Question: Who wrote the Lunar 100 and had it published in Sky & Telescope?

Context articles: Reber Radio Telescope
Hobby–Eberly Telescope
Exploration of the Moon
Lunar 100
Lunar Precursor Robotic Program
Stony Ridge Observatory
Fine Guidance Sensor (HST)
Sky &amp; Telescope
Lunar phase
Aristarchus (crater)

Reber Radio Telescope is a parabolic radio telescope built by astronomer Grote Reber in his back yard in Illinois in 1937, implementing an earlier proposal of Karl Jansky, the discoverer (1931) of radio waves emanating from the Milky Way.
 It was the second radio telescope ever built (after Jansky's dipole array), and the first parabolic radio telescope, serving as a prototype for the first large dish radio telescopes such as the Green Bank Telescope and Lovell Telescope constructed after World War 2.
 Made of sheet metal with a 31.4 foot (9 meter) aperture and 20 foot (6 meter) focal length, it was the largest parabolic dish in existence at the time.
 Reber was the world's only radio astronomer at the time, and his construction of the telescope and the sky surveys he did with it helped found the field of radio astronomy, revealing radio sources such as Cassiopeia A and Cygnus X-1 for the first time.
The Hobby–Eberly Telescope (HET) is a 10-meter (30-foot) aperture telescope located at the McDonald Observatory.
 It is one of the largest optical telescopes in the world and combines a number of features that differentiate it from most telescope designs, resulting in greatly lowered construction costs.
 For instance, the primary mirror is constructed from 91 hexagonal segments, which is less expensive than manufacturing a single large primary.
 Furthermore, the telescope's main mirror is fixed at a 55° angle and can rotate around its base.
 A target is tracked by moving the instruments at the focus of the telescope; this provides access to about 70–81% of the sky at its location and allows a single target to be tracked for up to two hours.
 The telescope is named for former Texas Lieutenant-Governor Bill Hobby and for Robert E. Eberly, a Penn State benefactor.
The physical exploration of the Moon began when Luna 2, a space probe launched by the Soviet Union, made an impact on the surface of the Moon on September 14, 1959.
 Prior to that the only available means of exploration had been observation from Earth.
 The invention of the optical telescope brought about the first leap in the quality of lunar observations.
 Galileo Galilei is generally credited as the first person to use a telescope for astronomical purposes; having made his own telescope in 1609, the mountains and craters on the lunar surface were among his first observations using it.
The Lunar 100 (L100) is a list of one hundred of the most interesting features to observe on the Moon.
 The list was first described by Charles A. Wood in the article "The Lunar 100" in Sky & Telescope magazine, April 2004.
The Lunar Precursor Robotic Program (LPRP) is a completed program of robotic spacecraft missions which NASA has used to prepare for future human spaceflight missions to the Moon by 2010.
 Two LPRP missions, the Lunar Reconnaissance Orbiter (LRO) and the Lunar Crater Observation and Sensing Satellite (LCROSS), were launched in June 2009.
 The lift off above Cape Canaveral Air Force Station in Florida was successful on June 18, 2009.
 The unmanned Atlas V rocket launched the two space probes towards the Moon, where they will provide a 3-D map and search for water in conjunction with the Hubble Space Telescope.
 The launch date, originally planned for October 2008, was shifted to Thursday from Wednesday (June 17) due to a postponement of the Saturday (June 13) launch of the Space Shuttle Endeavour, resulting from a hydrogen fuel leak.
 This lunar program marks the first United States mission to the Moon in over ten years.
 Neil Armstrong's first step on the Moon occurred July 20, 1969, and this launch was just 32 days shy of the 40th anniversary.
 The actual journey to the Moon will take about four days, at which time the LRO will enter a low orbit around the Moon, while the LCROSS mission will perform a "swing-by" to enter a much different orbit to set up for a collision with the Moon's surface several months later.
 Projected lunar impact of the Centaur and LCROSS spacecraft is on October 9, 2009 at 11:30 UT (7:30 a.m. EDT, 4:30 a.m. PDT), ± 30 minutes.
 The plume from the Centaur impact may be visible through telescopes with apertures as small as 10 to 12 in .
Stony Ridge Observatory is an astronomical observatory built by and for amateur astronomers in the mountains of Los Angeles County, California, in 1957.
 When installed, its 760 mm Newtonian-Cassegrain likely ranked as the largest amateur telescope in the United States.
 The telescope is designed so that one of four Newtonian foci, or a Cassegrain focus, can be used.
 Asteroids 10168 Stony Ridge and 144633 Georgecarroll were discovered at the observatory, and other scientific research (including an extensive lunar photography and mapping project in cooperation with Lockheed upon which the decision on the lunar lander touchdown site was based) has been conducted there.
 The observatory also has a 12 inch Cassegrain telescope and a number of accessory items, including CCD cameras and computer equipment.
Fine Guidance Sensor (FGS) for the Hubble Space Telescope is a system of three instruments used for pointing the telescope in space, and also for astrometry and its related sciences.
 Each FGS uses a combination of optics and electronics to provide for pointing the telescope at a certain location in the sky.
 There are three Hubble FGS, and they have been upgraded over the lifetime of the telescope by manned Space Shuttle missions.
 The instruments can support pointing of 2 milli-arc seconds (units of degree).
 The three FGS are part of the Hubble Space Telescope's pointing control system, aka PCS.
 The FGS function in combination with the Hubble main computer and gyroscopes, with the FGS providing data to the computer as sensors which enables the HST to track astronomical targets.
Sky & Telescope (S&T) is a monthly American magazine covering all aspects of amateur astronomy, including the following:
The lunar phase or phase of the moon is the shape of the illuminated (sunlit) portion of the Moon as seen by an observer on Earth.
 The lunar phases change cyclically as the Moon orbits the Earth, according to the changing positions of the Moon and Sun relative to the Earth.
 The Moon's rotation is tidally locked by the Earth's gravity, therefore the same lunar surface always faces Earth.
 This face is variously sunlit depending on the position of the Moon in its orbit.
 Therefore, the portion of this hemisphere that is visible to an observer on Earth can vary from about 100% (full moon) to 0% (new moon).
 The lunar terminator is the boundary between the illuminated and darkened hemispheres.
 Each of the four "intermediate" lunar phases (see below) is roughly seven days (~7.4 days) but this varies slightly due to the elliptical shape of the Moon's orbit.
 Aside from some craters near the lunar poles such as Shoemaker, all parts of the Moon see around 14.77 days of sunlight, followed by 14.77 days of "night".
 (The side of the Moon facing away from the Earth is sometimes called the "dark side of the Moon", although that is a misnomer.)
Aristarchus, named after the Greek astronomer Aristarchus of Samos, is a prominent lunar impact crater that lies in the northwest part of the Moon's near side.
 It is considered the brightest of the large formations on the lunar surface, with an albedo nearly double that of most lunar features.
 The feature is bright enough to be visible to the naked eye, and displays unusually bright features when viewed through a large telescope.
 It is also readily identified when most of the lunar surface is illuminated by earthshine.
 The crater is larger than the Grand Canyon.