Revealing the cold dust in low-metallicity environments - I. Photometry analysis of the Dwarf Galaxy Survey with Herschel

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Volume 557 (September 2013)

A&A, 557 (2013) A95

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201321602e]

Table 3

SPIRE flux densities for the DGS galaxies.

Source	F₂₅₀ (Jy)	σ₂₅₀ (Jy)	F₃₅₀ (Jy)	σ₃₅₀ (Jy)	F₅₀₀ (Jy)	σ₅₀₀ (Jy)

Haro 11	0.63	0.05	0.23	0.02	0.09	0.01
Haro 2	1.28^a	0.10	0.53^a	0.04	0.15^a	0.01
Haro 3	1.79^a	0.15	0.77^a	0.07	0.23^a	0.02
He 2-10	6.67^a	0.54	2.64^a	0.22	0.79^a	0.07
HS 0017+1055	≤0.030	−	≤0.050	−	≤0.045	−
HS 0052+2536^b	0.058	0.007	0.03	0.01	0.018	0.009
HS 0822+3542^c	−	−	−	−	−	−
HS 1222+3741^c	−	−	−	−	−	−
HS 1236+3937	≤0.030	−	≤0.050	−	≤0.045	−
HS 1304+3529	0.038	0.007	≤0.050	−	≤0.045	−
HS 1319+3224^c	−	−	−	−	−	−
HS 1330+3651^c	−	−	−	−	−	−
HS 1442+4250	≤0.030	−	≤0.050	−	≤0.045	−
HS 2352+2733	≤0.030	−	≤0.050	−	≤0.045	−
I Zw 18	≤0.030	−	≤0.050	−	≤0.045	−
IC 10^d	101.^a	31.	47.6^a	14.8	16.3^a	5.1
II Zw 40	1.33^a	0.12	0.58^a	0.06	0.18	0.02
Mrk 1089^b	1.75^a	0.15	0.78^a	0.07	0.24^a	0.03
Mrk 1450	0.049	0.007	≤0.050	−	≤0.045	−
Mrk 153	0.048^a	0.008	≤0.050	−	≤0.045	−
Mrk 209	0.062	0.007	0.03	0.01	≤0.045	−
Mrk 930	0.40^a	0.04	0.13^a	0.01	0.049^a	0.007
NGC 1140	1.97^a	0.17	0.94^a	0.08	0.28^a	0.03
NGC 1569	12.0^a	1.0	5.02^a	0.41	1.55^a	0.13
NGC 1705	0.60^a	0.05	0.29^a	0.03	0.10^a	0.01
NGC 2366	2.04^a	0.17	1.01^a	0.09	0.39^a	0.04
NGC 4214	18.6^a	1.5	9.92^a	0.80	3.79^a	0.31
NGC 4449	32.4^a	2.6	14.8^a	1.2	5.01^a	0.41
NGC 4861	1.10^a	0.10	0.54^a	0.05	0.20^a	0.03
NGC 5253	7.82^a	0.63	3.64^a	0.29	1.18^a	0.10
NGC 625	4.33^a	0.35	2.18^a	0.18	0.80^a	0.07
NGC 6822^d	48.4^a	15.0	29.7^a	9.2	13.6^a	4.2
Pox 186	0.045	0.007	≤0.050	−	≤0.045	−
SBS 0335-052	≤0.030	−	≤0.050	−	≤0.045	−
SBS 1159+545	≤0.030	−	≤0.050	−	≤0.045	−
SBS 1211+540	≤0.030	−	≤0.050	−	≤0.045	−
SBS 1249+493	≤0.030	−	≤0.050	−	≤0.045	−
SBS 1415+437^c	−	−	−	−	−	−
SBS 1533+574	≤0.122^a	−	≤0.050	−	≤0.045	−
Tol 0618-402^c	−	−	−	−	−	−
Tol 1214-277	≤0.030	−	≤0.050	−	≤0.045	−
UGC 4483	0.024	0.006	≤0.050	−	≤0.045	−
UGCA 20^c	−	−	−	−	−	−
UM 133	0.032	0.006	≤0.050	−	≤0.045	−
UM 311^b	3.84^a	0.31	1.87^a	0.16	0.66^a	0.06
UM 448	0.99^a	0.08	0.38^a	0.03	0.13	0.01
UM 461	0.027	0.006	0.03	0.01	≤0.045	−
VII Zw 403	0.14^a	0.01	0.053	0.008	0.028	0.009

Notes. When an upper limit is given, it is the 5σ upper limit computed in 3.2.3.

^(a)

The flux densities are derived from aperture photometry, with the same aperture used for PACS.

^(b)

These objects are galaxies within compact groups of galaxies or are parts of other galaxies and the photometry given here is for the whole group (see Sect. 3.1.1 for details).

^(c)

These sources were not observed at all by SPIRE.

^(d)

The quoted flux densities for these sources have been corrected for cirrus contamination.

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