The Hubble Catalog of Variables (HCV)

A. Z. Bonanos; M. Yang; K. V. Sokolovsky; P. Gavras; D. Hatzidimitriou; I. Bellas-Velidis; G. Kakaletris; D. J. Lennon; A. Nota; R. L. White; B. C. Whitmore; K. A. Anastasiou; M. Arévalo; C. Arviset; D. Baines; T. Budavari; V. Charmandaris; C. Chatzichristodoulou; E. Dimas; J. Durán; I. Georgantopoulos; A. Karampelas; N. Laskaris; S. Lianou; A. Livanis; S. Lubow; G. Manouras; M. I. Moretti; E. Paraskeva; E. Pouliasis; A. Rest; J. Salgado; P. Sonnentrucker; Z. T. Spetsieri; P. Taylor; K. Tsinganos

doi:10.1051/0004-6361/201936026

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Volume 630 (October 2019)

A&A, 630 (2019) A92

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201936026e]

Table 4.

Properties of the HCV Control Sample fields.

Field	Distance	Instrument	Filters	Δ_MJD ^(a)	# visits	N_sources	# known	Recovery	Type of	Reference ^(c)
Name				(days)			variables	rate (C)	variables
M 4	1.86 kpc	WFC3	F467M,	300	100	8460	38	0.32	RR Lyr,	1
			F775W						EB
IC 1613	760 kpc	ACS	F814W,	3	12	23 106	182	0.71	RR Lyr,	2
			F475W						Cepheids,
									EB
M31-Halo11	770 kpc	ACS	F814W,	40	32	10 059	115	0.80 ^(b)	RR Lyr,	3
			F606W						Dwarf Cepheids,
									LPVs,
									semiregulars
M31-Stream	770 kpc	ACS	F814W,	30	16	6792	24	0.88	RR Lyr	4
			F606W
M31-Disk	770 kpc	ACS	F814W,	39	15	10 644	23	0.83	RR Lyr	4
			F606W
M101-F1	6.4 Mpc	ACS	F814W,	>30	14	58 263	411	0.80	Cepheids	5
			F555W
NGC 4535	16 Mpc	WFPC2	F814W,	75	14	1032	50	0.09	Cepheids,	6,7
			F435W						supergiants
M 87	16.5 Mpc	ACS	F814W	30	48	15 731	32	0.63	Novae	8
NGC 1448	17.3 Mpc	WFC3	F350LP,	50	11	9228	54	0.44	Cepheids	5
			F160W
GOODS-S		ACS	several	50–3000	5–120	14 278	116	0.26	AGN,	9
		WFC3							SNe

Notes.

^(a)

The values for the Mean Julian Date (MJD) are approximate as they can differ among sources in the group.

^(b)

The recovery rate is 0.90 for RR Lyrae variables alone.

^(c)

References.(1) Nascimbeni et al. (2014), (2) Bernard et al. (2010), (3) Brown et al. (2004), (4) Jeffery et al. (2011), (5) Hoffmann et al. (2016), (6) Macri et al. (1999), (7) Spetsieri et al. (2018), (8) Shara et al. (2016), (9) Pouliasis et al. (2019).

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