ALMA Deep Field in SSA22: Survey Design and Source Catalog of a 20
  arcmin^2 Survey at 1.1mm
  To search for dust-obscured star-formation activity in the early Universe, it
is essential to obtain a deep and wide submillimeter/millimeter map. The advent
of the Atacama Large Millimeter/submillimeter Array (ALMA) has enabled us to
obtain such maps at sufficiently high spatial resolution to be free from source
confusion. We present a new 1.1mm map obtained by ALMA in the SSA22 field.
SSA22 contains a remarkable proto-cluster at z=3.09 and is therefore an ideal
region to investigate the role of large-scale cosmic web on dust-obscured star
formation. The typical 1sigma depth of our map is 73 uJy/beam at a 0.5
resolution; combined with earlier, archived observations, we map an area of 20
arcmin^2 (71 comoving Mpc^2 at z=3.09). Within the combined survey area we have
detected 35 sources at a signal-to-noise ratio (S/N) >5, with flux densities,
S1.1mm=0.43--5.6 mJy, equivalent to star-formation rates of >=100--1000 Msun/yr
at z=3.09, for a Chabrier initial mass function; of these, 17 are new
detections. The cumulative number counts show a factor 3--5x excess compared to
blank fields. The excess suggests enhanced dust-enshrouded star-formation
activity in the proto-cluster on a 10 comoving Mpc scale, indicating
accelerated galaxy evolution in this overdense region.
