Agenda Attachment Document August 2021

Total Page:16

File Type:pdf, Size:1020Kb

Agenda Attachment Document August 2021 Shire of Bruce Rock – Agenda Attachments 19 August 2021 Agenda Attachments Thursday 19 August 2021 Shire of Bruce Rock – Agenda Attachments 19 August 2021 HIRE O SHIRE OF BRUCE ROCK AGENDA ATTACHMENTS 19 AUGUST 2021 PAGE ITEM 9 MINUTES FROM PREVIOUS MEETINGS ATTACHMENT A – UNCONFIRMED COUNCIL MEETING MINUTES JULY 2021 3 ATTACHMENT B – WORKS AND SERVICES COMMITTEE MEETING 21 JULY 2021 45 ATTACHMENT C – UNCONFIRMED SPECIAL COUNCIL MEETING 29 JULY 2021 48 ATTACHMENT D – BUSH FIRE ADVISORY COMMITTEE MEETING 6 AUGUST 2021 53 ITEM 10.2 WEROC INC MEETING MINUTES AUGUST 2021 ATTACHMENT A – WEROC INC. BOARD MEETING MINUTES AUGUST 2021 56 ATTACHMENT B – LETTER FROM MINISTER SAFFIOTI 78 ATTACHMENT C – WEROC STRATEGIC WASTE MANAGEMENT PLAN AND LANDFILL RATIONALISM 79 STUDY ATTACHMENT D – WHEATBELT MEDICAL STUDENT IMMERSION PROGRAM 2022 PROGRAM 89 PROPOSAL ATTACHMENT E – WEROC INC. TOURISM AUDIT (FINAL DRAFT) 92 ITEM 11.1.1 DEVELOPMENT APPLICATIONS FOR THE INSTALLATION OF A COMMUNICATIONS REPEATER POINTS ON LOT 27457 CHAPMAN ROAD ARDATH, AND LOT 12460 HEALY ROAD, BABAKIN ATTACHMENT A – APPLICATION FOR DEVELOPMENT APPROVAL FOR A COMMUNICATIONS 211 REPEATER POINT TOWER & ASSOCIATED INFRASTRUCTURE LOT 27457, ARDATH ATTACHMENT B - APPLICATION FOR DEVELOPMENT APPROVAL FOR A COMMUNICATIONS 221 REPEATER POINT TOWER & ASSOCIATED INFRASTRUCTURE LOT 12460, BABAKIN ITEM 11.3.2 LIST OF PAYMENTS ATTACHMENT A – LIST OF PAYMENTS JULY 2021 231 ITEM 11.4.1 AMENDMENT TO COMMUNITY BUS HIRE POLICY ATTACHMENT A – POLICY 6.3 – COMMUNITY BUS HIRE 235 Shire of Bruce Rock – MINUTES 15 JULY 2021 ______________________________________________________________________________________________________ SHIRE OF BRUCE ROCK MINUTES – ORDINARY MEETING 15 JULY 2021 TABLE OF CONTENTS TABLE OF CONTENTS .................................................................................................................. 1 1. Declaration of Opening ....................................................................................................... 2 2. Record of Attendance/Apologies/Leave of Absence (Previously Approved) ......................... 2 3. Declarations of Interest ...................................................................................................... 2 4. Response to Previous Public Questions Taken on Notice ..................................................... 2 5. Public Question Time .......................................................................................................... 2 6. Petitions/Deputations/Presentations/Submissions ............................................................. 2 7. Applications for Leave of Absence ....................................................................................... 3 8. Announcements by Presiding Member ................................................................................ 3 9. Confirmation of Minutes ..................................................................................................... 3 10. Regional Reports ................................................................................................................ 4 10.1 WEROC Inc Meeting Minutes June 2021 ........................................................................ 4 10.2 WALGA Zone Minutes June 2021 ................................................................................... 7 11. Officers’ Reports ................................................................................................................. 9 11.1 Environmental Health Officer .............................................................................................. 9 11.1.1 Western Australian Planning Commission Subdivision Application No. 160975 for Lots 50, and 51 Venemore Street, Shackleton. .............................................................. 9 11.1.2 Western Australian Planning Commission Subdivision Application No. 160951 for Lots 15, and 19 Johnson Street, Bruce Rock. ................................................................ 12 11.2 Manager of Works and Services ........................................................................................ 15 11.2.1 Acquisition of Water Corp Low-Level Tank .................................................................. 