An image from the Karl G. Jansky Very Large Array of the Galaxy Hercules A (also known as
3C348) showing powerful synchrotron jets emerging from its core, the site of a supermassive …

Software correlation, where a correlation algorithm written in a high-level language such as
C++ is run on commodity computer hardware, has become increasingly attractive for small …

The Very Long Baseline Array (VLBA) consists of ten high performance antennas and a 20-
station correlator. The 25-m-diameter reflector antennas are located geographically to …

We report new interferometric observations of IRAS 04368+ 2557 (L1527) in 13 CO (J= 1–
0), C 18 O (J= 1–0), and 2.7 mm continuum emission using the Nobeyama Millimeter Array …

In this paper, we describe the architecture and performance of the GRAPE-4 system, a
massively parallel special-purpose computer for N-body simulation of gravitational …

The establishment of the Nobeyama Radio Observatory (NRO) in 1982 was an important
event that greatly influenced the subsequent development of Japanese astronomy. The 45 …

The significance of radio astronomy at millimeter and submillimeter wavelengths is
described, and some of the more important results are given. The limitations imposed by the …

We have developed an FX-architecture digital spectro-correlator for the Atacama Compact
Array of the Atacama Large Millimeter/submillimeter Array. The correlator is able to …

STARBURST galaxies are those that are presently forming stars at a higher rate than that
averaged over the galactic lifetime. Starburst galaxies usually exhibit strong CO line …

We report aperture synthesis C 18 OJ= 1–0 observations of L1551 IRS 5 with a spatial
resolution of 2 &farcs; 8× 2 &farcs; 5 using the Nobeyama Millimeter Array. We have …