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2881. Emma Kirby - Contact
. Homepage . Science . Outreach . Travel . Other . Contact Me . Postal Address: . Mt Stromlo Observatory . Cotter Road . Weston Creek . ACT 2611 . AUSTRALIA . Phone Numbers: . Work: +61 2 61250221 . Mob: +61 4 22283524 . Emails . emma AT mso.anu.edu.au (Replace AT with @ symbol) . Copyright 2007 Emma Kirby. Parts of the webpage design was obtained from Free CSS Templates. All Photos were taken by Emma Kirby unless otherwise stated.
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Ссылки http://www.mso.anu.edu.au/~emma/contact/contact.html -- 3.0 Кб -- 01.10.2012
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2882. Observational Techniques: Assignment 1
The aim of this assignment is to teach you how to carry out a very common programming task: reading in a bunch of data from a text file, doing something with it then writing the results out again. ... The goal of the assignment is to write a computer program which will select this sample for you. You will pick the micro-quasars to observe from a rather large catalogue, which can be found here: The catalogue is an ASCII (text) file - you can inspect it with a normal text editor. ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/ObsTech/Ass1.html -- 4.6 Кб -- 01.10.2012
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2883. Untitled Document
The new Mount Stromlo will offer three telescopes for public access, restored heritage buildings and improved research facilities. The Oddie Telescope in 1911 . ... Mount Stromlo Observatory is the oldest continuously operating research observatory in Australia, lost five telescopes, heritage buildings, workshops and houses in bushfires on January 18 this year. ... The Oddie Telescope will be restored for public use and the Old Administration Building will house offices and an astronomy library. ...
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Ссылки http://www.mso.anu.edu.au/~brian/press/Heritage.html -- 3.9 Кб -- 01.10.2012
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2884. GSAOI Red Supergiants Science Page
... GSAOI Home . ... Science . ... They used Cepheid variables out to 20 Mpc as the calibrating method for a host of secondary distance indicators such as Type Ia supernovae, surface brightness fluctuations, and the Tully Fisher method. ... Luminous red supergiants provide a new method of measuring the Hubble constant that is independent of the Cepheid distances. ... Larger spiral galaxies will yield larger numbers of red supergiants and hence a more accurate distance modulus. ...
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Ссылки http://www.mso.anu.edu.au/gsaoi/science/redsgs.shtml -- 6.7 Кб -- 01.10.2012
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2885. GSAOI Dwarf Galaxies Science Page
... GSAOI Home . ... Science . ... For example, among the Milky Way's dE companions we see systems with dominant old populations, systems with minor intermediate-age (age ~ 2 to 10 Gyr) components, and systems where the intermediate-age component dominates the old stars. ... This variety of star formation histories is not restricted to the Galaxy's companions. ... To make progress in understanding the processes that govern dwarf galaxy evolution, we need to study systems beyond the Local Group. ...
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Ссылки http://www.mso.anu.edu.au/gsaoi/science/dwarfs.shtml -- 9.5 Кб -- 01.10.2012
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2886. Gemini Near-Infrared Integral-Field Spectrograph (NIFS) IFU.
The first near-infrared IFU spectrograph was the 3D instrument , constructed by the Max Planck Institut f r Extraterrestrische Physik. ... An effective slit width of 0.1" was chosen in order to probe to spatial scales approaching the 0.07" diffraction-limited image core size expected from the Gemini adaptive optics system at 2.2 microns while maintaining an acceptable field-of-view. ... The field mirror array then feeds the spectrograph collimator mirror (seen at left in the above figure). ...
