Scientific Colonialism in Indigenous Spaces: a Case Study in Hawai´I
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Music and Identity Ofthe Cultural Renaissance of Hawai·I A
-022.\ CONNECT BACK TO DIS PIACE: Music and Identity ofthe Cultural Renaissance ofHawai·i A '!HESIS SUBMITTED TO '!HE GRADUATE DIVISION OF '!HE UNIVERSI1Y OF HAWAI·I IN PARTIAL FULFILLMENT OF '!HE REQUIREMENTS FOR '!HE DEGREE OF MASTER OF ARTS IN PACIFIC ISLAND STUDIES MAY 2005 By Andrea A Suzuki Thesis Conunittee: Kater1na Teaiwa. Chairperson George Teny Kanalu Young Jonathan K. 050110 Acknowledgements First and foremost I have to thank my parents. especIally Daddy MIke for the opJX>rtun1ties that they have gtven me and their sUpJX>rt gtven to my endeavors. I have to also thank Daddy Mitch for hIs sUPJX>rt and h1s stortes about "h1s days". I want to especIally thank my mom, an AM.A 1n her own rtght, for all ofher devoted time and sUPJX>rt. Secondly, I would l1ke to gIve my deepest thanks to Mel1nda Caroll wIthout whom th1s jOurney would have been a lot more d1ff1cult. Thankyou for your suggestions, your help, and your encouragement. I would also l1ke to thank my comm11tee, Katertna Tea1Wa, Kanalu Young, and John Osorto for their sUpJX>rt and theIr efforts 1n the completion ofth1s project. I'd l1ke to thank all ofthose that gave their time to me, tell1ng me their stortes. and allowtng me to share those stortes: Jeny Santos, Owana Salazar, Aunty CookIe, Uncle Cyr11. Hemy KapollO, John Demello. Gaylord Holomal1a, Keaum1k1 Akut. Peter Moon, and Joe Atpa. I'd l1ke to gIve my appreciation to the Pac1ftc Island StudIes Program that guIded me every' step ofthe way. F1nallly. I'd 11ke to thank all my frIends for their encouragement and tolerance ofmy 1nsan1ty, espec1ally Kamuela Andrade, for gJ.1nn1ng and beartng It and Kau1 for beIng my personal cheering section. -
University of Hawaii Telescopes at Mauna Kea Observatory
UNIVERSITY OF HAWAII TELESCOPES AT MAUNA KEA OBSERVATORY USER MANUAL Fourth Edition, April 1996 Last modi®ed, June 1997 Contents 1 INTRODUCTION 1 1.1 General : ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 1 1.2 About this Manual :: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 1 1.3 Observing TimeÐPolicy and Procedures : :::: ::: :::: ::: :::: ::: :::: ::: :::: : 1 1.3.1 Students and Assistants :: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 3 1.3.2 Information before Arrival : ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 3 1.3.3 Colloquia :: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 3 1.3.4 Reports to the Director ::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 3 1.3.5 Publications and Acknowledgments ::: ::: :::: ::: :::: ::: :::: ::: :::: : 3 1.4 Newsletter :: :::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 4 1.5 Information for Visiting Observers : ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 4 1.5.1 Transportation from Hilo to Hale Pohaku and Mauna Kea Observatory :: :::: ::: :::: : 4 1.6 AccommodationÐThe Mid-level Facility, Hale Pohaku :::: ::: :::: ::: :::: ::: :::: : 8 1.6.1 Telephone Service : :::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 8 1.6.2 Mail Service : ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 8 1.6.3 Library :::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 8 2 VISITING OBSERVER EQUIPMENT 11 2.1 Packing Goods for Shipping :::: ::: :::: ::: :::: ::: :::: ::: :::: ::: :::: : 11 2.2 Transport ::: :::: ::: :::: ::: :::: ::: -
In Honolulu's Christ Church in Kailua, Which Will Repeat Next Hemenway Theatre, UH Manoa Campus: Wed
