Capturing the Starlight
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Requirements of Timely Performance in Time and Voyage Charterparties
Graduate School REQUIREMENTS OF TIMELY PERFORMANCE IN TIME AND VOYAGE CHARTERPARTIES - AN EXPLORATION OF THEIR IDENTITY, SCOPE AND LIMITATIONS UNDER ENGLISH LAW Thesis submitted for the degree of Doctor of Philosophy at the University of Leicester by Tamaraudoubra Tom Egbe School of Law University of Leicester 2019 Abstract REQUIREMENTS OF TIMELY PERFORMANCE IN TIME AND VOYAGE CHARTERPARTIES - AN EXPLORATION OF THEIR IDENTITY, SCOPE AND LIMITATIONS UNDER ENGLISH LAW By Tamaraudoubra Tom Egbe The importance of time in the performance of contractual obligations under sea carriage of goods arrangements are until now little explored. For the avoidance of breach, certain obligations and responsibilities of the parties to the contract need to be performed promptly. Ocean transport is an expensive venture and a shipowner could suffer considerable financial losses if an unnecessary but serious delay interrupt the vessel’s earning power in the course of the charterer’s performance of his contractual obligation. On the other hand, a charterer could also incur a substantial loss if arrangements for the shipment and receipt of cargo fail to go according to plan as a result of the shipowner’s failure to perform his charterparty obligation timely and with reasonable diligence. With these considerations in mind, this thesis critically explores the concept of timely performance in the discharge of the contractual obligations of parties to a contract of carriage. While the thesis is not an expository of the occurrence of time in all the obligations of parties to the carriage contract, it focusses particularly on the identity, scope, and limitations of timeliness in the context of timely payment of hire, laytime and reasonable despatch. -
PACS Sky Fields and Double Sources for Photometer Spatial Calibration
Document: PACS-ME-TN-035 PACS Date: 27th July 2009 Herschel Version: 2.7 Fields and Double Sources for Spatial Calibration Page 1 PACS Sky Fields and Double Sources for Photometer Spatial Calibration M. Nielbock1, D. Lutz2, B. Ali3, T. M¨uller2, U. Klaas1 1Max{Planck{Institut f¨urAstronomie, K¨onigstuhl17, D-69117 Heidelberg, Germany 2Max{Planck{Institut f¨urExtraterrestrische Physik, Giessenbachstraße, D-85748 Garching, Germany 3NHSC, IPAC, California Institute of Technology, Pasadena, CA 91125, USA Document: PACS-ME-TN-035 PACS Date: 27th July 2009 Herschel Version: 2.7 Fields and Double Sources for Spatial Calibration Page 2 Contents 1 Scope and Assumptions 4 2 Applicable and Reference Documents 4 3 Stars 4 3.1 Optical Star Clusters . .4 3.2 Bright Binaries (V -band search) . .5 3.3 Bright Binaries (K-band search) . .5 3.4 Retrieval from PACS Pointing Calibration Target List . .5 3.5 Other stellar sources . 13 3.5.1 Herbig Ae/Be stars observed with ISOPHOT . 13 4 Galactic ISOCAM fields 13 5 Galaxies 13 5.1 Quasars and AGN from the Veron catalogue . 13 5.2 Galaxy pairs . 14 5.2.1 Galaxy pairs from the IRAS Bright Galaxy Sample with VLA radio observations 14 6 Solar system objects 18 6.1 Asteroid conjunctions . 18 6.2 Conjunctions of asteroids with pointing stars . 22 6.3 Planetary satellites . 24 Appendices 26 A 2MASS images of fields with suitable double stars from the K-band 26 B HIRES/2MASS overlays for double stars from the K-band search 32 C FIR/NIR overlays for double galaxies 38 C.1 HIRES/2MASS overlays for double galaxies . -
The Evening Sky Map
