Sentences with phrase «observed at optical wavelengths»

Not exact matches

According to Mather and other leading astronomers now working on a report to be released this summer by the Association of Universities for Research in Astronomy (AURA), that quest and others require an even bigger space telescope that would observe, as Hubble does, at optical, ultraviolet and near - infrared wavelengths.

Her research interests include structure, interactions, and star formation in galaxies in the local universe and at high redshift, and she observes in optical, near - infrared, and radio wavelengths.

The team used the GROND imager at the 2.2 m ESO / MPG telescope of the European Southern Observatory in Chile to observe the planet simultaneously at seven different wavelength bands spanning the optical and near - infrared.

We observed and spatially resolved the disk around the ~ 10 Myr old protoplanetary disk HD 100453 in polarized scattered light with SPHERE / VLT at optical and near - infrared wavelengths, reaching an angular resolution of ~ 0.02», and an inner working angle of ~ 0.09».

We observed and spatially resolved the disk around the ~ 10 Myr old protoplanetary disk HD 100453 in polarized scattered light with SPHERE / VLT at optical and near - infrared wavelengths, reaching an angular resolution of ~ 0.02», and an inner working angle... ▽ More Understanding the diversity of planets requires to study the morphology and the physical conditions in the protoplanetary disks in which they form.

Nuclei were stained with Hoechst 33342 (5 μg / ml) and observed by a fluorescence microscope equipped with U-MWU optical filters with a U-MWU optical filter at an excitation wavelength of 355 nm and an emission wavelength of 420 nm.

At these wavelengths, astronomers can peer at the disks of gas and dust around newborn stars, see into star - forming clouds, and observe early galaxies that are bright in submillimetre wavelengths but obscured by dust in optical lighAt these wavelengths, astronomers can peer at the disks of gas and dust around newborn stars, see into star - forming clouds, and observe early galaxies that are bright in submillimetre wavelengths but obscured by dust in optical lighat the disks of gas and dust around newborn stars, see into star - forming clouds, and observe early galaxies that are bright in submillimetre wavelengths but obscured by dust in optical light.

There is however a wavelength dependent component to the atmospheric turbulence, which can introduce optical path length errors when observing at a wavelength different from that of the fringe sensing camera.

The cocoon also explains other details of the event, such as the initial bright blue flash observed at ultraviolet and optical wavelengths, and the delay in the appearance of X-rays and radio waves.