15 11.3 Manager of Finance .......................................................................................................... 17 11.3.1 Statement of Financial Activity ..................................................................................... 17 11.3.2 List of Payments ............................................................................................................ 19 11.3.3 Community Budget Request – Bruce Rock Shackleton Ardath Cricket Club ................ 21 11.3.4 Extending Closure of Municipal Account held with Bendigo Bank Account ................ 23 11.4 Deputy Chief Executive Officer .......................................................................................... 25 11.4.1 Shire President Stamp .................................................................................................. 25 11.4.2 Shire Common Seal ....................................................................................................... 26 11.4.3 Recommendations for Appointment of Chief and Deputy Chief Bushfire Officers ..... 27 11.4.4 Extension of date/duration of Disability & Inclusion Plan ............................................ 29 11.4.5 Proposed Rectification of Boundaries of Reserve 14171 into Pikaring West Nature Reserve 23141, and dedication of constructed Road. ................................................. 31 11.4.6 Lease of the Equestrian Reserve................................................................................... 35 11.4.7 Amended Employee Code of Conduct .......................................................................... 37 11.5 Chief Executive Officer ...................................................................................................... 39 11.5.1 CEO Sick Leave and Appointment of Acting CEO .......................................................... 39 11.5.2 Approval for Special Meeting of Council ...................................................................... 40 12. New Business of an urgent nature introduced by discussion of the meeting ...................... 42 13. Confidential Items ............................................................................................................ 42 14. Closure of Meeting. .......................................................................................................... 42 1 Shire of Bruce Rock – MINUTES 15 JULY 2021 ______________________________________________________________________________________________________ SHIRE OF BRUCE ROCK MINUTES – ORDINARY MEETING 15 JULY 2021 1. Declaration of Opening The Shire President Cr SA Strange declared the meeting open at 3.30pm 2. Record of Attendance/Apologies/Leave of Absence (Previously Approved) President Cr SA Strange Deputy President Cr R Rajagopalan Councillors Cr AR Crooks Cr KP Foss Cr NC Kilminster Cr PG Negri Cr BJ Waight Cr RA Waye Chief Executive Officer Mr DRS Mollenoyux Deputy Chief Executive Officer Mr A O’Toole Executive Assistant Mrs MJ Schilling Environmental Health Officer Mr J Goldacre (3.45pm – 3.50pm) Manager of Works and Services Mr D Holland (3.50pm – 4.00pm) Manager of Finance Mrs JL Bow (4.00pm – 4.16pm) Leave of Absence Cr ISA Dolton 3. Declarations of Interest In accordance with Section 5.65 of the Local Government Act 1995 the following disclosures of financial interest were made at the Council meeting. Date Name Item No Reason In accordance with Section 5.65 of the Local Government Act 1995 the following disclosures of Closely Association Person and Impartiality interest were made at the Council meeting. Date Name Item No Reason 15.07.21 Darren Mollenoyux 11.5.1 Applying for Leave 15.07.21 Alan O’Toole 11.5.1 Recommended to be Acting CEO In accordance with Section 5.60B and 5.65 of the Local Government Act 1995 the following disclosures of Proximity interest were made at the Council meeting. Date Name Item No Reason 15.07.21 Cr KP Foss 11.4.5 Landowner neighbouring Pikaring Reserve 4. Response to Previous Public Questions Taken on Notice 5. Public Question Time 6. Petitions/Deputations/Presentations/Submissions 2 Shire of Bruce Rock – MINUTES 15 JULY 2021 ______________________________________________________________________________________________________ 7. Applications for Leave of Absence 8. Announcements by