On the observational bias of the Trojan swarms | Astronomy & Astrophysics (A&A)

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Volume 516 (June-July 2010)

A&A, 516 (2010) A22

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Table 2:

Photometry results for the observatories.
Site	Events^a	Grid miss^b	$\Delta_{\textrm{mag}}$	$\sigma$	limit^c	limit^d	$\Delta$ limi^e	Found^f	H^g	H^h	Hⁱ	H^j
Code	[pcs.]	[%]	[mag]	[mag]	[mag]	[mag]	[mag]	[pcs.]	[mag]	[mag]	[mag]	[mag]
644	8274	5.6	0.17	0.57	19.75	19.43	0.5	186	12.1	12.9	13.5	12.4
691^k	2611	11.1	0.30	0.48	20.30	20.10	0.8	35	12.4	13.4	13.5	12.9
691	5333	5.2	0.34	0.44	21.07	20.96	0.1	24	13.4	13.5	14.3	13.1
699	9030	2.9	-0.19	0.43	19.14	18.99	0.3	5	12.1	12.3	12.8	11.8
703	3896	3.7	0.17	0.54	19.79	19.53	0.4	73	11.7	12.4	13.5	12.4
704	28 456	4.6	0.77	0.73	18.69	18.63	0.3	694	11.3	12.3	12.6	11.3
G96	3423	6.4	0.06	0.42	21.19	20.94	0.3	5	12.7	13.5	14.1	13.8

Notes. ^(a) The cumulative number of matched Trojans with magnitude on a night to night basis.
^(b) The number of the integrated real Trojans which did not end up in the same grid-area as the observations.
^(c) Median of the faintest object in fields containing real Trojans.
^(d) Median of the faintest object in all fictitious Trojan containing fields.
^(e) Difference in using all fields with fictitious Trojans and those fields which contained 10 observations or more.
^(f) Number of simulated discoveries.
^(g) Median magnitude of simulated identifications.
^(h) Median magnitude of real discoveries.
⁽ⁱ⁾ Median magnitude of the deepest magnitude for identified objects.
^(j) Magnitude based on Col. 6 and a combined median distance and phase angle compensation (-7.36 mag).
^(k) Old instrument configuration.

Source LaTeX | All tables | In the text

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