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Ссылки http://www.mso.anu.edu.au/nifs/description/ifu.shtml -- 6.7 Кб -- 01.10.2012
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2887. GSAOI Contacts Page
RSAA Home . GSAOI Home . ... Contact Us . ... RSAA . 61 2 6125 0268 . ... 61 2 6125 8913 . ... 61 2 6125 0212 . ... 61 2 6125 8031 . ... 61 2 6125 0264 . ... 61 2 6125 8038 . Peter McGregor . ... 61 2 6125 8033 . ... 61 2 6125 8035 . ... 61 2 6125 8042 . ... Peter Wood . ... 61 2 6125 8032 . ... 61 2 6125 0238 . Peter Conroy . ... 61 2 6125 8022 . ... 61 2 6125 0239 . ... 61 2 6125 8046 . ... Project Engineer . ... Project Manager . ... Technical Programme Manager . Peter Young . ...
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Ссылки http://www.mso.anu.edu.au/gsaoi/contacts/index.shtml -- 9.6 Кб -- 01.10.2012
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2888. DBS Grating Calculator
Blue Grating (l/mm) 300(1) 600(1) 1200(1) 1200(2) . Red Grating (l/mm) 158(1) 316(1) 600(1) 1200(1) . Blue Central Wavelength ( ) Blue Grating Angle (deg) . Red Central Wavelength ( ) Red Grating Angle (deg) . ... Blue Arm . Red Arm . Grating Angle . deg. min. deg. min. Central Wavelength . ... Wavelength Range . ... It is maintained by Peter McGregor peter@mso.anu.edu.au This calculator requires a javascript-enabled browser. ...
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Ссылки http://www.mso.anu.edu.au/~peter/dbsang/dbsang.html -- 17.5 Кб -- 01.10.2012
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2889. High-Z SN Search
. Sorry, browsers with frames only...
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Ссылки http://www.mso.anu.edu.au/~brian/PUBLIC/public.html -- 1.4 Кб -- 01.10.2012
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2890. Sounds of the Universe
Here are links to several other web pages containing sounds from space. Unlike on my page, these are real acoustic (sound) waves, not electromagnetic waves converted to sounds. Sounds on Titan. Sounds of the Big Bang, acoustic oscillations converted into audible sounds. More sounds of the Big Bang . Sounds of Pulsars: pulsing signal amplitudes converted to sounds. More pulsar sounds . Sounds of our Sun , solar oscillations increased in frequency to become audible. Sounds of another star
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Ссылки http://www.mso.anu.edu.au/pfrancis/Music/links.html -- 2.3 Кб -- 01.10.2012
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2891. Sounds of the Universe
Sound waves cannot travel through the vacuum of space. ... These electromagnetic waves can be recorded by devices called spectrographs on many of the world's most powerful telescopes. On this web page, I have converted these electromagnetic waves into sound waves. I've also reduced the frequency 1.75 trillion times: the original frequencies are much too high for humans or even dogs to hear. This allows us to listen to many parts of the universe for the first time. ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/Music/intro.html -- 2.1 Кб -- 01.10.2012
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2892. GSAOI Orion Nebula Cluster Science Page
... GSAOI Home . ... Science . ... Deep imaging at J , H , and K is required to identify all stellar objects, brown dwarfs, and planetary mass objects in the central region of the Orion Nebula Cluster down to masses comparable to that of Jupiter. This is required to establish the initial mass function, i.e., the number of stars of each mass that have formed, in this region of intense massive star formation. ... The fields of the GSAOI detectors are shown as four green squares in each frame. ...
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Ссылки http://www.mso.anu.edu.au/gsaoi/science/orion.shtml -- 6.7 Кб -- 01.10.2012
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2893. GSAOI Disk Galaxies Science Page
... The formation of the disks of disk galaxies remains poorly understood. ... Many disk galaxies have only the thin disk component, with no bulge or significant thick disk. ... Almost all disk galaxies have an exponential radial surface brightness distribution. The reason for this exponential form is not known; nor is it known when the exponential form is established. ... We would compare low redshift galaxies observed in the I band with galaxies at z =0.5 in the J band and at z =1 in the H band. ...
