Jacob Noel-Storr

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Ser Amantio di Nicolao (talk | contribs) at 01:54, 25 April 2020 (→‎References: add authority control). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Jacob Noel-Storr
Born (1976-05-29) 29 May 1976 (age 47)
EducationPhD Astronomy, Columbia University (2004); MPhil Astronomy, Columbia University (2001); MA Astronomy, Columbia University (2000); MSci (Hons) Physics with Astrophysics, University of Birmingham (1998)
Employer(s)InsightSTEM, Inc., Rochester Institute of Technology (Former), University of Arizona (Former), Columbia University (Former)
Organization(s)AAS, Association for Astronomy Education, InsightSTEM
TitleSTEM Education and Outreach Professional

Dr. Jacob Noel-Storr is an astrophysics researcher and science education and outreach specialist researcher, Presently the President of InsightSTEM, Inc. He was a former assistant research professor at Rochester Institute of Technology, and assistant staff scientist in the Steward Observatory and Flandrau Science Center at the University of Arizona. He is known for his contributions to the study of Active Galactic Nuclei / Supermassive Black Holes, as well as science / astronomy education and outreach.

Published works

  • "VLBA Observations of MRK6: Probing the Jet-Lobe Connection", Kharb, P., O'Dea, C.P., Baum, S.A., Hardcastle, M.J., Dicken, D., Croston, J. H., Mingo, B., Noel-Storr, J. (2014), ApJ Accepted[1]
  • "Innovative Low Cost Science Education Technology Tools: Increasing Access to Science for All", Noel-Storr, J., Cole, B. N. (2012) in "Connecting People to Science: A National Congerence onf Science Education And Public Outreach." ASP Conference Series, Vol. 457. Eds. J.N. Jensen, J.G. Manning, M.G. Gibbs, and D. Daou. San Francisco: Astronomical Society of the Pacific, 2012., p. 317[2]
  • "VLBA and Chandra Observations of Jets in FR-I Radio Galaxies: Constraints on Jet Evolution", Kharb, P., O'Dea, C. P., Tilak, A., Baum, S. A., Haynes, E., Noel‐Storr, J., Fallon, C., Christiansen, K. (2012), ApJ 754:1 [3]
  • "Modeling the Infrared Emission in Cygnus A", Privon, G. C., Baum, S. A., O'Dea, C. P., Gallimore, J., Noel‐Storr, J., Axon, D. J., Robinson, A. (2012), ApJ 747:46[4]
  • "Hubble Space Telescope Far-ultraviolet Observations of Brightest Cluster Galaxies: The Role of Star Formation in Cooling Flows and BCG Evolution", O'Dea, K. P., et al. (Noel‐Storr, J. co‐author, 2010), ApJ 719:1619[5]
  • "Infrared Diagnostics for the Extended 12µm Sample of Seyferts", Baum, S. A., Gallimore, J.F., O'Dea, C. P., Buchanan, C. L., Noel-Storr, J., Axon, D. J., Robinson, A., Elitzur, M., Dorn, M., Staudaher, S. (2010), ApJ 710:298[6]
  • "Spitzer Observations of Star Formation in Brightest Cluster Galaxies", O'Dea, C. P., et al. (Noel-Storr, J. co-author, 2010), in "The Monster's Fiery Breath: Feedback in Galaxies, Groups and Clusters", AIP Conference Proceedings, Vol. 1201, p. 182[7]
  • "HST/ACS Emission Line Imaging of Low Redshift 3CR Radio Galaxies. I. The Data" Tremblay, G., et al. (Noel-Storr, J. co-author, 2009), ApJS 183:278[8]
  • "NASA Family Science Night: Changing Perceptions One Family at a Time", Mitchell, S., Drobnes, E., Collina-Trujillo, M. S., Noel-Storr, J. (2008) Adventures in Space Research 42:1844[9]
  • "An Infrared Survey of Brightest Cluster Galaxies II. Why are Some Brightest Cluster Galaxies Forming Stars?" O'Dea, C. P., Baum, S. A., Privon, G., Noel-Storr, J., et al. (2008) ApJ 681:1035[10]
  • "Family Astronomy: Improving Practices and Developing New Approaches" Noel-Storr, J., Drobnes, E., Mitchell, S. E. (2008), in "EPO and a Changing World: Creating Linkages and Expanding Partnerships: The 119th Annual Meeting of the Astronomical Society of the Pacific" Eds, Catharine Garmany and Michael G. Gibbs (vol. 389, p. 309)[11]
  • "An Infrared Survey of Brightest Cluster Galaxies I", Quillen et al., (Noel-Storr, J. co-author, 2008), ApJS 176:39[12]
  • "Unveiling the nature of Seyfert nuclei with 1–100 micron spectral energy distrobutions", Buchanan et al. (Noel-Storr, J. co-author, 2008), Memorie della Societa Astronomica Italiana, v. 79, p. 1140[13]

See also

References