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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. -
The Practice of Thresholds
Chapter 1 The Practice of Thresholds Thresholds were important to the ancient Irish monks whose wis- dom guides us on this path. Thresholds are the space between, when we move from one time to another, as in the threshold of dawn to day or of dusk to dark; one space to another, as in times of inner or outer journeying or pilgrimage; and one awareness to another, as in times when our old structures start to fall away and we begin to build something new. The Celts describe thresholds as “thin times or places” where heaven and earth are closer together and the veil between worlds is thin. In the Celtic imagination, thresholds are potent places. We expe- rience the thresholds of the year unfolding, so that each new season beckons us into a renewed awareness of the nearness of the holy presence. In the Celtic wheel of the year there are eight portals in time that mark the equinoxes and solstices, as well as the midway points between them. Each of these festivals held the possibility of deeper connection to the divine. We will explore this further in chap- ter 10. We encounter thresholds each day through the movement across the hinges of time. The turning of early morning and evening were thought to be especially graced times of day when the otherworld was near. There are physical places that evoke a sense of wonder. My hus- band, John, wonders if “thin places” means they were worn thin by the many souls who have been drawn to these liminal landscapes 1 THE SOUL’S SLOW RIPENING and sought prayer there. -
COMMISSION C4 WORLD HERITAGE and ASTRONOMY 1. Background
Transactions IAU, Volume XXXA Reports on Astronomy 2015-2018 c 2018 International Astronomical Union Piero Benvenuti, ed. DOI: 00.0000/X000000000000000X COMMISSION C4 WORLD HERITAGE AND ASTRONOMY PATRIMOINE MONDIAL ET ASTRONOMIE PRESIDENT Clive Ruggles VICE-PRESIDENT Gudrun Wolfschmidt PAST PRESIDENT N/A ORGANIZING COMMITTEE Roger Ferlet, Siramas Komonjinda, Mikhail Marov, Malcolm Smith COMMISSION C4 WORKING GROUPS Div. C / Commission C4 WG1 Windows to the Universe: High-Mountain Observatories and other Astronomical Sites of the late 20th and early 21st Centuries (Joint with Commission B7) Div. C / Commission C4 WG2 Classical Observatories from the Renaissance to the 20th Century Div. C / Commission C4 WG3 Heritage of Space Exploration Div. C / Commission C4 WG4 Astronomical Heritage in Danger Div. C / Commission C4 WG5 Intangible Heritage (Joint with Commission C1) Div. C / Commission C4 WGAAC Archaeoastronomy and Astronomy in Culture (Joint with Commission C3) TRIENNIAL REPORT 2015-2018 1. Background UNESCO's Astronomy and World Heritage Initiative (AWHI) (whc.unesco.org/en/ astronomy) has existed since 2004 to identify, promote and protect heritage, and potential World Heritage, connected with astronomy. A Memorandum of Understanding (MoU) between UNESCO and the IAU, under which the IAU undertook to implement the AWHI jointly with UNESCO, was signed in 2008 ahead of the IYA 2009. This commitment now continues indefinitely, UNESCO and the IAU having entered into a wider global partnership. The Astronomy and World Heritage Working Group -
The Skyscraper 2009 04.Indd
A Better Galaxy Guide: Early Spring M67: One of the most ancient open clusters known and Craig Cortis is a great novelty in this regard. Located 1.7° due W of mag NGC 2419: 3.25° SE of mag 6.2 66 Aurigae. Hard to find 4.3 Alpha Cancri. and see; at E end of short row of two mag 7.5 stars. Highly NGC 2775: Located 3.7° ENE of mag 3.1 Zeta Hydrae. significant and worth the effort —may be approximately (Look for “Head of Hydra” first.) 300,000 light years distant and qualify as an extragalactic NGC 2903: Easily found at 1.5° due S of mag 4.3 Lambda cluster. Named the Intergalactic Wanderer. Leonis. NGC 2683: Marks NW “crook” of coathanger-type triangle M95: One of three bright galaxies forming a compact with easy double star mag 4.2 Iota Cancri (which is SSW by triangle, along with M96 and M105. All three can be seen 4.8°) and mag 3.1 Alpha Lyncis (at 6° to the ENE). together in a low power, wide field view. M105 is at the NE tip of triangle, midway between stars 52 and 53 Leonis, mag Object Type R.A. Dec. Mag. Size 5.5 and 5.3 respectively —M95 is at W tip. Lynx NGC 3521: Located 0.5° due E of mag 6.0 62 Leonis. M65: One of a pair of bright galaxies that can be seen in NGC 2419 GC 07h 38.1m +38° 53’ 10.3 4.2’ a wide field view along with M66, which lies just E. -
