  We present the results of a high angular resolution (1.1") and sensitivity
(maximum of ~0.1 mJy) radio survey at 1-2 GHz in the Galactic Bulge. This
complements the X-ray Chandra Galactic Bulge Survey, and investigates the full
radio source population in this dense Galactic region. Radio counterparts to
sources at other wavelengths can aid in classification, as there are relatively
few types of objects that are reasonably detectable in radio at kiloparsec
distances, and even fewer that are detected in both X-rays and radio. This
survey covers about 3 square degrees of the Galactic Bulge Survey area
(spanning the Galactic coordinate range of -3deg < l < +3deg and +1.6deg < b <
+2.1deg as a first look into this region of the Galaxy with this combination of
frequency, resolution, and sensitivity. Spectral indices within the observed
band of 1-2 GHz were calculated for each source to assist in determining its
emission mechanism. We find 1617 unique sources in the survey, 25 of which are
radio counterparts to X-ray sources, and about 100 of which are steep-spectrum
(alpha <~ -1.4) point sources that are viable pulsar candidates. Four radio
sources are of particular interest: a compact binary; an infrared transient
with an inverted radio spectrum; a potential transitional millisecond pulsar
candidate; and a very steep spectrum radio source with an X-ray and bright
infrared counterpart. We discuss other notable sources, including possible
radio transients, potential new planetary nebulae, and active galactic nuclei.
