIS TEAM HAVE BUILT AND COMMISSIONED AN ADVANCED ADAPTIVE OPTICS (AO) SYSTEM AT THE 6.5-M MAGELLAN CLAY TELESCOPE AT LAS CAMPANAS OBSERVATORY CHILE. THIS SYSTEM IS CALLED MAGAO (PI LAIRD CLOSE) AND IT USES AN ADAPTIVE SECONDARY MIRROR (ASM) WITH 585 ACTUATORS TO APPLY THE CORRECTION MEASURED BY ITS HIGHORDER PYRAMID WAVEFRONT SENSOR (PWFS) 1000 TIMES EACH SECOND. BECAUSE WE CAN CORRECT AT WAVELENGTHS AS SHORT AS H-ALPHA (656.3 NM) THE MAGAO SYSTEM REGULARLY PRODUCES THE HIGHEST-SPATIAL-RESOLUTION DEEP IMAGES TO DATE. MAGAO HAS BEEN ON-SKY OVER 160 NIGHTS NOW AND HAS BEEN IN REGULAR SCIENCE OPERATIONS AT MAGELLAN FOR 3 YEARS. MAGAO IS THE ONLY TELESCOPIC SYSTEM (ON THE GROUND OR SPACE) THAT HAS PUBLISHED HIGH SPATIAL RESOLUTION ($48) 8/2/22 P00005 MOTIVATION TO DETECT PROTOPLANETS: THOUSANDS OF GAS-RICH EXOPLANETS ARE KNOWN TODAY. YET, UNTIL RECENTLY, NONE OF THESE WERE YOUNG FORMING/ACCRETING "PROTOPLANETS". MULTI WAVELENGTH OBSERVATIONS (AO AND JWST) OF SUCH PROTOPLANETS ARE THE BEST APPROACH TO UNRAVELING THE MYSTERY OF PLANET FORMATION. TECHNICAL BACKGROUND OF THE MAGAO INSTRUMENT: THE PI AND HIS TEAM HAVE BUILT AND COMMISSIONED AN ADVANCED ADAPTIVE OPTICS (AO) SYSTEM AT THE 6.5-M MAGELLAN CLAY TELESCOPE AT LAS CAMPANAS OBSERVATORY, CHILE. THIS SYSTEM IS CALLED MAGAO (PI LAIRD CLOSE) AND IT USES AN ADAPTIVE SECONDARY MIRROR (ASM) WITH 585 ACTUATORS TO APPLY THE CORRECTION MEASURED BY ITS HIGHORDER PYRAMID WAVEFRONT SENSOR (PWFS) 1000 TIMES EACH SECOND. BECAUSE WE CAN CORRECT AT WAVELENGTHS AS SHORT AS H-ALPHA (656.3 NM), THE MAGAO SYSTEM REGULARLY PRODUCES THE HIGHEST-SPATIAL-RESOLUTION DEEP IMAGES TO DATE. MAGAO HAS BEEN ON-SKY OVER 160 NIGHTS NOW AND HAS BEEN IN REGULAR SCIENCE OPERATIONS AT MAGELLAN FOR 3 YEARS. MAGAO IS THE ONLY TELESCOPIC SYSTEM (ON THE GROUND OR SPACE) THAT HAS PUBLISHED HIGH SPATIAL RESOLUTION Funding Only Action ($48) 8/2/22 Not listed MOTIVATION TO DETECT PROTOPLANETS: THOUSANDS OF GAS-RICH EXOPLANETS ARE KNOWN TODAY. YET UNTIL RECENTLY NONE OF THESE WERE YOUNG FORMING/ACCRETING "PROTOPLANETS". MULTI WAVELENGTH OBSERVATIONS (AO AND JWST) OF SUCH PROTOPLANETS ARE THE BEST APPROACH TO UNRAVELING THE MYSTERY OF PLANET FORMATION. TECHNICAL BACKGROUND OF THE MAGAO INSTRUMENT: THE PI AND HIS TEAM HAVE BUILT AND COMMISSIONED AN ADVANCED ADAPTIVE OPTICS (AO) SYSTEM AT THE 6.5-M MAGELLAN CLAY TELESCOPE AT LAS CAMPANAS OBSERVATORY CHILE. THIS SYSTEM IS CALLED MAGAO (PI LAIRD CLOSE) AND IT USES AN ADAPTIVE SECONDARY MIRROR (ASM) WITH 585 ACTUATORS TO APPLY THE CORRECTION MEASURED BY ITS HIGHORDER PYRAMID WAVEFRONT SENSOR (PWFS) 1000 TIMES EACH SECOND. BECAUSE WE CAN CORRECT