Application of Medical Imaging Software to 3D Visualization of Astronomical Data Michelle Borkin Alyssa Goodman, Mike Halle, Doug Alan ADASS 2006 Conference.

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Presentation transcript:

Application of Medical Imaging Software to 3D Visualization of Astronomical Data Michelle Borkin Alyssa Goodman, Mike Halle, Doug Alan ADASS 2006 Conference October 17, 2006

And more… Astronomy Visualization IDL DS9 Karma 3D Slicer GAIA Aipsview

Channel Map Movie

Imaging Image Analysis Big Data Sets Globally Distributed Data AstroMed at the Initiative in Innovative Computing ( ) at Harvard AstronomyMedicine Initiative in Innovative Computing Harvard-Smithsonian Center for Astrophysics Surgical Planning Laboratory at Brigham and Women’s Hospital Harvard Medical School Martinos Center for Biomedical Imaging at Mass. General Hospital

3D Slicer Open source Modular (easy to contribute) Dedicated development staff Widely used in the medical community

3D Slicer Demo Movie RA Velocity DEC RA DEC Velocity RA DEC Muench et al 2003

3D Slicer - Segmentation CLUMPFIND 3D Slicer

OsiriX

OsiriX Demo Movie RA Velocity DEC

Molecular Cloud HH jet ~ 1pc HH knots Outflow lobes Outflows Note: not drawn to scale.Based on H. Arce Thesis Protostar

A Survey of Velocity Features in Perseus Visualize 12 CO data cube in 3D Slicer Mark high velocity points in 3D space, and export to astronomical software Identify outflows and calculate statistics

Outflow Identification in B5 Velocity DEC RA-DEC integrated map of 12CO RA

Outflow Identification Red Shifted points Blue Shifted points HH Objects SCF points IRAS Sources Known Outflow Sources New outflows Known outflows or outflow regions (not analyzed yet)

Future Research 3D Slicer for Astronomy: the ability to run segmentation algorithms, more detailed display options (ex. spectra and average spectra), tools for data quantification, and interoperability with online data bases (ex. NVO). Use of 3D Slicer: find velocity features such as outflows, determine other physical properties of clouds such as the number of clumps (and their size, location, and mass) in star forming regions, and visualization of algorithm output. For more information, go to

Questions? For more information, go to:

Outflow Identification Red Shifted points Blue Shifted points HH Objects SCF points IRAS Sources Known Outflow Sources c2d Sources

Future Research Red Shifted points Blue Shifted points HH Objects SCF points IRAS Sources Known Outflow Sources Finish cataloging Calculate outflow statistics

B5 Results Summation of all the spectra in Region 1 Summation of the spectra associated with outflows Summation of all the spectra associated with previously known outflows Gaussian fit Region 1 (B5)

B5 Results Summation of all the spectra in Region 1 All outflows previously detected outflows Gaussian fit High velocity gas High velocity gas from detected outflows