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Situation Report: Insert Response Name
Cuyahoga County EOC Situation Report #18 - Coronavirus Date of Issue: 3/12/2020 Time Period: 1100-1900 Prepared by: Serena Steele, Situation Unit Leader Approved by: Mark Christie Incident Overview: On March 9, three patients in Cuyahoga County tested positive for COVID-19. All patients contracted the virus outside of the state of Ohio: two in Egypt and one in Washington, DC. Ohio Governor DeWine declared a state of emergency. On 3/11 a fourth case was confirmed in Stark County, OH. The Cuyahoga County EOC will be partially activated and staffed 0700-1900 on Tuesday 3/10 through at least Friday 3/13. Cuyahoga County Executive Armond Budish signed a Declaration of Emergency for Cuyahoga County. Mayor Frank Jackson released a proclamation of Civil Emergency for the City of Cleveland. Additional information can be found here: CDC- https://www.cdc.gov/coronavirus/2019-ncov/index.html Ohio Department of Health- https://coronavirus.ohio.gov/ Cuyahoga County Board of Health- https://www.ccbh.net/coronavirus/ County EOC Status: Partial Activation- staffed by: • ESF 1 Transportation- Greater Cleveland Regional Transit Authority • ESF 3 Public Works- Northeast Ohio Regional Sewer District/Cuyahoga County Public Works • ESF 4 Firefighting- Cuyahoga County Fire Chiefs Association • ESF 5 Info & Planning- Cuyahoga County Emergency Management, Cuyahoga County Public Safety/Justice Services • ESF 6 Mass Care- United Way/2-1-1, ARC • ESF 8 Public Health & Medical- Center for Health Affairs, Cuyahoga County Board of Health, Cleveland Department of Public Health • ESF 15 External Affairs- Cuyahoga County Communications Department, Cleveland Dept of Public Health Communications 1. Operations: Cuyahoga County EOC partially activated on 3/9/2020 after the first three cases were confirmed. -
Gaianir Combining Optical and Near-Infra-Red (NIR) Capabilities with Time-Delay-Integration (TDI) Sensors for a Future Gaia-Like Mission
Proposal title: GaiaNIR Combining optical and Near-Infra-Red (NIR) capabilities with Time-Delay-Integration (TDI) sensors for a future Gaia-like mission. PI: Dr. David Hobbs, Lund Observatory, Box 43, SE-221 00 Lund, Sweden. Email: [email protected]. Tel.: +46-46-22 21573 Core team members: The following minimum team is needed to initiate the project. D. Hobbs Lund Observatory, Sweden. A. Brown Leiden Observatory, Holland. A. Mora Aurora Technology B.V., Spain. C. Crowley HE Space Operations B.V., Spain. N. Hambly University of Edinburgh, UK. J. Portell Institut de Ciències del Cosmos, ICCUB-IEEC, Spain. C. Fabricius Institut de Ciències del Cosmos, ICCUB-IEEC, Spain. M. Davidson University of Edinburgh, UK. Proposal writers: See Appendix A. Other supporting scientists: See Appendix B and Appendix C. Senior science advisors: E. Høg Copenhagen University (Retired), Denmark. L. Lindegren Lund Observatory, Sweden. C. Jordi Institut de Ciències del Cosmos, ICCUB-IEEC, Spain. S. Klioner Lohrmann Observatory, Germany. F. Mignard Observatoire de la Côte d’Azur, France. arXiv:1609.07325v2 [astro-ph.IM] 22 May 2020 Fig. 1: Left is an IR image from the Two Micron All-Sky Survey (image G. Kopan, R. Hurt) while on the right an artist’s concept of the Gaia mission superimposed on an optical image, (Image ESA). Images not to scale. 1 1. Executive summary ESA recently called for new “Science Ideas” to be investigated in terms of feasibility and technological developments – for tech- nologies not yet sufficiently mature. These ideas may in the future become candidates for M or L class missions within the ESA Science Program. -
E X P L O R E OWNED by PLAYHOUSE SQUARE I D E a C E N T E R Participating in Economic Development in Greater Cleveland
