Edward A. Baltz, Ph.D.

2000 University of California, Berkeley, Berkeley, CA 
Astronomy and Astrophysics
"Edward Baltz"
Mean distance: 14.35


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Joseph Ivor Silk grad student 2000 UC Berkeley
 (Signatures of dark matter.)
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Shara MM, Doyle T, Lauer TR, et al. (2017) AHubble Space TelescopeSurvey for Novae in M87. II. Snuffing out the Maximum Magnitude–Rate of Decline Relation for Novae as a Non-standard Candle, and a Prediction of the Existence of Ultrafast Novae The Astrophysical Journal. 839: 109
Shara MM, Doyle TF, Pagnotta A, et al. (2017) A Hubble Space Telescope survey for novae in M87 – III. Are novae good standard candles 15 d after maximum brightness? Monthly Notices of the Royal Astronomical Society. 474: 1746-1751
Shara MM, Doyle TF, Lauer TR, et al. (2016) A HUBBLE SPACE TELESCOPE SURVEY FOR NOVAE IN M87. I. LIGHT AND COLOR CURVES, SPATIAL DISTRIBUTIONS, AND THE NOVA RATE The Astrophysical Journal Supplement Series. 227: 1
Baltz EA, Marshall P, Oguri M. (2009) Analytic models of plausible gravitational lens potentials Journal of Cosmology and Astroparticle Physics. 2009
Waters CZ, Zepf SE, Lauer TR, et al. (2009) Color bimodality in M87 globular clusters Astrophysical Journal. 693: 463-471
Hooper D, Baltz EA. (2008) Strategies for determining the nature of dark matter Annual Review of Nuclear and Particle Science. 58: 293-314
Baltz EA, Berenji B, Bertone G, et al. (2008) Pre-launch estimates for GLAST sensitivity to dark matter annihilation signals Journal of Cosmology and Astroparticle Physics. 2008
Baltz EA, Taylor JE, Wai LL. (2007) Can astrophysical gamma-ray sources mimic dark matter annihilation in galactic satellites? Astrophysical Journal. 659
Taylor JE, Baltz EA, Wai LL. (2007) Will GLAST identify dark matter? Aip Conference Proceedings. 921: 178-180
Baltz EA, Battaglia M, Peskin ME, et al. (2006) Determination of dark matter properties at high-energy colliders Physical Review D - Particles, Fields, Gravitation and Cosmology. 74
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