Presiding Member 9. Confirmation of Minutes COUNCIL DECISION Resolution OCM Jul 21 – 9.1 Moved: Cr Rajagopalan Seconded: Cr Foss That the minutes of the Annual Electors Meeting held Thursday 17 June 2021 be received. Carried 8/0 COUNCIL DECISION Resolution OCM Jul 21 – 9.2 Moved: Cr Waye Seconded: Cr Waight That the minutes of the Ordinary Meeting held Thursday 17 June 2021 be confirmed as a true and correct record. Carried 8/0 3 Shire of Bruce Rock – MINUTES 15 JULY 2021 ______________________________________________________________________________________________________ 10. Regional Reports Agenda Reference and Subject: 10.1 WEROC Inc Meeting Minutes June 2021 File Reference: 1.6.9.1 WEROC Inc. Agendas and Minutes Reporting Officer: Darren Mollenoyux, Chief Executive Officer Author: Darren Mollenoyux, Chief Executive Officer Disclosure of Interest Nil Attachments Item 10.1 Attachment A – WEROC Inc Board Meeting Minutes Summary Council is asked to receive the minutes from the previous
Recommended publications
  • The Photosphere and Circumstellar Environment of the Be Star Achernar
    New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry Proceedings IAU Symposium No. 307, 2014 c International Astronomical Union 2015 G.Meynet,C.Georgy,J.H.Groh&Ph.Stee,eds. doi:10.1017/S1743921314006905 The photosphere and circumstellar environment of the Be star Achernar Daniel M. Faes1,2, Armando Domiciano de Souza2,AlexC.Carciofi1 and Philippe Bendjoya2 1 Instituto de Astronomia, Geof´ısica e Ciˆencias Atmosf´ericas, Universidade de S˜ao Paulo, Rua do Mat˜ao 1226, Cidade Universit´aria, 05508-900, S˜ao Paulo, SP, Brazil email: [email protected] 2 Lab. J.-L. Lagrange, UMR 7293 - Observatoire de la Cˆote d’Azur (OCA), Univ. de Nice-Sophia Antipolis (UNS), CNRS, Valrose, 06108 Nice, France Abstract. Achernar is a key target to investigate high stellar rotation and the Be phenonemon. It is also the hottest star for which detailed photospheric information is available. Here we report our results to determine the photospheric parameters of Achernar and evaluate how the emission of a Viscous Decretion Disk (VDD) around it would be observable. The analysis is based on interferometric data (PIONIER and AMBER at ESO-VLTI), complemented by spectroscopy and polarimetry for the circumstellar emission. For the first time fundamental parameters of a Be photosphere were determined. The presence of a residual disk at the quiescent phase and some characteristics of the new formed disk (2013 activity) are also discussed. This is rare opportunity to precisely determine the stellar brightness distribution and evaluate the evolution of a just formed Be disk. Keywords. stars: individual (Achernar), stars: fundamental parameters, techniques: interfero- metric, circumstellar matter, stars: emission-line, Be 1.
    [Show full text]
  • 2021 Solar Rituality and Ephemerides
    HE LANETARY YSTEM T P S Ideas, Formulas and Forms for a new Culture/Civilization 2021 SOLAR RITUALITY AND EPHEMERIDES (December 2020) [email protected] 1 2021 SOLAR RITUALITY AND EPHEMERIDES A rhythmic and ritual coordination and sowing for a planetary Order The TPS solar Sowing Ia, Fa a F a C a Ca intends to a a a" a aa " a ba a " the cyclic pulsations of the higher Creators, the planetary, solar and cosmic Entities: the conscious Dream of a New Culture and Civilization, as a manifestation on Earth of the evolutionary Plan and of a new human planetary Order.1 By working we learn to work, and in this Workshop of spatial Thought we learn together to build more and more knowingly Harmonic Thought-forms, as a result of a right or heavenly way of being and existing, in order to set up a better Future and to progressively release our humanity from its lower trammels. Humanity can and has to spread, in an impersonal and disinterested way, Seeds or Ideas capable of fertilizing consciousness making it resound to infinity: "Culture is a treasure of consciousness, therefore the field of the sowing of the new Thought is the human consciousness ... It is a vast field like Heaven: no one knows its boundaries. Thus the seeds to be spread have no number or form ... Only with formless seeds an infinite field can be cultivated. And the soil of human consciousness is ready to welcome them: many signs prove it, both above and below, and sowing cannot be deferred".