Varro's Roman Seasons
Varro’s Roman Seasons Amelia Carolina Sparavigna To cite this version: Amelia Carolina Sparavigna. Varro’s Roman Seasons. 2019. hal-02387848 HAL Id: hal-02387848 https://hal.archives-ouvertes.fr/hal-02387848 Submitted on 30 Nov 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. HAL, Submitted 30 November 2019 Varro's Roman Seasons A. C. Sparavigna1 1 Dipartimento di Scienza Applicata e Tecnologia, Politecnico di Torino, Torino, Italy The four seasons of the Roman calendar, as described by Marcus Terentius Varro, are different from our seasons, in the sense that they start on days which differ from those that we are using today. In his Books on Agriculture, Varro shows that the Roman seasons started on the Cross Quarter-days instead than on the Quarter-days of the year as it happens today. Besides the classic subdivision in four parts, in the Books on Agriculture we can also find the year divided into eight parts, that is eight seasons having quite different lengths. In our discussion of Varro's seasons we will compare the days he mentions for the separation of seasons to the Cross Quarter- and Quarter-days that we find in Celtic calendars. -
Commission C4 Annual Report 2017
Commission C4 annual report 2017 Report for the period January to December 2017 The Commission's main achievements during 2017 are as follows. 1 The publication of the second ICOMOS-IAU Thematic Study on astronomical heritage ("TS2"). Heritage Sites of Astronomy and Archaeoastronomy in the Context of the World Heritage Convention: Thematic Study no. 2 was published as an e-book in June, in time for the 2017 UNESCO World Heritage Committee meeting in Kraków, and as a paperback in November, in time for the ICOMOS General Assembly in Delhi. ICOMOS Thematic Studies (sometimes produced in co-operation with specialist partner organisations) aim to provide a synthesis of current research and knowledge on a specific theme and/or region, and are useful to State Parties wishing to nominate a heritage property for inscription on the World Heritage List. TS2 examines a number of key questions relating to astronomical heritage sites and their potential recognition as World Heritage, attempting to identify what might constitute “outstanding universal value” (OUV) in relation to astronomy. It represents the culmination of several years' work to address some of the most challenging issues raised in the first ICOMOS-IAU Thematic Study ("TS1"), published in 2010. A particularly complex issue is the recognition and protection of dark skies. Dark sky areas cannot in themselves be considered as potential World Heritage Sites, but TS2 includes a thematic chapter by Michel Cotte of ICOMOS considering a range of ways in which dark sky values can be interrelated with broader cultural or natural values of a place and thereby contribute to its overall cultural or natural value and potential OUV. -
A Handbook of Double Stars, with a Catalogue of Twelve Hundred
The original of this bool< is in the Cornell University Library. There are no known copyright restrictions in the United States on the use of the text. http://www.archive.org/details/cu31924064295326 3 1924 064 295 326 Production Note Cornell University Library pro- duced this volume to replace the irreparably deteriorated original. It was scanned using Xerox soft- ware and equipment at 600 dots per inch resolution and com- pressed prior to storage using CCITT Group 4 compression. The digital data were used to create Cornell's replacement volume on paper that meets the ANSI Stand- ard Z39. 48-1984. The production of this volume was supported in part by the Commission on Pres- ervation and Access and the Xerox Corporation. Digital file copy- right by Cornell University Library 1991. HANDBOOK DOUBLE STARS. <-v6f'. — A HANDBOOK OF DOUBLE STARS, WITH A CATALOGUE OF TWELVE HUNDRED DOUBLE STARS AND EXTENSIVE LISTS OF MEASURES. With additional Notes bringing the Measures up to 1879, FOR THE USE OF AMATEURS. EDWD. CROSSLEY, F.R.A.S.; JOSEPH GLEDHILL, F.R.A.S., AND^^iMES Mt^'^I^SON, M.A., F.R.A.S. "The subject has already proved so extensive, and still ptomises so rich a harvest to those who are inclined to be diligent in the pursuit, that I cannot help inviting every lover of astronomy to join with me in observations that must inevitably lead to new discoveries." Sir Wm. Herschel. *' Stellae fixac, quae in ccelo conspiciuntur, sunt aut soles simplices, qualis sol noster, aut systemata ex binis vel interdum pluribus solibus peculiari nexu physico inter se junccis composita. -
