CDS

2003A&A...405..833S

Query : 2003A&A...405..833S

2003A&A...405..833S - Astronomy and Astrophysics, volume 405, 833-849 (2003/7-3)

A deep 6.7µm survey in the SSA13 field with ISO.

SATO Y., KAWARA K., COWIE L.L., TANIGUCHI Y., SANDERS D.B., MATSUHARA H., OKUDA H., WAKAMATSU K., SOFUE Y., JOSEPH R.D. and MATSUMOTO T.

Abstract (from CDS):

We present results of a deep mid-infrared survey in the SSA13 field with the Infrared Space Observatory (ISO). In order to probe the near-infrared light at high redshifts, we surveyed the field with the broad band LW2 (5-8.5µm) filter of the mid-infrared camera ISOCAM. Adopting a highly redundant imaging strategy for the 23 h observation and carefully treating gradual changes in the detector responsivity caused by a very high rate of cosmic ray impacts, we succeeded in reaching an 80% completeness limit of 16µJy in the central 7-arcmin2 region. Utilizing the signal-to-noise ratio map, we detected 65 sources down to 6µJy in the 16-arcmin2 field. Integral galaxy number counts at 6.7µm are then derived, reaching 1.3x104deg–2 at the faint limit with a slope of -1.6 between 13µJy and 130µJy. Integrating individual sources in this flux range, the resolved fraction of the extragalactic background light at 6.7µm is estimated to be 0.56n/Wm2/sr. These results, which reach a flux limit three times fainter than those in the Hubble Deep Fields, are in fairly good agreement with a model prediction by Franceschini et al. (1997, ESA SP401, 159). Finally, we discuss the relation of distant massive E/S0 galaxies to the faint 6.7µm galaxy population.

Abstract Copyright: ∼

Journal keyword(s): Galaxy: evolution - infrared: galaxies - cosmology: observations - surveys - galaxies: photometry - methods: data analysis

Nomenclature: Table 3: [SKC2003] NN (Nos 0-64).

