Square Kilometre Array (Ska) Swiss Interests and Contribution
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Line-Intensity Mapping: 2017 Status Report Arxiv:1709.09066V1
Line-Intensity Mapping: 2017 Status Report E. D. Kovetz1,*, M. P. Viero2, A. Lidz3, L. Newburgh4, M. Rahman1, E. Switzer5, M. Kamionkowski1, J. Aguirre3, M. Alvarez6, J. Bock7, J. R. Bond6, G. Bower8, C. M. Bradford9, P. C. Breysse6, P. Bull9, T. C. Chang9, Y. T. Cheng7, D. Chung2, K. Cleary7, A. Cooray10, A. Crites7, R. Croft11, O. Dor´e7,9, M. Eastwood7, A. Ferrara12, J. Fonseca13, D. Jacobs14, G. Keating15, G. Lagache16, G. Lakhlani6, A. Liu17,18, K. Moodley19, N. Murray6, A. Penin19, G. Popping20, A. Pullen21, D. Reichers22, S. Saito23, B. Saliwanchik19, M. Santos13,24, R. Somerville25,26, G. Stacey22, G. Stein6, F. Villaescusa-Navarro26, E. Visbal26, A. Weltman27, L. Wolz28, M. Zemcov29 1Department of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles St., Baltimore, MD 21218, USA 2Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305 3Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA 4Department of Physics, Yale University, New Haven, CT 06520 5NASA Goddard Space Flight Center, Greenbelt, MD, USA 6Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George st., Toronto, ON, M5S 3H8, Canada 7Division of Physics, Math and Astronomy, California Institute of Technology, 1200 E. California Blvd. Pasadena, CA 91125 8Academia Sinica Institute of Astronomy and Astrophysics, 645 N. A'ohoku Place, Hilo, HI 96720, USA 9Jet Propulsion Laboratory, California Institute of Technology, -
Journal Issue 26 | October 2019
journal Issue 26 | October 2019 Communicating Astronomy with the Public Spotlighting a Black Hole What did it take to create the largest outreach campaign for an astronomical result? Tactile Subaru A project to make telescope technology accessible Naming ExoWorlds Update on the IAU100 NameExoWorlds campaign www.capjournal.org As part of the 100th anniversary commemorations, the International Astronomical Union (IAU) is organising the IAU100 NameExoWorlds global competition to allow any country in the world to give a popular name to a selected exoplanet and its News News host star. The final results of the competion will be announced in Decmeber 2019. Credit: IAU/L. Calçada. Editorial Welcome to the 26th edition of the CAPjournal! To start off, the first part of 2019 brought in a radical new era in astronomy with the first ever image showing a shadow of a black hole. For CAPjournal #26, part of the team who collaborated on the promotion of this image hs written a piece to show what it took to produce one of the largest astronomy outreach campaigns to date. We also highlight two other large outreach campaigns in this edition. The first is a peer-reviewed article about the 2016 solar eclipse in Indonesia from the founder of the astronomy website lagiselatan, Avivah Yamani. Next, an update on NameExoWorlds, the largest IAU100 campaign, as we wait for the announcement of new names for the ExoWorlds in December. Additionally, this issue touches on opportunities for more inclusive astronomy. We bring you a peer-reviewed article about outreach for inclusion by Dr. Kumiko Usuda-Sato and the speech “Diversity Across Astronomy Can Further Our Research” delivered by award-winning astronomy communicator Dr. -
21 Cm Intensity Mapping: the Tianlai Project
21 cm intensity mapping: the Tianlai Project Yougang Wang1, Xulei Chen1, Fengquan Wu1, Shifan Zuo1, Jixia Li1, Shijie Sun1, Jiao Zhang 2, Stebbins Albert 3, Reza Ansari 4, Peter T. Timbie5, Jeffrey B. Peterson6, Juyong Zhang7, Santanu Das5 1Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China 2School of Physics and Electronic Engineering, Shanxi University, Taiyuan 030006, China 3 Fermi National Accelerator Laboratory, Batavia, IL 60510, USA 4 Universit´eParis-Sud, LAL, UMR 8607, F-91898 Orsay Cedex, France & CNRS/IN2P3, F-91405 Orsay, Franc 5Department of Physics, University of Wisconsin Madison, Madison, WI 53706, USA 6Department of Physics, Carnegie Mellon University, Pittsburgh, PA 15213, USA 7Hangzhou Dianzi University, Hangzhou, P. R. China The Tianlai project is a 21-cm intensity mapping experiment which is aimed at surveying the large-scale structure and use its baryon acoustic oscillation features to constrain dark energy models. The pathfinder of the Tianlai array has been built, which includes three cylinders and sixteen dishes. In this talk, we will give a review of the Tianlai experiment. 