5 The Fear Factor 8 Pritchett !ICalendar 13 Book Bonanza l!IStraight Dope Volume 3, Number 45, November 10, 1993 FREE Interview by JOHN WYTHE WHITE State Representative DaveHagino has spent 15 years fighting the system he's a partof- and theparty he belongs to. !JiORDERS BOOKS & MUSIC· BORDERS BOOKS & MUSIC· BORDERS BOOKS & MUSIC· BORDERS BOOKS & MUSIC· BORDERS BOOKS & MUSIC· BORDERS BOOKS & MUSIC· BORDERS BOOKS 8 ,,,, :,..: ;o 0 0 � �L � w ffi 8 Cl 0 ;,<; 0::: w 0 il,1.. � SELECTION: w 2 No Comparison 00 Cl 0::: i0 co co 0 ;o 0 -- -- co�:. 0 0 7' $�··· C nw oco ;o· · 0 m � co 0 0 w7' ::c: :::: C w 0:co 0 ;o 0 m � co 0 0 ci: � $ C w Borders® Books &Music. n ;o8 0 m The whole idea behind Finda book or music store the new Borders Books w;o co .- Borders Books & Music is to &Music. 0 with more titles and 0 w7' create an appealing place with Welcome to the new � $ we'll shop there. C more selection. So we brought Borders Books &Music. w () 100,000 in over book titles, more times the average store. Borders co 0 than 5 times the average bookstore. especially excels in classical and ;o It 0 CD m .r::;"' � OJ ;o What that means is that Borders jazz recordings. 0 E w (.) "' i co .r::; 'l' CD I 0 E 0 offersmore history, more com Borders also carries the area's (!) 0 """' 7' H-1 Fwy. w puters, more cooking. More of broadest selection of videotapes, � Waikele/Waipahu Exit 7 ::::: C everything, not just more copies including classic and foreign films. -
Effective Aperture 3.6–4.9 M) 4.7 M 186″ Segmented, MMT (6×1.8 M) F
Effective Effective Mirror type Name Site Built aperture aperture (m) (in) 10.4 m 409″ Segmented, Gran Telescopio Roque de los Muchachos 2006/9 36 Canarias (GTC) Obs., Canary Islands, Spain 10 m 394″ Segmented, Keck 1 Mauna Kea Observatories, 1993 36 Hawaii, USA 10 m 394″ Segmented, Keck 2 Mauna Kea Observatories, 1996 36 Hawaii, USA 9.8 m 386″ Segmented, Southern African South African Astronomical 2005 91 Large Telescope Obs., Northern Cape, South (SALT) Africa 9.2 m 362″ Segmented, Hobby-Eberly McDonald Observatory, 1997 91 Telescope (HET) Texas, USA (11 m × 9.8 m mirror) 8.4 m×2 330″×2 Multiple Large Binocular Mount Graham 2004 (can use mirror, 2 Telescope (LBT) Internationals Obs., Phased- Arizona array optics for combined 11.9 m[2]) 8.2 m 323″ Single Subaru (JNLT) Mauna Kea Observatories, 1999 Hawaii, USA 8.2 m 323″ Single VLT UT1 (Antu) Paranal Observatory, 1998 Antofagasta Region, Chile 8.2 m 323″ Single VLT UT2 (Kueyen) Paranal Observatory, 1999 Antofagasta Region, Chile 8.2 m 323″ Single VLT UT3 (Melipal) Paranal Observatory, 2000 Antofagasta Region, Chile 8.2 m 323″ Single VLT UT4 (Yepun) Paranal Observatory, 2001 Antofagasta Region, Chile 8.1 m 318″ Single Gemini North Mauna Kea Observatories, 1999 (Gillett) Hawaii, USA 8.1 m 318″ Single Gemini South Cerro Pachón (CTIO), 2001 Coquimbo Region, Chile 6.5 m 256″ Honeycomb Magellan 1 Las Campanas Obs., 2000 (Walter Baade) Coquimbo Region, Chile 6.5 m 256″ Honeycomb Magellan 2 Las Campanas Obs., 2002 (Landon Clay) Coquimbo Region, Chile 6.5 m 256″ Single MMT (1 x 6.5 M1) F. -
Arxiv:2009.11049V2 [Astro-Ph.IM] 24 Sep 2020
Research in Astronomy and Astrophysics manuscript no. (LATEX: ms2020-0197.tex; printed on September 25, 2020; 1:02) The estimate of sensitivity for large infrared telescopes based on measured sky brightness and atmospheric extinction Zhi-Jun Zhao1,4, Hai-Jing Zhou1, Yu-Chen Zhang2, Yun Ling3 and Fang-Yu Xu∗2 1 School of Physics, Henan Normal University,Xinxiang 453007, China; xu [email protected]; [email protected] 2 Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China; 3 Kunming Institute of Physics, Kunming 650216, China; 4 Henan Key Laboratory of Infrared Materials & Spectrum Measures and Applications, Xinxiang 453007, China Received 20xx month day; accepted 20xx month day Abstract : In order to evaluate the ground-based infrared telescope sensitivity affected by the noise from the atmosphere, instruments and detectors, we construct a sensitivity model that can calculate limiting magnitudes and signal-to-noise ratio (S/N). The model is tested with tentative measurements of M′-band sky brightness and atmospheric extinction obtained at the Ali and Daocheng sites. We find that the noise caused by an excellent scientific detector and instruments at 135◦C can be ignored compared to the M′-band sky background noise. − Thus, when S/N =3 and total exposure time is 1 second for 10 m telescopes, the magnitude limited by the atmosphere is 13.01m at Ali and 12.96m at Daocheng. Even under less-than- − arXiv:2009.11049v2 [astro-ph.IM] 24 Sep 2020 ideal circumstances, i.e., the readout noise of a deep cryogenic detector is less than 200e and the instruments are cooled to below 87.2◦C, the above magnitudes decrease by 0.056m − at most. -