Simbad objects: 66

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Number of rows : 66
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023 		#notes
1 [SKC2003] 0 IR 13 12 15.8 +42 44 00           ~ 2 0
2 SSA 13 reg 13 12 16.5 +42 44 39           ~ 107 0
3 [SKC2003] 1 IR 13 12 16.8 +42 44 21           ~ 2 0
4 [SKC2003] 2 IR 13 12 17.4 +42 44 53           ~ 2 0
5 [SKC2003] 3 IR 13 12 18.0 +42 43 45           ~ 2 0
6 [SKC2003] 4 IR 13 12 18.1 +42 45 28           ~ 2 0
7 [SKC2003] 5 IR 13 12 18.1 +42 46 15           ~ 2 0
8 [SKC2003] 6 IR 13 12 18.4 +42 43 20           ~ 2 0
9 [SKC2003] 7 IR 13 12 18.7 +42 42 48           ~ 2 0
10 [SKC2003] 8 IR 13 12 19.5 +42 45 00           ~ 2 0
11 [SKC2003] 9 IR 13 12 19.5 +42 45 37           ~ 2 0
12 [SKC2003] 10 IR 13 12 20.0 +42 44 38           ~ 2 0
13 [SKC2003] 11 IR 13 12 21.0 +42 44 33           ~ 2 0
14 [SKC2003] 12 IR 13 12 21.3 +42 46 24           ~ 2 0
15 [SKC2003] 13 IR 13 12 21.4 +42 44 24           ~ 2 0
16 MCBA 21 QSO 13 12 21.56064 +42 44 05.7768           ~ 5 0
17 [SKC2003] 15 IR 13 12 21.6 +42 45 19           ~ 2 0
18 [SKC2003] 16 IR 13 12 21.8 +42 43 48           ~ 2 0
19 MCBA 18 X 13 12 22.48 +42 44 50.0           ~ 4 0
20 [SKC2003] 18 IR 13 12 22.8 +42 43 15           ~ 2 0
21 [SKC2003] 19 IR 13 12 23.1 +42 46 07           ~ 2 0
22 [SKC2003] 21 IR 13 12 23.4 +42 44 31           ~ 2 0
23 FIRST J131223.6+424517 IR 13 12 23.638 +42 45 17.00           ~ 2 0
24 2MASS J13122387+4245438 * 13 12 23.8919060112 +42 45 43.810203132           ~ 2 0
25 [SKC2003] 23 IR 13 12 24.3 +42 43 59           ~ 2 0
26 [SKC2003] 24 IR 13 12 24.5 +42 43 23           ~ 2 0
27 [SKC2003] 25 IR 13 12 24.7 +42 44 15           ~ 2 0
28 [SKC2003] 26 IR 13 12 24.8 +42 45 10           ~ 2 0
29 [SKC2003] 27 IR 13 12 25.2 +42 46 00           ~ 2 0
30 [SKC2003] 29 IR 13 12 25.7 +42 43 19           ~ 2 0
31 [BCS99] J131225.7+424350 PaG 13 12 25.7 +42 43 50   24.3       ~ 5 0
32 [SKC2003] 30 IR 13 12 26.2 +42 42 27           ~ 2 0
33 [SKC2003] 32 IR 13 12 26.3 +42 44 06           ~ 2 0
34 [SKC2003] 31 IR 13 12 26.3 +42 45 26           ~ 2 0
35 [SKC2003] 33 IR 13 12 27.4 +42 44 49           ~ 2 0
36 [SKC2003] 36 IR 13 12 27.7 +42 45 09           ~ 2 0
37 [SKC2003] 35 IR 13 12 27.7 +42 45 35           ~ 2 0
38 [SKC2003] 34 IR 13 12 27.7 +42 46 32           ~ 2 0
39 [SKC2003] 37 IR 13 12 27.9 +42 42 20           ~ 2 0
40 MCBA 15 X 13 12 28.25 +42 44 54.5           ~ 6 0
41 [SKC2003] 38 IR 13 12 28.3 +42 44 30           ~ 2 0
42 [SKC2003] 39 IR 13 12 28.5 +42 46 02           ~ 2 0
43 [SKC2003] 41 IR 13 12 28.6 +42 44 00           ~ 2 0
44 [SKC2003] 42 IR 13 12 28.9 +42 46 19           ~ 2 0
45 [SKC2003] 43 IR 13 12 29.0 +42 43 07           ~ 2 0
46 [SKC2003] 44 IR 13 12 29.2 +42 45 59           ~ 2 0
47 [SKC2003] 45 IR 13 12 29.4 +42 44 40           ~ 2 0
48 [SKC2003] 46 IR 13 12 29.6 +42 43 01           ~ 2 0
49 [SKC2003] 47 IR 13 12 29.9 +42 44 08           ~ 2 0
50 [SKC2003] 48 IR 13 12 29.9 +42 45 14           ~ 2 0
51 [SKC2003] 49 IR 13 12 30.0 +42 44 20           ~ 2 0
52 [SKC2003] 50 IR 13 12 30.1 +42 44 59           ~ 2 0
53 [SKC2003] 51 IR 13 12 31.1 +42 43 33           ~ 2 0
54 [SKC2003] 53 IR 13 12 31.5 +42 42 36           ~ 2 0
55 [SKC2003] 52 IR 13 12 31.5 +42 42 44           ~ 2 0
56 [SKC2003] 54 IR 13 12 31.6 +42 45 51           ~ 2 0
57 [SKC2003] 55 IR 13 12 31.8 +42 43 48           ~ 2 0
58 [SKC2003] 56 IR 13 12 32.0 +42 45 05           ~ 2 0
59 NAME SMM J131232.1+424428.0 PaG 13 12 32.1 +42 44 28           ~ 6 1
60 [SKC2003] 58 IR 13 12 32.9 +42 43 11           ~ 2 0
61 [SKC2003] 59 IR 13 12 34.0 +42 44 42           ~ 2 0
62 [SKC2003] 60 IR 13 12 34.2 +42 46 02           ~ 2 0
63 MCBA 10 G 13 12 34.48 +42 43 09.3           ~ 5 0
64 [SKC2003] 61 IR 13 12 34.5 +42 43 41           ~ 2 0
65 [SKC2003] 63 IR 13 12 35.0 +42 45 05           ~ 2 0
66 2MASS J13123587+4243583 * 13 12 35.8859919528 +42 43 58.214879904           ~ 2 0

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2023.09.26-14:08:49

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