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Ссылки http://www.mso.anu.edu.au/gsaoi/science/disks.shtml -- 7.4 Кб -- 01.10.2012
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2894. Paul Francis: Publications
44: An 80 Mpc Filament of galaxies at redshift 2.38 . Woodgate, B.E., Palunas, P., Francis, P.J., Williger, G.M. Teplitz, H.I. 2003, AAS 203.8910 (abstract) . ... Francis, P.J., Wilson, G.M. Woodgate, B.E. 2000, in "Cosmic Evolution and Galaxy Formation: Structure, Interactions and Feedback", proceedings of the 3rd Guillermo Haro Astrophysics Conference (Puebla, Mexico, 15-19 Nov 1999), eds/ Franco, J., Terlevich, E., Lopez-Crus Aretxaga, I. 2000, 279-281 . ... 12: A Group of Galaxies at z=2.38 . ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/papers/conf.html -- 13.4 Кб -- 01.10.2012
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2895. GSAOI Picture Gallery Page
. RSAA Home . GSAOI Home . Instrument . Description . Science . Picture Gallery . Performance . Calculator . Contact Us . Internal . Other Links . Research School of Astronomy and Astrophysics . Gemini Telescopes . Multi-Conjugate Adaptive Optics . GSAOI Conceptual Design Review (August 2002)
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Ссылки http://www.mso.anu.edu.au/gsaoi/gallery/index.shtml -- 4.5 Кб -- 01.10.2012
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2896. Welcome to JonghwanтАЩs Home
. а . а . а . Welcome to JonghwanтАЩs Home . а . а . а . а
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Ссылки http://www.mso.anu.edu.au/~jrhee/Site/Welcome.html -- 7.5 Кб -- 01.10.2012
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2897. CHIAKI's Presentations
... Luminosity Evolution of the Milky Way Galaxy (gif 1.5MB), Kobayashi 2004 . Luminosity Evolution of Elliptical Galaxy that form through monolithically (gif 2.2MB), Kobayashi 2004 . Luminosity Evolution of Elliptical Galaxy that form through monolithically (mpg 1.1MB), Kobayashi 2004 . Luminosity Evolution of Elliptical Galaxy that form through major mergers (gif 2.5MB), Kobayashi 2004 . ... V-Luminosity Maps of 124 Elliptical Galaxies (gif 121KB), Kobayashi 2004 . ...
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Ссылки http://www.mso.anu.edu.au/~chiaki/works/index.html -- 6.3 Кб -- 01.10.2012
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2898. Emma Kirby - Travel
. Homepage . Science . Outreach . Travel . Other . Contact Me . Work . Other . 24 - 26 October 2008: Siding Spring . 17 - 28 November 2008: Winter School - Canary Islands . 1 - 5 December 2008: University Bonn? - Germany . 9 - 17 December 2008: LVHIS Observing & DA- ATCA, Narrabri . Copyright 2007 Emma Kirby. Parts of the webpage design was obtained from Free CSS Templates. All Photos were taken by Emma Kirby unless otherwise stated.
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Ссылки http://www.mso.anu.edu.au/~emma/travel/travel.html -- 3.0 Кб -- 01.10.2012
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2899. GSAOI Open Cluster Science Page
... GSAOI Home . ... Science . ... The goal of this project is to detect the termination of the white dwarf cooling sequence in nearby open star clusters, and hence derive cluster ages that are independent of the normal main sequence turnoff method. ... The potential for accurate proper motion measurements, i.e., measurements of transverse motion across the sky, with GSAOI offers a means of overcoming this difficulty. ...
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Ссылки http://www.mso.anu.edu.au/gsaoi/science/open.shtml -- 5.6 Кб -- 01.10.2012
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2900. GSAOI Bulk Motions Science Page
... GSAOI Home . ... Science . ... It is widely accepted that the evolution of the large scale structure of the Universe is driven by dark matter. Understanding this dark matter continues to be one of Astronomy's great unsolved problems. Measuring the bulk motions of galaxies allows us to map the overall mass distribution of the Universe in a way that is independent of the luminous matter in galaxies. ...
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Ссылки http://www.mso.anu.edu.au/gsaoi/science/bulk.shtml -- 6.9 Кб -- 01.10.2012
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