The Mopra Southern Galactic Plane CO Survey – Data Release 3. (arXiv:1902.04249v1 [astro-ph.GA])
<a href="http://arxiv.org/find/astro-ph/1/au:+Braiding_C/0/1/0/all/0/1">Catherine Braiding</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wong_G/0/1/0/all/0/1">G. F. Wong</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Maxted_N/0/1/0/all/0/1">N. I. Maxted</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Romano_D/0/1/0/all/0/1">D. Romano</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Burton_M/0/1/0/all/0/1">M. G. Burton</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Blackwell_R/0/1/0/all/0/1">R. Blackwell</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Filipovic_M/0/1/0/all/0/1">M. D. Filipović</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Freeman_M/0/1/0/all/0/1">M. S. R. Freeman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Indermuehle_B/0/1/0/all/0/1">B. Indermuehle</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lau_J/0/1/0/all/0/1">J. Lau</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rebolledo_D/0/1/0/all/0/1">D. Rebolledo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rowell_G/0/1/0/all/0/1">G. Rowell</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Snoswell_C/0/1/0/all/0/1">C. Snoswell</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tothill_N/0/1/0/all/0/1">N. F. H. Tothill</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Voisin_F/0/1/0/all/0/1">F. Voisin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wilt_P/0/1/0/all/0/1">P. de Wilt</a>
We present observations of fifty square degrees of the Mopra carbon monoxide
(CO) survey of the Southern Galactic Plane, covering Galactic longitudes $l =
300$-$350^circ$ and latitudes $|b| le 0.5^circ$. These data have been taken
at 0.6 arcminute spatial resolution and 0.1 km/s spectral resolution, providing
an unprecedented view of the molecular clouds and gas of the Southern Galactic
Plane in the 109-115 GHz $J = 1$-0 transitions of $^{12}$CO, $^{13}$CO,
C$^{18}$O and C$^{17}$O. We present a series of velocity-integrated maps,
spectra and position-velocity plots that illustrate Galactic arm structures and
trace masses on the order of $sim$10$^{6}$ M$_{odot}$ per square degree; and
include a preliminary catalogue of C$^{18}$O clumps located between
$l=330$-$340^circ$. Together with information about the noise statistics of
the survey these data can be retrieved from the Mopra CO website, the PASA data
store and the Harvard Dataverse (doi:10.7910/DVN/LH3BDN).
We present observations of fifty square degrees of the Mopra carbon monoxide
(CO) survey of the Southern Galactic Plane, covering Galactic longitudes $l =
300$-$350^circ$ and latitudes $|b| le 0.5^circ$. These data have been taken
at 0.6 arcminute spatial resolution and 0.1 km/s spectral resolution, providing
an unprecedented view of the molecular clouds and gas of the Southern Galactic
Plane in the 109-115 GHz $J = 1$-0 transitions of $^{12}$CO, $^{13}$CO,
C$^{18}$O and C$^{17}$O. We present a series of velocity-integrated maps,
spectra and position-velocity plots that illustrate Galactic arm structures and
trace masses on the order of $sim$10$^{6}$ M$_{odot}$ per square degree; and
include a preliminary catalogue of C$^{18}$O clumps located between
$l=330$-$340^circ$. Together with information about the noise statistics of
the survey these data can be retrieved from the Mopra CO website, the PASA data
store and the Harvard Dataverse (doi:10.7910/DVN/LH3BDN).
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