Linked from

The 14 pages that link to Submillimetre astronomy, each with the reason it gives.

• Infrared astronomyRelated: Its boundary with far-infrared astronomy is continuous, and both trace cold dust and gas.

• Event Horizon TelescopeRelated: The EHT’s short-wavelength observations reduce atmospheric and interstellar blurring of compact sources.

• Cosmic infrared backgroundRelated: Submillimeter surveys probe redshifted dust emission that forms part of the background.

• Cosmic dustRelated: Cold grains radiate at submillimeter wavelengths, allowing their mass and distribution to be mapped.

• Dark nebulaRelated: Cold dust in opaque clouds emits strongly at submillimeter wavelengths.

• Debris diskRelated: Long-wavelength observations trace cold dust and larger grains in outer disk regions.

• Ultraluminous infrared galaxyRelated: Submillimeter surveys identify distant, dust-rich galaxies related to ULIRGs.

• Rho Ophiuchi cloud complexRelated: These wavelengths trace cold dust and dense gas hidden within the complex.

• Atacama Large Millimeter/submillimeter ArrayRelated: Much of ALMA’s observing range lies in this atmospheric-sensitive part of the spectrum.

• Young stellar objectRelated: Its wavelengths trace the cold envelopes and disks surrounding young stellar objects.

• CW LeonisRelated: Submillimeter observations trace cool dust and molecules in the outer envelope.

• Infrared telescopeRelated: It borders infrared astronomy while requiring specialized high-altitude or space observatories.

• Mount GrahamRelated: The Submillimeter Telescope observes these wavelengths from the mountain.