An outburst from a forming massive star,
due to the sudden intake of material from its accretion disk, has been detected for the very first time
CALIFA project allowed to detect, in three early-type galaxies,
a very tenuous arms where stars are being formed
The TGO satellite has successfully completed the ignition needed
to be captured by Martian gravity
The United Nations General Assembly adopted a resolution declaring 11 February as the International Day of Women and Girls in Science. The Spanish National Research Council has proposed to all the institutes in CSIC to make a picture with all women in their research centers, to use this picture in their welcome web page, and a mosaic of them at the CSIC welcome web page, from 10 to 13 February 2017, with the aim of making visible CSIC and their research centers in their support for the participation of women and girls in Science.09/02/2017
The HI galaxy mass function represents a fundamental component of our understanding of the gas content of galaxies. How its form varies throughout the local Universe and as a function of redshift is key to developing a complete picture of galaxy evolution. We use the ALFALFA 70% catalogue, the largest uniform catalogue of extragalactic HI sources to date, to explore the environmental dependence of the HI mass function based on the projected neighbour densities in both SDSS and 2MRS.
Early-type galaxies are characterized by their spheroidal shape, lacking in remarkable features, and by their reddish color that comes from a very aged star population. They are very massive galaxies where star formation stopped billions of years ago. However, an international astronomers team has found, in three early-type galaxies from the close universe, a very tenuous structure similar to the spiral galaxies arms that has star under formation.19/01/2017
"Let's go to Mars" is a scientific graphic adventure in which you must land-off in Mars, explore the surface of the planet, build a permanent base for the arrival of your colleagues, collect and analyze Martian samples, and face the many dangers that exist in the red planet. Beware of maintaining your oxygen and energy levels or you will fail in your mission!29/12/2017
At 22:25 in the evening (local time) of December 11 a brilliant fireball crossed the south of Spain. The fireball, which overflew the provinces of Granada and Jaén, could be seen from much of the country. The phenomenon has been recorded from the Sierra Nevada Observatory (Granada), as well as from the meteor detection stations operating under the SMART Project from the observatories of La Hita (Toledo), Calar Alto (Almería), La Sagra (Granada) and Seville.12/12/2016
The ExoMars (ESA) mission has been in orbit around Mars since 19 October. Over the past two weeks, the first test observations of the instruments have been made. NOMAD, a spectrograph co-designed by the Institute of Astrophysics of Andalusia (IAA-CSIC) to solve the so-called methane problem on Mars has sent its first data confirming the excellent performance of the instrument.30/11/2016
An international team, with the participation of the Institute of Astrophysics of Andalusia (IAA-CSIC), has observed with the OSIRIS camera onboard the Rosetta mission changes in light reflected on the surface of comet 67P / Churyumov with different time scales, from minutes to several days. These changes in brightness are mainly due to the amount of ice present in the observation area.18/11/2016
Low mass stars, like the Sun, are formed from big fragments of clouds of gas and dust, which condense until a central object, or protostar, is formed, growing up by absorbing gas from a surround disk and expelling the surplus material through a couple of jets located on both poles. However, it was not known if the most massive stars, with tens of solar masses, are formed through the same mechanism. The study of an outburst detected in the forming massive star NIRS 3, and published today in Nature, has provided the most solid evidence that, indeed, all stars are formed the same way.14/11/2016
The mayor of Granada, Francisco Cuenca, has conducted a public event in which he has introduced the proposal submitted yesterday to the Secretary of State for Science and Innovation. Representatives of the Government of Andalusia, the University of Granada, The Technological Health Park, the Higher Council for Scientific Research and the Science Park have attended the event.
Lithium, the lightest solid element in existence, plays an important role in our lives, both at the biological and the technological level. Like the majority of chemical elements, its origins stem back to astrophysical phenomena, but its point of genesis was so far unclear. Recently, a group of researchers detected enormous quantities of beryllium-7 –an unstable element which decays into lithium in 53.2 days– inside nova Sagittarii 2015 N.2, which suggests that novae are the main source of lithium in the galaxy.02/11/2016
The UPWARDS project is coordinated by the Institute of Astrophysics of Andalusia (IAA-CSIC), with the participation of seven European scientific institutions. It will develop new analytical techniques to exploit the Mars Express and ExoMars data. Among the activities to publicize the project is the documentary "Rediscovering Mars: UPWARDS project", which airs today at 18h in La 2 of Spanish Television.19/10/2016
Calar Alto Observatory constitutes an astronomical reference for the international scientific community for the quality of its telescopes and astronomical instrumentation.10/10/2016
On Thursday September 15 the Delegate of Environment of the Junta de Andalucía, Inmaculada Oria, visited the Sierra Nevada Observatory (OSN). The visit is part of a collaboration agreement between the Institute of Astrophysics of Andalusia (IAA) and the Provincial Delegation which began following the First Day of Sky Quality held last June.
