Sr No DIPP No Entity Name 1 DIPP17 Vizortex R&D Pvt. Ltd 2 DIPP10 AUM PROJECT ENGINEERS PRIVATE LIMITED 3 DIPP15 BIOMATIQUES
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Crowdfunding in Asia
Crowdfunding in Asia May 2018 Introducing the first free directory of crowdfunding platforms across Asia. The data is based on the AlliedCrowds Capital Finder, a database of over 7,000 alternative finance capital providers across emerging markets. Our data has been used by organizations like FSD Asia, UNDP, World Green Economy Organization, GIZ, World Bank, and others in order to provide unique, actionable insights into the world of emerging market alternative finance. This is the latest of our regular reports on alternative finance in emerging markets; you can find all previous reports here. Crowdfunding rose in prominence in the post-financial crisis years (starting in 2012), and for good reason: a global credit crunch limited the amount of funding available to entrepreneurs and small businesses. Since then, crowdfunding has grown rapidly around the world. Crowdfunding is especially consequential in countries where SMEs find it difficult to raise capital to start or grow their businesses. This is the case in many Asian countries; according to the SME Finance Forum, there is a $2.3 trillion MSME credit gap in East Asia and the Pacific. Crowdfunding can help to fill this gap by offering individuals and small businesses an alternative source of capital. This can come in the form of donation-based as well as lending-based (peer-to-peer or peer-to-business) crowdfunding. In order to help entrepreneurs and small business owners to find the crowdfunding platform that’s right for them, we are releasing the first publicly available list of all crowdfunding platforms across Asia. The report is split into two key sections: the first one is an overview of crowdfunding platforms, and how active they are across the largest markets on the continent. -
A 21St Century Powerhouse Dick Forsberg Head of Strategy, Avolon
An in-depth analysis of the Indian air travel market Dick Forsberg | July 2018India A 21st Century Powerhouse Dick Forsberg Head of Strategy, Avolon ACKNOWLEDGEMENTS The author would like to acknowledge FlightGlobal Ascend as the source of the fleet data and OAG, through their Traffic Analyser and Schedules Analyser products, as the source of the airline traffic and capacity data used in this paper. DISCLAIMER This document and any other materials contained in or accompanying this document (collectively, the ‘Materials’) are provided for general information purposes only. The Materials are provided without any guarantee, condition, representation or warranty (express or implied) as to their adequacy, correctness or completeness. Any opinions, estimates, commentary or conclusions contained in the Materials represent the judgement of Avolon as at the date of the Materials and are subject to change without notice. The Materials are not intended to amount to advice on which any reliance should be placed and Avolon disclaims all liability and responsibility arising from any reliance placed on the Materials. Dick Forsberg has over 45 years’ aviation industry experience, working in a variety of roles with airlines, operating lessors, arrangers and capital providers in the disciplines of business strategy, industry analysis and forecasting, asset valuation, portfolio risk management and airline credit assessment. As a founding executive and Head of Strategy at Avolon, his responsibilities include defining the trading cycle of the business, primary interface with the aircraft appraisal and valuation community, industry analysis and forecasting, driving thought leadership initiatives, setting portfolio risk management criteria and determining capital allocation targets. Prior to Avolon, Dick was a founding executive at RBS (now SMBC) Aviation Capital and previously worked with IAMG, GECAS and GPA following a 20-year career in the UK airline industry. -
The Performance of Domestic Airlines for the Year 2016
