Proposal Identification No.: S2841 Date Received: 2013-Apr-26 18:15:52 Technical Page This proposal has not been submitted before. Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Director Discretionary Time Astronomy 10 Hours Bistatic radar testing We propose engineering tests of a bistatic radar system. ... Sp ecial Equipment or setup: none RFI Considerations Frequency Ranges Planned 200-2000 MHz 1 ...

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... A Date Received: 2004-Jun-01 18:43:58 Mail hard copies to: Dr. Sixto Gonzalez, Director Arecibo Observatory HC 3 Box 53995 Arecibo, PR 00612 U.S.A. ARECIBO OBSERVATORY NATIONAL ASTRONOMY AND IONOSPHERE CENTER OBSERVING TIME REQUEST COVER SHEET We are indebted to our user community for their continued support of the Arecibo Observatory, Puerto Rico. ... The total time request is 70 hours of observing time. ... Yes Queue Observing Section II - Time Request The following times are in AST. ...

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ARCSAT ID NUMBER: (leave this blank) DESCRIPTIVE TITLE: (self-explanatory) PI: (you) OBSERVER(S): (people who will be doing the observing) UNCERTIFIED/UNTRAINED OBSERVERS: (people who have not used ARCSAT before) COLLABORATORS: (people from other institutions) CONTACT INFORMATION: (PI/OBSERVER email, phone) NUMBER OF WEEKS REQUESTED: (from 1 to 3) TIME REQUESTED: (List at least 3 possibilities in priority order - or more if you are requesting more than one week of time. ...

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... The Large Telescopes Program Committee of Russian AS . ... Executive Secretary, e-mail: request@sao.ru . Telescope RATAN-600 Time Request deadline: I half-year (Jan. ... Program title .. ... Principal investigator .. ... Request status .. ... Retarded applications and ones not conforming to form will not be accepted by the Committee. ... In some exceptional cases the Program Committee Secretary can accept a request after deadline with permission of the Chairman of Committee or director of SAO RAS. ...

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RadioAstron AO-1 prop osal Submission dead line: February 8, 23:59 UT. ... Team contact name and e-mail address: Ivan Petrov (e-mail: Ivan.Peterov@gmail.com ) Total observing time request: 100 hrs Number of independent observing segments and typical range of pro jected baselines required: 20 (3-30 Earth diameters) Specific dates and time intervals requested : If your experiment requires specific dates and UT ranges, please, indicate them: February 1, 2014: 08:00-16:00 UT -- M87 imaging ...

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... The process of proposing for Hubble Space Telescope observing time has been revised, to make it simpler for proposers. We describe the simple, flexible, and robust prototype system created to handle proposal submission. ... Proposing for Hubble Space Telescope ( HST ) observing time proceeds in two phases: the scientific merits of the proposal are considered in Phase I; only accepted proposals enter Phase II, where the observations are described in complete detail. ...

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... The number of experiments in this proposal is: 6 (8) Details of proposed experiments Experiment 1 Experiment 2 Experiment 3 Experiment 4 Source name (Jhhmm\Sigmaddmm) J1939­6342 J0024­4202 J0240­2309 J1723­6500 Alternative name PKS 1934­638 PKS 0022­423 PKS 0237 ... 25.026 00 24 42.990 02 40 08.1747 17 23 41.029 Dec(J2000) (dd mm ss.ssss) ­63 42 45.63 ­42 02 03.95 ­23 09 15.736 ­65 00 36.61 Observing frequency band (GHz) 1.6 1.6 1.6 5 Continuum ...

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Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Chirp ionosonde main technical characteristics . ... Linear frequency modulated continuous signals sounding method is relatively simple and has wide application in various special-purpose systems. ... Chirp signals which are applying for ionosphere channel diagnostics usually have10KHz/s -- 1MHz/s. We must point out that under modulation speed increasing there is an increase in noise suppression and resolution power. ...

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... Partner Recommended Time: . ... Time Requested in this Proposal: . ... Abstract: The primary aim of this proposal is to determine accurate distances to two Extreme Gas-Rich Dwarfs selected by Blind 21cm Line surveys. These two galaxies are representative of a galaxy class with an apparent large HI gas mass fraction, which may be vastly under-represented in conventional catalogs. ... Thus it is crucial to find an independent distance estimator for at least a sub-sample of these galaxies. ... Time . ...

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... It was designed to observe the solar wind approaching Earth, from a position near the Lagrangian point L1, and it is part of the International Solar-Terrestrial Physics (ISTP) Initiative . ... The original plan called for "Wind" to approach its final station over two years, undergoing two close encounters with the Moon to boost its speed. ... If however the object is moving , the encounter is not symmetric, and in the end the spacecraft may have gained or lost speed, depending on its trajectory. ...

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CCD Forum Message . ... Eyepieces ћ Meade ћ Misc. ... CCD Tips and Techniques | ... Opinions Requested . ... I am planning on getting back into astronomy (used to use an 8" newtownian 20 years ago). ... After reviewing many scopes and cameras the following are my planned scopes and equipment thus far. ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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Click here for more about this recent image from Shared Skies. Moore Observatory of the University of Louisville and Mt. Kent Observatory of the University of Southern Queensland support teaching and research by their students and faculty in programs in Astronomy, Physics, and Atmospheric Sciences. ... The wide field telescope in the roll roof and the CDK20 in the Sirius dome at Moore Observatory offer live real-time use to university students, and to secondary school teachers, on request. ...

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