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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 ::: :::: ::: :::: ::: :::: ::: -
Arthropod and Botanical Inventory and Assessment Thirty
ARTHROPOD AND BOTANICAL INVENTORY AND ASSESSMENT THIRTY METER TELESCOPE PROJECT MAUNA KEA SCIENCE RESERVE NORTHERN PLATEAU AND HALE PŌHAKU HĀMĀKUA DISTRICT, ISLAND OF HAWAI‘I May 2009 Prepared for Parsons Brinckerhoff Honolulu, Hawai‘i Pacific Analytics, L.L.C. P.O. Box 1064 Corvallis, Oregon 97339 www.statpros.com Prepared by: Pacific Analytics, L.L.C. Post Office Box 1064 Corvallis, Oregon 97339 Tel. (541) 758-9352 [email protected] www.statpros.com Gregory Brenner Senior Associate / Project Manager The pictures contained in this report are for the exclusive use by Pacific Analytics, L.L.C. and its clients. All photographs are copyrighted by Pacific Analytics, L.L.C. and may not be reproduced or used without the express written permission of Pacific Analytics, L.L.C. TABLE OF CONTENTS 1.0 INTRODUCTION ................................................................................................................4 1.1 TMT Project .........................................................................................................................4 1.2 Physical Setting ....................................................................................................................6 1.3 Current Study .......................................................................................................................7 2.0 METHODS ...........................................................................................................................8 2.1 Permit ...................................................................................................................................8 -
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 Importance of Insect Monitoring to Conservation Actions in Hawaii
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by ScholarSpace at University of Hawai'i at Manoa CProceedingsonservation of relevan the hawaiianCe of inse entomologicalCt monitoring s ociety (2013) 45:149–166 149 The Importance of Insect Monitoring to Conservation Actions in Hawaii Matthew J. Medeiros1, 2*, Jesse A. Eiben3, William P. Haines4, Raina L. Kaholoaa5, Cynthia B.A. King6, Paul D. Krushelnycky4, Karl N. Magnacca7, Daniel Rubinoff4, Forest Starr8, and Kim Starr8 1Urban School of San Francisco, San Francisco, CA 94117. 2University of California, Department of Integrative Biology, Berkeley, CA 94720. 3University of Hawaii at Hilo, College of Agriculture, Forestry and Natural Resource Management, Hilo, HI 96720. 4University of Hawaii at Manoa, Dept. of Plant and Environmental Protection Sciences, Honolulu, HI 96822. 5Haleakala National Park, Makawao, HI 96768. 6Hawaii Division of Forestry and Wildlife Native Invertebrate Program, 1151 Punchbowl Street, Room 325, Honolulu, Hawaii 96813. 7Oahu Army Natural Resources Program, PCSU, Schofield Barracks, HI 96857. 8Starr Environmental, Makawao, HI 96768. *Author to whom correspondence should be addressed: [email protected] Abstract. Endemic insect species make up the overwhelming majority of Hawaii’s native fauna, and play many important ecological roles. Despite this, insects receive low levels of conservation funding, likely due to their small size, fluctuating popula- tion sizes, and lack of baseline data necessary to determine if they are threatened with extinction. To determine which insects are at risk, how insect populations fluctuate in natural areas, and which management actions are most beneficial to Hawaiian ecosystems, we propose that insects be monitored whenever possible. -
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 -
Wekiu Bug Mitigation Report
WĒKIU BUG MITIGATION REPORT Prepared for the Keck Outrigger Telescopes Project Jet Propulsion Laboratory California Institute of Technology Pasadena, California 91109 Pacific Analytics L.L.C. P.O. Box 219 Albany, Oregon 97321 541-926-0117 www.statpros.com Revised November 4, 2000 Prepared by: Pacific Analytics, L.L.C. Post Office Box 219 Albany, Oregon 97321 Tel. (541) 926-0117 [email protected] www.statpros.com _____________________________ Gregory Brenner Managing Partner ₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪ Wēkiu Bug Mitigation Report: Table of Contents ₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪₪ WĒKIU BUG MITIGATION REPORT TABLE OF CONTENTS page I. Executive Summary ............................................................................. 1 II. Introduction .......................................................................................... 2 III. Objectives ............................................................................................. 8 IV. Habitat Restoration and Protection ...................................................... 9 V. Dust Control ......................................................................................... 16 VI. Hazardous Materials Control ............................................................... 19 VII. Trash Control ........................................................................................ 24 VIII. Alien Arthropod Control ...................................................................... 27 IX. Monitoring ........................................................................................... -
First Recorded Hawaiian Occurrence of the Alien Ground Beetle, Agonum Muelleri (Coleoptera: Carabidae), from the Summit of Mauna Kea, Hawaii Island
AProcgonum. H AmuelleriwAiiAn e,ntomol New S.tate Soc .R (2009)ecoRd 41:97–103 97 First Recorded Hawaiian Occurrence of the Alien Ground Beetle, Agonum muelleri (Coleoptera: Carabidae), from the Summit of Mauna Kea, Hawaii Island J. K. Liebherr1, S. L. Montgomery2, R. A. Englund3, and G. A. Samuelson3 1Department of Entomology, Cornell University, Ithaca, NY 14853, USA; 2Montane Matters, 94-610 Palai St., Waipahu, HI 96797, USA; 3Hawaii Biological Survey, Bishop Museum, Honolulu, HI 96817, USA Abstract. Adults of the non-native species, Agonum muelleri (Herbst) (Coleoptera: Carabidae) were collected from the summit of Mauna Kea in 2006 and again dur- ing 2008, indicating that a population of this European species is established on Mauna Kea volcano, Hawaii island (NEW STATE RECORD). Agonum muelleri is a synanthropic species that has been accidentally introduced from Europe to both the east and west coasts of North America, with the known North American distribution including 24 provinces and states of Canada and the United States. Characters for the adults are provided to permit diagnosis of this non-native species from all other native and introduced carabid beetle species known from Hawaii. Recorded environmental conditions from Mauna Kea summit taken during the months when specimens were collected are consistent with conditions associated with winged flight by A. muelleri individuals in the species’ native European range. Hawaii is the geographically most isolated archipelago in the World, with approximately 250 insect colonists (Zimmerman 1948, Liebherr 2001) speciating to result in over 5,200 present-day native endemic insect species (Eldredge and Evenhuis 2003). Among these, the Nysius seed bug (Hemiptera: Lygaeidae) radiation includes two remarkable species known from the mature shield volcanoes Mauna Kea and Mauna Loa; N. -
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.