169 citations · 936 across the 33 of their papers we have counts for
6 papers · 1 filter
The Seahorse Nebula: New views of the filamentary infrared dark cloud G304.74+01.32 from SABOCA, Herschel, and WISE
Oskari Miettinen
We mapped the filamentary infrared dark cloud (IRDC) G304.74+01.32 at 350 m with the SABOCA bolometer. The new SABOCA data have a factor of 2.2 times higher resolution than our…
An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution
Drew Brisbin, Oskari Miettinen, Manuel Aravena +28
We carried out targeted ALMA observations of 129 fields in the COSMOS region at 1.25 mm, detecting 152 galaxies at S/N5 with an average continuum RMS of 150 Jy. These fiel…
An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling
Oskari Miettinen, Ivan Delvecchio, Vernesa Smolčić +25
We determine the physical properties of a sample of SMGs in the COSMOS field that were pre-selected at the observed wavelength of mm, and followed up at $λ_{\rm o…
On the Kennicutt-Schmidt scaling law of submillimetre galaxies
Oskari Miettinen, Ivan Delvecchio, Vernesa Smolčić +3
The star formation rate per unit area correlates well with the gas surface density for different types of galaxies. However, this Kennicutt-Schmidt law has not yet been examined fo…
The VLA-COSMOS 3 GHz Large Project: The cosmic star formation history since z~5
M. Novak, V. Smolcic, J. Delhaize +19
We make use of the deep Karl G. Jansky Very Large Array (VLA) COSMOS radio observations at 3 GHz to infer radio luminosity functions of star-forming galaxies up to redshifts of z~5…
An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array
Oskari Miettinen, Mladen Novak, Vernesa Smolčić +32
We determine the radio size distribution of a large sample of 152 SMGs in COSMOS that were detected with ALMA at 1.3 mm. For this purpose, we used the observations taken by the VLA…