Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters

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Volume 621 (January 2019)

A&A, 621 (2019) A34

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Table 1.

Non-comprehensive list of measurements of H₀ made since 2000 using observations of X-ray and Sunyaev-Zel’dovich galaxy clusters.

Article	Number	Redshift	Ω_m, Ω_Λ	Value	SZ data source	X-ray data source
Reese et al. (2000)	2	0.55	0.3, 0.7		OVRO, BIMA	ROSAT
Patel et al. (2000)	1	0.322	0.3, 0.7		OVRO, BIMA, MMT^a	ROSAT, ASCA^b
Mason et al. (2001)	7	< 0.1	0.3, 0.7		OVRO	ROSAT
Grainge et al. (2002)	1	0.143	1, 0		RT	ROSAT, ASCA
Reese et al. (2002)	18	0.14–0.78	0.3, 0.7		OVRO, BIMA	ROSAT
Saunders et al. (2003)	1	0.217	0.3, 0.7		RT	ROSAT, ASCA
Reese et al. (2004)	26	0–0.78	0.3, 0.7	61 ± 3 ± 18	RT, OVRO, BIMA	ROSAT
Battistelli et al. (2003)	1	0.0231	0.27, 0.73	84 ± 26	OVRO, WMAP^c, MITO^d	ROSAT
Udomprasert et al. (2004)	7	< 0.1	0.3, 0.7		CBI	ROSAT, ASCA, BeppoSAX^e
Schmidt et al. (2004)	3	0.09–0.45	0.3, 0.7	69 ± 8	Various	Chandra
Jones et al. (2005)	5	0.14–0.3	0.3, 0.7		RT	ROSAT, ASCA
Bonamente et al. (2006)	38	0.14–0.89	0.3, 0.7		OVRO, BIMA	Chandra
	Double β-model with HSE
	Isothermal β-model
	Isothermal β-model with excised core

Notes.

^(a)

Multiple Mirror Telescope Observatory, Arizona, USA.

^(b)

The Advanced Satellite for Cosmology and Astrophysics, X-ray astronomy mission, Japan, USA.

^(c)

Wilkinson Microwave Anisotropy Probe.

^(d)

Millimeter and Infrared Testagrigia Observatory, Val d’Aosta, Italy.

^(e)

“Beppo” Satellite per Astronomia a raggi X, X-ray Satellite, Italy, Holland.

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