1984
DOI: 10.1016/0009-2797(84)90033-4
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The effects of cis-platinum(II)diamminodichloride, UV light and N-methyl-N′-nitro-N-nitrosoguanidine on Escherichia coli: Plasmid mediated resistance to mutagens

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Cited by 20 publications
(25 citation statements)
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“…The best evidence for this involvement is the necessity of the umuC,D gene products for the expression of cisplatin induced mutagenesis 129,[131][132][133]. However, mutagenesis by cis-DDP in Escherichia coli is strongly reduced or abolished in either uvr A or uvrB mutants 25,127,130,133) while mutagenesis by classical SOS inducers such as ultraviolet irradiation are increased in uvr deficient strains 30).…”
Section: Mutagenic Platinum-dna Adductsmentioning
confidence: 96%
See 1 more Smart Citation
“…The best evidence for this involvement is the necessity of the umuC,D gene products for the expression of cisplatin induced mutagenesis 129,[131][132][133]. However, mutagenesis by cis-DDP in Escherichia coli is strongly reduced or abolished in either uvr A or uvrB mutants 25,127,130,133) while mutagenesis by classical SOS inducers such as ultraviolet irradiation are increased in uvr deficient strains 30).…”
Section: Mutagenic Platinum-dna Adductsmentioning
confidence: 96%
“…SOS mediated error-prone rapeir is implicated in the mutagenesis of both Salmonella typhimurium and Escherichia coli by cis-DDP 25,[129][130][131]. The best evidence for this involvement is the necessity of the umuC,D gene products for the expression of cisplatin induced mutagenesis 129,[131][132][133].…”
Section: Mutagenic Platinum-dna Adductsmentioning
confidence: 99%
“…We can obtain the value of the parameter m using the measured amplitude of temperature perturbations in the CMB [28,29] δ = 2 × 10 −5 , and as in [30,31], we get m = 7 × 10 −6 M pl (n − 1) 1/4 . The values for the slow roll parameters at the beginning of inflation can also be obtained by using (54) to give ǫ i = 8.3 × 10 −3 and η i = 8.3 × 10 −3 .…”
Section: A Inflation Driven By a Potential Fieldmentioning
confidence: 98%
“…Finally, we ran an additional set D simulation of another Milky Way-sized halo in a 67 Mpc comoving box with a mass resolution 8.2 × 10 4 M ⊙ and gravitational softening length 196 pc. Table 1 lists sets of cosmological parameters from measurements of the cosmic microwave background by WMAP and the Planck mission (Spergel et al 2003(Spergel et al , 2007Komatsu et al 2009;Larson et al 2010;Jarosik et al 2010;Komatsu et al 2011;Hinshaw et al 2012;Planck Collaboration et al 2013). "Bolshoi" are the parameters from the Bolshoi simulation (Klypin, Trujillo-Gomez & Primack 2011) which were chosen to be within 1σ of WMAP5, WMAP7, and consistent with the results of supernovae, and X-ray cluster surveys.…”
Section: Simulationsmentioning
confidence: 99%