Mapping the kinetic Sunyaev-Zel’dovich effect toward MACS J0717.5+3745 with NIKA

R. Adam; I. Bartalucci; G. W. Pratt; P. Ade; P. André; M. Arnaud; A. Beelen; A. Benoît; A. Bideaud; N. Billot; H. Bourdin; O. Bourrion; M. Calvo; A. Catalano; G. Coiffard; B. Comis; A. D’Addabbo; M. De Petris; J. Démoclès; F.-X. Désert; S. Doyle; E. Egami; C. Ferrari; J. Goupy; C. Kramer; G. Lagache; S. Leclercq; J.-F. Macías-Pérez; S. Maurogordato; P. Mauskopf; F. Mayet; A. Monfardini; T. Mroczkowski; F. Pajot; E. Pascale; L. Perotto; G. Pisano; E. Pointecouteau; N. Ponthieu; V. Revéret; A. Ritacco; L. Rodriguez; C. Romero; F. Ruppin; K. Schuster; A. Sievers; S. Triqueneaux; C. Tucker; M. Zemcov; R. Zylka

doi:10.1051/0004-6361/201629182

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Volume 598 (February 2017)

A&A, 598 (2017) A115

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Table 4

Coordinates, measured flux densities and predicted flux densities in the NIKA bands for the eleven submillimeter sources identified in our field.

			Measured flux densities (mJy)					NIKA prediction (mJy)
Label	RA^a	Dec^a	SPIRE (GHz)^a			NIKA (GHz)		NIKA (GHz)
			1200	857	600	260	150	260 (model)	150 (model)

SMG01	+07:17:32.11	+37:43:21.0	57.6±0.9	30.1±0.9	9.9±1.2	1.0±0.8	0.2±0.2	0.9±0.2	0.1±0.1
SMG02	+07:17:25.40	+37:47:05.7	25.2±0.9	14.7±0.9	1.3±1.4	0.7±1.3	-0.1±0.3	0.5±0.2	0.1±0.1
SMG03	+07:17:30.92	+37:46:50.6	15.2±0.9	13.9±0.9	6.2±1.2	0.1±0.9	0.6±0.2	0.8±0.2	0.1±0.1
SMG04	+07:17:34.91	+37:45:47.4	18.4±0.9	10.6±1.0	5.1±1.7	0.3±0.7	0.0±0.2	0.6±0.2	0.1±0.1
SMG05	+07:17:33.58	+37:44:01.9	14.3±0.8	16.8±0.9	13.3±1.2	1.3±0.7^b	0.2±0.2^b	1.8±0.3	0.4±0.1
SMG06	+07:17:25.06	+37:43:55.6	8.8±1.1	7.3±1.0	2.7±1.3	0.1±0.8	0.2±0.2	0.4±0.2	0.1±0.1
SMG07	+07:17:37.28	+37:45:34.1	12.1±0.9	12.7±1.0	14.1±1.2	0.1±0.7	0.4±0.2	1.6±0.3	0.3±0.1
SMG08	+07:17:30.87	+37:46:18.4	1.3±1.1	1.3±0.9	0.0±1.1	0.1±0.7	-0.1±0.2	<0.05	<0.02
SMG09^c	+07:17:31.24	+37:44:43.0	6.3±1.0	11.9±1.0	15.1±1.0	2.5±0.7^b	0.6±0.2^b	3.0±0.4	0.6±0.2
SMG10	+07:17:40.43	+37:45:26.7	4.2±0.9	5.3±0.8	3.1±1.2	−0.3±0.8	0.4±0.2	0.5±0.2	0.1±0.1
SMG11	+07:17:34.95	+37:44:33.1	4.7±1.1	4.8±0.8	4.9±1.4	0.0±0.7^b	−0.9±0.2^b	0.5±0.2	0.1±0.1

Notes. The measured flux densities are from SPIRE (Sayers et al. 2013) and NIKA (this work).

^(a)

From Sayers et al. (2013).

^(b)

Likely to be contaminated by SZ.

^(c)

High redshift lensed galaxy candidate with HST counterpart.

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