Subject: Performance of domestic airlines for the year 2016. Traffic data submitted by various domestic airlines has been analysed for the month of September 2016. Following are the salient features: Passenger Growth Passengers carried by domestic airlines during Jan-Sept 2016 were 726.98 lakhs as against 590.21 lakhs during the corresponding period of previous year thereby registering a growth of 23.17 % (Ref Table 1). 800.00 726.98 Growth: YoY = + 23.17 % MoM = + 23.46% 700.00 8 % 590.21 600.00 500.00 400.00 2015 2016 300.00 200.00 Pax Lakhs) Carried(in Pax 82.30 100.00 66.66 0.00 YoY MoM Passenger Load Factor The passenger load factors of various scheduled domestic airlines in Sept 2016 are as follows (Ref Table 2): 100.0 93.2 93.5 89.4 90.0 86.0 83.3 82.8 82.1 82.1 81.7 79.9 79.0 78.9 77.7 77.7 77.5 75.6 80.0 73.72 72.7 70.8 69.2 65.57 70.0 64.48 60.0 50.0 40.0 30.0 Pax Pax FactorLoad (%) 20.0 10.0 0 0.0 0.0 Air Jet JetLite Spicejet Go Air IndiGo Air Air Asia Vistara Air Trujet Air India Airways Costa Pegasus Carnival Aug-16 Sep-16 1 The passenger load factor in the month of Sept 2016 has almost remained constant compared to previous month primarily due to the end of tourist season. Cancellations The overall cancellation rate of scheduled domestic airlines for the month of Sept 2016 has been 0.42 %. -
69-22,173 MARKOWITZ, Allan Henry, 1941- a STUDY of STARS
This dissertation has been microfilmed exactly u received 6 9 -2 2 ,1 7 3 MARKOWITZ, Allan Henry, 1941- A STUDY OF STARS EXHIBITING COM POSITE SPECTRA. The Ohio State University, Ph.D., 1969 A stron om y University Microfilms, Inc., Ann Arbor, Michigan A STUDY OF STARS EXHIBITING COMPOSITE SPECTRA DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Allan Henry Markowitz, A.B., M.Sc. ******** The Ohio S ta te U n iv e rsity 1969 Approved by UjiIjl- A dviser Department of Astronomy ACKNOWLEDGMENTS It is a sincere pleasure to thank my adviser, Professor Arne Slettebak, who originally suggested this problem and whose advice and encouragement were indispensable throughout the course of the research. I am also greatly indebted to Professor Philip Keenan for help in classifying certain late-type spectra and to Professor Terry Roark for instructing me in the operation of the Perkins Observatory telescope, I owe a special debt of gratitude to Dr. Carlos Jaschek of the La Plata Observatory for his inspiration, advice, and encourage ment. The Lowell Observatory was generous in providing extra telescope time when the need arose. I wish to particularly thank Dr. John Hall for this and for his interest. I also gratefully acknowledge the assistance of the Perkins Observatory staff. To my wife, Joan, I owe my profound thanks for her devotion and support during the seemingly unending tenure as a student. I am deeply grateful to my mother for her eternal confidence and to my in-laws for their encouragement. -
Abd Al-Rahman Al-Sufi and His Book of the Fixed Stars: a Journey of Re-Discovery
ResearchOnline@JCU This file is part of the following reference: Hafez, Ihsan (2010) Abd al-Rahman al-Sufi and his book of the fixed stars: a journey of re-discovery. PhD thesis, James Cook University. Access to this file is available from: http://eprints.jcu.edu.au/28854/ The author has certified to JCU that they have made a reasonable effort to gain permission and acknowledge the owner of any third party copyright material included in this document. If you believe that this is not the case, please contact [email protected] and quote http://eprints.jcu.edu.au/28854/ 5.1 Extant Manuscripts of al-Ṣūfī’s Book Al-Ṣūfī’s ‘Book of the Fixed Stars’ dating from around A.D. 964, is one of the most important medieval Arabic treatises on astronomy. This major work contains an extensive star catalogue, which lists star co-ordinates and magnitude estimates, as well as detailed star charts. Other topics include descriptions of nebulae and Arabic folk astronomy. As I mentioned before, al-Ṣūfī’s work was first translated into Persian by al-Ṭūsī. It was also translated into Spanish in the 13th century during the reign of King Alfonso X. The introductory chapter of al-Ṣūfī’s work was first translated into French by J.J.A. Caussin de Parceval in 1831. However in 1874 it was entirely translated into French again by Hans Karl Frederik Schjellerup, whose work became the main reference used by most modern astronomical historians. In 1956 al-Ṣūfī’s Book of the fixed stars was printed in its original Arabic language in Hyderabad (India) by Dārat al-Ma‘aref al-‘Uthmānīa. -
