BL Lacertae objects beyond redshift 1.3 – UV-to-NIR photometry and photometric redshift for Fermi/LAT blazars

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Volume 538 (February 2012)

A&A, 538 (2012) A26

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Table 4

SED fits and photometric redshift solutions.


Name	z _phot,best ^a	z _spec,img ^b	Power law				Galaxy
			z _phot ^c	χ ²	P _z ^d	β ^e	z _phot ^c	χ ²	P _z ^c	model


CRATES J0001-0746	<1.25	–		5.6	36.5	1.20		6.9	77.5	pl_I22491_30_TQSO1_70
CRATES J0009+0628	<1.35	–		4.6	36.1	1.45		14.8	83.1	I22491_50_TQSO1_50
CRATES J0021-2550	<1.44	–		10.2	60.4	0.90		14.7	93.3	pl_I22491_20_TQSO1_80
1RXS J002209.2-185333	<1.38	–		5.8	77.4	0.95		16.8	47.9	pl_I22491_20_TQSO1_80
RX J0035.2+1515		–		2.6	90.1	0.90		8.7	75.5	I22491_60_TQSO1_40
FRBA J0037+1238	–	–		44.0	96.6	1.20		28.5	66.5	I22491_60_TQSO1_40
BZB J0045+2127	<1.06	–		21.6	28.9	0.85		11.6	85.6	pl_I22491_30_TQSO1_70
PKS 0047+023		–		10.8	94.9	1.60		13.6	80.5	pl_QSO_DR2_029_t0
PKS 0048-09	<1.34	0.64		5.6	44.9	1.25		7.3	74.1	pl_I22491_30_TQSO1_70
RBS 119	<1.12	–		4.5	26.5	0.65		23.0	69.1	I22491_60_TQSO1_40
FRBA J0054-2455	<1.14	–		16.9	31.3	0.60		13.1	73.8	pl_TQSO1_template_norm
PKS 0055-328		–		17.7	95.2	1.25		11.2	38.4	I22491_50_TQSO1_50
BZB J0114+1325	<1.22	–		6.3	37.0	0.75		27.7	56.0	pl_I22491_20_TQSO1_80
CLASS J0115+0356	<1.25	–		5.3	33.5	0.85		12.9	78.2	I22491_60_TQSO1_40
BZB J0115+2519	<1.45	–		12.8	63.4	0.90		18.6	96.3	I22491_60_TQSO1_40
AT20G J0124-0625	<2.46	–		12.1	69.0	1.30		7.4	54.9	pl_I22491_20_TQSO1_80
CRATES J0154+0823	<1.37	–		7.6	53.2	0.95		11.8	79.6	pl_I22491_20_TQSO1_80
RBS 259	<1.16	–		23.6	26.1	1.00		14.8	71.2	pl_I22491_20_TQSO1_80
CGRaBS J0158-3932	<1.35	–		13.3	25.0	1.10		5.3	75.4	pl_I22491_30_TQSO1_70
CRATES J0159-2740	<1.05	–		25.8	16.0	0.95		14.5	36.5	pl_I22491_20_TQSO1_80
BZB J0209-5229	<1.18	–		14.0	11.2	0.95		6.7	99.5	I22491_60_TQSO1_40
CGRaBS J0211+1051	–	–		49.9	32.3	1.05		27.0	99.5	I22491_60_TQSO1_40
CRATES J0216-6636	<1.25	–		10.4	38.2	0.85		10.0	66.4	I22491_60_TQSO1_40
RBS 334	<1.14	–		6.3	26.4	0.80		16.5	74.6	pl_I22491_20_TQSO1_80
BZB J0238-3116	<1.02	–		16.2	13.6	0.65		12.2	99.4	I22491_60_TQSO1_40
CRATES J0250+1708	<3.10	–		15.6	30.6	2.00		8.0	44.4	pl_I22491_20_TQSO1_80
AT20G J0314-5104	<1.43	–		1.8	70.8	1.20		6.8	56.6	I22491_40_TQSO1_60
BZB J0323-0111	<1.54	–		14.5	95.0	0.85		16.7	90.6	I22491_60_TQSO1_40
CRATES J0325-5629	<1.42	0.86		21.5	65.6	2.05		60.3	99.9	pl_QSOH_template_norm
CRATES J0325-5635	–	0.06		78.6	100.0	1.40		39.7	97.8	pl_I22491_20_TQSO1_80
PKS 0332-403		1.36		6.0	99.8	1.35		13.0	62.3	I22491_60_TQSO1_40
CRATES J0334-3725	<1.34	–		8.0	64.5	0.90		7.9	71.0	I22491_60_TQSO1_40
PKS 0355-500	<1.44	0.64		14.0	67.3	1.25		9.7	43.3	I22491_40_TQSO1_60
CRATES J0402-2615		–		8.6	100.0	1.25		9.5	48.9	I22491_60_TQSO1_40
