0000000000379936

AUTHOR

Mike Irwin

showing 3 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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A parametric description of the 3D structure of the Galactic bar/bulge using the VVV survey

2017

We study the structure of the inner Milky Way using the latest data release of the Vista Variables in Via Lactea (VVV) survey. The VVV is a deep near-infrared, multi-colour photometric survey with a coverage of 300 square degrees towards the Bulge/Bar. We use Red Clump (RC) stars to produce a high-resolution dust map of the VVV's field of view. From de-reddened colour-magnitude diagrams we select Red Giant Branch stars to investigate their 3D density distribution within the central 4 kpc. We demonstrate that our best-fit parametric model of the Bulge density provides a good description of the VVV data, with a median percentage residual of 5$\%$ over the fitted region. The strongest of the o…

Absolute magnitudeInitial mass functionastro-ph.GAMilky WayFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: bulgeBulge0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsRed clumpGalaxy: structureAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSLuminosity function (astronomy)Physics010308 nuclear & particles physicsGalactic CenterAstronomyAstronomy and AstrophysicsGalaxy: fundamental parametersAstrophysics - Astrophysics of GalaxiesGalaxy: centregalaxies: individual: Milky WayRed-giant branchSpace and Planetary ScienceGalaxy: formationAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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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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