1 Introduction Baryon acoustic oscillations (BAO) are a feature imprinted on the cosmic microwave background and the large-scale structures in the late universe by acoustic waves traveling in the plasma prior to the recombination epoch. The comoving characteristic scale of the BAO is determined by the sound horizon at the last scattering surface. The BAO scale can be taken as a standard ruler to measure the angular diameter distance and the Hubble parameter H(z), and hence to constrain the cosmological parameters. -
Square Kilometre Array Computational Challenges
Square Kilometre Array Computational Challenges Paul Alexander Paul Alexander SKA Computational Challenges What is the Square Kilometre Array (SKA) • Next Generation radio telescope – compared to best current instruments it is ... E-MERLIN • ~100 times sensitivity • ~ 106 times faster imaging the sky • More than 5 square km of collecting area on sizes 3000km eVLA 27 27m dishes Longest baseline 30km GMRT 30 45m dishes Longest baseline 35 km Paul Alexander SKA Computational Challenges What is the Square Kilometre Array (SKA) • Next Generation radio telescope – compared to best current instruments it is ... • ~100 times sensitivity • ~ 106 times faster imaging the sky • More than 5 square km of collecting area on sizes 3000km • Will address some of the key problems of astrophysics and cosmology (and physics) • Builds on techniques developed in Cambridge • It is an interferometer • Uses innovative technologies... • Major ICT project • Need performance at low unit cost Paul Alexander SKA Computational Challenges Dishes Paul Alexander SKA Computational Challenges Phased Aperture array Paul Alexander SKA Computational Challenges also a Continental sized Radio Telescope • Need a radio-quiet site • Very low population density • Large amount of space • Possible sites (decision 2012) • Western Australia • Karoo Desert RSA Paul Alexander SKA Computational Challenges Sensitivity comparison 12,000 Sensitivity Comparison 10,000 1 - K 2 8,000 SKA2 6,000 SKA2 SKA1 MeerKAT LOFAR ASKAP 4,000 Sensitivity: Aeff/Tsys m Sensitivity:Aeff/Tsys eVLA SKA1 2,000 -
Patrick Thaddeus
PUBLISHED: 19 JUNE 2017 | VOLUME: 1 | ARTICLE NUMBER: 0170 obituary Patrick Thaddeus A pioneer in the field of astrochemistry, Patrick Thaddeus discovered dozens of exotic molecules in space and helped revolutionize our view of the interstellar medium and star formation. atrick Thaddeus did more than anyone telescope operating from a rooftop just a else to demonstrate, as he was fond few hundred yards from Broadway. After Pof saying, that chemistry was not a over two decades of steady mapping with provincial subject that stopped five miles this instrument and a near-duplicate one above our heads. As a pioneer in the field that they installed in Chile in 1982, Pat and of astrochemistry, his elegant laboratory his students obtained what is still today work provided ironclad identifications the most extensive and widely used survey of hundreds of new molecules of of the molecular Milky Way. More than astronomical interest, and his observational 40 years later, both telescopes continue to programme discovered about one-sixth yield important scientific results, including of the ~200 molecules known to exist in the discovery over the past decade of two space. His early recognition that carbon THOMAS DAME new spiral arm features of the Galaxy. monoxide would be an excellent tracer of A total of 24 PhD dissertations have the cold dense regions of space led directly been written based on observations or to the discovery of giant molecular clouds instrumental work with the two telescopes. and a revolution in our understanding of In 1986, Pat, along with several the interstellar medium and star formation. -