Minutes Regular Meeting Mauna Kea Management Board Wednesday
University of Hawai‘i at Hilo 640 N. A‘ohoku Place, Room 203, Hilo, Hawai‘i 96720 Telephone: (808) 933-0734 Fax: (808) 933-3208 Mailing Address: 200 W. Kawili Street, Hilo, Hawai‘i 96720 Minutes Regular Meeting Mauna Kea Management Board Wednesday, May 19, 2010 ʻImiloa Astronomy Center Moana Hoku Hall 600 ʻImiloa Place Hilo, Hawaii 96720 Attending MKMB: Chair Barry Taniguchi, 2nd Vice Chair/Secretary Ron Terry, John Cross, Lisa Hadway, Herring Kalua, and Christian Veillet BOR: Dennis Hirota and Eric Martinson Kahu Kū Mauna: Ed Stevens OMKM: Stephanie Nagata and Dawn Pamarang Others: Robert Albarson, Jim Albertini, Laura Aquino, Dean Au, Madeline Balo-Keawe, Sean Bassle- Kukonu, David Byrne, Rob Christensen, Gregory Chun, Nan Chun, Vaughn Cook, Sandra Dawson, Donn delaCruz, Gerald DeMello, Richard Dods, Suzanne Frayser, Paul Gillett, MRC Greenwood, Richard Ha, Katherine Hall, Cory Harden, Inge Heyer, Clyde Higashi, Nelson Ho, Arthur Hoke, Jacqui Hoover, Stewart Hunter, Stew Hussey, Leslie Isemoto, Mark Ishii, Paul Kagawa, Mike Kaleikini, Ka’iu Kimura, Kyle Kinoshita, Ron Koehler, Randy Kurohara, Susan Law, Tim Law, Karina Leasure, Jonathan Lee, Pete Lindsey, George Martin, Tani Matsubara, Jeff Melrose, Jon Miyata, Delbert Nishimoto, Eugene Nishimura, James Nixon, Cynthia Nomura, Alton Nosaka, Derek Oshita, Tom Peek, Koa Rice, Helen Rogers, Skylark Rossetti, Gary Sanders, Ian Sandison, Bill Stormont, Leonard Tanaka, Rose Tseng, Ross Watson II, Josh Williams, Ross Wilson, Greg Wines, Harry Yada, Mason Yamaki, Miles Yoshioka I. CALL TO ORDER Chair Taniguchi called the meeting of the Mauna Kea Management Board (MKMB) to order at 9:03 a.m. II. APPROVAL OF MINUTES Upon motion by Herring Kalua and seconded by Ron Terry the minutes of the April 21, 2010 meeting of the MKMB were unanimously approved. -
The International Gemini Telescopes Project Has Made Giant Steps Forward, Despite Having Undergone Considerable Reassessment
THETHE GEMINIGEMINIINTERNATIONALINTERNATIONAL AnnualAnnual TELESCOPESTELESCOPES ReportReport 19951995 United States United Kingdom Canada Chile Brazil Argentina The photographs above show the first primary mirror at the Corning plant at Canton, NY, at the completion ceremony in October 1995, and the mirror being loaded onto a barge at Odgensburg Port on the St. Lawrence Seaway in December 1995, en route to the REOSC polishing plant in France. The cover photographs show (above) the Gemini site at Mauna Kea in October 1995 with the University of Hawaii telescope in the background, and (below) at Cerro Pachón in December 1995. Photograph credits: Susan Kayser, the International Gemini Project Office The Annual Report for 1995 was prepared by the National Science Foundation, the Executive Agency for the International Gemini 8-Meter Telescopes Project. Gemini Project Annual Report 1995 Message from the Gemini Board ...................................................................................................................... ii Introduction .......................................................................................................................................................... 1 Schedule............................................................................................................................................................. 1 Organization ......................................................................................................................................................... 3 The Gemini -
Ka Wai Ola O OHA – the Living Water of OHA Iulai (July) 2003