E X P L O R E OWNED BY PLAYHOUSE SQUARE I D E A C E N T E R Participating in economic development in Greater Cleveland 1375 Euclid Avenue, Cleveland, Ohio 44115 NUMBER OF FLOORS 6 FULL FLOOR SQUARE 36,700 RSF The Idea Center at FOOTAGE Playhouse Square is OFFICE RENTAL $18.00 per rentable SF, modified the result of a RATES gross partnership TENANT Negotiable between WVIZ/PBS IMPROVEMENTS and 90.3 WCPN OPERATING Tenants pay their pro rata share of ideastream and EXPENSE increases (if any) in operating ADJUSTMENTS expenses and real estate taxes over a PlayhouseSquare. base year UTILITIES Electric Individually controlled and Encompassing over separately metered for lights, wall plugs and air 243,035 SF, the conditioning building offers Water AC water separate annual innovative office charge for cooling tower space. PARKING Adjacent parking garage and many reasonably-priced surface lots surrounding the building BUILDING ACCESS / 24-hours, seven days per week SECURITY BUILDING Teleconferencing and distance The information contained herein was AMENITIES learning technology available. obtained from sources believed reliable; however, Playhouse Square Real Estate Services makes no guarantees, warranties 300-seat Westfield Insurance Studio For leasing information, contact or representations as to the completeness Theatre available for seminars and or accuracy thereof. The presentation of Joseph P. Fegen ▪ 216-640-8722 this property is submitted subject to errors, conferences. [email protected] omissions, change of price or conditions -
EUCLID Mission Assessment Study
EUCLID Mission Assessment Study Executive Summary ESA Contract. No. 5856/08/F/VS September 2009 EUCLID– Mapping the Dark Universe EUCLID is a mission to study geometry and nature of the dark universe. It is a medium-class mission candidate within ESA's Cosmic Vision 2015– 2025 Plan for launch around 2017. EUCLID has been derived by ESA from DUNE and SPACE, two complementary Cosmic Vision proposals addressing questions on the origin and the constitution of the Universe. 70% Dark Energy The observational methods applied by EUCLID are shape and redshift measure- ments of galaxies and clusters of galaxies. To 4% Baryonic Matter this end EUCLID is equipped with 3 scientific instruments: 26% Dark Matter • Visible Imager (VIS) • Near-Infrared Photometer (NIP) • Near-Infrared Spectrograph (NIS) The EUCLID Mission Assessment Study is the industrial part of the EUCLID assessment phase. The study has been performed by Astrium from September 2008 to September 2009 and is intended for space segment definition and programmatic evaluation. The prime responsibility is with Astrium GmbH (Friedrichshafen, Germany) with support from Astrium SAS (Toulouse, France) and Astrium Ltd (Stevenage, UK). EUCLID Mission EUCLID shall observe 20.000 deg2 of the extragalactic sky at galactic latitudes |b|>30 deg. The sky is sampled in step & b>30° stare mode with instantaneous fields of about 0.5 deg2 . Nominally a strip of about 20 deg in latitude is scanned per day (corresponding to about 1 deg in longitude). galactic plane step 1 b<30° step 2 step 3 The sky is nominally observed along great circles in planes perpendicular to the Sun- spacecraft axis (SAA=0). -
Tri-C Jazzfest Cleveland Adds New Features for 2017
Here is the indoor lineup, with show times and locations: Chris Botti Dianne Reeves Jane Bunnett and Maqueque Boz Scaggs Catherine Russell Thursday, June 22 Saturday, June 24 BOZ SCAGGS WITH CATHERINE CHRIS BOTTI WITH DIANNE JANE BUNNETT RUSSELL OPENING — 8:05 P.M. REEVES OPENING — 7:30 P.M. AND MAQUEQUE/ Connor Palace Connor Palace ALICIA OLATUJA — Boz Scaggs performed with the Steve Trumpeter Chris Botti is a Grammy winner, 1 P.M. Miller Band in the ’60s before embarking with four albums having reached No. 1 Allen Theatre on a solo career that produced classic on Billboard’s jazz charts. With a buttery- Saxophonist Jane albums such as Silk Degrees (1976) rich and fluid voice, the legendary Dianne Alicia Olatuja Bunnett, a Juno and Middle Man (1980). Catherine Reeves has won five Grammys for Best Award winner, Russell’s musical resume includes six Vocal Jazz Performance. routinely launches creative and exciting chart-topping albums and a Grammy as a projects with Cuban artists such as featured artist on the Boardwalk Empire Friday, June 23 the five young women in Maqueque. soundtrack. TERENCE Newcomer Alicia Olatuja earned praise BLANCHARD’S from the New York Times as “a singer TERENCE BLUE NOTE with a strong and luscious tone and an BLANCHARD’S SESSIONS — amiably regal presence on stage.” E-COLLECTIVE — 6 P.M. 10:15 P.M. Ohio Theatre Allen Theatre Terence Blanchard Trumpeter Terence Terence Blanchard’s Blanchard and a few E-Collective offers a Terence Blanchard musical friends — Kenny Barron, Ravi socially conscious Tri-C JazzFest Cleveland takes it to both the streets Coltrane, Carl Allen and David Pulphus journey into an and the theaters at Playhouse Square June 22–24. -
