He was the principal investigator of the BICEP2 telescope, which was part of the BICEP and Keck Array series of experiments.[3][4][5] Measurements announced on 17 March 2014 from the BICEP2 telescope appeared to support the idea of cosmic inflation, by reporting the first evidence for a primordial B-Mode pattern in the polarization of the CMB.[6][7][8] Further analysis revealed this result to be spurious, and that the signal had been contaminated by interstellar dust in the Milky Way.[9]
Prior to BICEP2, as a graduate student at the University of Chicago, Kovac worked on the Degree Angular Scale Interferometer led by John Carlstrom, which in 2002 announced the first detection of polarization in the CMB.[10] In 2003, Kovac moved to Caltech as a Millikan Postdoctoral Fellow, beginning work under Andrew Lange on the QUaD telescope and on BICEP1, the predecessor of BICEP2. After BICEP1's deployment to the South Pole in 2006, at Lange's invitation Kovac joined the research faculty of Caltech as a Kilroy Fellow and led the team that proposed BICEP2. In 2009 Kovac joined the faculty at Harvard University.[11]
^BICEP2 Collaboration, BICEP2; R Ade, P. A.; Aikin, R. W.; Barkats, D.; Benton, S. J.; Bischoff, C. A.; Bock, J. J.; Brevik, J. A.; Buder, I.; Bullock, E.; Dowell, C. D.; Duband, L.; Filippini, J. P.; Fliescher, S.; Golwala, S. R.; Halpern, M.; Hasselfield, M.; Hildebrandt, S. R.; Hilton, G. C.; Hristov, V. V.; Irwin, K. D.; Karkare, K. S.; Kaufman, J. P.; Keating, B. G.; Kernasovskiy, S. A.; Kovac, J. M.; Kuo, C. L.; Leitch, E. M.; Lueker, M.; et al. (2014). "BICEP2 I: Detection Of B-mode Polarization at Degree Angular Scales". Physical Review Letters. 112 (24): 241101. arXiv:1403.3985. Bibcode:2014PhRvL.112x1101B. doi:10.1103/PhysRevLett.112.241101. PMID24996078. S2CID22780831.{{cite journal}}: CS1 maint: numeric names: authors list (link)