Lincoln Near-Earth Asteroid Program (LINEAR)

By G. Stokes, J. Evans, H. Viggh, F. Shelly, E. Pearce. 2000

175 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/2d3bb595a06ee409bb544675694747e5cca189c4

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In Astronomy and Astrophysics

Citations in the corpus

Now You See It, Now You Don't: The Disappearing Central Engine of the Quasar J1011+5442 (2015, methodology): “19.0 18.5 18.0 17.5 17.0 V [ m ag ] 19.0 18.5 18.0 17.5 17.0 V [ m ag ] J1011+5442 was observed regularly between December 2002 and June 2008 as part of the MIT Lincoln Laboratory Lincoln Near-Earth Asteroid Research (LINEAR) survey (Stokes et al. 2000).”
PRELIMINARY RESULTS FROM NEOWISE: AN ENHANCEMENT TO THE WIDE-FIELD INFRARED SURVEY EXPLORER FOR SOLAR SYSTEM SCIENCE (2011, background): “…discover and characterize asteroids and comets have been conducted at visible wavelengths (e.g., the Catalina Sky Survey, the Lincoln Near-Earth Asteroid Research Program, the Near Earth Asteroid Tracking Program, and Spacewatch - Larsen 2007; Stokes et al. 2000; Helin et al. 1997; McMillan 2007).”
The Zwicky Transient Facility: System Overview, Performance, and First Results (2018, methodology): “…(OGLE; Udalski et al. 1992), the All-sky Automated Survey (ASAS; Pojmanski 1997), the Lincoln Near-Earth Asteroid Research survey (LINEAR; Stokes et al. 2000), the Supernova Legacy Survey (SNLS; Astier et al. 2006), Palomar-Quest (Djorgovski et al. 2008), the Catalina Sky Survey (CSS;…”
Dawes Review 6: The Impact of Companions on Stellar Evolution (2016, background): “In addition, surveys designed to detect near Earth objects (e.g., LINEAR, Stokes et al. 2000) are also used to detect transients (Palaversa et al., 2016).”
OSIRIS-REx: Sample Return from Asteroid (101955) Bennu (2017, background): “[Insert Figure 5 here] Asteroid (101955) Bennu was discovered on September 11, 1999 (Williams 1999) by the Lincoln Near-Earth Asteroid Research (LINEAR) survey using a 1.0-m telescope located in Socorro, New Mexico (Stokes et al. 2000).”
THE CATALINA SURVEYS PERIODIC VARIABLE STAR CATALOG (2014, methodology): “Data from the Lowell Observatory NearEarth Object Search (LONEOS; Bowell et al. 1995) has been searched by Miceli et al. (2008), while data from the Lincoln Near-Earth Asteroid Research (LINEAR; Stokes et al. 2000) was analysed by Sesar et al. (2013) and Palaversa et al. (2013).”
A First Catalog of Variable Stars Measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS) (2018, background): “…for optical counterparts of gamma-ray bursts (Akerlof et al. 2000); and asteroid surveys including the Lowell Observatory Near-Earth Object Search (LONEOS; Bowell et al. 1995), the Lincoln Near-Earth Asteroid Research (LINEAR; Stokes et al. 2000) and the Catalina Sky Survey (Larson et al. 2003).”
Bias-corrected population, size distribution, and impact hazard for the near-Earth objects (2004, methodology): “For the third piece, the most extensive set of NEO discovery statistics are provided by the LINEAR survey (Stokes et al., 2000; Stuart, 2001).”
NEOWISE OBSERVATIONS OF NEAR-EARTH OBJECTS: PRELIMINARY RESULTS (2011, background): “Bottke et al. (2002) were limited in their ability to model the NEO population by the fact that the Spacewatch data upon which their results were based provided them only a very small sample of optically-selected NEOs.”
Optical surveys for space debris (2007, methodology): “, to detect and track man-made objects in near-Earth space (Stokes et al. 2000)! Vice versa, the NEAT system in Maui has been successfully used to survey high-altitude artificial objects in space (Africano et al.”