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1 , quasars, pulsars, and the 3 degrees cosmic background radiation).
2 birds in the Chernobyl region in relation to background radiation.
3 ht 'ripples' as seen in the cosmic microwave background radiation.
4 ude reduction in correlated poisoning due to background radiation.
5 also negatively correlated with the level of background radiation.
6 , which is only slightly higher than typical background radiation (3 mSv/year).
7 detections of anisotropy in cosmic microwave background radiation and observations of the large-scale
8 ity roughly three times the intensity of the background radiation and that undergo at least one perio
9  in adult bank voles is affected by ionizing background radiation, and potentially causing elevated l
10 ved anisotropies of the cosmic near-infrared background radiation are expected to have contributions
11 s); this energy now forms part of the cosmic background radiation at wavelengths near 1 mm.
12 cidence of cataracts increased with level of background radiation both in analyses based on a dichoto
13 (submm) galaxies have been resolved from the background radiation, but they have been difficult to st
14     The risk differences due to variation in background radiation can be larger than the risks associ
15 equently, accurately modeling and estimating background radiation can significantly improve our nucle
16 luctuations in the surface brightness of the background radiation caused by clustering or supercluste
17 ult of a search for anisotropy in the cosmic background radiation (CBR).
18 l comes from studies of the cosmic microwave background radiation (CMBR), the remnant heat from the i
19 e were exposed to 0.0002 cGy/min (~ 400-fold background radiation) continuously over 5 weeks.
20 on indicates that under these conditions the background radiation could have been released from a nea
21  and lead to a safer PET tracer with reduced background radiation dose.
22 members has been shown to be in the range of background radiation, even without restrictions on conta
23 vers a higher dose of radiation, the average background radiation exposure in the United States is 3
24 und transmission [LSO-TX]) that uses (176)Lu background radiation from detector scintillators with lo
25 duces a new data-driven approach to modeling background radiation from spectral measurements.
26                                         This background radiation gives rise mainly to random coincid
27 erefore possible that the elevated levels of background radiation in Chernobyl affect the ecology and
28  populations in areas with varying levels of background radiation in Chernobyl.
29 ld have produced significant cosmic infrared background radiation in the near-infrared, whose fluctua
30 high-dose procedures (>/=3 mSv; ie, 1 year's background radiation), including 1 (IQR, 1-2; mean, 1.8)
31 ysfunctional telomeres in DNA-PKcs-deficient backgrounds, radiation-induced instability, and breast c
32 precise measurements of the cosmic microwave background radiation, large galaxy redshift surveys, bet
33 ria isolated from the site with intermediate background radiation levels survived better and produced
34  from other study sites with higher or lower background radiation levels.
35 that high levels of spatial heterogeneity in background radiation may hamper adaptive life history re
36 tical to nuclear security, the complexity of background radiation modeling is intensified by dynamica
37  primarily develop as a function of ionizing background radiation, most likely as a plastic response
38  with the average annual effective dose from background radiation of about 3 mSv.
39 nucleosynthesis provides (with the microwave background radiation) one of the two quantitative experi
40 n studies of health hazards from exposure to background radiation, radon in homes, radiation in the w
41 nature of radiation emissions makes modeling background radiation structure a particularly challengin
42 tive relationship between bird abundance and background radiation when the frequency of cataracts was