Observatorio de Sierra Nevada Susana Martín Ruiz (IAA-CSIC)

Slides:



Advertisements
Similar presentations
Radio Astronomy By looking at the radio part of the EM spectrum, we can get a different perspective on the nature of the universe. the atmospheric window.
Advertisements

Research Centre of Astronomy and Geophysics Mongolian Academy of Sciences Study of near-earth objects in Mongolia. Space debris, asteroids and comets Outreach.
The Properties of Young Brown Dwarfs John D. Shaw.
Return to Hubble: Servicing Mission 4 Dr. Frank Summers Space Telescope Science Institute April 2, 2009.
Observational techniques meeting #7. Detectors CMOS (active pixel arrays) Arrays of pixels, each composed on a photodetector (photodiode), amplifier,
Chapter 6 Telescopes: Portals of Discovery. 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning How does your eye form an image? How do.
Extragalactic science with the Herschel Space Observatory Marc Sauvage CEA/DSM/DAPNIA Service d'Astrophysique UMR AIM.
The SOAR Telescope MSU’s Laboratory for Astronomical Discovery.
ATACAMA. At September Faculty Meeting we proposed: A project of scientific excitement and uniqueness, in the IR niche; with focus that emphasizes Cornell’s.
Instituto de Astrofísica de Andalucía – C.S.I.C Research Institute of the Consejo Superior de Investigaciones Cientificas Main activities devoted to Astrophysics.
SOFIA — The Observatory open cavity (door not shown) TELESCOPE pressure bulkhead scientific instrument (1 of 7) Scientist work stations, telescope and.
The active Sun. The magnetic Sun White lightMagnetic field.
The Universe in the Infrared What is the Spitzer Space Telescope, and how does it work? Funded by NASA’s Spitzer Science Center Images courtesy NASA/JPL.
Agile: A Time-Series CCD Photometer to Study Variables Anjum Mukadam, Russell Owen, Ed Mannery University of Washington, Seattle.
OSN Archive: Current status and future implementations José Miguel Ibáñez Instituto de Astrofísica de Andalucía - CSIC Sierra Nevada Observatory First.
Modern Telescopes Lecture 12. Imaging Astronomy in 19c Photography in 19c revolutionize the astronomy Photography in 19c revolutionize the astronomy 
COROT TARGETS: PROGRESS REPORT ON THE PHOTOMETRIC AND SPECTROSCOPIC MONITORING OF DSCT, GDOR AND BCEP VARIABLE STARS.
Space Infrared Astronomy in Japan 2009 UN BSS & IHY Workshop, September 22, 2009 MATSUMOTO, Toshio Seoul National University, ISAS/JAXA.
Big Bear Solar Observatory NST Main Features  All reflecting, off-axis Gregory optical configuration  PM: 1.6 m clear aperture with f/2.4  Figuring.
Further Advancements of the PARI Optical Ridge Telescopes for Education and Public Outreach M. W. Castelaz, J. D. Cline Pisgah Astronomical Research Institute.
Sternberg Astronomical Institute of Lomonosov Moscow State University.
A visible-light AO system for the 4.2 m SOAR telescope A. Tokovinin, B. Gregory, H. E. Schwarz, V. Terebizh, S. Thomas.
Optics and Telescopes. Optics and Telescopes: Guiding Questions 1.How do reflecting and refracting telescopes work? 2.Why is it important that professional.
Hvar Observatory Faculty of Geodesy Kačićeva 26, Zagreb.
Ch. 28 Sec. 1 Tools of Astronomy. Tools  Radiation  Light is the best tool used to observe and learn about the universe  Before telescopes, scientist.
15 October Observational Astronomy Direct imaging Photometry Kitchin pp ,
Astronomy & Astrophysics Division Research Programmes - IR/Optical IS Matter & Star Formation Active Galaxies Sun; Solar Wind; Comets Quasars & Pulsars.
Matt Carter Joseph Owen.  Located in Ashland, Va  Randolph Macon College.
HD This star is found periodic. The possible period is days. We present the phase curve with this period. HD This star is not variable.
INSTRUMENTATION/ OID / L. Pasquini/ 1 ____________________________________________________________ FLAMES COORDINATION AND INTERFACES. FIELD CORRECTOR.
ASTRO-F Survey as an Input Catalogue for FIRST Takao Nakagawa (ISAS, Japan) & ASTRO-F Team.
Andreas Quirrenbach and the CARMENES Consortium Searching for Blue Planets Orbiting Red Dwarfs.
Tools of Modern Astronomy Chapter 21 Section 1 Pages Chapter 21 Section 1 Pages
Chapter 6 Telescopes: Portals of Discovery. 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning How does your eye form an image? How do.
is transparent ERAU Astronomical Observatory Meade inch Schmidt Cassegrain Reflecting Telescope.
Exploring the far reaches of the universe. Hubble Telescope By Blake Shaffer.
6.3 Telescopes and the Atmosphere 6.4 Eyes and Cameras: Everyday Light Sensors Our goals for learning How does Earth’s atmosphere affect ground-based observations?
In p42 Visible light questions: 1.What colors are on the visible light spectrum? 2.What units are the wavelengths of light measured in? 3.What is the range.
VLST workshop; STScI February UV astronomy in the post- GALEX era Noah Brosch Wise Observatory Tel Aviv University Israel.
SITE PARAMETERS RELEVANT FOR HIGH RESOLUTION IMAGING Marc Sarazin European Southern Observatory.
The Taiwanese-American Occultation Survey (TAOS) Matthew Lehner ASIAA.
Observations of aerosol concentration, properties and chemical composition Sandro Fuzzi Institute for Atmospheric Sciences and Climate National Research.
Existing Facilities of IIA Vainu Bappu Observatory, Kavalur M.K. V. Bappu, the founder Director of IIA had set up an observatory for the night time observations.
The Scientific Goals for Astronomical Satellite
Virtual Visits to Astronomical Observatories M. Serra-Ricart L. Martínez L. Cuesta Instituto de Astrofísica de.
All-sky camera of the ALFA project: common points and interests with the Wide Field Astronomical Observations E. Séran & M. Godefroy CETP, St-Maur June.
1 Small Telescopes and the Photometric Calibration of the Sloan Digital Sky Survey (SDSS) Douglas Tucker.
Daily observation of dust aerosols infrared optical depth and altitude from IASI and AIRS and comparison with other satellite instruments Christoforos.
Robo-AO Overview: System, capabilities, performance Christoph Baranec (PI)
July 12, 2004Pulsating PMS stars Pulsating Pre-Main Sequence Stars in Young Open Clusters K. Zwintz Institute of Astronomy, Univ. Vienna, Austria
ISUAL Design Concept S. Mende. SDR 7 Jun NCKU UCB Tohoku ISUAL Design Concept S. Mende Sprite Example Sprite Image obtained by Berkeley/NCKU 1999.
Wide-field Infrared Survey Explorer (WISE) is a NASA infrared- wavelength astronomical space telescope launched on December 14, 2009 It’s an Earth-orbiting.
Star Map 3D+: Guide to the Night Sky, Planets, Constellations, and Astronomy.
Infrared Spectroscopy (and the Cassini Composite Infrared spectrometer) Adam Ginsburg September 25, 2007.
Existing Facilities of IIA
V. Agapov, N. Sakva, D.Davydov, E.Katkova
Indian Astronomical Observatory
Chapter 6 Telescopes: Portals of Discovery
SOFIA — The Observatory
Chapter 6 Telescopes: Portals of Discovery
Observing Facilities of IIA
6.3 Telescopes and the Atmosphere
An IFU slicer spectrometer for SNAP
The pointing calibration of the WFCTA tracking system
Solar Physics and the Total Solar Eclipse of 2017 August 21
Announcements No lab this week since we had an observing night Tuesday. Next week: 1st Quarter Nights Tuesday and Thursday. Set-up will start at 6:30pm.
How do humans observe and explore space?
Observational techniques meeting #6
Caucasian Mountain Observatory SAI MSU
Observational Astronomy
Presentation transcript:

