Galactic bulge population II Cepheids in the VVV survey: period-luminosity relations and a distance to the Galactic centre

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Volume 605 (September 2017)

A&A, 605 (2017) A100

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Table 1

Properties of Type II Cepheids in the Galactic bulge.

VVV ID	OGLE ID	P	Class	Mean magnitudes					σ			E _{J K _s}
		(days)		V	I	J	H	K _S	J	H	K _S

515601356315	OGLE-002	2.268	BLH	15.188	13.909	13.116	12.766	12.521	0.072	0.072	0.072	0.173
515601679485	OGLE-003	1.484	BLH	16.519	15.061	14.240	13.855	13.387	0.104	0.104	0.104	0.290
515594023082	OGLE-005	2.008	BLH	18.666	16.842	15.845	15.354	14.788	0.152	0.153	0.150	0.388
515520862858	OGLE-008	1.183	BLH	17.765	15.970	–	14.205	13.935	–	0.060	0.058	0.410
515555436341	OGLE-009	1.896	BLH	17.630	15.608	13.887	13.343	13.134	0.098	0.098	0.098	0.461
515534145302	OGLE-013	1.517	BLH	18.525	16.193	14.550	13.951	13.676	0.117	0.117	0.116	0.588
515543870338	OGLE-014	1.239	BLH	15.376	13.590	12.306	11.905	11.613	0.003	0.004	0.092	0.534
515490128302	OGLE-015	1.279	BLH	18.087	15.907	14.291	13.712	13.438	0.008	0.010	0.111	0.591
515522173203	OGLE-017	1.098	BLH	18.533	16.251	14.371	13.850	13.669	0.091	0.092	0.090	0.636
515490198825	OGLE-018	1.620	BLH	18.072	15.990	14.187	13.630	13.339	0.113	0.113	0.113	0.580

Notes. The OGLE ID, period, subtype, and optical mean magnitudes are taken from OGLE-III (Soszyński et al. 2011). The values of E_{JK_s}: E(J−K_s), are taken from extinction maps of Gonzalez et al. (2011b). The first ten lines of the table are shown here and the entire table is available at the CDS.

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