    [Show full text]
  • The Spinning-Top Be Star Achernar from VLTI-VINCI
    A&A 407, L47–L50 (2003) Astronomy DOI: 10.1051/0004-6361:20030786 & c ESO 2003 Astrophysics The spinning-top Be star Achernar from VLTI-VINCI A. Domiciano de Souza1,P.Kervella2,S.Jankov3,L.Abe1, F. Vakili1,3,E.diFolco4, and F. Paresce4 1 Laboratoire Univ. d’Astroph. de Nice (LUAN), CNRS UMR 6525, Parc Valrose, 06108 Nice Cedex 02, France 2 European Southern Observatory (ESO), Alonso de Cordova 3107, Casilla 19001, Vitacura, Santiago 19, Chile 3 Observatoire de la Cˆote d’Azur, D´epartement FRESNEL, CNRS UMR 6528, Boulevard de l’Observatoire, Letter to the Editor BP 4229, 06304 Nice, France 4 European Southern Observatory (ESO), Karl-Schwarzschild str. 2, 85748 Garching, Germany Received 5 May 2003 / Accepted 22 May 2003 Abstract. We report here the first observations of a rapidly rotating Be star, α Eridani, using Earth-rotation synthesis on the Very Large Telescope (VLT) Interferometer. Our measures correspond to a 2a/2b = 1.56 0.05 apparent oblate star, 2a and 2b being the equivalent uniform disc angular diameters in the equatorial and polar direction. Considering± the presence of a circum- stellar envelope (CSE) we argue that our measurement corresponds to a truly distorted star since α Eridani exhibited negligible Hα emission during the interferometric observations. In this framework we conclude that the commonly adopted Roche approx- imation (uniform rotation and centrally condensed mass) should not apply to α Eridani. This result opens new perspectives to basic astrophysical problems, such as rotationally enhanced mass loss and internal angular momentum distribution. In addition to its intimate relation with magnetism and pulsation, rapid rotation thus provides a key to the Be phenomenon: one of the outstanding non-resolved problems in stellar physics.
    [Show full text]
  • The Fundamentals of Stargazing Sky Tours South
    The Fundamentals of Stargazing Sky Tours South 01 – The March Sky Copyright © 2014-2016 Mintaka Publishing Inc. www.CosmicPursuits.com -2- The Constellation Orion Let’s begin the tours of the deep-southern sky with the most famous and unmistakable constellation in the heavens, Orion, which will serve as a guide for other bright constellations in the southern late-summer sky. Head outdoors around 8 or 9 p.m. on an evening in early March, and turn towards the north. If you can’t find north, you can ask someone else, or get a small inexpensive compass, or use the GPS in your smartphone or tablet. But you need to face at least generally northward before you can proceed. You will also need a good unobstructed view of the sky in the north, so you may need to get away from structures and trees and so on. The bright stars of the constellation Orion (in this map, south is up and east is to the right) And bring a pair of binoculars if you have them, though they are not necessary for this tour. Fundamentals of Stargazing -3- Now that you’re facing north with a good view of a clear sky, make a 1/8th of a turn to your left. Now you are facing northwest, more or less. Turn your gaze upward about halfway to the point directly overhead. Look for three bright stars in a tidy line. They span a patch of sky about as wide as your three middle fingers held at arm’s length. This is the “belt” of the constellation Orion.
    [Show full text]
  • Introduction to Astronomy Lecture 3: the Birth of Stars and Planets
    Introduction to Astronomy Lecture 3: The birth of stars and planets Presented by Dr Helen Johnston School of Physics Spring 2015 The University of Sydney Page In tonight’s lecture • Forming stars – where stars come from • Forming planets – how the planets come together • Measuring stars – how we find the brightness and distance of stars The University of Sydney Page !2 Forming stars Our story begins with the vast clouds of gas between the stars. The University of Sydney The Great Nebula in Orion, M42 Page !4 This gas is made up mostly of hydrogen and helium, formed in the Big Bang. However, a small but vital fraction consists of heavier elements like oxygen, carbon and silicon. As we will see in coming weeks, these elements were manufactured deep in the cores of stars, and returned to the interstellar medium when those stars expired. Without these heavier elements, no rocky planets could form. The Crab Nebula, left behind by the supernovaThe University of Sydney explosion of 1054 AD Page !5 The interstellar material from which the solar system formed consists mostly of hydrogen and helium, with other elements less than one-thousandth as abundant as hydrogen. The “Astronomer’s Periodic table”, with the size of the element indicating its abundance byThe Universityweight. of Sydney (Figure by Ben McCall) Page !6 Star formation takes place in the densest regions of clouds, called dark nebulae. A famous example is the Horsehead Nebula. In these regions, shrouded by dust, molecular gas forms and clumps together and the density increases, until the densest regions start to collapse under their own gravity.