List Stranica 1 Od
list product_i ISSN Primary Scheduled Vol Single Issues Title Format ISSN print Imprint Vols Qty Open Access Option Comment d electronic Language Nos per volume Available in electronic format 3 Biotech E OA C 13205 2190-5738 Springer English 1 7 3 Fully Open Access only. Open Access. Available in electronic format 3D Printing in Medicine E OA C 41205 2365-6271 Springer English 1 3 1 Fully Open Access only. Open Access. 3D Display Research Center, Available in electronic format 3D Research E C 13319 2092-6731 English 1 8 4 Hybrid (Open Choice) co-published only. with Springer New Start, content expected in 3D-Printed Materials and Systems E OA C 40861 2363-8389 Springer English 1 2 1 Fully Open Access 2016. Available in electronic format only. Open Access. 4OR PE OF 10288 1619-4500 1614-2411 Springer English 1 15 4 Hybrid (Open Choice) Available in electronic format The AAPS Journal E OF S 12248 1550-7416 Springer English 1 19 6 Hybrid (Open Choice) only. Available in electronic format AAPS Open E OA S C 41120 2364-9534 Springer English 1 3 1 Fully Open Access only. Open Access. Available in electronic format AAPS PharmSciTech E OF S 12249 1530-9932 Springer English 1 18 8 Hybrid (Open Choice) only. Abdominal Radiology PE OF S 261 2366-004X 2366-0058 Springer English 1 42 12 Hybrid (Open Choice) Abhandlungen aus dem Mathematischen Seminar der PE OF S 12188 0025-5858 1865-8784 Springer English 1 87 2 Universität Hamburg Academic Psychiatry PE OF S 40596 1042-9670 1545-7230 Springer English 1 41 6 Hybrid (Open Choice) Academic Questions PE OF 12129 0895-4852 1936-4709 Springer English 1 30 4 Hybrid (Open Choice) Accreditation and Quality PE OF S 769 0949-1775 1432-0517 Springer English 1 22 6 Hybrid (Open Choice) Assurance MAIK Acoustical Physics PE 11441 1063-7710 1562-6865 English 1 63 6 Russian Library of Science. -
Detection Statistics of the Radioastron AGN Survey
Available online at www.sciencedirect.com ScienceDirect Advances in Space Research 65 (2020) 705–711 www.elsevier.com/locate/asr Detection statistics of the RadioAstron AGN survey Y.Y. Kovalev a,b,c,⇑, N.S. Kardashev a,†, K.V. Sokolovsky a,d,e, P.A. Voitsik a,T.Anf, J.M. Anderson g,h, A.S. Andrianov a, V.Yu. Avdeev a, N. Bartel i, H.E. Bignall j, M.S. Burgin a, P.G. Edwards k, S.P. Ellingsen l, S. Frey m, C. Garcı´a-Miro´ n, M.P. Gawron´ski o, F.D. Ghigo p, T. Ghosh p,q, G. Giovannini r,s, I.A. Girin a, M. Giroletti r, L.I. Gurvits t,u, D.L. Jauncey k,v, S. Horiuchi w, D.V. Ivanov x, M.A. Kharinov x, J.Y. Koay y, V.I. Kostenko a, A.V. Kovalenko aa, Yu.A. Kovalev a, E.V. Kravchenko r,a, M. Kunert-Bajraszewska o, A.M. Kutkin a,z, S.F. Likhachev a, M.M. Lisakov c,a, I.D. Litovchenko a, J.N. McCallum l, A. Melis ab, A.E. Melnikov x, C. Migoni ab, D.G. Nair t, I.N. Pashchenko a, C.J. Phillips k, A. Polatidis z, A.B. Pushkarev a,ad, J.F.H. Quick ae, I.A. Rakhimov x, C. Reynolds j, J.R. Rizzo af, A.G. Rudnitskiy a, T. Savolainen ag,ah,c, N.N. Shakhvorostova a, M.V. Shatskaya a, Z.-Q. Shen f,ac, M.A. Shchurov a, R.C. Vermeulen z, P. de Vicente ai, P. -
Dynamics of the Arecibo Radio Telescope
