More than 160 near Earth asteroids observed in the EURONEAR network

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Volume 511 (February 2010)

A&A, 511 (2010) A40

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Table 1:

Telescopes and detectors used for follow-up, recovery and secure orbits of NEAs.
Telescope	Aperture (m)	CCD	Pixels	FOV (arcmin)	Scale ( $\hbox {$^{\prime \prime }$ }$ /pixel)
Pic du Midi	1.05	THX7863	$384\times288$	$5.2\times3.9$	0.820
Haute Provence	1.20	TK1024	$1024\times1024$	11. $7\times11.7$	0.685
Cerro Armazones	0.85	SBIG ST-10	$2184\times1472$	$15.6\times8.3$	0.430
Cerro Tololo	1.0	Y4KCam	$4096\times4096$	$20\times20$	0.289
Las Campanas	1.02	SIT#3	$2048\times3650$	$15.1\times26.5$	0.435
La Silla	1.00	SBIG ST-10	$2184\times1472$	$3.3\times2.2$	0.090
La Silla	2.20	WFI mosaic	$8\times(2184\times1472)$	$34\times33$	0.238
Vasile Urseanu,
Bucharest	0.30	TC273-home made	$640\times500$	$21.6\times16.9$	2.30
York University	0.60	SBIG ST-9	$512\times512$	$4.3\times4.3$	0.505

Notes. The observatory is given in the first column and the aperture in the second one. The CCD camera (third column), the pixel size (fourth column), the field of view (FOV), and the scale (in $\hbox {$^{\prime \prime }$ }$ /pixel) are also presented.

Source LaTeX | All tables | In the text

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