Palomar–Leiden survey

The Palomar–Leiden survey (PLS) was a successful

The original PLS-survey took place in 1960, and was followed by three Palomar–Leiden Trojan survey campaigns, launched in 1971, 1973 and 1977. Its principal investigators were the astronomers

PLS was one of the most productive minor planet surveys ever conducted: five new

• P-L  Palomar–Leiden survey (1960), discovered more than 2,000 asteroids (1,800 with orbital information) in eleven nights. This number was increased to 2,400 including 19 Trojans after further analysis of the plates.[3] A total of 130 photographic plates were taken.
• T-1   the first Palomar–Leiden Trojan survey (1971), discovered approximately 500 asteroids including 4 Jupiter trojans in nine nights.^[3] A total of 54 photographic plates were taken.
• T-2   the second Palomar–Leiden Trojan survey (1973), discovered another 1,200 asteroids including 18 Jupiter trojans in eight nights.^[3] A total of 78 photographic plates were taken.
• T-3   the third Palomar–Leiden Trojan survey (1977), discovered an additional 1,400 asteroids including 24 Jupiter trojans in seven nights.^[3] A total of 68 photographic plates were taken.

Naming

The discovered bodies received a custom provisional designation. For example, the asteroid

Surveys

The PLS was originally intended as an extension of the Yerkes–McDonald asteroid survey (1950–1952), which was initiated by Dutch–American astronomer Gerard Kuiper. While this survey was limited to a magnitude of up to 16, PLS could study minor planets up to a visual magnitudes of 20. However, it only covered a portion of the ecliptic about the vernal equinox, with the target areas selected to minimize the number of background stars.

Photographic plates taken by Tom Gehrels at the Lunar and Planetary Laboratory in Arizona using the 48-inch Schmidt camera at Palomar Observatory. The orbital elements were computed at the Cincinnati Observatory, which was the site of the Minor Planet Center at the time. All other aspects of the program were conducted at Leiden Observatory in the Netherlands.

Original PLS-survey

During September and October 1960, the first 130 photographic plates were taken, with each plate spanning 35.6 × 35.6 cm and having a limiting magnitude of 20.5. The observed region covered an area of 36° × 18°. The Zeiss blink comparator from the Heidelberg Observatory was adapted to perform blink comparison of the plates. This resulted in the discovery of a large number of asteroids; typically 200–400 per plate. A subset of these objects had sufficient data to allow orbital elements to be computed. The mean error in their positions was as small as 0.6″, which corresponded to 0.009 mm on the plates. The resulting mean error in magnitude estimation was 0.19.^[2]

Trojan surveys

The third Palomar–Leiden Trojan survey was performed in 1977, resulting in the discovery of 26 Jupiter trojans.^[4] In total, there were three Trojan campaigns, designated T-1, T-2, and T-3, which discovered 3570 asteroids.^{[citation needed]} Another small extension of the survey was reported in 1984, adding 170 new objects for a combined total of 2,403.^[5]

List of discovered minor planets