186 research outputs found

    Characterization of magnesium requirement of human 5'-tyrosyl DNA phosphodiesterase mediated reaction

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    <p>Abstract</p> <p>Background</p> <p>Topo-poisons can produce an enzyme-DNA complex linked by a 3'- or 5'-phosphotyrosyl covalent bond. 3'-phosphotyrosyl bonds can be repaired by tyrosyl DNA phosphodiesterase-1 (TDP1), an enzyme known for years, but a complementary human enzyme 5'-tyrosyl DNA phosphodiesterase (hTDP2) that cleaves 5'-phosphotyrosyl bonds has been reported only recently. Although hTDP2 possesses both 3'- and 5'- tyrosyl DNA phosphodiesterase activity, the role of Mg<sup>2+ </sup>in its activity was not studied in sufficient details.</p> <p>Results</p> <p>In this study we showed that purified hTDP2 does not exhibit any 5'-phosphotyrosyl phosphodiesterase activity in the absence of Mg<sup>2+</sup>/Mn<sup>2+</sup>, and that neither Zn<sup>2+ </sup>or nor Ca<sup>2+ </sup>can activate hTDP2. Mg<sup>2+ </sup>also controls 3'-phosphotyrosyl activity of TDP2. In MCF-7 cell extracts and de-yolked zebrafish embryo extracts, Mg<sup>2+ </sup>controlled 5'-phosphotyrosyl activity. This study also showed that there is an optimal Mg<sup>2+ </sup>concentration above which it is inhibitory for hTDP2 activity.</p> <p>Conclusion</p> <p>These results altogether reveal the optimal Mg<sup>2+ </sup>requirement in hTDP2 mediated reaction.</p

    Observational Constraints on the Merger History of Galaxies since z ≈ 6: Probabilistic Galaxy Pair Counts in the CANDELS Fields

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    Galaxy mergers are expected to have a significant role in the mass assembly of galaxies in the early Universe, but there are very few observational constraints on the merger history of galaxies at z>2z>2. We present the first study of galaxy major mergers (mass ratios >> 1:4) in mass-selected samples out to z≈6z\approx6. Using all five fields of the HST/CANDELS survey and a probabilistic pair count methodology that incorporates the full photometric redshift posteriors and corrections for stellar mass completeness, we measure galaxy pair-counts for projected separations between 5 and 30 kpc in stellar mass selected samples at 9.7<log⁥10(M∗/M⊙)<10.39.7 < \log_{10}(\rm{M}_{*}/\rm{M}_{\odot}) < 10.3 and log⁥10(M∗/M⊙)>10.3\log_{10}(\rm{M}_{*}/\rm{M}_{\odot}) > 10.3. We find that the major merger pair fraction rises with redshift to z≈6z\approx6 proportional to (1+z)m(1+z)^{m}, with m=0.8±0.2m = 0.8\pm0.2 (m=1.8±0.2m = 1.8\pm0.2) for log⁥10(M∗/M⊙)>10.3\log_{10}(\rm{M}_{*} / \rm{M}_{\odot}) > 10.3 (9.7<log⁥10(M∗/M⊙)<10.39.7 < \log_{10}(\rm{M}_{*}/\rm{M}_{\odot}) < 10.3). Investigating the pair fraction as a function of mass ratio between 1:20 and 1:1, we find no evidence for a strong evolution in the relative numbers of minor to major mergers out to z<3z<3. Using evolving merger timescales we find that the merger rate per galaxy (R\mathcal{R}) rises rapidly from 0.07±0.010.07\pm 0.01 Gyr−1^{-1} at z<1z < 1 to 7.6±2.77.6\pm 2.7 Gyr−1^{-1} at z=6z = 6 for galaxies at log⁥10(M∗/M⊙)>10.3\log_{10}(\rm{M}_{*}/\rm{M}_{\odot}) > 10.3. The corresponding co-moving major merger rate density remains roughly constant during this time, with rates of Γ≈10−4\Gamma \approx 10^{-4} Gyr−1^{-1} Mpc−3^{-3}. Based on the observed merger rates per galaxy, we infer specific mass accretion rates from major mergers that are comparable to the specific star-formation rates for the same mass galaxies at z>3z>3 - observational evidence that mergers are as important a mechanism for building up mass at high redshift as in-situ star-formation.Comment: 36 pages, 17 figures. Accepted for publication in Ap

    Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations

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