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3mm spectral-line observing with Mopra. Tony Wong. ATNF & UNSW ... Interpolate to timestamps of spectra in aips reader (or better yet, using ...
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Tsys (at zenith) 143 K 177 K 299 K. Sensitivity (Jy/K) 43 62 111. Zenith opacity 0.102 0.121 0.180. Continuum flux sensitivity 0.54 Jy 1.34 Jy 2.99 Jy ...
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Contours: MAGMA CO data. Greyscale: IR excess map. Tracing H2 with NIR Extinction. Method outline: ... Peak HI Temp (contour) on Integrated CO. CO vs. HI in LMC ...
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multiply and accumulate. Synthesis Array Correlators. XF. For each baseline ( ~N2 ) ... Multiply corresponding frequencies. FX correlator has advantages for ...
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Calibration and Data reduction Strategies. Cormac Purcell & Ned Ladd. Mopra Training Weekend ... Pon-src = C [ Isrc e-t J(Tatm)(1-e-t) Ibg e-t IRx ] ...
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Chris Phillips & Juergen Ott at Mopra. Steve Tingay & Bob Sault at ATCA ... Observed continuum calibrator 1921-293 and SiO maser oCeti at 86 GHz ...
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ATNF Parkes, ATCA, Mopra, LBA-Correlator. UTas Hobart, Ceduna ... Tracy Getts effectively left. Paul Jones 6 months LBA correlator ...
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Title: Can extra-solar planets be detected with mm interferometry? Author: Vincent Minier Last modified by: Vincent Minier Created Date: 12/4/2001 4:30:19 AM
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Optical Near-Infrared (1 3.5 m, COBE) Far Infrared (12 100 m, IRAS) Methanol Masers ... Science with Antarctic Infrared and Sub-millimetre Telescopes
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What place for millimetre-wave in Australian radio astronomy for the next decade? ... directions for southern hemisphere mm-wave astronomy' meeting 30-31/03/06 ...
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Application for time via. http://opal.atnf.csiro.au. Proposal deadlines. June 15 (summer time) December 15 (mm) CABB - Present mm capabilities ...
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More clearly stated outreach goals for all ATNF ... May 2003: Transfer of a refurbished heliograph dish to St Columba High School ...
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First results from HOPS (The H2O southern Galactic Plane Survey) Andrew Walsh (JCU) ... Kate Brooks (ATNF) Chris Phillips (ATNF) Shari Breen (UTas) ...
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Polar molecules (have dipole moment) eg CO (E1 = 5K), HCN, CS, HCO ... Must Nod No chopping. OTF Mapping. Methanol Maser-selected Hot Molecular Core Survey ...
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Radio Astronomy an exciting science. May 2004. A. Tzioumis. 3. Oz ... Radio Astronomy is an exciting science - many 'weird and wonderful' objects. May 2004 ...
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Compute processes (Core) Incoming data stream is time divided and copied round ... 5 node, dual processor dual core. 4 (Intel) NICs for network flexibility ...
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Star Formation and Millimetre Astronomy Michael Burton School of Physics University of New South Wal
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Follow philosophy of MALT pilot study: Observe range of targets in variety ... molecular species towards various finder charts of high mass star forming cores. ...
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Galactic Molecular Survey (in progress)? Objectives: ... (3) bootstrap = Galactic properties = nearby extragalactic = distant galaxies ...
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Choose time to fringe check. Transfer some data to central processor ... Feedback from fringe checking into model. Monitoring of Clock Rate drifts (EVN style) ...
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Goal: In situ determination of zonal wind speed along Huygens ... VLBA Brewster. DWE: No nodding on Titan continuously. 14:49:14. 09:30:09. VLBA Owens Valley ...
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Summary of Australian e-VLBI activities. Steven Tingay. e-VLBI workshop, 31 May, 2004 ... Between various antennas, semi-regular real-time and delayed ...
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Massive Young Stars in the Galaxy Melvin Hoare University of Leeds UK
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... Plane Survey. Image Courtesy: Cormac Purcell. Andrew Walsh (JCU) ... Kate Brooks (ATNF) Chris Phillips (ATNF) Shari Breen (UTas) Maria Cunningham (UNSW) ...
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mixer. Local. oscillator. OMT. feed. fsignal ... Historically, when amplifers aren't available whack in a mixer anyway and do some science. ...
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... {7|7}7~77 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 ... WoXoYoo[oo]o^o_o`oaobocodoeofogohoiojokolomonooopoqorosotouovowoxoyozo{o|o }o~o ...