List of Easy Double Stars for Winter and Spring = Easy = Not Too Difficult = Difficult but Possible
List of Easy Double Stars for Winter and Spring = easy = not too difficult = difficult but possible 1. Sigma Cassiopeiae (STF 3049). 23 hr 59.0 min +55 deg 45 min This system is tight but very beautiful. Use a high magnification (150x or more). Primary: 5.2, yellow or white Seconary: 7.2 (3.0″), blue 2. Eta Cassiopeiae (Achird, STF 60). 00 hr 49.1 min +57 deg 49 min This is a multiple system with many stars, but I will restrict myself to the brightest one here. Primary: 3.5, yellow. Secondary: 7.4 (13.2″), purple or brown 3. 65 Piscium (STF 61). 00 hr 49.9 min +27 deg 43 min Primary: 6.3, yellow Secondary: 6.3 (4.1″), yellow 4. Psi-1 Piscium (STF 88). 01 hr 05.7 min +21 deg 28 min This double forms a T-shaped asterism with Psi-2, Psi-3 and Chi Piscium. Psi-1 is the uppermost of the four. Primary: 5.3, yellow or white Secondary: 5.5 (29.7), yellow or white 5. Zeta Piscium (STF 100). 01 hr 13.7 min +07 deg 35 min Primary: 5.2, white or yellow Secondary: 6.3, white or lilac (or blue) 6. Gamma Arietis (Mesarthim, STF 180). 01 hr 53.5 min +19 deg 18 min “The Ram’s Eyes” Primary: 4.5, white Secondary: 4.6 (7.5″), white 7. Lambda Arietis (H 5 12). 01 hr 57.9 min +23 deg 36 min Primary: 4.8, white or yellow Secondary: 6.7 (37.1″), silver-white or blue 8. -
Varro's Roman Seasons
HAL, Submitted 30 November 2019 Varro's Roman Seasons A. C. Sparavigna1 1 Dipartimento di Scienza Applicata e Tecnologia, Politecnico di Torino, Torino, Italy The four seasons of the Roman calendar, as described by Marcus Terentius Varro, are different from our seasons, in the sense that they start on days which differ from those that we are using today. In his Books on Agriculture, Varro shows that the Roman seasons started on the Cross Quarter-days instead than on the Quarter-days of the year as it happens today. Besides the classic subdivision in four parts, in the Books on Agriculture we can also find the year divided into eight parts, that is eight seasons having quite different lengths. In our discussion of Varro's seasons we will compare the days he mentions for the separation of seasons to the Cross Quarter- and Quarter-days that we find in Celtic calendars. Keywords: Chronology, Roman Chronology, Julian Calendar, Celtic festivals. DOI:10.5281/zenodo.3559524 Marcus Terentius Varro (116 - 27 BC) was a Roman scholar and writer. In his political career, he became tribune of the people, quaestor and curule aedile. Supporting Pompey, Varro reached the office of praetor [1,2]. He was also one of the members of the commission that carried out the agrarian plan of Julius Caesar for the resettlement of Capua and Campania (59 BC) [2]. During the civil war, Varro commanded one of Pompey's armies in Spain. After the battle of Pharsalus, he reconciled with Julius Caesar, and Caesar appointed him to oversee the public library of Rome [1]. -
April 14 2018 7:00Pm at the April 2018 Herrett Center for Arts & Science College of Southern Idaho
Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting President’s Message Tim Frazier Saturday, April 14th 2018 April 2018 7:00pm at the Herrett Center for Arts & Science College of Southern Idaho. It really is beginning to feel like spring. The weather is more moderate and there will be, hopefully, clearer skies. (I write this with some trepidation as I don’t want to jinx Public Star Party Follows at the it in a manner similar to buying new equipment will ensure at least two weeks of Centennial Observatory cloudy weather.) Along with the season comes some great spring viewing. Leo is high overhead in the early evening with its compliment of galaxies as is Coma Club Officers