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Table 3

Characteristics and optical-to-MIR and VLA 20 cm counterparts of the SMGs identified in the PdBI 1.3 mm maps.

Source α 2000.0 δ 2000.0 S 1.3 mm S / N 1.3 mm Offset Candidate r
[h:m:s] [°::] [mJy] [] counterpart IDa []

AzTEC16 09 59 50.069 +02 44 24.50 2.07 ± 0.62 5.0 9.0 501 (ACS-I) 0.35
AzTEC17a 09 59 39.194 +02 34 03.83 1.58 ± 0.43 6.2 4.5 613229 (GALEX) 1.29
1496 (ACS-I) 1.36
1475165 (COSMOS+UltraVISTA) 1.38
271694 (New UltraVISTA) 1.47
250117 (IRAC) 0.30
J095939.19+023403.6 (VLA Deep) 0.22
AzTEC17b 09 59 38.904 +02 34 04.69 1.53 ± 0.46 4.5 6.8 1475223 (COSMOS+UltraVISTA) 1.25
AzTEC18 09 59 42.607 +02 35 36.96 1.78 ± 0.54 4.5 7.3 1044 (ACS-I) 0.76
1471053 (COSMOS+UltraVISTA) 0.82
AzTEC19a 10 00 28.735 +02 32 03.84 3.98 ± 0.91 10.3 4.4 1593 (ACS-I) 0.40
1455882 (COSMOS+UltraVISTA) 0.20
262214 (New UltraVISTA) 0.20
242501 (IRAC) 0.63
2158 (MIPS 24 μm) 0.15
J100028.70+023203.7 (VLA Deep) 0.53
AzTEC19b 10 00 29.256 +02 32 09.82 5.21 ± 1.30 9.7 10.6 597821 (GALEX) 0.66
1486 (ACS-I) 0.68
1455681 (COSMOS+UltraVISTA) 0.63
262766 (New UltraVISTA) 0.74
AzTEC20 10 00 20.251 +02 41 21.66 1.85 ± 0.49 6.0 5.9 ... ...
AzTEC21a 10 00 02.558 +02 46 41.74 3.37 ± 1.03 5.8 4.3 711447 (GALEX) 0.35
1688587 (COSMOS+UltraVISTA) 0.15
328878 (New UltraVISTA) 1.00
297396 (IRAC) 1.11
7262 (MIPS 24 μm) 1.46
AzTEC21b 10 00 02.710 +02 46 44.51 1.34 ± 0.38 4.2 0.7 711786 (GALEX) 0.53
1688585 (COSMOS+UltraVISTA) 0.45
AzTEC21c 10 00 02.856 +02 46 40.80 1.27 ± 0.40 4.5 4.5 712026 (GALEX) 1.49
297223 (IRAC) 1.46
AzTEC22 09 59 50.681 +02 28 19.06 1.82 ± 0.59 5.1 10.5 ... ...
AzTEC23 09 59 31.399 +02 36 04.61 0.99 ± 0.29 4.9 4.0 1494354 (COSMOS+UltraVISTA) 1.24
AzTEC24a 10 00 38.969 +02 38 33.90 1.79 ± 0.53 4.9 10.6 ... ...
AzTEC24b 10 00 39.410 +02 38 46.97 1.72 ± 0.53 5.0 10.8 ... ...
AzTEC24c 10 00 39.194 +02 38 54.46 2.85 ± 0.78 5.1 12.8 ... ...
AzTEC25b ... ... ... ... ... ... ...
AzTEC26a 09 59 59.386 +02 38 15.36 0.98 ± 0.28 5.4 4.4 647670 (GALEX) 1.05
930 (ACS-I) 1.07
1709726 (COSMOS+UltraVISTA) 0.94
291786 (New UltraVISTA) 0.83
AzTEC26b 09 59 59.657 +02 38 21.08 0.90 ± 0.26 4.8 2.8 ... ...
AzTEC27 10 00 39.211 +02 40 52.18 3.36 ± 0.97 c 6.0 1.4 666 (ACS-I) 1.15
AzTEC28 10 00 04.680 +02 30 37.30 2.38 ± 0.77 5.5 3.5 ... ...
AzTEC29a 10 00 26.351 +02 37 44.15 2.45 ± 0.67 4.7 10.8 736 (ACS-I) 1.41
AzTEC29b 10 00 26.561 +02 38 05.14 9.01 ± 2.39 7.3 11.6 1685295 (COSMOS+UltraVISTA) 0.76
AzTEC30 10 00 03.552 +02 33 00.94 1.53 ± 0.45 4.6 9.3 ... ...

Notes. The coordinates given in Cols. (2) and (3) refer to the peak position determined by the three-parameter point-source model fit for all sources with peak surface brightness of S/N> 4. The flux densities given in Col. (4) are primary-beam corrected, and the quoted errors include the 20% calibration uncertainty. For the (marginally) resolved sources AzTEC21a, AzTEC27, and AzTEC28, the total flux density was derived from the best-fit six-parameter source model. The S/N ratio given in Col. (5) refers to the extracted value in the non-primary-beam-corrected map. In Col. (6), we give the PdBI source offset from the phase centre, i.e. the AzTEC 1.1 mm centroid. The last column gives the projected angular separation between the 1.3 mm peak position and the counterpart position.

(a)

The references for the different source catalogues are as follows: ACS I-band (Leauthaud et al. 2007); GALEX (Zamojski et al. 2007); COSMOS photometry catalogue (Capak et al. 2007); UltraVISTA (Capak et al. 2007; McCracken et al. 2012; Ilbert et al. 2013); Spitzer IRAC/MIPS (S-COSMOS team); VLA Deep (Schinnerer et al. 2010).

(b)

The 1.3 mm features in AzTEC25 did not fulfil our detection criteria.

(c)

AzTEC27 is probably subject to gravitational lensing (see Appendices C and D), and our lens modelling suggests a magnification factor of μ = 2.04 ± 0.16. In this case, AzTEC27’s intrinsic flux density at observing-frame 1.3 mm would be 1.65 ± 0.49 mJy.

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