Table 2: P-mode frequencies for HD 160691 ( $\mu$ Hz). The frequency resolution of the time series is 1.56 $\mu$ Hz. Frequencies with label ^a correspond to peaks with a signal-to-noise ratio in the range 2.5-3 and have to be considered with caution.
l = 0 l = 1 l = 2 l = 3

n = 13 .... .... 1381.8^a ....

n = 14 .... 1424.5 .... ....

n = 15 1478.4 1513.7 1555.1^a/1557.0^a 1592.9^a

n = 16 1562.3 1600.2 .... 1682.5^a

n = 17 .... .... 1731.8/1734.9 1772.2

n = 18 1740.9 1780.8 1824.2/1826.6 1862.3

n = 19 1831.6 .... 1914.5 1954.7

n = 20 1922.0 1960.4 2005.9/2007.8 2042.5

n = 21 2010.1 2051.0 2094.9/2096.7 2132.8

n = 22 2101.0 2140.8 2182.9/2184.9 ....

n = 23 2189.7^a 2231.0 2274.4^a/2276.0^a 2315.7^a

n = 24 2280.3 2322.7 .... ....

n = 25 .... .... .... ....

n = 26 .... 2504.5^a .... ....

**Table 2:** P-mode frequencies for HD 160691 ( $\mu$ Hz). The frequency resolution of the time series is 1.56 $\mu$ Hz. Frequencies with label ^a correspond to peaks with a signal-to-noise ratio in the range 2.5-3 and have to be considered with caution.
	l = 0	l = 1	l = 2	l = 3
n = 13	....	....	1381.8^a	....
n = 14	....	1424.5	....	....
n = 15	1478.4	1513.7	1555.1^a/1557.0^a	1592.9^a
n = 16	1562.3	1600.2	....	1682.5^a
n = 17	....	....	1731.8/1734.9	1772.2
n = 18	1740.9	1780.8	1824.2/1826.6	1862.3
n = 19	1831.6	....	1914.5	1954.7
n = 20	1922.0	1960.4	2005.9/2007.8	2042.5
n = 21	2010.1	2051.0	2094.9/2096.7	2132.8
n = 22	2101.0	2140.8	2182.9/2184.9	....
n = 23	2189.7^a	2231.0	2274.4^a/2276.0^a	2315.7^a
n = 24	2280.3	2322.7	....	....
n = 25	....	....	....	....
n = 26	....	2504.5^a	....	....

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 A low-mass-planetary companion
	4 Acoustic spectrum analysis
	5 Conclusions
	References