Berenices and Virgo with that dense cluster of extragalactic objects. Tim Frazier, President One of my first forays into the Coma-Virgo cluster was in the early 1960’s with my [email protected] new 4 ¼ inch f/10 reflector and my first star chart, the epoch 1960 version of Norton’s Star Atlas. I figured from the maps I couldn’t miss seeing something since Robert Mayer, Vice President there were so many so closely packed. That became the real problem as they all [email protected] appeared as fuzzy spots and the maps were not detailed enough to distinguish one galaxy from another. I still have that atlas as it was a precious Christmas gift from Gary Leavitt, Secretary my grandparents but now I use better maps, larger scopes and GOTO to make sure [email protected] it is M84 or M86. -
Materiały Sekcji Obserwacji Pozycji I Zakryć Polskiego Towarzystwa Miłośników Astronomii
Materiały Sekcji Obserwacji Pozycji i Zakryć Polskiego Towarzystwa Miłośników Astronomii Nr 81 (1/2007) Brzegówkowy początek roku Uczestnicy wypraw obserwacyjnych 21 kwietnia Wydawnictwo dofinansowane ze środków Ministerstwa Nauki i Szkolnictwa Wyższego Sekcja Obserwacji Pozycji i Zakryć Polskiego Towarzystwa Miłośników Astronomii (SOPiZ PTMA) członek Międzynarodowego Towarzystwa Rejestracji Momentów Zakryć / Sekcja Europejska (International Occultation Timing Association / European Section) Sekcja istnieje od roku 1979 jako organizacja wewnętrzna Polskiego Towarzystwa Miłośników Astronomii. Sekcja zajmuje się prowadzeniem prac obserwacyjnych, obliczeniowych i analitycznych w dziedzinie zakryć - zaćmień oraz obserwacji pozycyjnych. Raz do roku SOPiZ organizuje konferencję poświęconą tematyce zakryć, zagadnień astrometrycznych i innych pokrewnych. Sekcja wydaje własny biuletyn „Materiały". Każdy członek Towarzystwa może przystąpić do aktywnej pracy w SOPiZ, stając się jej pełnoprawnym członkiem poprzez wykonywanie cennych obserwacji czy prac obliczeniowo - analitycznych. Bogate doświadczenie SOPiZ, jej zaangażowanie w prace techniczne, aktywna współpraca analityczna i koordynacyjna z innymi grupami z całego świata spowodowały, że od wielu lat Sekcja cieszy się uznaniem w międzynarodowym środowisku zajmującym się jej dziedziną działalności. Siedziba SOPiZ PTMA mieści się w Łodzi. Korespondencję należy kierować na adres: Sekcja Obserwacji Pozycji i Zakryć PTMA Planetarium i Obserwatorium Astronomiczne im. Arego Sternfelda ul. Pomorska 16 -
Arxiv:2006.10868V2 [Astro-Ph.SR] 9 Apr 2021 Spain and Institut D’Estudis Espacials De Catalunya (IEEC), C/Gran Capit`A2-4, E-08034 2 Serenelli, Weiss, Aerts Et Al
Noname manuscript No. (will be inserted by the editor) Weighing stars from birth to death: mass determination methods across the HRD Aldo Serenelli · Achim Weiss · Conny Aerts · George C. Angelou · David Baroch · Nate Bastian · Paul G. Beck · Maria Bergemann · Joachim M. Bestenlehner · Ian Czekala · Nancy Elias-Rosa · Ana Escorza · Vincent Van Eylen · Diane K. Feuillet · Davide Gandolfi · Mark Gieles · L´eoGirardi · Yveline Lebreton · Nicolas Lodieu · Marie Martig · Marcelo M. Miller Bertolami · Joey S.G. Mombarg · Juan Carlos Morales · Andr´esMoya · Benard Nsamba · KreˇsimirPavlovski · May G. Pedersen · Ignasi Ribas · Fabian R.N. Schneider · Victor Silva Aguirre · Keivan G. Stassun · Eline Tolstoy · Pier-Emmanuel Tremblay · Konstanze Zwintz Received: date / Accepted: date A. Serenelli Institute of Space Sciences (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E- 08193, Spain and Institut d'Estudis Espacials de Catalunya (IEEC), Carrer Gran Capita 2, Barcelona, E-08034, Spain E-mail: [email protected] A. Weiss Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany C. Aerts Institute of Astronomy, Department of Physics & Astronomy, KU Leuven, Celestijnenlaan 200 D, 3001 Leuven, Belgium and Department of Astrophysics, IMAPP, Radboud University Nijmegen, Heyendaalseweg 135, 6525 AJ Nijmegen, the Netherlands G.C. Angelou Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany D. Baroch J. C. Morales I. Ribas Institute of· Space Sciences· (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E-08193, arXiv:2006.10868v2 [astro-ph.SR] 9 Apr 2021 Spain and Institut d'Estudis Espacials de Catalunya (IEEC), C/Gran Capit`a2-4, E-08034 2 Serenelli, Weiss, Aerts et al.