DYNAMICS OF THE ARECIBO RADIO TELESCOPE Ramy Rashad 110030106 Department of Mechanical Engineering McGill University Montreal, Quebec, Canada February 2005 Under the supervision of Professor Meyer Nahon Abstract The following thesis presents a computer and mathematical model of the dynamics of the tethered subsystem of the Arecibo Radio Telescope. The computer and mathematical model for this part of the Arecibo Radio Telescope involves the study of the dynamic equations governing the motion of the system. It is developed in its various components; the cables, towers, and platform are each modeled in succession. The cable, wind, and numerical integration models stem from an earlier version of a dynamics model created for a different radio telescope; the Large Adaptive Reflector (LAR) system. The study begins by converting the cable model of the LAR system to the configuration required for the Arecibo Radio Telescope. The cable model uses a lumped mass approach in which the cables are discretized into a number of cable elements. The tower motion is modeled by evaluating the combined effective stiffness of the towers and their supporting backstay cables. A drag model of the triangular truss platform is then introduced and the rotational equations of motion of the platform as a rigid body are considered. The translational and rotational governing equations of motion, once developed, present a set of coupled non-linear differential equations of motion which are integrated numerically using a fourth-order Runge-Kutta integration scheme. In this manner, the motion of the system is observed over time. A set of performance metrics of the Arecibo Radio Telescope is defined and these metrics are evaluated under a variety of wind speeds, directions, and turbulent conditions. -
Fact Sheet Fact Sheet
FactFact sheet sheet What is the SKA? The Square Kilometre Array (SKA) is a next-generation radio telescope that will be vastly more sensitive than the best present-day instruments. It will give astronomers remarkable insights into the formation of the early Universe, including the emergence of the first stars, galaxies and other structures. This will shed light on the birth, and eventual death, of the cosmos. The SKA will require new technology and progress in Why build the SKA? fundamental engineering in fields such as information and communication technology, high performance computing In order to answer some fundamental questions about the and production manufacturing techniques. It will comprise origin and evolution of the Universe, a more sensitive radio a vast array of antennas, arranged in clusters to be spread telescope is needed that can detect the very weak signals over 3000 kilometres or more. The antennas will be linked coming from the edge of the cosmos. A telescope such as the electronically to form one enormous telescope. The SKA will be able to “see” distant objects in the very young combination of unprecedented collecting area, versatility Universe and provide answers to questions such as the and sensitivity will make the SKA the world’s premier imaging emergence of the first stars, galaxies and other structures. and survey telescope over a wide range of radio frequencies, Because the speed of light is finite and the size of the Universe producing the sharpest pictures of the sky of any telescope. is so large, telescopes are effectively time machines, enabling astronomers to look into the past and study the Universe as it The SKA will: was billions of years ago. -
SETI@Home Completes a Decade of ET Search 1 May 2009
SETI@home completes a decade of ET search 1 May 2009 Over the years, improvements to the Arecibo telescope have significantly improved the quality of data available to SETI@home, and the continuous increase in the speed of the average PC has made it possible to use more sensitive and sophisticated analysis techniques. Today, SETI@home continues its search for evidence of extraterrestrial life, with greater sensitivity than ever, and its hundreds of thousands of volunteers continue to engage in lively on-line forums and in a spirited competition The SETI@home project, which has involved the for most data processed. worldwide public in a search for radio-wave evidence of life outside Earth, marks its 10th More information: anniversary on May 17, 2009. setiathome.berkeley.edu/index.php The project, based at the Space Sciences Provided by SETI@home Laboratory at the University of California, Berkeley, records and analyzes data from the world's largest radio telescope, the Arecibo Observatory