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The European Southern Observatory Your Talk
The European Southern Observatory Your talk Your name Overview What is astronomy? ESO history What is ESO? La Silla VLT ALMA E-ELT ESO Visitor Centre | 9 October 2013 Why are we here? What is astronomy? And what it all is good for? ESO Visitor Centre | 9 October 2013 What is astronomy? Astronomy is the study of all celestial objects. It is the study of almost every property of the Universe from stars, planets and comets to the largest cosmological structures and phenomena; across the entire electromagnetic spectrum and more. It is the study of all that has been, all there is and all that there ever will be. From the effects of the smallest atoms to the appearance of the Universe on the largest scales. ESO Visitor Centre | 9 October 2013 Astronomy in the ancient world Astronomy is the oldest of the natural sciences, dating back to antiquity, with its origins in the religious, mythological, and astrological practices of the ancient civilisations. Early astronomy involved observing the regular patterns of the motions of visible celestial objects, especially the Sun, Moon, stars and naked eye observations of the planets. The changing position of the Sun along the horizon or the changing appearances of stars in the course of the year was used to establish agricultural or ritual calendars. ESO Visitor Centre | 9 October 2013 Astronomy in the ancient world Australian Aboriginals belong to the oldest continuous culture in the world, stretching back some 50 000 years… It is said that they were the first astronomers. “Emu in the sky” at Kuringai National Park, Sydney -Circa unknown ESO Visitor Centre | 9 October 2013 Astronomy in the ancient world Goseck Circle Mnajdra Temple Complex c. -
Orthoptera: Tristiridae), En La Zona Costera Sur De La Región De Antofagasta
Boletín del Museo Nacional de Historia Natural, Chile, 57: 133-138 (2008) REGISTRO EN ALTURA DE ENODISOMACRIS CURTIPENNIS CIGLIANO, 1989 (ORTHOPTERA: TRISTIRIDAE), EN LA ZONA COSTERA SUR DE LA REGIÓN DE ANTOFAGASTA MARIO ELGUETA¹ y CONSTANZA BARRÍA² ¹ Entomología, Museo Nacional de Historia Natural, Casilla 787, Santiago, Chile; [email protected] ² Instituto de Geografía, Universidad Católica de Chile, Av. Vicuña Mackenna 4860, Santiago, Chile. [email protected] RESUMEN Se documenta el hallazgo de ejemplares de Enodisomacris curtipennis Cigliano, 1989 (Tristiridae: Elasmoderini) a una altitud de 2.700 m en el Cerro Armazones en 24º34’53”S; 70º11’56”O (Datum PSAD 56) equivalente a 378.600 E y 7.280.850 S (UTM); este constituye un nuevo registro altitudinal y a la vez es la máxima altura reportada para esta especie. El Cerro Armazones forma parte de la sierra Vicuña Mackenna y se ubica al NE de la localidad costera de Paposo, a 37 km hacia el interior, en la zona sur de la Provincia de Antofagasta. Se entregan además algunos antecedentes del ambiente en que se encuentra este ortóptero. ————— Palabras clave: Tristiridae, Enodisomacris curtipennis, distribución geográfica. ABSTRACT A high altitude record for Enodisomacris curtipennis Cigliano, 1989 (Orthoptera: Tristiridae), in the Southern coastal area of Antofagasta Region. The grasshopper Enodisomacris curtipennis Cigliano, 1989 is reported for the first time at 2,700 meters of altitude in the Cerro Armazones, 24º34’53” S; 70º11’56” W (Datum PSAD 56) or 378.600 E; 7.280.850 S (UTM). This is the highest altitudinal record for this species. The hill belongs to the Vicuña Mackenna range and is located at NE of Paposo locality, in the Southern coastal area of Antofagasta Province of Chile. -
The Case for Irish Membership of the European Southern Observatory Prepared by the Institute of Physics in Ireland June 2014
The Case for Irish Membership of the European Southern Observatory Prepared by the Institute of Physics in Ireland June 2014 The Case for Irish Membership of the European Southern Observatory Contents Summary 2 European Southern Observatory Overview 3 European Extremely Large Telescope 5 Summary of ESO Telescopes and Instrumentation 6 Technology Development at ESO 7 Big Data and Energy-Efficient Computing 8 Return to Industry 9 Ireland and Space Technologies 10 Astrophysics and Ireland 13 Undergraduate Teaching 15 Outreach and Astronomy 17 Education and Training 19 ESO Membership Fee 20 Conclusions 22 References 24 1 Summary The European Southern Observatory (ESO) is universally acknowledged as being the world leading facility for observational astronomy. The astrophysics community in Ireland is united in calling for Irish membership of ESO believing that this action would strongly support the Irish government’s commitment to its STEM (science, technology, engineering and maths) agenda. An essential element of the government’s plans for the Irish economy is to substantially grow its high-tech business sector. Physics is a core part of that base, with 86,000 jobs in Ireland in this sector1 while astrophysics, in particular, is a key driver both of science interest and especially of innovation. To support this agenda, Irish scientists and engineers need access to the best research facilities and with this access comes the benefits of spin-off technology, contracts and the jobs which this can bring. ESO is currently expanding its membership to include Brazil and is considering some eastern European countries. The cost of membership will increase as more states join and as Ireland’s GDP increases. -
Esoshop Catalogue
