CoRoT's view of newly discovered B-star pulsators: results for 358 candidate B pulsators from the initial run's exoplanet field data

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Table A.1:

CoRoT 102804522 shows rich variability on varying timescales, but many of the frequencies can be connected through the same frequency spacing ( $\epsilon =f_2-f_1-\Delta f$ ).
Type	f₁ (d^-1)	$\Delta f$ (d^-1)	f₂ (d^-1)	$\epsilon$ (d^-1)
Single	1.0891	0.5320	1.6213	0.0002
Single	1.2350	0.5248	1.7595	-0.0003
Single	1.4445	0.5248	1.9697	0.0004
Single	1.7595	0.5320	2.2914	-0.0002
Single	1.8758	0.5320	2.4077	-0.0002
Single	3.1081	0.5248	3.6325	-0.0004
Single	3.6325	0.5248	4.1572	-0.0001
Single	3.7455	0.5248	4.2703	-0.0001
Single	3.8578	0.5320	4.3899	0.0001
Single	3.9212	0.5248	4.4458	-0.0003
Single	4.3259	0.5248	4.8512	0.0004
Single	4.7765	0.5320	5.3088	0.0003
Single	9.0494	0.5248	9.5741	-0.0001
Triplet	14.2073	0.5320	14.7395	0.0001
	14.7395	0.5320	15.2719	0.0004

Source LaTeX | All tables | In the text

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