I N E D R I A C A S T N E O D I T A C L E O R N I G D S T S H A E P H M O O R C I . Z N O p l f e i n h d o P t O o N ) l h a r g Z i u s , o I l C t P h R I r e o R N ( O o r C r H e t L p h p E E i s t D H a ( r g T F i . O B NORTH D R e N M h t E A X O e s A H U M C T . I P N S L E E P Z “ E A N H O NORTHERN HEMISPHERE M T R T Y N H E ” K E η ) W S . T T E W U B R N W D E T T W T H h A The Evening Sky Map e MAY 2021 E . C ) Cluster O N FREE* EACH MONTH FOR YOU TO EXPLORE, LEARN & ENJOY THE NIGHT SKY r S L a o K e Double r Y E t B h R M t e PERSEUS A a A r CASSIOPEIA n e S SKY MAP SHOWS HOW Get Sky Calendar on Twitter P δ r T C G C A CEPHEUS r E o R e J s O h Sky Calendar – May 2021 http://twitter.com/skymaps M39 s B THE NIGHT SKY LOOKS T U ( O i N s r L D o a j A NE I I a μ p T EARLY MAY PM T 10 r 61 M S o S 3 Last Quarter Moon at 19:51 UT. -
Extrasolar Planets and Their Host Stars
Kaspar von Braun & Tabetha S. Boyajian Extrasolar Planets and Their Host Stars July 25, 2017 arXiv:1707.07405v1 [astro-ph.EP] 24 Jul 2017 Springer Preface In astronomy or indeed any collaborative environment, it pays to figure out with whom one can work well. From existing projects or simply conversations, research ideas appear, are developed, take shape, sometimes take a detour into some un- expected directions, often need to be refocused, are sometimes divided up and/or distributed among collaborators, and are (hopefully) published. After a number of these cycles repeat, something bigger may be born, all of which one then tries to simultaneously fit into one’s head for what feels like a challenging amount of time. That was certainly the case a long time ago when writing a PhD dissertation. Since then, there have been postdoctoral fellowships and appointments, permanent and adjunct positions, and former, current, and future collaborators. And yet, con- versations spawn research ideas, which take many different turns and may divide up into a multitude of approaches or related or perhaps unrelated subjects. Again, one had better figure out with whom one likes to work. And again, in the process of writing this Brief, one needs create something bigger by focusing the relevant pieces of work into one (hopefully) coherent manuscript. It is an honor, a privi- lege, an amazing experience, and simply a lot of fun to be and have been working with all the people who have had an influence on our work and thereby on this book. To quote the late and great Jim Croce: ”If you dig it, do it. -
The Minor Planet Bulletin, We Feel Safe in Al., 1989)
THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 43, NUMBER 3, A.D. 2016 JULY-SEPTEMBER 199. PHOTOMETRIC OBSERVATIONS OF ASTEROIDS star, and asteroid were determined by measuring a 5x5 pixel 3829 GUNMA, 6173 JIMWESTPHAL, AND sample centered on the asteroid or star. This corresponds to a 9.75 (41588) 2000 SC46 by 9.75 arcsec box centered upon the object. When possible, the same comparison star and check star were used on consecutive Kenneth Zeigler nights of observation. The coordinates of the asteroid were George West High School obtained from the online Lowell Asteroid Services (2016). To 1013 Houston Street compensate for the effect on the asteroid’s visual magnitude due to George West, TX 78022 USA ever changing distances from the Sun and Earth, Eq. 1 was used to [email protected] vertically align the photometric data points from different nights when constructing the composite lightcurve: Bryce Hanshaw 2 2 2 2 George West High School Δmag = –2.5 log((E2 /E1 ) (r2 /r1 )) (1) George West, TX USA where Δm is the magnitude correction between night 1 and 2, E1 (Received: 2016 April 5 Revised: 2016 April 7) and E2 are the Earth-asteroid distances on nights 1 and 2, and r1 and r2 are the Sun-asteroid distances on nights 1 and 2. CCD photometric observations of three main-belt 3829 Gunma was observed on 2016 March 3-5. Weather asteroids conducted from the George West ISD Mobile conditions on March 3 and 5 were not particularly favorable and so Observatory are described. -
Determination of the Spectroscopic Stellar Parameters for 257 Field Giant
