The Bolocam Galactic Plane Survey: Survey Description and Data Reduction

dc.contributor.utaustinauthorDunham, Miranda K.en_US
dc.contributor.utaustinauthorEvans, Neal J., IIen_US
dc.creatorAguirre, James E.en_US
dc.creatorGinsburg, Adam G.en_US
dc.creatorDunham, Miranda K.en_US
dc.creatorDrosback, Meredith M.en_US
dc.creatorBally, Johnen_US
dc.creatorBattersby, Caraen_US
dc.creatorBradley, Eric Todden_US
dc.creatorCyganowski, Claudiaen_US
dc.creatorDowell, Darrenen_US
dc.creatorEvans, Neal J., IIen_US
dc.creatorGlenn, Jasonen_US
dc.creatorHarvey, Paulen_US
dc.creatorRosolowsky, Eriken_US
dc.creatorStringfellow, Guy S.en_US
dc.creatorWalawender, Joshen_US
dc.creatorWilliams, Jonathan P.en_US
dc.date.accessioned2016-10-28T19:35:57Z
dc.date.available2016-10-28T19:35:57Z
dc.date.issued2011-01en_US
dc.description.abstractWe present the Bolocam Galactic Plane Survey (BGPS), a 1.1 mm continuum survey at 33 '' effective resolution of 170 deg(2) of the Galactic Plane visible from the northern hemisphere. The BGPS is one of the first large area, systematic surveys of the Galactic Plane in the millimeter continuum without pre-selected targets. The survey is contiguous over the range-10.5 <= l <= 90.5, vertical bar b vertical bar <= 0.5. Toward the Cygnus X spiral arm, the coverage was flared to vertical bar b vertical bar <= 1.5 for 75.5 <= l <= 87.5. In addition, cross-cuts to vertical bar b vertical bar <= 1.5 were made at l = 3, 15, 30, and 31. The total area of this section is 133 deg(2). With the exception of the increase in latitude, no pre-selection criteria were applied to the coverage in this region. In addition to the contiguous region, four targeted regions in the outer Galaxy were observed: IC1396 (9 deg(2), 97.5 <= l <= 100.5, 2.25 <= b <= 5.25), a region toward the Perseus Arm (4 deg(2) centered on l = 111, b = 0 near NGC 7538), W3/4/5 (18 deg(2), 132.5 <= l <= 138.5), and Gem OB1 (6 deg(2), 187.5 <= l <= 193.5). The survey has detected approximately 8400 clumps over the entire area to a limiting non-uniform 1s noise level in the range 11-53 mJy beam(-1) in the inner Galaxy. The BGPS source catalog is presented in a previously published companion paper. This paper details the survey observations and data reduction methods for the images. We discuss in detail the determination of astrometric and flux density calibration uncertainties and compare our results to the literature. Data processing algorithms that separate astronomical signals from time-variable atmospheric fluctuations in the data timestream are presented. These algorithms reproduce the structure of the astronomical sky over a limited range of angular scales and produce artifacts in the vicinity of bright sources. Based on simulations, we find that extended emission on scales larger than about 5'.9 is nearly completely attenuated (>90%) and the linear scale at which the attenuation reaches 50% is 3'.8. Comparison with other millimeter-wave data sets implies a possible systematic offset in flux calibration, for which no cause has been discovered. This presentation serves as a companion and guide to the public data release (http://irsa.ipac.caltech.edu/Missions/bolocam.html) through NASA's Infrared Processing and Analysis Center (IPAC) Infrared Science Archive (IRSA). New data releases will be provided through IPAC-IRSA with any future improvements in the reduction. The BGPS provides a complementary long-wavelength spectral band for the ongoing ATLASGAL and Herschel-SPIRE surveys, and an important database and context for imminent observations with SCUBA-2 and ALMA.en_US
dc.description.departmentAstronomyen_US
dc.description.sponsorshipNSF AST-0838261en_US
dc.description.sponsorshipNational Science Foundation NSF AST-0708403, AST-0607793en_US
dc.description.sponsorshipNational Radio Astronomy Observatory (NRAO)en_US
dc.identifierdoi:10.15781/T24X54K18
dc.identifier.citationAguirre, James E., Adam G. Ginsburg, Miranda K. Dunham, Meredith M. Drosback, John Bally, Cara Battersby, Eric Todd Bradley et al. "The Bolocam Galactic Plane Survey: survey description and data reduction." The Astrophysical Journal Supplement Series, Vol. 192, No. 1 (Jan., 2011): 4.en_US
dc.identifier.doi10.1088/0067-0049/192/1/4en_US
dc.identifier.issn0067-0049en_US
dc.identifier.urihttp://hdl.handle.net/2152/42997
dc.language.isoEnglishen_US
dc.relation.ispartofen_US
dc.relation.ispartofserialAstrophysical Journal Supplement Seriesen_US
dc.rightsAdministrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en_US
dc.rights.restrictionOpenen_US
dc.subjectism: cloudsen_US
dc.subjectmethods: data analysisen_US
dc.subjectstars: Formationen_US
dc.subjectstars: massiveen_US
dc.subjectsubmillimeter: ismen_US
dc.subjectsurveysen_US
dc.subjectinfrared-dark cloudsen_US
dc.subjectdust continuum emissionen_US
dc.subjectc2d legacy cloudsen_US
dc.subjectstar-forming regionsen_US
dc.subjectmolecular clouden_US
dc.subjectphysical-propertiesen_US
dc.subjectdense coresen_US
dc.subjectmilky-wayen_US
dc.subjectmu-men_US
dc.subjectsubmillimeteren_US
dc.subjectastronomy & astrophysicsen_US
dc.titleThe Bolocam Galactic Plane Survey: Survey Description and Data Reductionen_US
dc.typeArticleen_US

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