Astrometry: Revealing the Other Two Dimensions of
... observations showed relative motion. Others, for example Bode, held onto the accidental alignment hypothesis and advanced the utility of double stars for parallax and proper ...
... observations showed relative motion. Others, for example Bode, held onto the accidental alignment hypothesis and advanced the utility of double stars for parallax and proper ...
test methods for secondary mirrors of cassegrain telescopes with
... Disadvantages: Two telescopes must be available at the same time and in the same place. ...
... Disadvantages: Two telescopes must be available at the same time and in the same place. ...
Celestron Telescope Accessory Catalog
... These are Celestron’s top of the line eyepieces, utilizing a hybrid design of five elements. They feature long eye relief and a wide field, and each air-to-glass surface is fully multicoated to enhance contrast levels. These special eyepieces are computer designed to keep visual aberrations to an ab ...
... These are Celestron’s top of the line eyepieces, utilizing a hybrid design of five elements. They feature long eye relief and a wide field, and each air-to-glass surface is fully multicoated to enhance contrast levels. These special eyepieces are computer designed to keep visual aberrations to an ab ...
Projects
... NMG Gemini Near Infrared Spectrograph (GNIRS) DESCRIPTION: The Gemini Near Infrared Spectrograph is a $4.2 million long-slit spectrometer that has been mounted on the Gemini South 8-meter Telescope on Cerro Pachon, Chile. It will operate from 1 to 5 um and will offer two plate scales and a range of ...
... NMG Gemini Near Infrared Spectrograph (GNIRS) DESCRIPTION: The Gemini Near Infrared Spectrograph is a $4.2 million long-slit spectrometer that has been mounted on the Gemini South 8-meter Telescope on Cerro Pachon, Chile. It will operate from 1 to 5 um and will offer two plate scales and a range of ...
Sample pages 1 PDF
... roughly 100 GB of data every night, the reduction of which requires fast computers and vast storage capacities. The largest astronomical CCD camera currently is that of the PanSTARRS-1 telescope, with more than 1.4 billion pixels, covering about 6 deg2 on the sky. But it is not only optical astronom ...
... roughly 100 GB of data every night, the reduction of which requires fast computers and vast storage capacities. The largest astronomical CCD camera currently is that of the PanSTARRS-1 telescope, with more than 1.4 billion pixels, covering about 6 deg2 on the sky. But it is not only optical astronom ...
8 m Club Meeting - Adaptive optics
... NIRSPEC K-band image & spectra Closest ultracool companion around a main sequence star m = 8.6 mag ...
... NIRSPEC K-band image & spectra Closest ultracool companion around a main sequence star m = 8.6 mag ...
An Adaptive Secondary Mirror Demonstrator: Construction and
... mirror technology. An attractive application of this outside astronomy is the compensation of selfinduced free-air turbulent in very high power laser systems, where the adaptive metal mirror lends itself ideally to liquid cooling. The demonstrator is planned to be tested on the optical bench in the ...
... mirror technology. An attractive application of this outside astronomy is the compensation of selfinduced free-air turbulent in very high power laser systems, where the adaptive metal mirror lends itself ideally to liquid cooling. The demonstrator is planned to be tested on the optical bench in the ...
Lecture ppt - UCO/Lick Observatory
... – Shape of mirror surface when you push just one actuator (like a Greens’ function) – Can optimize your AO system with a particular influence function, but performance is pretty forgiving Page 10 ...
... – Shape of mirror surface when you push just one actuator (like a Greens’ function) – Can optimize your AO system with a particular influence function, but performance is pretty forgiving Page 10 ...
Experimental FLIR study Gruber, James Powell Calhoun: The NPS Institutional Archive 1979-06
... light and then switched to the infrared wavelengths. The FLIR has imaged scenes with a temperature difference of 9°K above ambient. MTF measurements havp shown it to be diffraction ...
... light and then switched to the infrared wavelengths. The FLIR has imaged scenes with a temperature difference of 9°K above ambient. MTF measurements havp shown it to be diffraction ...
