0000000000379934

AUTHOR

Steven Phillipps

showing 2 related works from this author

The VST Photometric Hα Survey of the Southern Galactic Plane and Bulge (VPHAS+)

2014

The VST Photometric Halpha Survey of the Southern Galactic Plane and Bulge (VPHAS+) is surveying the southern Milky Way in u, g, r, i and Halpha at 1 arcsec angular resolution. Its footprint spans the Galactic latitude range -5 < b < +5 at all longitudes south of the celestial equator. Extensions around the Galactic Centre to Galactic latitudes +/-10 bring in much of the Galactic Bulge. This ESO public survey, begun on 28th December 2011, reaches down to 20th magnitude (10-sigma) and will provide single-epoch digital optical photometry for around 300 million stars. The observing strategy and data pipelining is described, and an appraisal of the segmented narrowband Halpha filter in us…

media_common.quotation_subjectMilky WayAstronomyFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energyPhotometry (optics)BulgeQB460Astrophysics::Solar and Stellar AstrophysicsQCAstrophysics::Galaxy Astrophysicsmedia_commonQBPhysicsCelestial equatorWhite dwarfAstronomyAstronomy and AstrophysicsGalactic planeAstrophysics - Astrophysics of GalaxiesStars13. Climate actionSpace and Planetary ScienceSkyAstrophysics of Galaxies (astro-ph.GA)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics::Earth and Planetary Astrophysics
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The second data release of the INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS DR2)

2014

The INT/WFC Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS) is a 1800 square degrees imaging survey covering Galactic latitudes |b| < 5 deg and longitudes l = 30 to 215 deg in the r, i and H-alpha filters using the Wide Field Camera (WFC) on the 2.5-metre Isaac Newton Telescope (INT) in La Palma. We present the first quality-controlled and globally-calibrated source catalogue derived from the survey, providing single-epoch photometry for 219 million unique sources across 92% of the footprint. The observations were carried out between 2003 and 2012 at a median seeing of 1.1 arcsec (sampled at 0.33 arcsec/pixel) and to a mean 5\sigma-depth of 21.2 (r), 20.0 (i) and 20.3 (H-a…

InfraredAstronomyFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionRoot mean squarePhotometry (optics)surveyslaw0103 physical sciencesQB460stellar content [Galaxy]010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)cataloguesPhysics010308 nuclear & particles physicsNewtonian telescopeVegaAstronomyAstronomy and AstrophysicsBeGalactic planeemission-line [stars]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics - Instrumentation and Methods for AstrophysicsData releaseData reduction
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