Vol. 20, No. 07 Ka Wai Ola o OHA – The Living Water of OHA Iulai (July) 2003 OHA refocuses nationhood campaign Arakaki plaintiffs’ in light of recognition bill amendments attorney Hanifin dies; hearing By Derek Ferrar rescheduled esponding to recent amend- By Naomi Sodetani ments to the U.S. Senate bill Rseeking federal recognition for June 16 hearing on native Hawaiians, OHA has refocused motions submitted in the the timeline of its own campaign to AArakaki v. Lingle case has facilitate Hawaiian self-governance, been rescheduled because of the known as Ho‘oulu Lähui Aloha, or “To sudden death of one of the plain- Raise a Beloved Nation.” tiffs’ attorneys. In early May, OHA’s Trustees, Patrick Hanifin, 48, suffered a together with a variety of Hawaiian heart attack on June 13 and died community groups, announced the the following day. process of public discussion and par- Federal Judge Susan Oki ticipation leading to a community- Mollway has rescheduled the based ‘aha, or gathering of delegates, hearing to Sept. 8. which would frame the founding docu- The three-month delay means ments of a governing entity to repre- the case could be affected by the sent the Hawaiian people. OHA’s outcome of the Hawaiian Board has several times affirmed its Recognition Bill. The bill is pend- view that federal recognition and the ing before the U.S. Senate, and formation of a Hawaiian governing OHA Trustee Boyd Mossman and Sen. Daniel Akaka during the trustees’ recent visit to action could be taken on it before body are the best ways to defend Washington, D.C., to lobby in favor of the Akaka-sponsored Hawaiian Recognition Bill. -
The Mauna Kea Observatories Near-Infrared Filter Set. II. Specifications for a New JHKL!
Publications of the Astronomical Society of the Pacific, 114:180–186, 2002 February ᭧ 2002. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A. The Mauna Kea Observatories Near-Infrared Filter Set. II. Specifications for a New JHKLЈMЈ Filter Set for Infrared Astronomy A. T. Tokunaga Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822; [email protected] D. A. Simons Gemini Observatory, Northern Operations Center, 670 North A‘ohoku Place, Hilo, HI 96720; [email protected] and W. D. Vacca Max-Planck-Institut fu¨r extraterrestrische Physik, Postfach 1312, D-85741 Garching, Germany; [email protected] Received 2001 July 28; accepted 2001 October 17 ABSTRACT. We present a description of a new 1–5 mm filter set similar to the long-used JHKLM filter set derived from that of Johnson. The new Mauna Kea Observatories Near-Infrared filter set is designed to reduce background noise, improve photometric transformations from observatory to observatory, provide greater accuracy in extrapolating to zero air mass, and reduce the color dependence in the extinction coefficient in photometric reductions. We have also taken into account the requirements of adaptive optics in setting the flatness specification of the filters. A complete technical description is presented to facilitate the production of similar filters in the future. 1. INTRODUCTION baru Telescopes, all of the optical/infrared observatories at Mauna Kea are currently using these filters (NASA Infrared The rationale for a new set of infrared filters was presented Telescope Facility, United Kingdom Infrared Telescope, Canada- by Simons & Tokunaga (2002, hereafter Paper I). -
Mauna Kea Public Access Plan January 2010
PUBLIC ACCESS PLAN FOR THE UH MANAGEMENT AREAS ON MAUNA KEA A Sub-Plan of the Mauna Kea Comprehensive Management Plan January 2010 Prepared for: Office of Mauna Kea Management University of Hawai‘i-Hilo 200 W. Kawili Street Hilo, Hawaii 96720 Prepared by: Sustainable Resources Group Intn’l, Inc. Island Planning Island Transitions, LLC 111 Hekili Street, Suite A373 1405 Waianuenue Avenue P.O. Box 202 Kailua, HI 96734 Hilo, HI 96720 Pa‘auilo, HI 96776 Acknowledgements The Public Access Plan was funded by the Office of Mauna Kea Management (OMKM). Interim Director Stephanie Nagata was instrumental in setting up and overseeing all aspects of the contract with Sustainable Resources Group Intn’l Inc (SRGII). She provided critical reviews of plan drafts and insight to the operational history and current policies that have shaped activities in the UH Management Areas on Mauna Kea over the years. Ms. Nagata and her assistant, Dawn