Joint UV Survey Telescope
S. Basa, Laboratoire d’Astrophysique de Marseille, France distant sample of SMBHs, which in turn, hold the greatest promise of extending the existing M-σ relation beyond current limitations by revealing dormant SMBHs in galactic nuclei [15,16]. Finally is the class of unknown transients for which we currently lack both predictions and detections. This class represents a significant area of discovery space that only a wide-field The transientand sensitivesky X-ray transient “machine” can uniquely explore. In the sections below, we outline the importance of extending our knowledge of known, predicted, and unknown X-ray transients, on par with the on-going ground-based technological efforts to advance our understanding of the dynamic sky at optical (LSST) and radio (SKA pathfinders) wavelengths. Sky is intrinsically variable!! • Hard X-ray monitoring instruments show a restless X-ray sky (Swift-BAT, INTEGRAL, MAXI).! ! distant sample of SMBHs, which in turn, hold the greatest promise of extending the existing ! M-σ relation beyond current limitations by revealing dormant SMBHs in galactic nuclei [15,16]. Finally is the class of unknown transients for which we currently lack both predictions and Time domain astronomy still in its infancy, but detections. This class represents a significant area of discovery space that only a wide-field and sensitive X-ray transient “machine” can uniquely explore. In the sections below, we outline theSoderberg et al. 2009 importance of extending our knowledge of known, predicted, and unknown X-ray should quickly evolve especially at optical (PTF, transients, on par with the on-going ground-based technological efforts to advance our understanding of the dynamic sky at optical (LSST) and radio (SKA pathfinders)EXPLORING wavelengths. -
NASA Program & Budget Update
NASA Update AAAC Meeting | June 15, 2020 Paul Hertz Director, Astrophysics Division Science Mission Directorate @PHertzNASA Outline • Celebrate Accomplishments § Science Highlights § Mission Milestones • Committed to Improving § Inspiring Future Leaders, Fellowships § R&A Initiative: Dual Anonymous Peer Review • Research Program Update § Research & Analysis § ROSES-2020 Updates, including COVID-19 impacts • Missions Program Update § COVID-19 impact § Operating Missions § Webb, Roman, Explorers • Planning for the Future § FY21 Budget Request § Project Artemis § Creating the Future 2 NASA Astrophysics Celebrate Accomplishments 3 SCIENCE Exoplanet Apparently Disappears HIGHLIGHT in the Latest Hubble Observations Released: April 20, 2020 • What do astronomers do when a planet they are studying suddenly seems to disappear from sight? o A team of researchers believe a full-grown planet never existed in the first place. o The missing-in-action planet was last seen orbiting the star Fomalhaut, just 25 light-years away. • Instead, researchers concluded that the Hubble Space Telescope was looking at an expanding cloud of very fine dust particles from two icy bodies that smashed into each other. • Hubble came along too late to witness the suspected collision, but may have captured its aftermath. o This happened in 2008, when astronomers announced that Hubble took its first image of a planet orbiting another star. Caption o The diminutive-looking object appeared as a dot next to a vast ring of icy debris encircling Fomalhaut. • Unlike other directly imaged exoplanets, however, nagging Credit: NASA, ESA, and A. Gáspár and G. Rieke (University of Arizona) puzzles arose with Fomalhaut b early on. Caption: This diagram simulates what astronomers, studying Hubble Space o The object was unusually bright in visible light, but did not Telescope observations, taken over several years, consider evidence for the have any detectable infrared heat signature. -