Mon. Not. R. Astron. Soc. 000, 1–18 (2015) Printed 10 May 2018 (MN LATEX style file v2.2) Determination of the spectroscopic stellar parameters for 257 field giant stars⋆⋆ S. Alves1,2†, L. Benamati3,4,5, N. C. Santos3,4,5, V. Zh. Adibekyan3,4, S. G. Sousa3,4,5, G. Israelian6,7, J. R. De Medeiros8, C. Lovis9, S. Udry9 1 Instituto de Astrof´ısica, Pontificia Universidad Cat´olica de Chile, Av. Vicu˜na Mackenna 4860, 782-0436, Macul, Santiago, Chile 2 CAPES Foundation, Ministry of Education of Brazil, Bras´ılia / DF, Brazil 3 Centro de Astrof´ısica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal 4 Instituto de Astrof´ısica e Ciˆencias do Espa¸co, Universidade do Porto, Rua das Estrelas, PT4150-762 Porto, Portugal 5 Departamento de F´ısica e Astronomia, Faculdade de Ciˆencias da Universidade do Porto, Portugal 6 Instituto de Astrof´ısica de Canarias, 38200 La Laguna, Tenerife, Spain 7 Departamento de Astrof´ısica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain 8 Departamento de F´ısica Te´orica e Experimental, Universidade Federal do Rio Grande do Norte, Campus Universit´ario Lagoa Nova, 59072-970 Natal, RN, Brasil 9 Observatoire de Gen`eve, Universit´ede Gen`eve, 51 ch. des Maillettes, 1290, Sauverny, Switzerland Accepted 2015 January 26. Received 2015 January 20; in original form 2014 November 26 ABSTRACT The study of stellar parameters of planet-hosting stars, such as metallicity and chemical abun- dances, help us to understand the theory of planet formation and stellar evolution. Here, we present a catalogue of accurate stellar atmospheric parameters and iron abundances for a sam- ple of 257 K and G field evolved stars that are being surveyed for planets using precise radial– velocity measurements as part of the CORALIE programme to search for planets around giants. -
The Minor Planet Bulletin
THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 34, NUMBER 3, A.D. 2007 JULY-SEPTEMBER 53. CCD PHOTOMETRY OF ASTEROID 22 KALLIOPE Kwee, K.K. and von Woerden, H. (1956). Bull. Astron. Inst. Neth. 12, 327 Can Gungor Department of Astronomy, Ege University Trigo-Rodriguez, J.M. and Caso, A.S. (2003). “CCD Photometry 35100 Bornova Izmir TURKEY of asteroid 22 Kalliope and 125 Liberatrix” Minor Planet Bulletin [email protected] 30, 26-27. (Received: 13 March) CCD photometry of asteroid 22 Kalliope taken at Tubitak National Observatory during November 2006 is reported. A rotational period of 4.149 ± 0.0003 hours and amplitude of 0.386 mag at Johnson B filter, 0.342 mag at Johnson V are determined. The observation of 22 Kalliope was made at Tubitak National Observatory located at an elevation of 2500m. For this study, the 410mm f/10 Schmidt-Cassegrain telescope was used with a SBIG ST-8E CCD electronic imager. Data were collected on 2006 November 27. 305 images were obtained for each Johnson B and V filters. Exposure times were chosen as 30s for filter B and 15s for filter V. All images were calibrated using dark and bias frames Figure 1. Lightcurve of 22 Kalliope for Johnson B filter. X axis is and sky flats. JD-2454067.00. Ordinate is relative magnitude. During this observation, Kalliope was 99.26% illuminated and the phase angle was 9º.87 (Guide 8.0). Times of observation were light-time corrected. -
Meteor 0 2 Csillagászati Évkönyv 2011 V Y N Ö K V É
1 1 meteor 0 2 csillagászati évkönyv 2011 v y n ö k v é i t a z s á g a l l i s c r o e t e m ISSN 0866 - 2851 9 7 7 0 8 6 6 2 8 5 0 0 2 Ár: 2400 Ft A Magyar Csillagászati Egyesület lapja meteor a tengerfenéktõl a „Marsig” olvassák! meteor.mcse.hu METEOR CSILLAGÁSZATI ÉVKÖNYV 2011 METEOR CSILLAGÁSZATI ÉVKÖNYV 2011 MCSE – 2010. NOVEMBER METEOR CSILLAGÁSZATI ÉVKÖNYV 2011 MCSE – 2010. NOVEMBER meteor csillagászati évkönyv 2011 Szerkesztette: Benkõ József Mizser Attila Magyar Csillagászati Egyesület www.mcse.hu Budapest, 2010 METEOR CSILLAGÁSZATI ÉVKÖNYV 2011 MCSE – 2010. NOVEMBER Az évkönyv kalendárium részének összeállításában közremûködött: Butuza Tamás Görgei Zoltán Hegedüs Tibor Kaposvári Zoltán Kovács József Sánta Gábor Sárneczky Krisztián Szabó Sándor Szôllôsi Attila A kalendárium csillagtérképei az Ursa Minor szoftverrel készültek. www.ursaminor.hu Az elongációs grafikonok készítéséhez egyedi szoftvert használtunk, melyet Butuza Tamás készített. Szakmailag ellenôrizte: Szabados László A kiadvány támogatói: Mindazok, akik az SZJA 1%-ával támogatják a Magyar Csillagászati Egyesületet. Adószámunk: 19009162-2-43 Felelôs kiadó: Mizser Attila Nyomdai elôkészítés: Kármán Stúdió, www.karman.hu Nyomtatás, kötészet: OOK-Press Kft., www.ookpress.hu Terjedelem: 20 ív fekete-fehér+1ívszínes melléklet 2010. november ISSN 0866-2851 METEOR CSILLAGÁSZATI ÉVKÖNYV 2011 MCSE – 2010. NOVEMBER Tartalom Bevezetô ................................................... 