2010•Unpublished venueOpen access

NIBLES: an HI census of SDSS galaxies in the Local Volume

Wim van Driel, Stephen Edward Schneider, M. D. Lehnert, Simon Blyth, Antoine Bouchard, K. J. van der Heyden, W. J. G. de Blok, R. C. Kraan‐Korteweg, M. Ramatsoku

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Abstract

Improving our knowledge of the H I Universe will improve our readiness to use the SKA and its Precursors to their full potential.NIBLES (Nançay Interstellar Baryons Legacy Extragalactic Survey) is a targeted survey of 3000 SDSS galaxies in the Local Volume (900<cz<12,000 km/s) that are distributed evenly over their entire range of total stellar mass (absolute z-band magnitude M z ∼ -13 to -24 mag, for H 0 =70 km s -1 Mpc -1 ).Using mainly the 100-m Nançay Radio Telescope, after 3500 hours of telescope time in the period 2007-2009 it has produced spectra deeper than the blind ALFALFA survey, and it uniformly samples the local galaxy stellar mass distribution.NIBLES will allow us to address a number of outstanding questions in astrophysics, such as: the global baryon budget within the local volume, gas properties as a function of galaxy dynamical mass, stellar mass, and various galaxy morphology parameters.A combination of short initial and longer follow-up observations is expected to yield an overall detection rate of 75%, which appears to be rather independent of galaxy mass and colour -except for the most luminous (M z = -23 to -24), gas-poor ellipticals.NIBLES is an open collaboration and anyone interested in the science and willing to contribute to the project is welcome to join the score of NIBLErS.

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Improving our knowledge of the H I Universe will improve our readiness to use the SKA and its Precursors to their full potential.NIBLES (Nançay Interstellar Baryons Legacy Extragalactic Survey) is a targeted survey of 3000 SDSS galaxies in the Local Volume (900<cz<12,000 km/s) that are distributed evenly over their entire range of total stellar mass (absolute z-band magnitude M z ∼ -13 to -24 mag, for H 0 =70 km s -1 Mpc -1 ).Using mainly the 100-m Nançay Radio Telescope, after 3500 hours of telescope time in the period 2007-2009 it has produced spectra deeper than the blind ALFALFA survey, and it uniformly samples the local galaxy stellar mass distribution.NIBLES will allow us to address a number of outstanding questions in astrophysics, such as: the global baryon budget within the local volume, gas properties as a function of galaxy dynamical mass, stellar mass, and various galaxy morphology parameters.A combination of short initial and longer follow-up observations is expected to yield an overall detection rate of 75%, which appears to be rather independent of galaxy mass and colour -except for the most luminous (M z = -23 to -24), gas-poor ellipticals.NIBLES is an open collaboration and anyone interested in the science and willing to contribute to the project is welcome to join the score of NIBLErS.

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Available abstract

Improving our knowledge of the H I Universe will improve our readiness to use the SKA and its Precursors to their full potential.NIBLES (Nançay Interstellar Baryons Legacy Extragalactic Survey) is a targeted survey of 3000 SDSS galaxies in the Local Volume (900<cz<12,000 km/s) that are distributed evenly over their entire range of total stellar mass (absolute z-band magnitude M z ∼ -13 to -24 mag, for H 0 =70 km s -1 Mpc -1 ).Using mainly the 100-m Nançay Radio Telescope, after 3500 hours of telescope time in the period 2007-2009 it has produced spectra deeper than the blind ALFALFA survey, and it uniformly samples the local galaxy stellar mass distribution.NIBLES will allow us to address a number of outstanding questions in astrophysics, such as: the global baryon budget within the local volume, gas properties as a function of galaxy dynamical mass, stellar mass, and various galaxy morphology parameters.A combination of short initial and longer follow-up observations is expected to yield an overall detection rate of 75%, which appears to be rather independent of galaxy mass and colour -except for the most luminous (M z = -23 to -24), gas-poor ellipticals.NIBLES is an open collaboration and anyone interested in the science and willing to contribute to the project is welcome to join the score of NIBLErS.

Key concepts: Galaxy, Physics, Astrophysics, Stellar mass, Astronomy, Baryon, Universe, Galaxy formation and evolution

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