in Puerto Rico. The collected computing power of hundreds of thousands of volunteer PCs is used to search this data for narrow-band signals (similar to TV or cell-phone transmissions) and other types of signals of possible extraterrestrial origin. SETI@home was conceived in 1995. Development began in 1998, with initial funding from The Planetary Society and Paramount Pictures. It was publicly launched on May 17, 1999, and the number of volunteers quickly grew to about one million. Because of the presence of noise and man-made radio interference, SETI@home doesn't get excited by individual signals. -
Why SETI Will Fail ‡
Why SETI Will Fail z B. Zuckerman1 1Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA E-mail: [email protected] Abstract. The union of space telescopes and interstellar spaceships guarantees that if extraterrestrial civilizations were common, someone would have come here long ago. PACS numbers: 97.10.Tk arXiv:1912.08386v1 [physics.pop-ph] 18 Dec 2019 z This article originally appeared in the September/October 2002 issue of Mercury magazine (published by the Astronomical Society of the Pacific). Why SETI Will Fail 2 1. Introduction Where do humans stand on the scale of cosmic intelligence? For most people, this question ranks at or very near the top of the list of "scientific things I would like to know." Lacking hard evidence to constrain the imagination, optimists conclude that technological civilizations far in advance of our own are common in our Milky Way Galaxy, whereas pessimists argue that we Earthlings probably have the most advanced technology around. Consequently, this topic has been debated endlessly and in numerous venues. Unfortunately, significant new information or ideas that can point us in the right direction come along infrequently. But recently I have realized that important connections exist between space astronomy and space travel that have never been discussed in the scientific or popular literature. These connections clearly favor the more pessimistic scenario mentioned above. Serious radio searches for extraterrestrial intelligence (SETI) have been conducted during the past few decades. Brilliant scientists have been associated with SETI, starting with pioneers like Frank Drake and the late Carl Sagan and then continuing with Paul Horowitz, Jill Tarter, and the late Barney Oliver. -
Intensity Mapping with Neutral Hydrogen and the Hidden Valley Simulations
Prepared for submission to JCAP Intensity mapping with neutral hydrogen and the Hidden Valley simulations Chirag Modi,a;b Emanuele Castorina,a;b Yu Feng,a;b Martin Whitea;b;c aDepartment of Physics, University of California, Berkeley, CA 94720 bBerkeley Center for Cosmological Physics, Berkeley, CA 94720 cDepartment of Astronomy, University of California, Berkeley, CA 94720 E-mail: [email protected], [email protected], [email protected], [email protected] Abstract. This paper introduces the HiddenValley simulations, a set of trillion-particle N-body simulations in gigaparsec volumes aimed at intensity mapping science. We present details of the simulations and their convergence, then specialize to the study of 21-cm fluctuations between redshifts 2 and 6. Neutral hydrogen is assigned to halos using three prescriptions, and we investigate the clustering in real and redshift-space at the 2-point level. In common with earlier work we find the bias of HI increases from near 2 at z = 2 to 4 at z = 6, becoming more scale dependent at high z. The level of scale-dependence and decorrelation with the matter field are as predicted by perturbation theory. Due to the low mass of the hosting halos, the impact of fingers of god is small on the range relevant for proposed 21-cm instruments. We show that baryon acoustic oscillations and redshift-space distortions could be well measured by such instruments. Taking advantage of the large simulation volume, we assess the impact of fluctuations in the ultraviolet background, which change HI clustering