The US Air Force Academy Falcon Telescope Network
... small aperture telescopes called the Falcon Telescope Network (FTN). Led by the Department’s Center for Space Situational Awareness Research (CSSAR), the FTN will provide USAFA cadets and faculty with world-class capability to conduct research in satellite characterization and astronomy. Partnering ...
... small aperture telescopes called the Falcon Telescope Network (FTN). Led by the Department’s Center for Space Situational Awareness Research (CSSAR), the FTN will provide USAFA cadets and faculty with world-class capability to conduct research in satellite characterization and astronomy. Partnering ...
Site testing for the Discovery Channel Telescope
... Figure 7. Cross-correlations of measured velocities at 11.6m and 9.8m (upper), and 4.9m (lower). Due a overly large deadband gaps in several of the direction sensors, and the fact that two types of potentiometers were in use, extraneous direction readings required filtering. Direction cross-correlat ...
... Figure 7. Cross-correlations of measured velocities at 11.6m and 9.8m (upper), and 4.9m (lower). Due a overly large deadband gaps in several of the direction sensors, and the fact that two types of potentiometers were in use, extraneous direction readings required filtering. Direction cross-correlat ...
ISNS3371_040507_bw - The University of Texas at Dallas
... eyepiece (ocular). Incident light rays (from the left) are refracted by the objective and the eyepiece and reach the eye of the person looking through the telescope (to the right of the eyepiece). If the focal length of the objective (f1) is bigger than the focal length of the eyepiece (f1), the ref ...
... eyepiece (ocular). Incident light rays (from the left) are refracted by the objective and the eyepiece and reach the eye of the person looking through the telescope (to the right of the eyepiece). If the focal length of the objective (f1) is bigger than the focal length of the eyepiece (f1), the ref ...
Cvetojevic_PIMMS_11 - School of Physics
... through and approaching the noise floor of our detector. Our detector was not sensitive enough ...
... through and approaching the noise floor of our detector. Our detector was not sensitive enough ...
ppt
... of young, blue stars. Astronomers now believe that Andromeda has one core. The two bright blobs are actually the ring of red stars and the disk of blue stars. ...
... of young, blue stars. Astronomers now believe that Andromeda has one core. The two bright blobs are actually the ring of red stars and the disk of blue stars. ...
Optical Fabrication and Testing - National Optical Astronomy
... – Science: 3-D map of the early universe Near IR Deployable Integral Field Spectrograph NIRDIF – Science: deconstructing young galaxies and pre-galactic fragments Mid-IR, High Dispersion, AO Spectrograph MIHDAS – Science: origins of planetary systems Near IR, AO Echelle Spectrograph NIrES – Science: ...
... – Science: 3-D map of the early universe Near IR Deployable Integral Field Spectrograph NIRDIF – Science: deconstructing young galaxies and pre-galactic fragments Mid-IR, High Dispersion, AO Spectrograph MIHDAS – Science: origins of planetary systems Near IR, AO Echelle Spectrograph NIrES – Science: ...
Active mirror technology for large space telescopes
... holding the actuators will show up in the mirror surface. System performance is maintained by sensing the wavefront and applying a real time correction to the optical surface, via the actuators. Unlike the rigid mirrors, the thin mirrors are controlled using the local influence from actuators, rathe ...
... holding the actuators will show up in the mirror surface. System performance is maintained by sensing the wavefront and applying a real time correction to the optical surface, via the actuators. Unlike the rigid mirrors, the thin mirrors are controlled using the local influence from actuators, rathe ...
solartele
... Keplerian telescope). Another mounts the drawing easel in a framework and slides on a rail. The fully developed helioscope is on an equatorial mount with a circle graduated into 24 hours for right ascension, and a graduated sector for declination. All of these instruments are built to maintain the d ...
... Keplerian telescope). Another mounts the drawing easel in a framework and slides on a rail. The fully developed helioscope is on an equatorial mount with a circle graduated into 24 hours for right ascension, and a graduated sector for declination. All of these instruments are built to maintain the d ...