Cosmic Vision and Other Missions for Space Science in Europe 2015-2035
Cosmic Vision and other missions for Space Science in Europe 2015-2035 Athena Coustenis LESIA, Observatoire de Paris-Meudon Chair of the Solar System and Exploration Working Group of ESA Member of the Space Sciences Advisory Committee of ESA Cosmic Vision 2015 - 2025 The call The call for proposals for Cosmic Vision missions was issued in March 2007. This call was intended to find candidates for two medium-sized missions (M1, M2 class, launch around 2017) and one large mission (L1 class, launch around 2020). Fifty mission concept proposals were received in response to the first call. From these, five M-class and three L- class missions were selected by the SPC in October 2007 for assessment or feasibility studies. In July 2010, another call was issued, for a medium-size (M3) mission opportunity for a launch in 2022. Also about 50 proposals were received for M3 and 4 concepts were selected for further study. Folie Cosmic Vision 2015 - 2025 The COSMIC VISION “Grand Themes” 1. What are the conditions for planetary formation and the emergence of life ? 2. How does the Solar System work? 3. What are the physical fundamental laws of the Universe? 4. How did the Universe originate and what is it made of? 4 COSMIC VISION (2015-2025) Step 1 Proposal selection for assessment phase in October 2007 . 3 M missions concepts: Euclid, PLATO, Solar Orbiter . 3 L mission concepts: X-ray astronomy, Jupiter system science, gravitational wave observatory . 1 MoO being considered: European participation to SPICA Selection of Solar Orbiter as M1 and Euclid JUICE as M2 in 2011. -
ARIEL Payload Design Description
Doc Ref: ARIEL-RAL-PL-DD-001 ARIEL Payload ARIEL Payload Design Issue: 2.0 Consortium Description Date: 15 February 2017 ARIEL Consortium Phase A Payload Study ARIEL Payload Design Description ARIEL-RAL-PL-DD-001 Issue 2.0 Prepared by: Date: Paul Eccleston (RAL Space) Consortium Project Manager Reviewed by: Date: Kevin Middleton (RAL Space) Payload Systems Engineer Approved & Date: Released by: Giovanna Tinetti (UCL) Consortium PI Page i Doc Ref: ARIEL-RAL-PL-DD-001 ARIEL Payload ARIEL Payload Design Issue: 2.0 Consortium Description Date: 15 February 2017 DOCUMENT CHANGE DETAILS Issue Date Page Description Of Change Comment 0.1 09/05/16 All New document draft created. Document structure and headings defined to request input from consortium. 0.2 24/05/16 All Added input information from consortium as received. 0.3 27/05/16 All Added further input received up to this date from consortium, addition of general architecture and background section in part 4. 0.4 30/05/16 All Further iteration of inputs from consortium and addition of section 3 on science case and driving requirements. 0.5 31/05/16 All Completed all additional sections except 1 (Exec Summary) and 8 (Active Cooler), further updates and iterations from consortium including updated science section. Added new mass budget and data rate tables. 0.6 01/06/16 All Updates from consortium review of final document and addition of section 8 on active cooler (except input on turbo-brayton alternative). Updated mass and power budget table entries for cooler based on latest modelling. 0.7 02/06/16 All Updated figure and table numbering following check. -
Special Spitzer Telescope Edition No
INFRARED SCIENCE INTEREST GROUP Special Spitzer Telescope Edition No. 4 | August 2020 Contents From the IR SIG Leadership Council In the time since our last newsletter in January, the world has changed. 