Open Access

Table 1

ALMA sources.

ID IDCLS RACLS, DecCLS Offset
3h 32m...,−27°... arcsec
(1) (2) (3) (4)
GS1 3280 14.55 s, 5256.54′′ 0.176,−0.188
GS2 5339 54.69 s, 5140.70′′ 0.052,−0.232
GS3 2619 39.25 s, 5325.71′′ 0.083,−0.173
GS4 7184 17.21 s, 5037.07′′ 0.161,−0.280
GS5 9834 35.72 s, 4916.04′′ 0.089,−0.248
GS6 14 876 28.51 s, 4658.14′′ 0.091,−0.269
GS7 8409 37.74 s, 5000.41′′ 0.067,−0.225
GS8 5893b 46.84 s, 5121.12′′ 0.081,−0.184

UDF1 15 669 44.03 s, 4635.70′′ 0.066,−0.277
UDF2 15 639 43.53 s, 4639.00′′ 0.057,−0.277
UDF3 15 876 38.54 s, 4634.06′′ 0.083,−0.243
UDF4 15 844 41.03 s, 4631.45′′ 0.063,−0.250
UDF5 13 508 36.97 s, 4727.21′′ 0.101,−0.239
UDF6 15 010 34.43 s, 4659.57′′ 0.100,−0.254
UDF7 15 381 43.32 s, 4646.80′′ 0.050,−0.250
UDF8 16 934 39.74 s, 4611.25′′ 0.043,−0.289
UDF11 12 624 40.05 s, 4755.46′′ 0.090,−0.242
UDF13 15 432 35.08 s, 4647.58′′ 0.098,−0.260
UDF16 14 638 42.38 s, 4707.61′′ 0.069,−0.242

Notes. Theupper part of the table lists the 8 galaxies (GS1 to GS8) observed with ALMA at 870 μm at a 0.2 arcsec resolution in our ALMA program. The lower part lists the 11 galaxies (UDF#) from the 1.3 mm ALMA survey of the HUDF by Dunlop et al. (2017) at a resolution of 0.35 arcsec. Column (1) simplified ID. For the UDF galaxies, we use the same IDs as in Dunlop et al. (2017). Columns (2) and (3) CANDELS ID and coordinates from Guo et al. (2013). GS8, initially associated with the galaxy with the CANDELS ID 5893, was found to be associated with a background galaxy that we will call 5893b (see Sect. 3.1). Column (4) offset to be applied to the HST CANDELS coordinates to match the ALMA astrometry.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.