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The 3D dust complexity maps used in the main result of Section 4 <a href="https://arxiv.org/abs/2404.11009">"Imprints of the Local Bubble and Dust Complexity on Polarized Dust Emission," Halal et al. 2024</a>. Use of these data must cite that paper. We provide 12 maps, corresponding to the 12 posterior sample 3D dust extinction maps of <a href="https://www.aanda.org/articles/aa/full_html/2024/05/aa47628-23/aa47628-23.html">Edenhofer et al. 2023</a>, which extend radially out to 1.25 kpc. The maps we provide are in Galactic coordinates and are only defined over the masks described in <a href="https://arxiv.org/abs/2404.11009">Halal et al. 2024</a>.
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Halal et al. 2023 3D HI-based Stokes Parameter Maps
The HI-based Stokes parameter maps used in (https://arxiv.org/abs/2306.10107) Filamentary Dust Polarization and the Morphology of HI Structures, Halal et al. 2023. Use of these data must cite that paper and (https://ui.adsabs.harvard.edu/abs/2019ApJ...887..136C/abstract) Clark & Hensley 2019. There are four sets of data cubes: one at Nside=1024 based on the 4' GALFA-HI data computed using the Spherical RHT algorithm, one at Nside=2048 based on the 4' GALFA-HI data smoothed to 7' computed using the Hessian algorithm, and two at Nside=1024 based on the 16.2' HI4PI data (one computed using the Spherical RHT algorithm and the other using the Hessian algorithm). A map based on the Hessian algorithm and the 16.2' HI4PI data, integrated over the velocity range -13 km/s to 16 km/s (Section 4.1 in Halal et al. 2023), is also available. The provided data cubes can be used to produce integrated maps over any velocity range desired. <br/><br/> These maps are given in units of K km/s and follow the Galactic IAU polarization convention. Multiply U by -1 to obtain maps corresponding to the COSMO convention as those provided by Planck. Multiply both Q and U by -1 to obtain maps corresponding to the magnetic field orientation in the IAU convention. <br/><br/> Please see (https://github.com/seclark/ClarkHensley2019) for code that demonstrates the use of data of the same format. The velocity binning of this data follows that of <a href="https://dataverse.harvard.edu/dataset.xhtml?persistentId=doi:10.7910/DVN/P41KDE">Clark & Hensley 2019</a> and can be found <a href="https://github.com/seclark/ClarkHensley2019/tree/master/data">here</a>.
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- Award ID(s):
- 2106607
- PAR ID:
- 10562788
- Publisher / Repository:
- Harvard Dataverse
- Date Published:
- Subject(s) / Keyword(s):
- Astronomy Astrophysics Dust Polarization
- Format(s):
- Medium: X Size: 2474900413; 343115439; 1440378273; 18543664; 2063599616; 2598113379; 18599423; 1458937575; 2517324464; 343756902; 301996800 Other: application/x-hdf5; application/x-hdf5; application/x-hdf5; application/x-hdf5; application/x-hdf5; application/x-hdf5; application/x-hdf5; application/x-hdf5; application/x-hdf5; application/x-hdf5; application/fits
- Size(s):
- 2474900413 343115439 1440378273 18543664 2063599616 2598113379 18599423 1458937575 2517324464 343756902 301996800
- Right(s):
- Creative Commons Zero v1.0 Universal
- Sponsoring Org:
- National Science Foundation
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{"Abstract":["The PPT survey extended from the Ross Ice Shelf, southward over the TAM along 150W between the Scott and Reedy Glaciers, and through the South Pole. Approximately 15,000 line km were flown. North-south oriented transects were flown 10 km apart and west-east tie lines were flown with a 30 km line spacing. Fifteen km long transect 'run-ins' and 'run-outs' were added to each line, thus ensuring data collection to survey boundaries. Laser altimetry, ice-penetrating radar, gravity and magnetic field intensity data were collected. This work was funded by NSF-OPP grant 9615832 with the project title: Collaborative Research: Contrasting Architecture and Dynamics of the Transantarctic Mountains (Pensacola-Pole Transect). Principal Investigators were D.D. Blankenship, University of Texas Institute for Geophysics, and R.E. Bell and W.R. Buck, Lamont-Doherty Earth Observatory.\n<br>\n<br>\nThis work was conducted by the Support Office for Aerogeophysical Research (SOAR) NSF facility under cooperative agreement OPP-9319379. The 1998/1999 field season <a href="http://hdl.handle.net/2152/65412"> report </a>(Holt et al 1999) describes the field work in more detail.\n<br>\n<br>\nThese data are gridded orthogonal data with a point every 850 m. Data is in a space delimited ASCII table with three columns: Longitude, Latitude and geophysical observation. Grids are smoothed using a Gaussian filter (2.125 km for gravity, magnetic field anomaly, surface elevation and 8.5 km for ice thickness) and surfaced using a bicubic spline method.\n<br>\nObservations include:\n<ol>\n<li> Bed elevation (m, WGS-84) </li> \n<li> Gravity disturbance (mGal, WGS-84) </li> \n<li> Ice Thickness (m) </li> \n<li> Laser Derived Surface Elevation (m, WGS-84) </li> \n<li> Magnetic Anomaly (nT, IGRF) </li> \n<li> Radar Derived Surface Elevation (m, WGS-84) </li> \n</ol>\nA browse image is included. \n<br><br>\n<i>Acknowledgement: </i><br>\nIn keeping with NSF Grant Policy, any publication using these data (including web documents) must contain the following acknowledgment: "This material is based on work supported by the National Science Foundation under cooperative agreement OPP-9319379." Also, any oral presentation utilizing these materials should acknowledge the support of the National Science Foundation. In addition, we request that any oral presentation, web page or publication also acknowledge SOAR and the University of Texas. A suitable citation for PPT data is:\n<br>\n<i>Davis, M.B., 2001, Subglacial Morphology and Structural Geology in the Southern Transantarctic Mountains from Airborne Geophysics, M.S. Thesis, Univ. of Texas, 133 pp.<a href="http://dx.doi.org/10.26153/tsw/2786">doi:10.26153/tsw/2786</a></i>\n<br>\nThese data represent the data that was hosted on the UTIG webpage at https://www-udc.ig.utexas.edu/external/facilities/aero/data/soar/PPT/SOAR_ppt.htm."]}more » « less