1 From the SIG Leadership Travel restrictions and quarantine have necessitated online-conferences, web-based meetings, and working from home. Upturned semesters, constantly shifting deadlines and schedules, and the evolving challenge of Science Highlights keeping our families and communities safe have all taken their toll. We hope this newsletter offers a moment of respite and a reminder that our community 2 Mysteries of Exoplanet continues its work even in the face of great uncertainty and upheaval. Atmospheres In January we said goodbye to the Spitzer Space Telescope, which 4 Relevance of Spitzer in the completed its mission after sixteen years in space. In celebration of Spitzer, Era of Roman, Euclid, and in recognition of the work of so many members of our community, this Rubin & SPHEREx newsletter edition specifically highlights cutting edge science based on and inspired by Spitzer. In the words of Dr. Paul Hertz, Director of Astrophysics 6 Spitzer: The Star-Formation at NASA: Legacy Lives On "Spitzer taught us how important infrared light is to our 8 AKARI Spitzer Survey understanding of our universe, both in our own cosmic 10 Science Impact of SOFIA- neighborhood and as far away as the most distant galaxies. HIRMES Termination The advances we make across many areas in astrophysics in the future will be because of Spitzer's extraordinary legacy." Technical Highlights Though Spitzer is gone, our community remains optimistic and looks forward to the advances that the next generation of IR telescopes will bring. -
The Cosmic Vision Process
The Cosmic Vision Process Jean Clavel Head of Astronomy & Fundamental Physics Missions Division Science & Robotic Exploration Directorate of ESA Cosmic Vision Process - EUCLID Conference - 17-18 Nov 2009 - ESTEC 05/02/2010 1 Cosmic Vision process • First “Call for Missions” issued in 1st Q 2007 • 50 proposals received by June 2007 deadline – LISA de facto L mission candidate • Selection process by scientific community during summer • Final selection in October 2007 Cosmic Vision Process - EUCLID Conference - 17-18 Nov 2009 - ESTEC 05/02/2010 2 Selected concepts for first slice of Cosmic Vision program (1/2) • L mission concepts – IXO (large collecting area X-ray observatory) – Laplace (mission to the Jupiter system) – LISA (ex officio, gravitational wave observatory) • All of them require significant technology development • All of them are proposed to ESA as international collaborations Cosmic Vision Process - EUCLID Conference - 17-18 Nov 2009 - ESTEC 05/02/2010 3 Selected concepts for first slice of Cosmic Vision program (2/2) • M mission concepts – Plato (exoplanets finding by planetary transits and asteroseismology) – Euclid (Dark energy) – Marco Polo (NEO sample return) – Cross Scale (Magnetospheric physics) – Solar Orbiter (remnant of Horizon 2000+ added in 2008) • Mission of opportunity – Spica (contribution to JAXA MIR-NIR observatory) • No strong technology development required Cosmic Vision Process - EUCLID Conference - 17-18 Nov 2009 - ESTEC 05/02/2010 4 Cosmic vision process for 1st slice: Initial planning • 2 launch opportunities, -
Lessons Learned from Past & Current ESA-NASA Collaborations
Lessons Learned ! from Past & Current ESA-NASA Collaborations" NRC Committee on NASA Participation in Euclid" January 2011" " George Helou" IPAC, Caltech" NRC Committee on Euclid Participation, January 2011 Helou-1 OUTLINE" Question: What are the successes and failures of previous missions where NASA astrophysics has contributed to an ESA mission (ISO, Herschel, Planck)?" u Study Cases:" v Infrared Space Observatory (ISO) v Spitzer Space Telescope v Herschel Space Telescope v Planck Surveyor " Question: What are your recommendations for the framework for US role in Euclid?" u Suggestions for Euclid Participation" NRC Committee on Euclid Participation, January 2011 Helou-2 IRAS: First mid-to-far-IR All-Sky Survey u IRAS was the first IR all-sky survey, at 12, 25, 60 and 100µm: Si and Ge photo-conductors u Collaboration between US, Netherlands, UK, 1983 Main data products: u Point Source Catalog ~1 Jy sensitivity u Faint Source Catalog, a few times deeper u All-Sky Image Atlas at 4΄ resolution u On-demand co-added survey data v Compact sources v Resolution enhancement NRC Committee on Euclid Participation, January 2011 Helou-3 ISO: First Pointed IR Observatory in Space u Four versatile instruments, 2 imagers, 2 spectrometers, covering 3-240µm: Si, Ge photoconductors (1995-98) u ESA mission with minor NASA, ISAS participation NRC Committee on Euclid Participation, January 2011 Helou-4 Spitzer: the NASA IR Great Observatory u Three instruments, imaging at {3.6, 4.5, 6.8, 8}, {24, 70 and 160} µm, 1 spectrometer 5-38µm, SED mode 60-120µm: Si,