Click on this image or any of those below to obtain a larger version.
See Locations page for more information
on what part of the sky the Survey covers.
![]() 74cm Continuum (274k) |
![]() 21cm Continuum (377k) |
![]() 21cm Polarization (533k) |
![]() 60µm Dust Emission (235k) |
![]() HI Line (0 km/s) (360k) |
![]() CO Line (116k) |
![]() HI Line (-14 km/s) (390k) |
![]() CO Line (133k) |
![]() HI Line (-41 km/s) (399k) |
![]() CO Line (115k) |
These images were generated with the Karma software package. The 2.6mm CO maps are truncated due to coverage limitations of CO data; see Locations page for details.
![]() Red = 100µm Green = 60µm Blue = 21cm Cont (363k) |
![]() Red = 60µm Green = HI -40 km/s Blue = CO -40 km/s (475k) |
These images were generated with the IDL and Astronomy User's Library software packages.
These are available through the Pilot Project page.
![]() 74cm Continuum, Stokes I (102k) |
![]() 21cm Continuum, Stokes I (217k) |
![]() 21cm Line, -35.3 km/s (260k) |
![]() 21cm Continuum, Stokes Q (221k) |
These images were generated with the Karma, IRAF, and SAOimage software packages.
![]() 21cm Continuum, Stokes I (140k) |
![]() 21cm Continuum, Stokes Q (362k) |
![]() 21cm Line, +20.8 km/s (437k) |
![]() 21cm Line, -0.6 km/s (509k) |
These images were generated with the Karma, IRAF, and SAOimage software packages.
Large-scale structure information has not yet been included in these images; this is the reason for the dark areas found adjacent to narrow, bright sources. The Hydrogen maps are also less extensive than the continuum maps, lacking four fields on the east (left) edge -- see overview image at top of page.