Kim Coble's Publications
Here are some of my publications, talks and posters. See my CV for a full listing of publications, talks, and meetings.
Physics and Astronomy Education Research
Cosmology Education and Outreach
CMB: SZE
CMB: Boomerang
CMB: Python V
CMB: MSAM
Dark Energy
Light Element Abundances
Physics and Astronomy Education Research:
- Transferring Instructional Reforms into New Urban Learning Environments in Physics and Astronomy (AAPT National meeting, talk, July 2008)
- Applying Successful Techniques to Transform Physics and Astronomy in Urban Classrooms (PERC, poster, July 2008)
- Improvements in the Introductory Physics Courses at Chicago State University Part II : Evaluating the Effectiveness of Our Implementation (AAPT National meeting, talk, July 2006)
Cosmology Education and Outreach:
- The Big Bang Hapened Here: Cosmology for Non-Scientists (AAS talk, June 2004)
- Why Everyone Should Learn Something About the Universe and What We Can Do to Help (Fort Lewis College, Durango, CO, talk, Mar. 2004)
- Teaching Cosmology: What, Why, and How (University of Arizona, talk for CAPER team, Mar. 2004)
- What People Should Learn About Cosmology and Why (NSF AAPF Fellows Symposium talk, Jan. 2004)
- What Everyone Should Know About Cosmology (Lecture, Oct. 2003)
- Mapping the Universe from Antarctica (California Academy of Sciences, Dean Lecture, Sept. 2003; Carthage College, Oct. 2003; Lafayette College, Feb. 2004; DePaul University, Feb. 2004; Union College, Mar. 2004; includes some bonus slides not shown in talk)
- Museum Audiences and Virtual Environments (Collaboration Between Researchers and Museums Conference, June 2003)
- What Should People Learn About Cosmology and Why? (Boulder talk, May 2003)
- Mapping the Universe from Antarctica (Fort Lewis College, Durango, CO, talk, April 2003)
- Why Should People Learn Cosmology? (AAS poster, Jan 2003)
- The Big Picture: An Overview of Modern Cosmology (SII Lecture, Oct 2002)
- Research and Education in Cosmology: What I Am Doing and Why (AAS talk, June 2002)
- Astronomy Education: A Museum - University Partnership (AAS poster, June 2002)
- Python, Boomerang and Acbar: Different Ways of Mapping the Ancient Universe (Adler Planetarium Antarctica Day talk, May 2002)
- Mapping the Universe from Antarctica (Adler Planetarium Far Out Friday talk, Dec 2001)
- Setting the Stage: From the Big Bang to Galaxy Formation (Science Integration Origins workshop, Nov 2001)
- The Big Picture: A Perspective From Modern Cosmology (Science Integration/Education conference talk, Sept 2000)
- Radio Sources Toward Galaxy Clusters at 30 GHz (paper published in AJ)
- Radio Sources Toward Galaxy Clusters at 30 GHz (talk at Cosmic Cartography Conference, 2007)
- Observations of Galactic and Extra-galactic Sources From the BOOMERANG and SEST Telescopes
- BOOMERANG: A Balloon-borne Millimeter Wave Telescope and Total Power Receiver for Mapping Anisotropy in the Cosmic Microwave Background
- The BOOMERanG experiment and the curvature of the Universe
- Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology
- A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background
- Noise estimation in CMB time-streams and fast map-making. Application to the BOOMERanG98 data
- First results from the BOOMERanG experiment
- Detection of anisotropy in the Cosmic Microwave Background at horizon and sub-horizon scales with the BOOMERanG experiment
- The Cosmic Background Radiation circa nu2K
- The Quintessential CMB, Past & Future
- CMB Analysis of Boomerang & Maxima & the Cosmic Parameters {Omega_tot,Omega_b h^2,Omega_cdm h^2,Omega_Lambda,n_s}
- Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations
- First Estimations of Cosmological Parameters From BOOMERANG
- A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
- Galactic Foreground Constraints from the Python V Cosmic Microwave Background Anisotropy Data (analysis includes cross-correlations)
- Cosmic Microwave Background Anisotropy Measurement From Python V (analysis includes cross-correlations)
- The Data Reduction and Analysis of the Python V Cosmic Microwave Background Anisotropy Experiment (my thesis)
- Anisotropy in the Cosmic Microwave Background at Degree Angular Scales: Python V Results (astro-ph version) ApJ Letters version
- Anisotropy in the Cosmic Microwave Background at Degree Angular Scales: Python V Results (proceedings from the Texas Symposium on Relativistic Astrophysics, December 1998; similar to above but includes more pretty pictures)
- Cosmic Microwave Background Anisotropy: Python V Results (poster from AAS meeting, June 1998; updated figures April 5, 1999)
- Get Python V Window Functions
- New CMB Power Spectrum Constraints from MSAMI (ApJ version) astro-ph version
- CMB Window Functions and MSAM Results (poster from UCSB workshop, Nov 1997)
Home Research Education Publications Links Hobbies Travel
Disclaimer: Any opinions expressed here are are not the responsibility
of Chicago State University or the Department of Chemistry and Physics.
Some of this material is based upon work supported by the National Science Foundation
under the AAPF program. Any opinions, findings and conclusions or recomendations expressed
in this material do not necessarily reflect the views of the
National Science Foundation (NSF).
Last Modified Aug. 12, 2008
