The UKIDSS galactic plane survey

By P. Lucas, M. Hoare, A. Longmore, A. Schroder, C. Davis, A. Adamson, R. Bandyopadhyay, Richard de Grijs, M. Smith, A. Gosling and 21 more. 2007

410 citations recorded by the source corpus.

'The definitive version is available at www.blackwell-synergy.com .' Copyright Blackwell Publishing DOI: 10.1111/j.1365-2966.2008.13924.x

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/fce528f8dcee945c401a0ceece5e866885b6936d

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Citations in the corpus

• The structure of the Milky Way's bar outside the bulge (2015, methodology): “In the Ks-band we use data from (i) the United Kingdom Infrared Deep Sky Survey (UKIDSS) Galactic Plane Survey (GPS, Lucas et al. 2008), (ii) the VVV survey (Saito et al. 2012) and, (iii) to extend the study further from the galactic plane than previous studies, we augment this with 2MASS data…”
• The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs (2020, methodology): “The WFCAM archives searched were those of the UKIDSS Large Area Survey (ULAS), the UKIDSS Galactic Plane Survey (UGPS; Lucas et al. 2008), the UKIDSS Galactic Clusters Survey (UGCS), and the UKIRT Hemisphere Survey (UHS; Dye et al. 2018).”
• LIFTING THE DUSTY VEIL WITH NEAR- AND MID-INFRARED PHOTOMETRY. I. DESCRIPTION AND APPLICATIONS OF THE RAYLEIGH–JEANS COLOR EXCESS METHOD (2011, background): “Obviously, with the advent of deeper, publicly-available NIR surveys in the future (such as UKIDSS), the limitations of the NIR photometry seen here can be mitigated; given the limited sky coverage for high-resolution MIR photometry, such surveys have the capability of improving the extinction reach”
• VISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way (2009, methodology): “In addition, we will be able to identify the counterparts of high-energy (γ-, and X-ray) sources: accreting black holes, microquasars, binary-pulsar companions, low mass X-ray binaries (LMXBs), and high mass X-ray binaries (HMXBs) (e.g., Mirabel & Rodrı́guez, 1998; Lucas et al., 2008).”
• A 3D Dust Map Based on Gaia, Pan-STARRS 1, and 2MASS (2019, background): “Incorporation of deep infrared photometry—e.g., from the Spitzer GLIMPSE surveys (Churchwell et al. 2009), the UKIDSS Galactic Plane Survey (Lucas et al. 2008) in the north, the VISTA Variables in the Via Lactea survey in the south (Minniti et al. 2010), and the recently published unWISE catalog (Sc”
• THE DISTANCE, MASS, AND RADIUS OF THE NEUTRON STAR IN 4U 1608−52 (2008, methodology): “The 2MASS JHK photometry is slightly shallower than that provided by the more recent UKIDSS Galactic Plane Survey (Lucas et al. 2008).”
• The VST Photometric Hα Survey of the Southern Galactic Plane and Bulge (VPHAS (2014, methodology): “Beyond the VVV sky area, there is a synergy to be exploited in bringing VPHAS+ data together with those of the all-sky 2MASS survey (Skrutskie et al. 2006) and with the UKIDSS Galactic Plane Survey (Lucas et al. 2008), in those parts of the first and third Galactic quadrants the latter has covered.”
• THE RED MSX SOURCE SURVEY: THE MASSIVE YOUNG STELLAR POPULATION OF OUR GALAXY (2013, methodology): “These data come from two surveys, the UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Plane Survey (GPS: Lucas et al. 2008) and the Vista Variables in the Via Lactea Survey (VVV: Minitti et al. 2010), both of which are deeper and have better spatial resolution than 2MASS. UKIDSS uses the UKIRT…”
• Hi-GAL, the Herschel infrared Galactic Plane Survey: Photometric maps and compact source catalogues: First data release for the inner Milky Way: +68° ≥ l ≥ -70° (2016, background): “The UKIDSS Galactic Plane Survey (Lucas et al., 2008) on the 4m UK Infrared Telescope on Hawaii covered the three near-IR photometric bands (J, H and K) to 18th magnitude, producing catalogues of over a billion stars.”
• The second data release of the INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS DR2) (2014, background): “There is a significant degree of overlap between the footprints of UKIDSS Galactic Plane Survey (GPS; Lucas et al. 2008) and IPHAS, and hence by adopting a similar catalogue format we hope to facilitate scientific applications which combine both data sets.”
• ATLASGAL — towards a complete sample of massive star forming clumps ⋆ (2014, methodology): “For this process, we start with near-infrared photometry from the 2MASS (Skrutskie et al. 2006), UKIDSS (Lucas et al. 2008) or Vista-VVV (Minniti et al. 2010) surveys and mid-infrared photometry taken from MSX (Egan et al. 2003) and WISE (Wright et al. 2010) – see Lumsden et al. (2013) for a discuss”
• ATLASGAL - The APEX telescope large area survey of the galaxy at 870 μm (2009, methodology): “The ATLASGAL data will thus be cross-correlated with similar large-scale Galactic sur- veys at other wavelengths, in the near- to far-infrared range, for example with theJ,H,K UKIDSS Galactic Plane Survey (Lucas et al. 2008), providing spectral energy distributions from ∼1 to 870µm.”
• Vvv dr1: the first data release of the milky way bulge and southern plane from the near-infrared eso public survey vista variables in the via lactea (2011, methodology): “The VVV Survey was designed to complement the UKIDSSGPS (Lucas et al. 2008), VPHAS+ (see Arnaboldi et al. 2007), and the GLIMPSE-II surveys (Benjamin et al. 2003).”