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dc.contributor.authorKing, RR
dc.contributor.authorNaylor, T
dc.contributor.authorBroos, PS
dc.contributor.authorGetman, KV
dc.contributor.authorFeigelson, ED
dc.date.accessioned2016-06-14T12:55:44Z
dc.date.issued2013-11-14
dc.description.abstractWe present JHK infrared data from the UK InfraRed Telescope (UKIRT) for a subset of the regions of the Massive Young Star-Forming Complex Study in Infrared and X-ray (MYStIX) survey. Some of the data were obtained specifically for the MYStIX project, and some as part of the UKIRT Infrared Deep Sky Survey's Galactic Plane Survey. In most of these fields, crowding is a significant issue for aperture photometry, and so we have re-extracted the photometry from the processed images using an optimal extraction technique, and we describe how we adapt the optimal technique to mitigate the effects of crowding. © 2013. The American Astronomical Society. All rights reserved.en_GB
dc.description.sponsorshipThe MYStIX project is supported at Penn State by NASA grant NNX09AC74G, NSF grant AST-0908038, and the Chandra ACIS Team contract SV4-74018 (G. Garmire & L. Townsley, Principal Investigators), issued by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of NASA under contract NAS8-03060. This research made use of data products from the Chandra Data Archive.en_GB
dc.identifier.citationAstrophysical Journal, Supplement Series, Vol. 209, Number 2en_GB
dc.identifier.doi10.1088/0067-0049/209/2/28
dc.identifier.urihttp://hdl.handle.net/10871/22090
dc.language.isoenen_GB
dc.publisherAmerican Astronomical Societyen_GB
dc.rightsThis is the final version of the article. Available from the American Astronomical Society via the DOI in this record.en_GB
dc.titleThe MYStIX wide-field near-infrared data: Optimal photometry in crowded fieldsen_GB
dc.typeArticleen_GB
dc.date.available2016-06-14T12:55:44Z
dc.identifier.issn0067-0049
dc.identifier.journalAstrophysical Journal, Supplement Seriesen_GB


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