Editing Lowell Observatory Near-Earth-Object Search (section)

== Technique ==

Asteroids were found by obtaining four pictures (frames) of the same region of sky, each frame temporally separated by 15 to 30 minutes. The set of four frames were then submitted to reduction software which located all star-like sources on the frame and identified sources that moved with asteroid-like motion. The observer visually examined all asteroid detections that had motion different from a typical main-belt asteroid. Human examination was required because most putative NEO detections were not real but some kind of imaging artifact.

All asteroid positions were converted to [[equatorial coordinates]]. Various USNO star catalogs<ref>{{Cite web |url=http://www.nofs.navy.mil/data/fchpix/ |title=USNO Image and Catalogue Archive<!-- Bot generated title --> |access-date=2008-03-02 |archive-url=https://web.archive.org/web/20171104204050/http://www.nofs.navy.mil/data/fchpix/ |archive-date=2017-11-04 |url-status=dead }}</ref> were used for this conversion until 2007. Then the [[Sloan Digital Sky Survey]] catalog was used, along with supplemental information from the Carlsberg Catalog<ref>[http://www.ast.cam.ac.uk/~dwe/SRF/cmc14.html CMC14<!-- Bot generated title -->]</ref> and the [[2MASS]] catalog. Asteroid brightness was converted to standard [[visual magnitude]]. These data, along with the time of the observations, were sent to the [[Minor Planet Center]] (MPC) from which they were distributed to the scientific community. Potential near-Earth objects were handled expeditiously so that other observers could locate the asteroid on the same night and make further observations.

Telescope operation was automated to the extent that the survey could be run all night without observer intervention. However, the telescope was seldom operated in the automatic mode because an observer was required to reduce data promptly and to correct any malfunctions that might have occurred.