7 Kalendárium ............................................... 11 Cikkek Kálmán Béla: A napkutatás új eredményeibôl .................... 175 Kovács József: „Theoria motus corporum coelestium…” ........... 187 Benkô József – Szabó Róbert: Idôsorok az ûrbôl .................. 207 Kun Mária: Új ablakok a csillagközi anyagra ..................... 233 Hegedüs Tibor: A Tejútrendszer napjainkban .................... 240 Budavári Tamás: A Világegyetem színe ........................ -
January 9 2016 7:00Pm at the Herrett Center for Arts & Science Colleagues, College of Southern Idaho
Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting President’s Message Saturday, January 9th 2016 7:00pm at the Colleagues, Herrett Center for Arts & Science College of Southern Idaho. As 2016 opens up, it's time to talk about an old tradition and hopefully a new one. Public Star Party Follows at the First of all, the annual telescope clinic conducted by Tom Gilbertson will be Centennial Observatory Saturday, Jan. 9, at 7 p.m. at the Herrett Center. This is a great chance to help Club Officers friends out who may have received telescopes for Christmas. Please encourage them to come, and please feel free on attending. The more participation we get, the Robert Mayer, President better the chance we have of connecting to the public. [email protected] 208-312-1203 Then there's the new tradition we're hoping to carry out. On Friday, March 4th, we're planning on renting out the Lodge at Castle Rocks State Park. According to the Paul McClain, Vice President Park's website, the Lodge can hold up to eight people in four rooms. Jay Naegele [email protected] went there a couple of months ago, and reported back that the experience was worth it. What we'd do then, is just hold a members' star party at the Lodge. Gary Leavitt, Secretary [email protected] To help offset the cost, we are asking for $15 from each person who attends. 208-731-7476 If you are interested in going, please let me know, for the sooner we can make Jim Tubbs, Treasurer / ALCOR reservations, the better. -
The Minor Planet Bulletin 40 (2013) 125 CS3 Observations on Jan 13 and 14 Were Made with a 0.35-M Schmidt-Cassegrain and SBIG ST-9XE
THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 40, NUMBER 3, A.D. 2013 JULY-SEPTEMBER 119. SOMETHING OLD, SOMETHINGS NEW: figure shows the lightcurve after removing the rotation of the THREE BINARY DISCOVERIES primary, thus revealing the mutual events and other features due to FROM THE PALMER DIVIDE OBSERVATORY the satellite. The latter often includes an upward bowing between the events, indicating an elongated satellite that is tidally-locked to Brian D. Warner its orbital period. Palmer Divide Observatory 17995 Bakers Farm Rd., Colorado Springs, CO 80908 4383 Suruga. Observations of 4383 Suruga were made from 2013 [email protected] Feb 2-13. Initial observations were made with a 0.35-m Schmidt- Cassegrain and Finger Lakes FLI-1001E CCD camera. When (Received: 10 March) indications of a satellite were seen in those first data sets, the target was moved to a 0.5-m Ritchey-Chretien with FLI-1001E to improve the signal-to-noise ratio. Data on the order of 0.01-0.02 Analysis of new CCD photometric observations in early mag are usually required for reliable detections of mutual events 2013 of the Vestoid asteroid 4383 Suruga and Hungaria (occultations and/or eclipses) caused by a satellite. asteroid (53432) 1999 UT55 showed that the two are binary systems. A review of data from 2005 for the The results of the analysis are shown in Figures 1-3. The period of Hungaria asteroid 4440 Tchantches indicates that the the primary is 3.4068 ± 0.0003 h with an amplitude of 0.14 ± 0.01 original analysis probably overlooked a satellite. -