    [Show full text]
  • Basic Astronomy Labs
    Astronomy Laboratory Exercise 31 The Magnitude Scale On a dark, clear night far from city lights, the unaided human eye can see on the order of five thousand stars. Some stars are bright, others are barely visible, and still others fall somewhere in between. A telescope reveals hundreds of thousands of stars that are too dim for the unaided eye to see. Most stars appear white to the unaided eye, whose cells for detecting color require more light. But the telescope reveals that stars come in a wide palette of colors. This lab explores the modern magnitude scale as a means of describing the brightness, the distance, and the color of a star. The earliest recorded brightness scale was developed by Hipparchus, a natural philosopher of the second century BCE. He ranked stars into six magnitudes according to brightness. The brightest stars were first magnitude, the second brightest stars were second magnitude, and so on until the dimmest stars he could see, which were sixth magnitude. Modern measurements show that the difference between first and sixth magnitude represents a brightness ratio of 100. That is, a first magnitude star is about 100 times brighter than a sixth magnitude star. Thus, each magnitude is 100115 (or about 2. 512) times brighter than the next larger, integral magnitude. Hipparchus' scale only allows integral magnitudes and does not allow for stars outside this range. With the invention of the telescope, it became obvious that a scale was needed to describe dimmer stars. Also, the scale should be able to describe brighter objects, such as some planets, the Moon, and the Sun.
    [Show full text]
  • INTENDED DEREGISTERATION &CANCELLATION of Pins
    INTENDED DEREGISTERATION &CANCELLATION OF PINs S/No.
    [Show full text]
  • A Simple Method of Determining Archaeoastronomical Alignments in the Field
    UC Merced Journal of California and Great Basin Anthropology Title A Simple Method of Determining Archaeoastronomical Alignments in the Field Permalink https://escholarship.org/uc/item/7vd4h0xw Journal Journal of California and Great Basin Anthropology, 1(1) ISSN 0191-3557 Authors Seymour, Timothy P Edberg, Stephen J Publication Date 1979-12-01 Peer reviewed eScholarship.org Powered by the California Digital Library University of California A Simple Method of Determining Archaeoastronomical Alignments in the Field TIMOTHY P. SEYMOUR STEPHEN J. EDBERG As an aid in achieving this goal, we have EDITOR'S NOTE: While it is not nor­ developed the following simplified algebraic mally our policy to publish papers of a purely expressions, derived from spherical trigo­ methodological nature, the following paper is nometry, which can be used to determine useful to archaeologists with an interest in whether or not a celestial object (such as the archaeoastronotny and can be employed in sun, moon, or particular star) of possible sig­ making observations of the type described in nificance will rise or set at a point on the the preceding paper. horizon indicated by an apparent alignment. The only field equipment required consists of ECAUSE of the recent interest on the a surveyor's transit, a book of trigonometric B part of archaeologists in the possible tables or hand calculator with trigonometric astronomical significance of various archaeo­ functions, and an inexpensive star atlas. In logical features, field archaeologists are addition, a great deal of preliminary analysis beginning to look for possible archaeoastro­ can be accomplished prior to going into the nomical alignments with ever-increasing field with nothing more complex than a topo­ vigilance.