PKS 0422+00	<1.25	–		7.0	31.2	1.10		10.2	78.4	pl_I22491_30_TQSO1_70
CRATES J0430-2507	<1.46	0.52		6.6	65.8	1.15		9.1	67.6	pl_I22491_30_TQSO1_70
CRATES J0434-2015	<1.26	0.93		12.8	34.8	1.45		17.5	76.2	pl_I22491_20_TQSO1_80
BZB J0448-1632	<1.25	–		5.5	35.8	0.65		24.5	96.6	I22491_60_TQSO1_40
CRATES J0505+0415	<1.26	–		3.0	37.6	0.95		8.6	59.6	pl_I22491_20_TQSO1_80
RBS 621	<1.07	–		7.8	28.6	0.60		7.7	99.5	pl_TQSO1_template_norm
CGRaBS J0509+0541	<1.24	–		17.1	86.7	0.95		20.6	97.7	pl_I22491_20_TQSO1_80
PKS 0516-621	<1.44	1.30		10.4	82.7	1.20		11.9	77.3	pl_I22491_20_TQSO1_80
FRBA J0536-3343	<1.16	–		20.1	35.2	0.60		14.5	73.0	pl_TQSO1_template_norm
SUMSS J053748-571828		–		20.5	99.9	0.80		21.5	99.6	pl_I22491_30_TQSO1_70
1RXS J053810.0-390839	<1.71	–		5.6	17.9	1.20		5.8	37.6	I22491_40_TQSO1_60
BZB J0543-5532	<1.08	–		4.8	28.8	0.75		15.2	34.9	pl_I22491_20_TQSO1_80
PKS 0600-749		–		6.9	98.1	1.20		7.5	58.1	I22491_60_TQSO1_40
1ES 0602-482	<0.99	–		25.3	32.2	0.80		8.9	88.2	pl_I22491_30_TQSO1_70
CRATES J0630-2406		–		9.3	100.0	0.85		24.6	83.7	I22491_60_TQSO1_40
CRATES J0647-6058	<1.69	–		19.2	16.0	1.35		10.3	88.8	I22491_60_TQSO1_40
1ES 0647+250	<1.47	–		9.5	75.9	0.65		24.5	92.3	pl_QSOH_template_norm
PKS 0700-661	<1.46	–		10.5	73.1	1.05		6.7	98.6	I22491_60_TQSO1_40
CRATES J0705-4847	–	–		0.0	15.7	1.50		0.0	11.0	S0_80_QSO2_20
CRATES J0718-4319	<1.26	–		4.0	38.1	0.85		8.4	90.2	I22491_60_TQSO1_40
CRATES J0811-7530	<1.40	–		10.7	41.5	1.05		8.8	68.4	pl_I22491_30_TQSO1_70
AT20G J0814-1012	<1.54	–		10.0	75.2	0.95		17.3	61.1	pl_I22491_20_TQSO1_80
BZB J0816-1311	–	–		51.4	31.6	0.75		17.1	96.2	pl_I22491_20_TQSO1_80
CGRaBS J0817-0933	<1.64	–		10.0	88.0	1.35		7.3	69.3	pl_I22491_20_TQSO1_80
CRATES J0856+2057	<1.41	–		5.0	42.6	1.15		5.8	55.0	pl_I22491_20_TQSO1_80
CGRaBS J0856-1105	<1.54	–		6.2	82.7	1.15		7.5	69.7	pl_I22491_20_TQSO1_80
SDSS J090226.91+205046.4	<1.21	–		7.4	31.1	0.90		6.3	91.9	I22491_60_TQSO1_40
CRATES J0905+1358	<1.35	–		8.3	46.1	0.85		17.3	93.5	I22491_60_TQSO1_40
CRATES-Va J0906-0905	<1.51	–		10.5	98.9	1.05		13.7	92.2	pl_I22491_30_TQSO1_70
CRATES J0953-0840	<1.28	–		7.7	45.6	0.75		30.9	91.7	pl_I22491_20_TQSO1_80
CGRaBS J1008+0621	<1.44	–		6.0	81.6	1.25		6.5	57.4	pl_I22491_30_TQSO1_70
BZB J1022-0113	<1.14	–		13.6	26.4	0.60		14.1	83.7	pl_TQSO1_template_norm
BZB J1023-4336	<1.54	–		8.6	88.6	0.60		19.3	96.4	pl_QSOH_template_norm
PKS 1029-85	–	–		76.8	30.8	1.20		51.9	99.4	I22491_70_TQSO1_30
PKS B1035-281	–	1.07		55.8	89.8	0.25		25.0	100.0	pl_QSOH_template_norm
CLASS J1049+2338	–	0.32		30.5	32.7	1.55		31.2	45.3	I22491_50_TQSO1_50
CLASS J1054+2210	<1.36	–		13.8	55.0	0.95		22.0	31.8	I22491_50_TQSO1_50
BZB J1107+0222	<1.45	–		11.0	78.6	0.90		9.9	54.3	pl_I22491_30_TQSO1_70
OM 235		1.55		18.2	99.9	1.10		11.9	94.9	pl_I22491_30_TQSO1_70
