95 datasets found

The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures....

SCUBA, the Submillimetre Common-User Bolometer Array, built by the Royal Observatory Edinburgh for the James Clerk Maxwell Telescope, is the most versatile and powerful of a new...

Planck is ESA's mission to observe the first light in the Universe. Planck was launched on 14 May 2009, and the minimum requirement for success was for the spacecraft to...

Planck is ESA's mission to observe the first light in the Universe. Planck was launched on 14 May 2009, and the minimum requirement for success was for the spacecraft to...

The Low Frequency Array (LOFAR) is the only existing radio interferometer able to observe at ultra-low frequencies (<100MHz) with high resolution (<15-arcsec) and high...

Radio observation from LOFAR PL610 station in Borowiec. The LOw Frequency ARray (LOFAR) is a radio interferometer operating at a low frequency range from 10 to 240 MHz. Single...

Decametric radio observation from Nancay decameter array. The Nancay Decameter Array (NDA) at the Station de Radioastronomie de Nancay (SRN) is a phased array of 144 "Teepee"...

This is the B component of a low-resolution map representing a weighted average of the f090 and f150 linear polarization. For a slightly deeper map, we combine the DR4 based on...

This is the U component of a low-resolution map representing a weighted average of the f090 and f150 linear polarization. For a slightly deeper map, we combined the DR4 based on...

This is the second field (f150) of an unpolarized map with three components corresponding to f090, f150 and f220 bands which are broad bands with center frequency roughly at 95...

This is the first field (f090) of an unpolarized map with three components corresponding t f090, f150 and f220 bands which are broad bands with center frequency roughly at 95...

This is the B component of a low-resolution map representing a weighted average of the f090 and f150 linear polarization. For a slightly deeper map, we combin the DR4 based on...

This is the third field (f220) of an unpolarized map with three components corresponding to f090, f150 and f220 bands which are broad bands with center frequency roughly at 95...

This is the Q component of a low-resolution map representing a weighted average of the f090 and f150 linear polarization. For a slightly depper map, we combine the DR4 based on...

This is the first field (f090) of an unpolarized map with three components corresponding to f090, f150 and f220 bands which are broad bands with center frequency roughly at 95...