Pamarang, were of great assistance throughout the project. Special appreciation is due to several groups and individuals. Members of Kahu Kū Mauna generously contributed their time as a group and in subcommittee and roundtable discussions to assist in this planning process. David Byrne, Visitor Information Station (VIS) Supervisor, was readily available and enabled his staff to meet with the planners, resulting in better understanding of the ranger program, daily operations at the VIS and appreciation of how the current management of public use on the mountain has evolved over the years. The Mauna Kea Rangers, both past and present, shared quality data, observations, suggestions and concerns that can only come from daily interactions with the public on Mauna Kea. -
Big Glass and the Age of New Astronomy | Space | Air & Spac
Big Glass and the Age of New Astronomy | Space | Air & Spac... http://www.airspacemag.com/space/big-astronomy-how-built-1... AirSpaceMag.com Big Glass and the Age of New Astronomy The fight to put a monster telescope on Mauna Kea is part of a bigger war looming among astronomers. By Dennis Hollier Air & Space Magazine | Subscribe September 2016 The tallest island mountain in the world is Hawaii’s Mauna Kea, where the thin atmosphere and absence of light pollution create some of the best observing conditions for astronomers. At the summit, 13 telescopes sit along a ridge of formations that have built up around volcanic vents. The oldest telescope on site, and still the smallest, is the University of Hawaii’s 2.2-meter (7.2-foot) UH88, built in 1968. Mauna Kea is best known as the home of the twin 10-meter Keck telescopes, which saw first light in the 1990s and remain two of the largest optical and infrared telescopes in the world. Collectively, this baker’s dozen of observatories has dominated ground-based astronomy for four decades. But recently, Mauna Kea has become embroiled in a dispute that could radically alter the future of astronomy, and serve as a cautionary example of what we might lose if it keeps going down this path. In 2009, Mauna Kea was chosen as the site for the Thirty Meter Telescope, a mega-observatory proposed by the California Institute of Technology, the University of California, and national science agencies in Japan, Canada, India, and China. Its massive mirror will be made from 492 segments and have 81 times the sensitivity of the Keck telescopes. -
The Fight for Mauna Kea," Spectrum: Vol
Recommended Citation Coleman, Audrey (2020) "The Fight for Mauna Kea," Spectrum: Vol. 9 : Iss. 1 , Article 9. Available at: https://scholars.unh.edu/spectrum/vol9/iss1/9 This Article is brought to you for free and open access by the Student Journals and Publications at University of New Hampshire Scholars' Repository. It has been accepted for inclusion in Spectrum by an authorized editor of University of New Hampshire Scholars' Repository. For more information, please contact [email protected]. Spectrum Volume 9 Issue 1 Spectrum 2020 Article 9 6-2-2020 The Fight for Mauna Kea Audrey Coleman [email protected] Follow this and additional works at: https://scholars.unh.edu/spectrum Coleman: The Fight for Mauna Kea Audrey Coleman The Fight for Mauna Kea Question: Should the Thirty Meter Telescope (TMT) be built on Mauna Kea? Methods: I am an astrophysics major, and as such follow several astrophysicists on social media. I read through many of the articles they posted, positive or negative. I also sought out native Hawaiian voices, particularly in relation to the ways in which Mauna Kea is sacred. This led me to several published papers on native Hawaiian traditions regarding Mauna Kea. For the accompanying drawing I used artwork depicting the volcano goddess Pele as references. I also referenced several pictures of the summit of Mauna Kea to get a better idea of how to draw the mountain. Introduction: Mauna Kea, often translated as “White Mountain”, is the tallest mountain on the Big Island and is currently stewarded by the University of Hawaii (Institute for Astronomy: University of Hawaii, n.d.).