    [Show full text]
  • Epsilon Eridani's Planetary Debris Disk: Structure and Dynamics Based on Spitzer and Caltech Submillimeter Observatory Observa
    The Astrophysical Journal,690:1522–1538,2009January10 doi:10.1088/0004-637/690/2/1522 c 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A. ! EPSILON ERIDANI’S PLANETARY DEBRIS DISK: STRUCTURE AND DYNAMICS BASED ON SPITZER AND CALTECH SUBMILLIMETER OBSERVATORY OBSERVATIONS D. Backman1,M.Marengo2,K.Stapelfeldt3,K.Su4, D. Wilner2,C.D.Dowell3, D. Watson5,J.Stansberry4, G. Rieke4,T.Megeath2,6,G.Fazio2,andM.Werner3 1 Stratospheric Observatory for Infrared Astronomy & SETI Institute, 515 North Whisman Road, Mountain View, CA 94043, USA 2 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 3 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA 4 Steward Observatory, University of Arizona, Tucson, AZ 85721, USA 5 Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA Received 2008 May 25; accepted 2008 September 8; published 2008 December 22 ABSTRACT Spitzer and Caltech Submillimeter Observatory images and spectrophotometry of ! Eridani at wavelengths from 3.5 to 350 µmrevealnewdetailsofitsbrightdebrisdisk.The350µmmapconfirmsthepresenceofaring at r 11""–28""(35–90 AU), observed previously at longer sub-mm wavelengths. The Spitzer mid-IR and far- IR images= do not show the ring, but rather a featureless disk extending from within a few arcsec of the star across the ring to r 34"" (110 AU). The spectral energy distribution (SED) of the debris system implies acomplexstructure.AmodelconstrainedbythesurfacebrightnessprofilesandtheSEDindicatesthatthe∼ sub-mm ring emission is primarily from large (a 135 µm) grains, with smaller (a 15 µm) grains also present in and beyond the ring.
    [Show full text]
  • Uranometría Argentina Bicentenario
    URANOMETRÍA ARGENTINA BICENTENARIO Reedición electrónica ampliada, ilustrada y actualizada de la URANOMETRÍA ARGENTINA Brillantez y posición de las estrellas fijas, hasta la séptima magnitud, comprendidas dentro de cien grados del polo austral. Resultados del Observatorio Nacional Argentino, Volumen I. Publicados por el observatorio 1879. Con Atlas (1877) 1 Observatorio Nacional Argentino Dirección: Benjamin Apthorp Gould Observadores: John M. Thome - William M. Davis - Miles Rock - Clarence L. Hathaway Walter G. Davis - Frank Hagar Bigelow Mapas del Atlas dibujados por: Albert K. Mansfield Tomado de Paolantonio S. y Minniti E. (2001) Uranometría Argentina 2001, Historia del Observatorio Nacional Argentino. SECyT-OA Universidad Nacional de Córdoba, Córdoba. Santiago Paolantonio 2010 La importancia de la Uranometría1 Argentina descansa en las sólidas bases científicas sobre la cual fue realizada. Esta obra, cuidada en los más pequeños detalles, se debe sin dudas a la genialidad del entonces director del Observatorio Nacional Argentino, Dr. Benjamin A. Gould. Pero nada de esto se habría hecho realidad sin la gran habilidad, el esfuerzo y la dedicación brindada por los cuatro primeros ayudantes del Observatorio, John M. Thome, William M. Davis, Miles Rock y Clarence L. Hathaway, así como de Walter G. Davis y Frank Hagar Bigelow que se integraron más tarde a la institución. Entre éstos, J. M. Thome, merece un lugar destacado por la esmerada revisión, control de las posiciones y determinaciones de brillos, tal como el mismo Director lo reconoce en el prólogo de la publicación. Por otro lado, Albert K. Mansfield tuvo un papel clave en la difícil confección de los mapas del Atlas. La Uranometría Argentina sobresale entre los trabajos realizados hasta ese momento, por múltiples razones: Por la profundidad en magnitud, ya que llega por vez primera en este tipo de empresa a la séptima.