Exep Science Plan Appendix (SPA) (This Document)
ExEP Science Plan, Rev A JPL D: 1735632 Release Date: February 15, 2019 Page 1 of 61 Created By: David A. Breda Date Program TDEM System Engineer Exoplanet Exploration Program NASA/Jet Propulsion Laboratory California Institute of Technology Dr. Nick Siegler Date Program Chief Technologist Exoplanet Exploration Program NASA/Jet Propulsion Laboratory California Institute of Technology Concurred By: Dr. Gary Blackwood Date Program Manager Exoplanet Exploration Program NASA/Jet Propulsion Laboratory California Institute of Technology EXOPDr.LANET Douglas Hudgins E XPLORATION PROGRAMDate Program Scientist Exoplanet Exploration Program ScienceScience Plan Mission DirectorateAppendix NASA Headquarters Karl Stapelfeldt, Program Chief Scientist Eric Mamajek, Deputy Program Chief Scientist Exoplanet Exploration Program JPL CL#19-0790 JPL Document No: 1735632 ExEP Science Plan, Rev A JPL D: 1735632 Release Date: February 15, 2019 Page 2 of 61 Approved by: Dr. Gary Blackwood Date Program Manager, Exoplanet Exploration Program Office NASA/Jet Propulsion Laboratory Dr. Douglas Hudgins Date Program Scientist Exoplanet Exploration Program Science Mission Directorate NASA Headquarters Created by: Dr. Karl Stapelfeldt Chief Program Scientist Exoplanet Exploration Program Office NASA/Jet Propulsion Laboratory California Institute of Technology Dr. Eric Mamajek Deputy Program Chief Scientist Exoplanet Exploration Program Office NASA/Jet Propulsion Laboratory California Institute of Technology This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. © 2018 California Institute of Technology. Government sponsorship acknowledged. Exoplanet Exploration Program JPL CL#19-0790 ExEP Science Plan, Rev A JPL D: 1735632 Release Date: February 15, 2019 Page 3 of 61 Table of Contents 1. -
Charitable Crowdfunding: Who Gives, to What, and Why?
APRIL 2021 Charitable Crowdfunding: Who Gives, to What, and Why? RESEARCHED AND WRITTEN BY Indiana University Lilly Family School of Philanthropy RESEARCHED AND WRITTEN BY — Indiana University Lilly Family School of Philanthropy The Indiana University Lilly Family School of Philanthropy is dedicated to improving philanthropy to improve the world by training and empowering students and professionals to be innovators and leaders who create positive and lasting change. The school offers a comprehensive approach to philanthropy through its academic, research and international programs, and through The Fund Raising School, Lake Institute on Faith & Giving, Mays Family Institute on Diverse Philanthropy, and Women’s Philanthropy Institute. Learn more at www.philanthropy.iupui.edu INDIANA UNIVERSITY LILLY FAMILY SCHOOL OF PHILANTHROPY PROJECT TEAM — Una O. Osili, PhD Associate Dean for Research and International Programs Jonathan Bergdoll, MA Applied Statistician Andrea Pactor, MA Project Consultant Jacqueline Ackerman, MPA Associate Director of Research, Women’s Philanthropy Institute Peter Houston, MBA Visiting Research Associate With special thanks to Dr. Wendy Chen, Dr. Debra Mesch, and Dr. Pamala Wiepking for reviewing the survey questionnaire. The survey was fielded by AmeriSpeak at NORC. The report was designed by Luke Galambos at Galambos + Associates. This research was completed with funding from Facebook. The findings and conclusions contained within are those of the authors and do not necessarily reflect official positions or policies of Facebook. INDIANA UNIVERSITY LILLY FAMILY SCHOOL OF PHILANTHROPY — 301 University Boulevard, Suite 3000, Indianapolis, IN 46202 317.278.8902 / [email protected] / @IUPhilanthropy / www.philanthropy.iupui.edu Contents Introduction ................................................... 02 Key Findings ................................................. 02 Background ................................................... 05 What is Crowdfunding? ...................................... -
Open Batalha-Dissertation.Pdf