Observatorio de Sierra Nevada Susana Martín Ruiz (IAA-CSIC)

Located at Loma de Dilar in the Sierra Nevada mountain range (Granada) Altitude: 2900 m above sea level 100% Spanish (IAA- CSIC)

Telescopes  Main building: Nasmyth telescopes T150 (1.5m) and T90 (90cm) T150: a low resolution spectrograph (Albireo) and a CCD camera with a FoV of 8’ x 8’ T90: six channel photoelectric photometer (Strömgren photometer) and a CCD camera with a FoV of 17’x 17’  Other installations (projects): T60: robotic telescope with a IR camera (BOOTES-IR project) T35: 14’’ telescope with a wide field CCD camera (variable stars) SATI: interferometer (dynamic of the high layers of the Earth atmosphere) Spectrometer (study of the sky at infrared and sub-mm wavelengths)

Observing modes For T150 and T90 telescopes - Service - In-situ - Remote Very important: the telescopes can not be operated in service mode at the same time! Why?. The personnel is reduced: 3 night assistants (1 assistant/night)

The OSN is a modest observatory In favour...  Long term observations Photometric multisite campaigns, studies of comets, catalogues of stars, surveys, etc.  Outreach activities (guide visits in summer)  To get started in the use of telescopes But against...  Difficult access during the winter  Lack of technical personnel with plain dedication  The OSN has no assigned budget.

Future?...