    [Show full text]
  • Transits of Mercury, 1605–2999 CE
    Appendix A Transits of Mercury, 1605–2999 CE Date (TT) Int. Offset Date (TT) Int. Offset Date (TT) Int. Offset 1605 Nov 01.84 7.0 −0.884 2065 Nov 11.84 3.5 +0.187 2542 May 17.36 9.5 −0.716 1615 May 03.42 9.5 +0.493 2078 Nov 14.57 13.0 +0.695 2545 Nov 18.57 3.5 +0.331 1618 Nov 04.57 3.5 −0.364 2085 Nov 07.57 7.0 −0.742 2558 Nov 21.31 13.0 +0.841 1628 May 05.73 9.5 −0.601 2095 May 08.88 9.5 +0.326 2565 Nov 14.31 7.0 −0.599 1631 Nov 07.31 3.5 +0.150 2098 Nov 10.31 3.5 −0.222 2575 May 15.34 9.5 +0.157 1644 Nov 09.04 13.0 +0.661 2108 May 12.18 9.5 −0.763 2578 Nov 17.04 3.5 −0.078 1651 Nov 03.04 7.0 −0.774 2111 Nov 14.04 3.5 +0.292 2588 May 17.64 9.5 −0.932 1661 May 03.70 9.5 +0.277 2124 Nov 15.77 13.0 +0.803 2591 Nov 19.77 3.5 +0.438 1664 Nov 04.77 3.5 −0.258 2131 Nov 09.77 7.0 −0.634 2604 Nov 22.51 13.0 +0.947 1674 May 07.01 9.5 −0.816 2141 May 10.16 9.5 +0.114 2608 May 13.34 3.5 +1.010 1677 Nov 07.51 3.5 +0.256 2144 Nov 11.50 3.5 −0.116 2611 Nov 16.50 3.5 −0.490 1690 Nov 10.24 13.0 +0.765 2154 May 13.46 9.5 −0.979 2621 May 16.62 9.5 −0.055 1697 Nov 03.24 7.0 −0.668 2157 Nov 14.24 3.5 +0.399 2624 Nov 18.24 3.5 +0.030 1707 May 05.98 9.5 +0.067 2170 Nov 16.97 13.0 +0.907 2637 Nov 20.97 13.0 +0.543 1710 Nov 06.97 3.5 −0.150 2174 May 08.15 3.5 +0.972 2644 Nov 13.96 7.0 −0.906 1723 Nov 09.71 13.0 +0.361 2177 Nov 09.97 3.5 −0.526 2654 May 14.61 9.5 +0.805 1736 Nov 11.44 13.0 +0.869 2187 May 11.44 9.5 −0.101 2657 Nov 16.70 3.5 −0.381 1740 May 02.96 3.5 +0.934 2190 Nov 12.70 3.5 −0.009 2667 May 17.89 9.5 −0.265 1743 Nov 05.44 3.5 −0.560 2203 Nov
    [Show full text]
  • Development and Utilization of the HRIV Point Spread Function for the EPOXI Mission
    Development and Utilization of the HRIV Point Spread Function for the EPOXI Mission R. K. Barry [email protected] NASA/Goddard Space Flight Center, Greenbelt, MD 20771 ABSTRACT The Extrasolar Planet Observation Characterization and the Deep Impact Extended Investigation missions (EPOXI) are currently observing the transits of exoplanets, a comet nucleus at short range, and Earth using the High Resolution Instrument (HRI) - a 0.3 m f/35 telescope – on the Deep Impact flyby spacecraft. The HRI is in a permanently defocused state with the instrument point of focus about 0.6 cm before the focal plane due to the use of a reference flat mirror that became a powered optic due to thermal warping during ground thermal-vacuum testing. Consequently, the point spread function (PSF) for the HRI Visible CCD (HRIV) covers approximately nine pixels FWHM and is characterized by a patch with three-fold symmetry due to the three-point support structures of the primary and secondary mirrors. The PSF is also strongly color dependent varying in shape and size with change in filtration and target color. While defocus is highly desirable for exoplanet transit observations to limit sensitivity to intra-pixel variation, it is suboptimal for observations of spatially resolved targets. Consequently, all HRIV images used in our analysis of such objects were deconvolved with an instrument PSF. The instrument PSF is also being used to optimize transit analysis. We discuss development and usage of an instrument PSF for these observations. 1. INTRODUCTION The Extrasolar Planet Observation Characterization and the Deep Impact Extended Investigation (EPOXI) mission is the successful merging of the DIXI and EPOCh science investigations into a single affordable mission.
    [Show full text]