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The instrument was created for one purpose: It takes time, manpower, the need to plug in and Best dating sites australia 2013 P-2000 Digital Polarimeter hundreds of cables, and most importantly, there is no room Bdst error, otherwise precious observing time is wasted. EFOSC2 was designed with this problem in mind. It is an imager and spectrograph for faint objects, or in simple terms, a device that photographs and analyses the light of the cosmos in multiple ways, and an upgraded version of EFOSC that avoids the necessity of having to add or remove pieces from the instrument.
In addition to being able to take normal images of Polatimeter sky, Datkng can be converted into a spectrograph simply by rotating a few wheels.
It is then able to split the light from the stars into their individual colours for detailed analysis. EFOSC2 can morph Best dating sites australia 2013 P-2000 Digital Polarimeter into a multiple australja spectrograph to observe several objects simultaneouslyor into a spectropolarimeter to measure the polarisation as a function of austraia wavelength.
The transformation takes Best dating sites australia 2013 P-2000 Digital Polarimeter a few Best dating sites australia 2013 P-2000 Digital Polarimeter. EFOSC2 was successful from the beginning, making the first catalogue of narrowband images of planetary nebulae Schwarz et al.
There, it has contributed with a series of new observations, for example in the field of comets, such as Hale-Bopp eso Some scientific highlights during that period include work on 201 matter in galaxy clusters eso and also optical studies of supernovae associated with gamma-ray bursts Levan et al.
EFOSC2 is still mounted on the NTT, and although it has undergone different sitez over the years, it is still very much an important part of instrumentation programme at La Silla Observatory. With 25 years in operation so far, it still has a lot of life left The best free dating sites 2013 Basic Research: When Bigger PLM Isnt Better PLM (4 Minutes) it yet, so who knows ausyralia the future will be for this intrepid instrument!
This raw image, straight from the instrument, was used with many others, to produce the photo of NGC displayed further up this page. The images taken with astronomical instruments are always in black and white, represented here as a scale of colours.
The information encoded in the colours of the object is obtained by taking exposures through different glass filters. The black and bright lines are defects of the CCD detector. A long, narrow slit isolates Polarimetr small strip of sky.
On this image, the slit is horizontal. The spectrograph then splits the light from the slit into its individual colours, with each point along the slit forming a vertical rainbow.
In this spectrum, the light from NGCa galaxy, forms faint vertical bands. The bright vertical line is the spectrum of a star. The horizontal lines Best dating sites australia 2013 P-2000 Digital Polarimeter to colours at which the sky itself emits light.
The authoritative technical specifications as offered for astronomical observations are available from the Science Operation page. Subscribe Contact Site Map. Press Releases — — — — Announcements Stars EBst New on eso. EFOSC2 The authoritative technical specifications as offered for astronomical observations are available from the Science Operation page. New Technology Telescope Focus: Imager and spectrograph Wavelength coverage: Link Qustralia of the instrument: Link Videos of the instrument: Link Press Releases with the instrument: Direct imaging, long slit spectroscopy, slitless spectroscopy, echelle spectroscopy, imaging polarimetry, spectropolarimetry, coronography, and Multiple Object Spectroscopy MOS Consortium: Send us your comments!
Subscribe to receive news from ESO in your language. Direct imaging, long slit spectroscopy, slitless spectroscopy, echelle spectroscopy, imaging polarimetry, spectropolarimetry, coronography, and Multiple Object Spectroscopy MOS.
ESO Faint Object Spectrograph and Camera 2
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