Equation of state constraints for the cold dense matter inside neutron stars using the cooling tail method

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Table 1

X-ray bursts used in the M-R analysis.

Source	N _H	Obsid	Date	K _td2 / K _td ^a
	(10²² cm^-2)		(MJD)

4U 1702−429	1.87^b	50 025-01-01-00	51 781.333039	2.2
		80033-01-01-08	52 957.629763	2.0
		80033-01-19-04	53 211.964665	2.2
		80033-01-20-02	53 212.794286	2.1
		80033-01-21-00	53 311.806086	2.1

4U 1724−307	0.78^c	93044-06-04-00	54526.679905	2.3

SAX J1810.8−2609	0.35^d	93044-02-04-00	54325.894492	3.1

Notes.

^(a)

Ratio of the blackbody normalizations at half-touchdown flux and at the touchdown (see Kajava et al. 2014; Poutanen et al. 2014);

^(b)

Worpel et al. (2013);

^(c)

Kuulkers et al. (2003);

^(d)

Natalucci et al. (2000).

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