PASS prototype observations in 2005

Bibcode
2006tafp.conf..187D
Deeg, H. J.; Alsubai, K.; Horne, K.; Alonso, R.; Belmonte, J. A.; Collier Cameron, A.
Bibliographical reference

"Tenth Anniversary of 51 Peg-b: Status of and prospects for hot Jupiter studies. Colloquium held at Observatoire de Haute Provence, France, August 22-25, 2005. Edited by L. Arnold, F. Bouchy and C. Moutou. Published by Frontier Group, Paris (ISBN-2-914601-17.4). Proceedings of the colloquium in PDF format can be downloaded from the URL: http://www.obs-hp.fr/www/pubs/Coll51Peg/proceedings.html (courtesy of Frontier Group), p.187-189"

Advertised on:
2
2006
Number of authors
6
IAC number of authors
0
Citations
0
Refereed citations
0
Description
The Permanent All Sky Survey (PASS) will consist of arrays of wide angle CCD cameras, that will permanently survey the entire visible sky from several observing sites. Its major objectives are the detection of all giant-planet transits across bright stars and the detection and continuous tracking of any variable or transient phenomena in the full sky. A prototype with one CCD camera has been set up at Teide Observatory, Tenerife, and has been in regular operation since April 2005. Here is given an overview over the ongoing observations and the quality control that has been implemented.
Type
Non-refereed

It may interest you

  • Non-refereed
    Convection, rotation, and magnetic activity of solar-like stars from asteroseismology
    During the last decade, our understanding of stellar physics and evolution has undergone a tremendous revolution thanks to asteroseismology. Space missions such as CoRoT, Kepler, K2, and TESS have already been observing millions of stars providing high-precision photometric data. With these data, it is possible to study the convection of stars
    Mathur, Savita

    Advertised on:

    0
    2024
    Bibcode
    2024IAUS..365..195M
    Citations
    0
  • Non-refereed
    Tales of stellar & binary co-evolution, told by stellar oscillations
    Stellar binarity and stellar oscillations are mostly seen and studied as two separate phenomena. Sometimes, one process is even complicating the analysis of the other beyond the liking of one or the other research community. However, the complete picture painted by the physical constraints provided by the combination of both processes represents a
    Beck, Paul G.

    Advertised on:

    10
    2024
    Bibcode
    2024bss..confE..35B
    Citations
    0
  • Non-refereed
    The Multimodal Universe: 100 TB of Machine Learning Ready Astronomical Data
    We present the Multimodal Universe, a new framework collating over 100 TB of multimodal astronomical data for its first release, spanning images, spectra, time series, tabular and hyper-spectral data. This unified collection enables a wide variety of machine learning (ML) applications and research across astronomical domains. The dataset brings
    Angeloudi, Eirini et al.

    Advertised on:

    12
    2024
    Bibcode
    2024RNAAS...8..301A
    Citations
    0