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Table 1:

A list of campaigns where TNOs were found.

$\Omega$ [deg2]
N m50 $\varepsilon$[ ${}^{\circ}$] $\alpha$ [ ${}^{\circ}$] Reference
0.7 2 23.5 0.42 0.84 Irwin et al. (1995)$^\star$
1.2 7 24.85 0.55 1.1 Jewitt & Luu (1995)
3.9 12 24.2 0.99 1.97 Jewitt et al. (1996)$^\star$
4.4 3 23.2 1.05 2.1 Jewitt et al. (1996)$^\star$
0.35 1 24.6 0.30 0.59 Gladman et al. (1998)
0.049 4 25.6 0.11 0.22 Gladman et al. (1998)$^\star$
0.075 0 25 0.14 0.27 Gladman et al. (1998)
51.5 13 23.4 3.6 7.2 Jewitt et al. (1998)
0.01 2 27.94 0.05 0.1 Chiang & Brown (1999)
20.2 3 23.6 2.25 4.5 Trujillo et al. (2000)
1.5 24 24.9$\dots$ 25.9 0.61 1.22 Allen et al. (2001)$^\star$
0.012 0 26.7 0.06 0.11 Gladman et al. (2001)$^\star$
0.31 17 25.93 0.28 0.56 Gladman et al. (2001)$^\star$
73 86 24.0 4.25 8.5 Trujillo et al. (2001a)$^\star$
164 3 21.1 6.40 12.8 Trujillo et al. (2001b)$^\star$
5108 19 20.7 10 255.4 Trujillo & Brown (2003)$^\star$
0.02 3 28.7 0.07 0.14 Bernstein et al. (2004)$^\star$
550 183 22.5 5 55 Elliot et al. (2005)$^\star$
8000 1 big 20$\dots$21 10 400 Larsen et al. (2007)$^\star$
3.0 70 26.4 0.87 1.73 Fraser et al. (2008)
2.8 82 25.7 1.67 1.67 Fuentes & Holman (2008)
0.255 20 26.76 0.25 0.5 Fuentes et al. (2009)
0.33 36 26.8 0.29 0.57 Fraser & Kavelaars (2009)

Notes. The sky area covered ($\Omega$), the number of the objects discovered (N), the limiting magnitude (m50), an estimated half-opening angle  $\varepsilon$, and the ecliptic longitude coverage $\alpha$are given. Papers that provide enough data for objects discovered in that survey to identify them in the MPC database are marked with an asterisk.


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