Star Dust National Capital Astronomers, Inc
Star Dust National Capital Astronomers, Inc. May 2012 Volume 70, Issue 9 http://capitalastronomers.org Next Meeting May 2012: Soebur Razzaque When: Sat. May 12, 2012 George Mason University Time: 7:30 pm Neutrino Astronomy Where: UMD Observatory Abstract: Giant kilometer-scale telescopes in places like Antarctica Speaker: Soebur Razzaque, and the Mediterranean Sea are currently operating or being built to GMU catch neutrinos, one of the most elusive known particles in nature. Table of Contents Because neutrinos interact so feebly with matter, neutrino telescopes need to be big to catch neutrinos from galactic and extragalactic Preview of May 2012 Talk 1 astrophysical objects. Neutrino astronomy is still in its infancy: the Sun MASPG Talk May 16 2 and Supernova 1987A are the only sources that have been detected so far. But the detections from those two sources have already Hopewell Open House May 19 3 revealed much about the inner working of the Sun's core and about the Exploring the Sky Schedule 3 mechanism of supernova explosions, information that is inaccessible Occultations 4 to optical telescopes. Black Holes 6 High-energy neutrinos are produced by the interactions of cosmic rays. Owens Planetarium Shows 6 Cosmic rays are charged particles, so they are deflected by the galactic and extragalactic magnetic fields. Their directions of arrival tell NCA Volunteers 7 us nothing about the directions of their source objects. Thus the Calendar 7 sources of cosmic rays still have not been identified. In contrast, neutrinos are rarely deflected, so they point directly back to their Directions to Dinner/Meeting sources. -
0 Return of Private Foundation
16 0 OMB No 1545.0052 Form 990 -PF Return of Private Foundation or Section 4947(aXl) Nonexempt Charitable Trust Treated as a Private Foundation 2011 Department of the Treasury Internal Revenue Service Note . The foundation may be able to use a copy of this return to satisfy state reporting requi For calendar year 2011 , or tax year beginning 7/01 , 2011, and ending 6/30 , 2012 BAUMAN FAMILY FOUNDATION, INC. A Employer identification number 2040 S STREET, NW 13-3119290 WASHINGTON, DC 20009-1110 B Telephone number (see the instructions) (202) 328-2040 C If exemntlon aonllcatlon Is oendlna. check here n G Check all that apply Initial return Initial Return of a former public charity D 1 Foreign organizations, check here Final return Amended return Address change Name change 2 Foreign organizations meeting the 85% test, check q here and attach computation H Check type of organization X Section 501 (c)(3) exempt private foundation Section 4947(a)(1 ) nonexem pt charitable trust Other taxable p rivate foundation E If private foundation status was terminated q Fair market value of all assets at end of year J Accounting method: X Cash Accrual under section 507(b)(1)(A), check here (from Part ll, column (c), line 16) [] Other (specify) F If the foundation is in a 60-month termination $ 93, 310, 166. I (Part 1, column (d) must be on cash basis under section 507(b)(1)(B'. check here ;Part:I T Analysis of Revenue and (a) Revenue and (b) Net investment (c) Adjusted net (d) Disbursements Expenses (The total of amounts in expenses per books income income for charitable columns (b), (c), and (d) may not neces- purposes sarily equal the amounts in column (a) (cash basis only) (see instructions) ) 1 Contributions, gifts, grants, etc, received (att sch) 2 Ck rf the toundn is not req to att Sch B = = ? .= -_ - - 3 Interest on savings and temporary '-_ ' - - cash investments 314 545.