PKS B1130+008	<1.26	0.68		7.7	33.3	1.30		11.6	45.2	pl_I22491_30_TQSO1_70
PKS 1216-010	<1.23	–		8.7	34.7	1.30		10.2	78.8	pl_QSO_DR2_029_t0
BZB J1233-0144	<1.46	–		13.7	73.2	1.15		12.7	46.5	pl_I22491_20_TQSO1_80
SDSS J125117.88+103907.2	<1.06	0.25		13.4	15.9	1.00		12.9	40.9	pl_I22491_20_TQSO1_80
1RXS J130421.2-435308	–	–		525.0	33.5	1.25		347.1	100.0	I22491_70_TQSO1_30
1RXS J130737.8-425940	<1.53	–		15.0	90.6	0.75		21.3	99.7	I22491_60_TQSO1_40
4C +12.46	<1.40	–		5.7	67.8	1.35		11.1	88.4	pl_I22491_30_TQSO1_70
CRATES J1312-2156		1.49		7.1	100.0	0.95		18.4	100.0	I22491_60_TQSO1_40
CRATES J1314+2348	<1.30	–		15.8	52.3	1.10		14.3	33.3	I22491_50_TQSO1_50
BZB J1351+1114	<1.12	–		16.2	15.3	0.75		15.4	59.9	pl_I22491_20_TQSO1_80
PKS 1350+148	<1.43	–		9.8	63.8	1.00		14.6	35.1	I22491_50_TQSO1_50
CRATES J1359-3746	<1.26	0.33		5.1	36.4	1.25		12.5	34.0	I22491_40_TQSO1_60
SDSS J141826.33-023334.1	<1.37	–		5.2	69.3	0.70		25.4	99.9	pl_I22491_20_TQSO1_80
PKS 1424+240	<1.11	–		10.4	38.4	0.70		19.4	99.9	I22491_60_TQSO1_40
CRATES J1440+0610	<1.31	–		5.9	42.7	0.95		11.1	77.5	pl_I22491_20_TQSO1_80
PKS 1514+197	–	–		40.1	30.2	1.55		31.6	98.4	I22491_90_TQSO1_10
PG 1553+113	<1.35	–		6.0	80.8	0.65		29.7	99.5	I22491_60_TQSO1_40
SUMSS J195945-472519	<1.31	–		4.1	53.1	0.80		11.5	97.4	I22491_60_TQSO1_40
PKS 2012-017	<1.22	–		3.6	24.2	1.45		17.3	89.6	I22491_50_TQSO1_50
CRATES J2039-1046	–	–		259.6	34.4	1.30		174.9	99.3	I22491_80_TQSO1_20
CRATES J2103-6232	<1.24	–		5.2	39.4	0.90		8.4	65.3	I22491_60_TQSO1_40
PKS 2104-668	<1.20	–		10.6	25.4	1.25		12.8	90.4	pl_I22491_30_TQSO1_70
PKS B2147+031	<1.42	–		3.8	80.1	1.15		9.3	65.1	pl_I22491_20_TQSO1_80
BZB J2221-5225	<1.17	–		7.5	15.6	0.70		17.9	59.2	I22491_60_TQSO1_40
PKS 2233-148	<1.55	–		17.5	66.5	1.80		23.1	18.4	pl_QSO_DR2_029_t0
BZB J2255+2410	<1.25	–		8.1	33.1	0.90		8.7	69.6	I22491_60_TQSO1_40
PKS 2312-505	<1.29	0.81		7.2	34.1	1.65		25.0	85.2	I22491_60_TQSO1_40
BZB 2313+1444	<1.28	0.16		22.0	32.6	1.60		20.1	86.5	I22491_50_TQSO1_50
1ES 2322-409	<1.37	0.17		17.3	69.1	0.50		53.6	90.7	pl_TQSO1_template_norm
CLASS J2352+1749		–		7.5	91.8	1.15		7.1	64.2	pl_I22491_20_TQSO1_80

Notes.

^(a)

Best photometric redshift, see text.

^(b)

Spectroscopic or imaging redshift (if known) from Ackermann et al. (2012).

^(c)

Photometric redshift with 90% confidence uncertainties.

^(d)

Redshift probability density at z_phot ± 0.1(1 + z_phot).

^(e)

Spectral slope for power law model of the form F_λ ∝ λ^−β.

^(f)

Starburst/QSO hybrid templates with varying contributions of the two components. Template names reflect the relative contribution of the starburst (I22491_NN) and AGN (TQSO1_NN) models to the hybrid. “pl” marks an additional power-law component at short wavelengths. See Salvato et al. (2011) for details on the templates.

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