First step to detect an extrasolar planet using simultaneous observations with the VLTI instruments AMBER and MIDI

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Volume 515 (June 2010)

A&A, 515 (2010) A69

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Table 1:

Log of the observing sequences (left table: November 17 2007; right table: November 24 2007).
Object	Time (UT)	$B\cos(Z_{\rm p})$ (m)	$B\sin(Z_{\rm p})$ (m)	Object	Time (UT)	$B\cos(Z_{\rm p})$ (m)	$B\sin(Z_{\rm p})$ (m)
HD 9362	00h05min	129.6	-12.9	HD 9362	00h00min	130.0	-7.5
HD 9362	00h11min	129.7	-11.5	HD 9362	00h15min	130.1	-3.8
HD 9362	00h22min	129.9	-8.6	HD 9362	00h28min	130.2	0.5
HD 9362	00h31min	130.0	-6.6	GL 86	01h04min	130.2	1.7
HD 9362	00h40min	130.1	-4.3	HD 12524	01h36min	130.1	4.7
HD 9362	00h48min	130.2	-2.3	HD 9362	01h52min	127.8	24.9
HD 9362	00h57min	130.2	-0.3	GL 86	02h05min	128.8	18.9
GL 86	02h13min	129.5	13.2	GL 86	02h24min	127.8	24.7
GL 86	02h18min	129.4	14.5	GL 86	02h42min	126.6	30.4
GL 86	02h26min	129.1	16.7	HD 12524	02h56min	126.1	32.4
GL 86	02h33min	128.8	18.9	GL 86	03h28min	122.2	45.0
GL 86	02h40min	128.5	21.2	GL 86	03h33min	121.6	46.6
HD 12524	03h02min	127.8	24.6	GL 86	03h44min	120.2	50.1
HD 12524	03h10min	127.3	27.3	GL 86	03h52min	119.2	52.5
GL 86	03h32min	124.7	37.5	GL 86	04h00min	117.9	55.1
GL 86	03h41min	123.8	40.2
HD 12524	03h59min	121.1	47.8
GL 86	04h15min	119.8	51.1
GL 86	04h22min	118.7	53.4

Source LaTeX | All tables | In the text

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