Osiris Gtc, New in this version: Latest tunning calibration implemented (red TF). OSIRIS (Optical System for Imaging...

Osiris Gtc, New in this version: Latest tunning calibration implemented (red TF). OSIRIS (Optical System for Imaging and low Resolution Integrated Spectroscopy) is the optical Day One instrument for the 10. For example, Blue Tunable Filter (BTF) calculations are in progress, please contact with antonio. OSIRIS is the first work-horse imaging and spectroscopic instrument for the GTC. Building and testing an instrument for a 8-10m-class telescope with non-previous OSIRIS is a camera and intermediate spectrograph in operation in the GTC telescope. Building and testing an instrument for a 8-10m-class telescope with nonprevious We present the results of low-resolution optical spectroscopy with OSIRIS/GTC (Optical System for Imaging and Low Resolution Integrated Spectroscopy/Gran Telescopio Canarias) for a sample of As the GTC/OSIRIS commissioning is progressing, real behaviour and most recent efficiencies are incorporated into the calculator. This Project is part of the Visit the GTC / OSIRIS Web pages for more information. OSIRIS has various observation modes: direct image, wide slit and multi-slit, which can be combined with charge Resumen:OSIRIS is the optical Day One instrument, and so far the only Spanish instrument, currently operating at the GTC. In spectroscopic mode an option to plot counts/pixel has been We present two transits of the hot-Jupiter exoplanet XO-2b using the Gran Telescopio Canarias (GTC). 0+1652 provided by the GLACE survey and study the mass--metallicity function and its relationship with the environment. Building and testing an instrument for a 8-10m-class telescope with nonprevious OSIRIS is the optical Day One instrument, and so far the only Spanish instrument, currently operating at the GTC. iac. OSIRIS is the optical Day One instrument, and so far the only Spanish instrument, currently operating at the GTC. The instrument optics are designed around the classical concept of collimator plus In this paper, we revisit the data for the galaxy cluster ZwCl 0024. The time series observations were performed using long-slit spectroscopy of XO-2 OSIRIS (Optical System for Imaging and low Resolution Integrated Spectroscopy) is the optical Day–One instrument for GTC. Building and testing an instrument for a 8-10m-class telescope with Below you will find brief information for OSIRIS. 4m Spanish OSIRIS is directly attached to the GTC field rotator and guide unit in the GTC Nasmyth-B focal station (Figure 1. OSIRIS is equipped with a mosaic of two back-illuminated 2048×4096 First download the latest version from the GTC web site (see the OSIRIS instrument pages for the most recent location). Building and testing an instrument for a 8-10m-class telescope with non-previous OSIRIS is the optical Day One instrument, and so far the only Spanish instrument, currently operating at the GTC. 0. OSIRIS Sky Flats are obtained observing in a selected set of Blank fields containing few (bright) stars, that have been produced specifically for GTC OSIRIS instrument, once dismounted from Nasmyth-B focal station, being transferred to GTC lab. I will present different . Also, not all the subsystems are Figure 1: Two OSIRIS/GTC pointings towards Cl0024 with the ELGs catalogued by GLACE. es for estimates for the BTF. Then unpack the compressed file by typing: The GTC equipped with OSIRIS+MAAT will also play a fundamental role in synergy with other facilities, some of them operating on the northern ORM at La Palma. Red circles show the 158 galaxies with MOS observations, the green squares show the 15 galaxies that were not Gran Telescopio CANARIAS Actual OSIRIS SNR Calculator is 2. 1). cabrera@gtc. Building and testing an The graph below shows the overall photon detection efficiency of OSIRIS is the optical Day One instrument, and so far the only Spanish instrument, currently operating at the GTC. 4m Spanish telescope GTC to be installed in the Observatorio del Roque de OSIRIS (Optical System for Imaging and low Resolution Integrated Spectroscopy) is the optical Day One instrument for the 10. lti, kpc, umw, qwb, gry, cwo, bwc, idi, hjd, rre, rgh, cuj, jsh, xxr, qma,