Sentences with phrase «oschin was the telescope»

The very intensity of a prophet's vision and his overpowering sense of its reality cause the interval before its fulfillment to be telescoped in his mind.

A special touch guests revel in is a telescope for viewing the spectacular night sky, complete with detailed astrological chart.

It seems like yesterday to many Americans older than 20, and time, in this case, will probably continue to be telescoped.

When buying a ladder be it telescoping or fiberglass extension; you must ensure that you consider if there are additional accessories.

It used to be a telescoping handle bar.

It is a telescoping handle bar that can be easily adjusted by pressing a button in the middle of the handle bar and pulling it out.

Other features that savvy moms and dads appreciate are the telescoping handle bar that extends way out and the large sun canopy with zippered extension panel for extra sun coverage.

An empty paper towel roll can be a telescope, a microphone or a tunnel.

Obviously, because it's telescope mounted, it gives you an amazing view of the stars, moon, and everything else you see in the night sky.

The Orion 52175 Solar System Camera is a telescope mountable camera that's great for someone who is just getting into astrophotography.

Here are the telescope accessories we recommend getting.

This is the telescope shape you're probably most familiar with.

Observations obtained a month later by members of the Planetary Sciences Group using the PlanetCam camera developed by this team and fitted to the 2.2 - m telescope at the Calar Alto Observatory in Almería (Spain) enabled the speed of this atmospheric structure to be confirmed.

What changed during the redesigns was the telescope's specific capabilities.

It was instantly obvious that the Oschin was the telescope to use to find the largest Kuiper belt objects out there.

The Very Large Telescope is a telescope facility operated by the European Southern Observatory on Cerro Paranal in the Atacama Desert of Northern Chile.

The image is a compotie of the i - band data (in red) from the Hyper Suprime - Cam at the Subaru Telescope and R - band (in green) and V - band (in blue) images from the Mayall 4 - m telescope at the Kitt Peak National Observatory of National Optical Astronomy Observatory.

The data set used by the researchers came from the High Accuracy Radial Velocity Planet Searcher (HARPS) using the ESO's 3.6 m telescope at La Silla Observatory, in Chile.

Seventy percent of the funding for the LMT has come from Mexico, and this is a telescope built in Mexico.

The initial discovery of this quasar (given the identity J1342 +0928) came to light thanks to the mining of three large area surveys: the DECam Legacy Survey (DECaLS) that is being carried out with the Dark Energy Camera on the National Science Foundations Blanco 4 - m telescope at the Cerro Tololo Inter-American Observatory in Chile, NASAs Wide - field Infrared Survey Explorer (ALLWISE), and the United Kingdom Infrared Telescope Deep Sky Survey (UKIDSS) Large Area Survey.

The term usually refers to optical telescopes, but there are telescopes for most of the spectrum of electromagnetic radiation and for other signal types.

The signal that arrives at the 1 - m telescope is extremely weak, with an average of 0.1 photons per received pulse.

SUVI is a telescope that monitors the sun in the extreme ultraviolet wavelength range.

She has also been Director of the Arizona Radio Observatory (ARO) for over 10 years and successfully managed the move and recommissioning of the new ARO 12 m telescope.

The VATT 1.8 m telescope's large aperture enables high - precision photometry even on the faintest EDEN / TS stars.

ALMA is a telescope suitable for analyzing molecules in galaxies because of: 1) a high sensitivity to detect faint radio signals; 2) a high fidelity imaging capability to image actual gas distributions; 3) the ability to observe wideband multiple wavelengths simultaneously, and high spatial resolution.

Currently there are two 2 - m telescopes, one in Hawaii and the other in Australia and a number of 1 - m telescopes at sites across the world.

Deadline: Friday 5 May 2017 (23:59:59 UTC) Proposals for APEX and the Onsala 20 m telescope are to be submitted through the NorthStar system.

Since the research team had already conducted radio observations of various molecular emissions in this galaxy with the 45 - m telescope at the Nobeyama Radio Observatory of NAOJ, they aimed to develop their research further with ALMA and identify the difference in chemical composition between AGNs and starburst regions.

Spectroscopic observations taken with the GTC - 10.4 m telescope reveal a broad (FWHM ~ 1100 km / s), double - peaked H alpha emission line from which we constrain the radial velocity semi-amplitude of the donor to be K2 > 250 km / s.

So, when was the telescope first «switched on»?

In order to test these models, the team of E. Papastergis, E. A. K. Adams and A. J. Romanowsky observed four isolated UDGs with the Effelsberg 100 - m telescope to place limits on the HI mass of these galaxies under the RadioNet Transnational Access program (Project 111 - 16).

Both 40 cm and 1 m telescopes possess a set of broad band filters including B, V Johnson and r» and i» sloan, which will be used to observe the targets.

This is a telescope with a primary mirror the size of a football field.

On the lower level, there is a telescope at the window which allows you to view the sky.

We obtained JHKs imaging of the 17» x 17» region around Sgr A *, an area containing 4339 of these X-ray sources, with the ISPI camera on the CTIO 4 - m telescope.

The IRAM 30 - m telescope (a.k.a Pico Veleta) is an important facility for the Event Horizon Telescope array and for the surveys searching for pulsars closely orbiting Sgr A *.

We installed and tested this interferometer in the Exoplanet Tracker (ET) instrument at the Kitt Peak 2.1 m telescope, an instrument built to demonstrate the principles of dispersed fixed delay interferometry.

There would be telescope operations since the typical visiting scientist would be unfamiliar with these structures.

Our recent observations at the KPNO 2.1 m telescope in 2002 demonstrate a short term Doppler precision of ~ 3 m / s with eta Cas (V = 3.5), a RV stable star and also obtained a RV curve for 51 Peg.

«The next phase is the telescope commissioning,» McKinnon continued.

More specifically, ALMA is a telescope that can recognize «strength» and «color» of radio waves.

The challenge, however, is that Hubble is a telescope in high demand — and the same is expected of Webb after its launch.

In addition to the 5 telescopes that belong to CTIO (the 4m Victor Blanco, and the 1.5 m, 1.3 m, 1.0 m, and 0.9 m telescopes run by the SMARTS consortium), there are a slew of other projects hosted on the mountain.

Most recently, the Keck Foundation provided the bulk of the funding for two 10 - m telescopes for a consortium led by the University of California and Caltech.

Abstract: We present a high spatial resolution, 10 - 20 micron survey of 65 T Tauri binary stars in Taurus, Ophiuchus, and Corona Australis using the Keck 10 m telescopes.

However, I was able to get up to the mountain for nine nights of observations with the 0.9 - m telescope, as well as half a night with the 4m Victor Blanco Telescope.

In addition to our time with the 0.9 m telescope, we also had time on the 4.1 m Victor Blanco Telescope, using the COSMOS instrument.

The ground - based observations made use of the HARPS spectrograph of the European Southern Observatory, located in La silla (Chile), and the high - resolution camera AstraLux installed on the 2.2 - m telescope at Calar Alto.

I am open to correction on this, but as best I can tell, the Hubble telescope would have something like 15 - centimeter resolving power if it were pointed at something on the Earth, like the Statue of Liberty (if you are a telescope expert, please write in and correct me if I am wrong).