The visit was also attended by the Mayor of Monachil, Jose Morales, Councilman Environment of the City of Monachil, Franciso Alvarez, and the Director of the Sierra Nevada National Park, Javier Sanchez.19/09/2016
The scientific activities of the Instituto de Astrofísica de Andalucía require the analysis, design, prototyping, manufacture and integration of astrophysical instrumentation. To carry out all these tasks the Instrumental and Technological Development Unit UDIT has a Mechanical department, Optics laboratories, Electronics and Software as well as two clean rooms of ISO 8 class.
Contribution in the technological areas of Electronics, Mechanics, Optics, Project Management and Software.
Among our facilities we have clean rooms for testing and assembly equipment that require special conditions of environmental cleanup.
We provide related to optical metrology and optical engineering consultancy services.
Designed to study the dispersion of light in dust samples that are of interest in the field of astrophysics.
Dedicated to the maintenance and development of optical telescopes and astronomical instrumentation in the visible and near infrared.
Companies and technology centers collaborators in projects carried out in the center.
The Instituto Astrofísica Andalucía (IAA) is an institute belonging to the Consejo Superior de Investigaciones Científicas (CSIC) in Granada - Andalucía. The activities of the IAA - CSIC are related to research in the field of astrophysics and the development of instrumentation for telescopes and spacecraft.
General overview of the activities carried out in the IAA - CSIC, organization and internal structure, as well as some of its history.
Jobs, scholarships and contracts granted, and any relevant administrative information for members of the IAA - CSIC.
General aims and composition of the external scientific advisory board in IAA - CSIC
Description and composition of groups and scientific units associated with the IAA - CSIC.
Responsible for the communications and computing infrastructure needed in scientific research and business partnerships.
Check out the different activities in the IAA - CSIC through the annual reports published in recent years.
List of personnel assigned to IAA - CSIC through its scientific departments and internal units.
The main goal of the IAA International Office is to improve the fund raising level of the centre by securing funds beyond the support already provided by national and international grants.
Scientific and technological projects led by IAA - CSIC members
Access to restricted information for personnel assigned to IAA - CSIC through its intranet.
The Sierra Nevada Observatory (OSN) is a high mountain observatory located in Loma de Dilar, in the ski resort of the Sierra Nevada mountain range (Granada). The OSN is operated, maintained and supplied by the Instituto de Astrofísica de Andalucía (IAA-CSIC). It consists of a main building which hosts two Nasmyth optical telescopes of 90-cm and 1.50-m diameter each, as well as a 60-cm IR semi-automated telescope and a 35-cm telescope.
The German-Spanish Astronomical Center at Calar Alto is located in the Sierra de Los Filabres (Andalucía, Southern Spain) north of Almeria. It is operated jointly by the Max-Planck-Institut für Astronomie (MPIA) in Heidelberg, Germany, and the Instituto de Astrofísica de Andalucía (CSIC) in Granada/Spain. Calar Alto provides three telescopes with apertures of 1.23m, 2.2m and 3.5m to the general community. A 1.5m-telescope, also located on the mountain, is operated under the control of the Observatory of Madrid.
Instituto de Astrofísica de Andalucía
Glorieta de la Astronomía s/n, 18008 Granada
Telephone: (+34) 958 12 13 11
Fax: (+34) 958 814 530
Instituto de Astrofísica de Andalucía
Apartado 3004,18080 Granada
Take a taxi to the IAA or your hotel directly. There are some buses from the aiport to Granada, but they are not syncronous with the planes...
At the train station, ask for Av. de la Constitución and get on bus LAC to Palacio de Congresos. Get off Palacio de Congresos stop and change to bus S2, direction to Villa Argaz. This bus has a stop very close to the IAA, only a few meters.
At the bus station, get on bus SN2 to Palacio de Congresos. Get off at the bus stop Tierno Galván - Palacio de Congresos and change to bus S2 to Villa Argaz. The S2 route passes in front of the IAA. Get off at the first stop of Camino Bajo de Huétor Street, then walk for a few seconds and you'll be here.