Open Universe for Blazars: a new generation of astronomical products based on 14 years of Swift-XRT data

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Volume 631 (November 2019)

A&A, 631 (2019) A116

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Table 1.

Blazars observed by Swift with short and frequent, mostly daily XRT exposures in PC mode.

Blazar name	No. of XRT	No. of detections	⟨rate⟩ ^(b)	MAD ^(c)
	observations ^(a)	below pileup limit	(cts s⁻¹)	(%)
OJ 287	304	303	0.202	23.3
3C 279	282	261	0.355	17.5
PKS 1510−089	218	218	0.217	16.6
S5 0716+714	185	156	0.294	34.0
PG 1553+113	165	33	1.040	41.3
PKS 0235+164	158	155	0.048	40.5
PKS 0208−512	140	140	0.063	23.3
BZQJ 1635+3808	130	130	0.105	47.1
1ES 2344+514	126	64	0.599	26.7
PKS 0528+134	116	116	0.035	48.0
ON 231	113	112	0.057	25.8
CTA 102	110	89	0.322	50.9
1H 0323+342	108	88	0.426	23.7
MS 1207.9+3945	103	103	0.084	21.5
PKS 0921−213	94	94	0.216	19.9
NRAO 530	89	89	0.045	19.0
3C 66A	83	83	0.100	28.1
PKS 1222+216	73	73	0.111	22.2
TXS 0506+056 ^(d)	49	49	0.053	23.5

Notes.

^(a)

Integrated with one day time interval executed in PC mode with exposure time longer than 200 s.

^(b)

Median count rate in the total 0.3 − 10 keV band.

^(c)

Median Absolute Deviation about the median count rate.

^(d)

Blazar associated with the IceCube high-energy neutrino IC170922 and other IceCube neutrinos (Padovani et al. 2018).

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