The Pennsylvania State University The Graduate School Eberly College of Science A SYNERGISTIC APPROACH TO INTERPRETING PLANETARY ATMOSPHERES A Dissertation in Astronomy and Astrophysics by Natasha E. Batalha © 2017 Natasha E. Batalha Submitted in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy August 2017 The dissertation of Natasha E. Batalha was reviewed and approved∗ by the following: Steinn Sigurdsson Professor of Astronomy and Astrophysics Dissertation Co-Advisor, Co-Chair of Committee James Kasting Professor of Geosciences Dissertation Co-Advisor, Co-Chair of Committee Jason Wright Professor of Astronomy and Astrophysics Eric Ford Professor of Astronomy and Astrophysics Chris Forest Professor of Meteorology Avi Mandell NASA Goddard Space Flight Center, Research Scientist Special Signatory Michael Eracleous Professor of Astronomy and Astrophysics Graduate Program Chair ∗Signatures are on file in the Graduate School. ii Abstract We will soon have the technological capability to measure the atmospheric compo- sition of temperate Earth-sized planets orbiting nearby stars. Interpreting these atmospheric signals poses a new challenge to planetary science. In contrast to jovian-like atmospheres, whose bulk compositions consist of hydrogen and helium, terrestrial planet atmospheres are likely comprised of high mean molecular weight secondary atmospheres, which have gone through a high degree of evolution. For example, present-day Mars has a frozen surface with a thin tenuous atmosphere, but 4 billion years ago it may have been warmed by a thick greenhouse atmosphere. Several processes contribute to a planet’s atmospheric evolution: stellar evolution, geological processes, atmospheric escape, biology, etc. Each of these individual processes affects the planetary system as a whole and therefore they all must be considered in the modeling of terrestrial planets. -
E-Register: November, 2019
E-Register: November, 2019 S. No. Diary No. RoC No. Date Title of Work Category Applicant 1 14316/2019-CO/L L-86607/2019 01/11/2019 Design of five busbar half Literary/ BHARAT HEAVY ELECTRICALS LIMITED cut metallization pattern Dramatic 2 14319/2019-CO/L L-86608/2019 01/11/2019 Designfor mono of crystallinefive busbar silicon half Literary/ BHARAT HEAVY ELECTRICALS LIMITED cut metallization pattern Dramatic for multi crystalline silicon 3 13525/2019-CO/L L-86609/2019 01/11/2019 JIBANKRISHNERsolar cells GAAN Literary/ MR. JIBAN KRISHNA MAJUMDAR Dramatic 4 14150/2019-CO/L L-86610/2019 01/11/2019 TEM CHATA...! Literary/ Nitin Kava Dramatic 5 13804/2019-CO/L L-86611/2019 01/11/2019 2000 (Script) Literary/ Ajaykumar S. Parasu Dramatic 6 13757/2019-CO/L L-86612/2019 01/11/2019 TUZYAVINA Literary/ MS. SHRINIDHI GHATATE Dramatic 7 13842/2019-CO/SW SW-12939/2019 01/11/2019 INSURANCE CLAIM Computer Transasia Soft Tech Private Limited ANALYTICS Software 8 13480/2019-CO/L L-86613/2019 01/11/2019 dusri galti Literary/ Anand kumar Dramatic 9 13410/2019-CO/L L-86614/2019 01/11/2019 Class X- Unleashing Literary/ EDUCATION QUALITY FOUNDATION OF Aptitudes With Biology Dramatic INDIA 10 13615/2019-CO/L L-86615/2019 01/11/2019 BRUSH LETTERING BASICS Literary/ SURBHI ARORA Dramatic 11 13368/2019-CO/SW SW-12940/2019 01/11/2019 Edutrack Computer DIPTE RANJAN Software 12 13652/2019-CO/SW SW-12941/2019 01/11/2019 KisaanSe Computer Siddharth Sudhakar Software 13 13393/2019-CO/L L-86616/2019 01/11/2019 SOLAR PANEL CLEANING Literary/ VAIBHAV A PATANKAR MECHANISM Dramatic 14 11512/2019-CO/L L-86617/2019 01/11/2019 Somoy Nei Literary/ Tapan Kumar Ganguli Dramatic 15 14228/2019-CO/L L-86618/2019 01/11/2019 English Literary/ M/s Spectrum Educational Books Dramatic 16 14190/2019-CO/L L-86619/2019 01/11/2019 Engineering Graphics Literary/ M/s Spectrum Publications Dramatic 17 12967/2019-CO/L L-86620/2019 01/11/2019 Dr. -
Mètodes De Detecció I Anàlisi D'exoplanetes
