TY - JOUR
T1 - The ATLAS 5.5 gHz survey of the extended chandra deep field south
T2 - Catalogue, source counts and spectral indices
AU - Huynh, M. T.
AU - Hopkins, A. M.
AU - Lenc, E.
AU - Mao, M. Y.
AU - Middelberg, E.
AU - Norris, R. P.
AU - Randall, K. E.
PY - 2012/11/1
Y1 - 2012/11/1
N2 - Star-forming galaxies are thought to dominate the sub-mJy radio population, but recent work has shown that low-luminosity active galactic nuclei (AGNs) can still make a significant contribution to the faint radio source population. Spectral indices are an important tool for understanding the emission mechanism of the faint radio sources. We have observed the extended Chandra Deep Field South at 5.5 GHz using a mosaic of 42 pointings with the Australia Telescope Compact Array. Our image reaches an almost uniform sensitivity of ∼12 μJy rms over 0.25 deg 2 with a restoring beam of 4.9 arcsec × 2.0 arcsec, making ATLAS 5.5 GHz survey one of the deepest 6 cm surveys to date. We present the 5.5 GHz catalogue and source counts from this field. We take advantage of the large amount of ancillary data in this field to study the 1.4 to 5.5 GHz spectral indices of the sub-mJy population. For the full 5.5 GHz selected sample we find a flat median spectral index, α med = -0.40, which is consistent with previous results. However, the spectral index appears to steepen at the faintest flux density levels (S 5.5 GHz < 0.1mJy), where α med =-0.68. We performed stacking analysis of the faint 1.4 GHz selected sample (40 < S 1.4 GHz < 200 μJy) and found a steep average spectral index, α = -0.8, consistent with synchrotron emission. We also found a weak trend of steepening spectral index with redshift. Several young AGN candidates are identified using spectral indices, suggesting that gigahertz peaked-spectrum sources are as common in the mJy population as they are at Jy levels.
AB - Star-forming galaxies are thought to dominate the sub-mJy radio population, but recent work has shown that low-luminosity active galactic nuclei (AGNs) can still make a significant contribution to the faint radio source population. Spectral indices are an important tool for understanding the emission mechanism of the faint radio sources. We have observed the extended Chandra Deep Field South at 5.5 GHz using a mosaic of 42 pointings with the Australia Telescope Compact Array. Our image reaches an almost uniform sensitivity of ∼12 μJy rms over 0.25 deg 2 with a restoring beam of 4.9 arcsec × 2.0 arcsec, making ATLAS 5.5 GHz survey one of the deepest 6 cm surveys to date. We present the 5.5 GHz catalogue and source counts from this field. We take advantage of the large amount of ancillary data in this field to study the 1.4 to 5.5 GHz spectral indices of the sub-mJy population. For the full 5.5 GHz selected sample we find a flat median spectral index, α med = -0.40, which is consistent with previous results. However, the spectral index appears to steepen at the faintest flux density levels (S 5.5 GHz < 0.1mJy), where α med =-0.68. We performed stacking analysis of the faint 1.4 GHz selected sample (40 < S 1.4 GHz < 200 μJy) and found a steep average spectral index, α = -0.8, consistent with synchrotron emission. We also found a weak trend of steepening spectral index with redshift. Several young AGN candidates are identified using spectral indices, suggesting that gigahertz peaked-spectrum sources are as common in the mJy population as they are at Jy levels.
KW - Galaxies:evolution
KW - Radio continuum:galaxies
UR - http://www.scopus.com/inward/record.url?scp=84867606534&partnerID=8YFLogxK
U2 - 10.1111/j.1365-2966.2012.21894.x
DO - 10.1111/j.1365-2966.2012.21894.x
M3 - Article
AN - SCOPUS:84867606534
SN - 0035-8711
VL - 426
SP - 2342
EP - 2358
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 3
ER -