#format jsmath = Night Vision - Exploration of the Infrared Universe = === Michael Rowan-Robinson, 2013 === ------- This is a book about the marvelous objects we can observe in the infrared, and the people who discovered them - not much technical detail about the instruments that make the measurements. The graphs are interesting, and tell us about instrument sensitivity: * p51 - Planetary nebula, λ 2 to 14 μm, 0 to 6e-16 W cm^2^μm. Sharp peaks (chemical resonances?), many less than 0.1μm wide, 1e-16 to 4e-16 on top of a broad 10μm thermal(?) peak, 300K? p-p noise 2e-17 Fred Gillette at UCSD, The Two Micron Survey, terrestrial telescopes, 1967? * p57 - two graphs, PAH (Polycyclic Aromatic Hydrocarbon) peaks. 3 to 18 μm <
>NGC 2023: $S^0_v$ 0 to 2500e-31 W/Hz<
>M17-SW: 0 to 8000e-31 W/Hz <
>est 300e-31 p-p noise. Leger, Puget, Allamandola around 1985. * p111 - KOBE 2.7K black body background. Presumably lots of averaging. * p175 - Herschel 190 to 315 μm wavelength * Other graphs, only relative vertical units. The book discusses these infrared observatories, extra information from wikipedia: * IRAS Infrared Astronomical Satellite, 1983 * 0.202 m^2^, 12/25/60/100 μm, 30as to 2am resolution, 2K, superfluid He * WMAP space telescope - microwave * KOBE space telescope - microwave * Hubble space telescope - optical * Spitzer space telescope IR * Herschel space telescope mid IR ESA * ISO Infrared Space Observatory, 1995-1998 ESA * 60 cm, 2.5 to 17 μm, 3.4K/1.9K superfluid He * JWST mid IR, 2018? * James Clerk Maxwell telescope on Mauna Kea * Altacama Large Millimeter/Submillimeter Telescope array * European Extremely Large Telescope, proposed 39 meter