A Bluetooth Telescope Controller - ATM
... The 30F4011 DSC contains the software that basically converts LX-200 commands into pulses for the steppers. This sounds simpler than it is in reality: the command “go to this RA-Dec coordinate” requires these equatorial coordinates to be transformed into telescope based Hor-Ele reference system, whi ...
... The 30F4011 DSC contains the software that basically converts LX-200 commands into pulses for the steppers. This sounds simpler than it is in reality: the command “go to this RA-Dec coordinate” requires these equatorial coordinates to be transformed into telescope based Hor-Ele reference system, whi ...
- ALMA Observatory
... Since the beginning of time, human beings have been fascinated by the sky and stars. However, it was only with the invention of the telescope in 1609 that humans could begin to study astronomical objects in detail, transforming astronomy and taking discoveries to unprecedented levels thanks to techn ...
... Since the beginning of time, human beings have been fascinated by the sky and stars. However, it was only with the invention of the telescope in 1609 that humans could begin to study astronomical objects in detail, transforming astronomy and taking discoveries to unprecedented levels thanks to techn ...
CIN_602
... Similar to S2, but early science should include at least one bright-time instrument. The 'softest' requirement for WFOS is FoV. In other words, WFOS science must achieve the specified spectral resolution and wavelength coverage, but FoV is negotiable WFOS, as a D2 science instrument, must achieve ve ...
... Similar to S2, but early science should include at least one bright-time instrument. The 'softest' requirement for WFOS is FoV. In other words, WFOS science must achieve the specified spectral resolution and wavelength coverage, but FoV is negotiable WFOS, as a D2 science instrument, must achieve ve ...
Aryabhatta Research Institute of Observational Sciences
... expanding research in the key areas of it’s past activities, a major programme of highaltitude (∼ 2 km) atmospheric physics studies in the Central Himalayas as part of ISRO’s Geosphere-Biosphere Programme (GBP) is proposed as the Institute has about 50 years of night atmospheric extinction data obta ...
... expanding research in the key areas of it’s past activities, a major programme of highaltitude (∼ 2 km) atmospheric physics studies in the Central Himalayas as part of ISRO’s Geosphere-Biosphere Programme (GBP) is proposed as the Institute has about 50 years of night atmospheric extinction data obta ...
James Webb Space Telescope
The James Webb Space Telescope (JWST), previously known as Next Generation Space Telescope (NGST), is a space observatory under construction and scheduled to launch in October 2018. The JWST will offer unprecedented resolution and sensitivity from long-wavelength visible to the mid-infrared, and is a successor instrument to the Hubble Space Telescope and the Spitzer Space Telescope. The telescope features a segmented 6.5-meter (21 ft) diameter primary mirror and will be located near the Earth–Sun L2 point. A large sunshield will keep its mirror and four science instruments below 50 K (−220 °C; −370 °F).JWST's capabilities will enable a broad range of investigations across the fields of astronomy and cosmology. One particular goal involves observing some of the most distant objects in the Universe, beyond the reach of current ground and space based instruments. This includes the very first stars, the epoch of reionization, and the formation of the first galaxies. Another goal is understanding the formation of stars and planets. This will include imaging molecular clouds and star-forming clusters, studying the debris disks around stars, direct imaging of planets, and spectroscopic examination of planetary transits.In gestation since 1996, the project represents an international collaboration of about 17 countries led by NASA, and with significant contributions from the European Space Agency and the Canadian Space Agency. It is named after James E. Webb, the second administrator of NASA, who played an integral role in the Apollo program.The JWST has a history of major cost overruns and delays. The first realistic budget estimates were that the observatory would cost $1.6 billion and launch in 2011. NASA has now scheduled the telescope for a 2018 launch. In 2011, the United States House of Representatives voted to terminate funding, after about $3 billion had been spent and 75 percent of its hardware was in production. Funding was restored in compromise legislation with the US Senate, and spending on the program was capped at $8 billion. As of December 2014, the telescope remained on schedule and within budget, but at risk of further delays.