MÈTODES DE DETECCIÓ I ANÀLISI D’EXOPLANETES Rubén Soussé Villa 2n de Batxillerat Tutora: Dolors Romero IES XXV Olimpíada 13/1/2011 Mètodes de detecció i anàlisi d’exoplanetes . Índex - Introducció ............................................................................................. 5 [ Marc Teòric ] 1. L’Univers ............................................................................................... 6 1.1 Les estrelles .................................................................................. 6 1.1.1 Vida de les estrelles .............................................................. 7 1.1.2 Classes espectrals .................................................................9 1.1.3 Magnitud ........................................................................... 9 1.2 Sistemes planetaris: El Sistema Solar .............................................. 10 1.2.1 Formació ......................................................................... 11 1.2.2 Planetes .......................................................................... 13 2. Planetes extrasolars ............................................................................ 19 2.1 Denominació .............................................................................. 19 2.2 Història dels exoplanetes .............................................................. 20 2.3 Mètodes per detectar-los i saber-ne les característiques ..................... 26 2.3.1 Oscil·lació Doppler ........................................................... 27 2.3.2 Trànsits -
Effect of Different Stellar Galactic Environments on Planetary Discs I.The Solar Neighbourhood and the Birth Cloud of the Sun
Zurich Open Repository and Archive University of Zurich Main Library Strickhofstrasse 39 CH-8057 Zurich www.zora.uzh.ch Year: 2011 Effect of different stellar galactic environments on planetary discs I.The solar neighbourhood and the birth cloud of the sun Jiménez-Torres, J J ; Pichardo, B ; Lake, G ; Throop, H Abstract: We have computed trajectories, distances and times of closest approaches to the Sun by stars in the solar neighbourhood with known position, radial velocity and proper motions. For this purpose, we have used a full potential model of the Galaxy that reproduces the local z-force, the Oort constants, the local escape velocity and the rotation curve of the Galaxy. From our sample, we constructed initial conditions, within observational uncertainties, with a Monte Carlo scheme for the 12 most suspicious candidates because of their small tangential motion. We find that the star Gliese 710 will have the closest approach to the Sun, with a distance of approximately 0.34 pc in 1.36 Myr in the future. We show that the effect of a flyby with the characteristics of Gliese 710 on a 100 au test particle disc representing the Solar system is negligible. However, since there is a lack of 6D data for a large percentage of stars in the solar neighbourhood, closer approaches may exist. We calculate parameters of passing stars that would cause notable effects on the solar disc. Regarding the birth cloud of the Sun, we performed experiments to reproduce roughly the observed orbital parameters such as eccentricities and inclinations of the Kuiper belt. -
Atlas Menor Was Objects to Slowly Change Over Time
C h a r t Atlas Charts s O b by j Objects e c t Constellation s Objects by Number 64 Objects by Type 71 Objects by Name 76 Messier Objects 78 Caldwell Objects 81 Orion & Stars by Name 84 Lepus, circa , Brightest Stars 86 1720 , Closest Stars 87 Mythology 88 Bimonthly Sky Charts 92 Meteor Showers 105 Sun, Moon and Planets 106 Observing Considerations 113 Expanded Glossary 115 Th e 88 Constellations, plus 126 Chart Reference BACK PAGE Introduction he night sky was charted by western civilization a few thou - N 1,370 deep sky objects and 360 double stars (two stars—one sands years ago to bring order to the random splatter of stars, often orbits the other) plotted with observing information for T and in the hopes, as a piece of the puzzle, to help “understand” every object. the forces of nature. The stars and their constellations were imbued with N Inclusion of many “famous” celestial objects, even though the beliefs of those times, which have become mythology. they are beyond the reach of a 6 to 8-inch diameter telescope. The oldest known celestial atlas is in the book, Almagest , by N Expanded glossary to define and/or explain terms and Claudius Ptolemy, a Greco-Egyptian with Roman citizenship who lived concepts. in Alexandria from 90 to 160 AD. The Almagest is the earliest surviving astronomical treatise—a 600-page tome. The star charts are in tabular N Black stars on a white background, a preferred format for star form, by constellation, and the locations of the stars are described by charts.