AT WAVELENGTHS AS SHORT AS H-ALPHA (656.3 NM) THE MAGAO SYSTEM REGULARLY PRODUCES THE HIGHEST-SPATIAL-RESOLUTION DEEP IMAGES TO DATE. MAGAO HAS BEEN ON-SKY OVER 160 NIGHTS NOW AND HAS BEEN IN REGULAR SCIENCE OPERATIONS AT MAGELLAN FOR 3 YEARS. MAGAO IS THE ONLY TELESCOPIC SYSTEM (ON THE GROUND OR SPACE) THAT HAS PUBLISHED HIGH SPATIAL RESOLUTION $0 12/11/20 P00004 MOTIVATION TO DETECT PROTOPLANETS: THOUSANDS OF GAS-RICH EXOPLANETS ARE KNOWN TODAY. YET, UNTIL RECENTLY, NONE OF THESE WERE YOUNG FORMING/ACCRETING "PROTOPLANETS". MULTI WAVELENGTH OBSERVATIONS (AO AND JWST) OF SUCH PROTOPLANETS ARE THE BEST APPROACH TO UNRAVELING THE MYSTERY OF PLANET FORMATION. TECHNICAL BACKGROUND OF THE MAGAO INSTRUMENT: THE PI AND HIS TEAM HAVE BUILT AND COMMISSIONED AN ADVANCED ADAPTIVE OPTICS (AO) SYSTEM AT THE 6.5-M MAGELLAN CLAY TELESCOPE AT LAS CAMPANAS OBSERVATORY, CHILE. THIS SYSTEM IS CALLED MAGAO (PI LAIRD CLOSE) AND IT USES AN ADAPTIVE SECONDARY MIRROR (ASM) WITH 585 ACTUATORS TO APPLY THE CORRECTION MEASURED BY ITS HIGHORDER PYRAMID WAVEFRONT SENSOR (PWFS) 1000 TIMES EACH SECOND. BECAUSE WE CAN CORRECT AT WAVELENGTHS AS SHORT AS H-ALPHA (656.3 NM), THE MAGAO SYSTEM REGULARLY PRODUCES THE HIGHEST-SPATIAL-RESOLUTION DEEP IMAGES TO DATE. MAGAO HAS BEEN ON-SKY OVER 160 NIGHTS NOW AND HAS BEEN IN REGULAR SCIENCE OPERATIONS AT MAGELLAN FOR 3 YEARS. MAGAO IS THE ONLY TELESCOPIC SYSTEM (ON THE GROUND OR SPACE) THAT HAS PUBLISHED HIGH SPATIAL RESOLUTION Other Administrative Action $0 12/11/20 P00003 MOTIVATION TO DETECT PROTOPLANETS: THOUSANDS OF GAS-RICH EXOPLANETS ARE KNOWN TODAY. YET, UNTIL RECENTLY, NONE OF THESE WERE YOUNG FORMING/ACCRETING "PROTOPLANETS". MULTI WAVELENGTH OBSERVATIONS (AO AND JWST) OF SUCH PROTOPLANETS ARE THE BEST APPROACH TO UNRAVELING THE MYSTERY OF PLANET FORMATION. TECHNICAL BACKGROUND OF THE MAGAO INSTRUMENT: THE PI AND HIS TEAM HAVE BUILT AND COMMISSIONED AN ADVANCED ADAPTIVE OPTICS (AO) SYSTEM AT THE 6.5-M MAGELLAN CLAY TELESCOPE AT LAS CAMPANAS OBSERVATORY, CHILE. THIS SYSTEM IS CALLED MAGAO (PI LAIRD CLOSE) AND IT USES AN ADAPTIVE SECONDARY MIRROR (ASM) WITH 585 ACTUATORS TO APPLY THE CORRECTION MEASURED BY ITS HIGHORDER PYRAMID WAVEFRONT SENSOR (PWFS) 1000 TIMES EACH SECOND. BECAUSE WE CAN CORRECT AT WAVELENGTHS AS SHORT AS H-ALPHA (656.3 NM), THE MAGAO SYSTEM REGULARLY PRODUCES THE HIGHEST-SPATIAL-RESOLUTION DEEP IMAGES TO DATE. MAGAO HAS BEEN ON-SKY OVER 160 NIGHTS NOW AND HAS BEEN IN REGULAR SCIENCE OPERATIONS AT MAGELLAN FOR 3 YEARS. MAGAO IS THE ONLY TELESCOPIC SYSTEM (ON THE GROUND OR SPACE) THAT HAS PUBLISHED HIGH SPATIAL RESOLUTION Funding Only Action $94.7k 3/20/20