ESOshop Catalogue www.eso.org/esoshop Annual Report 2 Annual Report Annual Report Content 4 Annual Report 33 Mounted Images 6 Apparel 84 Postcards 11 Books 91 Posters 18 Brochures 96 Stickers 20 Calendar 99 Hubbleshop Catalogue 22 Media 27 Merchandise 31 Messenger Annual Report 3 Annual Report Annual Report 4 Annual Report Annual Report ESO Annual Report 2018 This report documents the many activities of the European Southern Observatory during 2018. Product ID ar_2018 Price 4 260576 727305 € 5.00 Annual Report 5 Apparel Apparel 6 Apparel Apparel Running Tank Women Running Tank Men ESO Cap If you love running outdoors or indoors, this run- If you love running outdoors or indoors, this run- The official ESO cap is available in navy blue and ning tank is a comfortable and affordable option. ning tank is a comfortable and affordable option. features an embroidered ESO logo on the front. On top, it is branded with a large, easy-to-see On top, it is branded with a large, easy-to-see It has an adjustable strap, measuring 46-60 cm ESO logo and website on the back and a smaller ESO logo and website on the back and a smaller (approx) in circumference, with a diameter of ESO 50th anniversary logo on the front, likely to ESO 50th anniversary logo on the front, likely to 20 cm (approx). raise the appreciation or the curiosity of fellow raise the appreciation or the curiosity of fellow runners. runners. Product ID apparel_0045 Product ID apparel_0015 (M) Product ID apparel_0020 (M) Price Price Price € 8.00 4 260576 720306 € 14.00 4 260576 720047 € 14.00 4 260576 720092 Product ID apparel_0014 (L) Product ID apparel_0019 (L) Price Price € 14.00 4 260576 720030 € 14.00 4 260576 720085 Product ID apparel_0013 (XL) Price € 14.00 4 260576 720023 Apparel 7 Apparel ESO Slim Fit Fleece Jacket ESO Slim Fit Fleece Jacket Men ESO Astronomical T-shirt Women This warm long-sleeve ESO fleece jacket is perfect This warm long-sleeve ESO fleece jacket is perfect This eye-catching nebular T-shirt features stunning for the winter. -
EGU2014-12008-3, 2014 EGU General Assembly 2014 © Author(S) 2014
Geophysical Research Abstracts Vol. 16, EGU2014-12008-3, 2014 EGU General Assembly 2014 © Author(s) 2014. CC Attribution 3.0 License. OH temperatures and intensities from astronomical spectra taken at Cerro Paranal in Chile Stefan Noll (1), Stefanie Unterguggenberger (1), Wolfgang Kausch (1,2), Stefan Kimeswenger (3,1), and Amy M. Jones (1) (1) Institute for Astro- and Particle Physics, University of Innsbruck, Innsbruck, Austria ([email protected]), (2) University of Vienna, Department of Astrophysics, Vienna, Austria, (3) Instituto de Astronomía, Universidad Católica del Norte, Antofagasta, Chile OH airglow is an important indicator for the properties and variability of the mesopause at about 87 km. OH bands cover a wide range of wavelengths from the optical to the near-infrared. The lines can be used to study intensities, vibrational temperatures, and rotational temperatures. The latter are expected to be close to the climate- related thermal temperatures of the band-specific emission layers. Most spectroscopic OH measurements focus on the determination of the rotational temperature for a single band by using a few lines with a low rotational upper level in a narrow wavelength range. Therefore, the specialised instruments that are typically used for airglow spectroscopy observe only a small fraction of the OH spectrum with limited information on the state of the upper atmosphere. In contrast, echelle spectrographs used at large astronomical observatories have the wavelength coverage, reso- lution, and sensitivity to study many OH bands and other airglow lines simultaneously. Since each ground-based observation from an astronomical telescope includes an observation of the night-sky emission, these data are also very valuable for upper atmosphere research, even though the timing and direction of the observations are not optimised and the targeted astronomical objects have to be removed from the spectra. -
European Extremely Large Telescope Site Chosen 26 April 2010
European Extremely Large Telescope site chosen 26 April 2010 and may, eventually, revolutionise our perception of the Universe, much as Galileo's telescope did 400 years ago. The final go-ahead for construction is expected at the end of 2010, with the start of operations planned for 2018. The decision on the E-ELT site was taken by the ESO Council, which is the governing body of the This night-time panorama shows Cerro Armazones in Organisation composed of representatives of the Chilean desert, near ESO's Paranal Observatory, ESO's fourteen Member States, and is based on an site of the Very Large Telescope. Cerro Armazones was extensive comparative meteorological investigation, chosen as the site for the planned European Extremely which lasted several years. The majority of the data Large Telescope, which, with its 42-meter diameter collected during the site selection campaigns will be mirror, will be the world’s biggest eye on the sky. Credit: ESO/S. Brunier made public in the course of the year 2010. Various factors needed to be considered in the site selection process. Obviously the "astronomical On April 26, 2010, the ESO Council selected Cerro quality" of the atmosphere, for instance, the number Armazones as the baseline site for the planned of clear nights, the amount of water vapour, and the 42-meter European Extremely Large Telescope (E- "stability" of the atmosphere (also known as seeing) ELT). Cerro Armazones is a mountain at an played a crucial role. But other parameters had to altitude of 3060 meters in the central part of Chile's be taken into account as well, such as the costs of Atacama Desert, some 130 kilometers south of the construction and operations, and the operational town of Antofagasta and about 20 kilometers from and scientific synergy with other major facilities Cerro Paranal, home of ESO's Very Large (VLT/VLTI, VISTA, VST, ALMA and SKA etc).