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Comet 19P/Borrelly ... Comet C/1999 H1 (Lee) ... For these comet observations (compared to say Galactic molecular clouds) it ...
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ALMA TAC and the proposal process Lister Staveley-Smith Member, ALMA Review Panel
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... a distributed, large-scale astronomical instrument of continental and inter ... Station Unit crashes: rewrote software, SU reboot during correlation job is now ...
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Dell PowerEdge 1600SC Apple XRaid. Server class computer. Currently ~2.05TB storage ... Dell PowerEdge machines. Capable of ~600Mb/sec sustained to disk ...
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Observat rio do CDCC - USP/SC
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Last report Nov 2002 4 months ago. Early ATUC late AT steering committee ... Prelude to international 'radio quiet reserves'? Follow up at ITU-R ...
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Australian Astronomy MNRF
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Richard Schilizzi, Tony Beasley, Don Campbell, ... Chief Investigator: Michael Etheridge. Project Scientist: Kurt Lambeck / Paul Tregonning ...
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Software correlation of full experiment on Swinburne supercomputer. SKA simulations. Provide supercomputing resources and software development to the national and ...
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History and Technical Development of VLBI = Very Long Baseline ... of a quasar at z=1.2. ... frame defined by the distant quasars and active galaxy nuclei. ...
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The APT network aims to provide a forum to discuss issues ... E-VLBI within Japan - Geodesy and astronomy. China. Internal e-VLBI network - rapidly developing ...
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The Red MSX Source Survey. RMS Team: Stuart Lumsden, Rene Oudmaijer, James ... Toby Moore, James Allsopp (Liverpool JMU) Cormac Purcell, Michael Burton (UNSW) ...
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... extra-solar systems (Minier, Lineweaver, Burton, Purcell, Longmore, Norris, 2003) ... Plane (Minier, Burton, Wong, Purcell, Hill, Longmore, Barnes, 2002 2003) ...
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The Research School of Astronomy & Astrophysics. the Australian National University ... Each proposal is introduced (summarised) by one member of the TAC, discussed, ...
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The Nature of Light. Light travels through space at a finite speed ... VIPER: cosmic microwave background. AMANDA (particle astronomy) Neutrinos. Cosmic Rays ...
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Three common maser species. H2O. OH. CH3OH two types of maser sources ... Pumped by mid-infrared radiation. High density. High methanol abundance ( 10-8) ...
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Maximum resolution of an instrument is proportional to ... image courtesy Crystal Brogan. Dodson, Legge et al, ApJ, 2003. Edward Fomalont & Sergei Kopeikin ...
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All have equatorial bulges except one. It is perfectly round. ... High-sensitivity observations: big antennas! Pulsar gate would help ...
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(Replaced test systems on Dell 1600SC servers) Apple Xserve hardware ... 300 Dell computers in cluster. Real time correlation ('normal' modes) - 30-50 nodes ...
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Modelled free-free absorption in 17 compact radio sources (HII and SNR). Resolved an SNR. ... Online Wide-field Imaging Calculator. http://astronomy.swin.edu.au ...
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... other AGN in June with the ATCA at high resolution (22 GHz) ... VLBI can provide high resolution images but unless careful only over small fields of view. ...
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Research ... THE SEARFE RADIO SCIENCE & ASTRONOMY AWARENESS PROJECT ... [3] Faculty of Engineering, University of Technology Sydney ...
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Richard Schilizzi, Tony Beasley, Don Campbell, ... What can VLBI ... Chief Investigator: Michael Etheridge. Project Scientist: Kurt Lambeck / Paul Tregonning ...
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Data rate improvements
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Need simple, cheap system. Want international compatibility. Do not need 100% reliability ... Cheap ~$1000. Needed at both ends ...
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Luminous ( 104 L ), embedded IR source. Bipolar molecular outflow ... MERLIN 5 GHz 0.1' 2mm speckle 0.2' Monopolar reflection nebula in a massive YSO ...
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Introduction. The Magellanic System, comprising the Small and Large Magellanic ... In contrast to other phases of the ISM, the molecular gas in the Magellanic ...
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Injection: shear, pulsation and precession. Size: 0.04 pc Time scale: 500 years ... 400yr Precession : pulsed. CO 2-1: 230 GHz. Atomic: optical. H2: 2.12, mm, ...
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Dome C the best astronomical site in the world
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