Present and future of the OTELO project

Bibcode
2015hsa8.conf..304R
Ramón-Pérez, M.; Bongiovanni, A.; Cepa, J.; Pérez García, A.; Alfaro, E. J.; Castañeda, H.; Ederoclite, A.; González-Serrano, J. I.; González, J. J.; Gallego, J.; Sánchez-Portal, M.
Bibliographical reference

Highlights of Spanish Astrophysics VIII, Proceedings of the XI Scientific Meeting of the Spanish Astronomical Society held on September 8-12, 2014, in Teruel, Spain, ISBN 978-84-606-8760-3. A. J. Cenarro, F. Figueras, C. Hernández-Monteagudo, J. Trujillo Bueno, and L. Valdivielso (eds.), p. 304-309

Advertised on:
5
2015
Number of authors
11
IAC number of authors
4
Citations
0
Refereed citations
0
Description
OTELO is an emission-line object survey carried out with the red tunable filter of the instrument OSIRIS at the GTC, whose aim is to become the deepest emission-line object survey to date. With 100 % of the data of the first pointing finally obtained in June 2014, we present here some aspects of the processing of the data and the very first results of the OTELO survey. We also explain the next steps to be followed in the near future.
Type
Non-refereed

It may interest you

  • Non-refereed
    JWST and cross-correlation techniques: A faster alternative for atmospheric studies
    The application of cross-correlation techniques to JWST transmission spectra has opened an alternate pathway to study exoplanet atmospheres with JWST observations, which will contribute to pave the road for the first atmospheric studies with ELTs. JWST observed for the first time the hot-Jupiter WASP-39b on July 2022 as part of the JWST Transiting
    Esparza-borges, Emma et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1005E
    Citations
    0
  • Non-refereed
    The population of barred galaxies in the MACS J0647.8+7015 galaxy cluster at z=0.59
    We study the bar fraction in the MACS J0647.8+7015 cluster of galaxies at z=0.59 using the observations obtained with the NIRCam instrument mounted on the JWST telescope. We visually inspected the near infrared images obtained with the F200W filter of all the cluster members to identify the presence of bars. The cluster member selection was based
    Lera, Margherita et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1560L
    Citations
    0
  • Non-refereed
    Performance and first measurements of the MAGIC Stellar Intensity Interferometer
    In recent years, a technology developed between the 1950s and 1970s by the pioneering experiments of Hanbury Brown and Twiss has (re)emerged: the Stellar Intensity Interferometry (SII). Unlike amplitude interferometry, SII exploits a second-order effect that can be measured by correlating the light intensities at different detectors without the
    Fiori, Michele et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1256F
    Citations
    0