We have investigated origin firing and replicon dynamics in response to DSB formation. Following a transient induction of
HO in G1, wt
HO and
HO inc cells were released into S phase. Replication intermediates were analyzed by 2D-gels (
Brewer and Fangman, 1987). To preserve the replication intermediates we have psoralen-crosslinked the chromatin
in vivo prior to DNA extraction (
Sogo et al., 2002). We analyzed the fate of the replication intermediates arising from
ARS305 (). At 30 min. from G1 release, both
HO and
HO-inc strains accumulated bubble intermediates indicating that
ARS305 had fired (). Hence DSB formation close to an origin of replication does not prevent it from firing. The fact that very large bubble intermediates can be visualized indicates that the
ARS305 right fork (305R) reaches the proximity of the break site. In the
HO inc strain bubbles and large Y intermediates (that form when one of the forks migrates beyond the restriction fragment), gradually diminished in intensity. At 100 min. the replication intermediates are barely detectable but reappear at 150 min. due to a new round of DNA synthesis ( and data not shown). In the
HO strain, bubble and large Y signals are more intense than in the
HO-inc strain. At least two hypotheses, not mutually exclusive, may explain the relative increase in the intensity of bubble and Y structures in the
HO strain. The DSB may transiently slow down the progression of one or both
ARS305 forks. For instance, the accumulation of large Ys may result from the transient pausing of the 305R fork in proximity of the DSB. Alternatively, at each time point, a larger population of cells is replicating the
ARS305 region following DSB formation. To address whether the 305R fork transiently stalls in front of the DSB, we monitored the replication intermediates within a restriction fragment in which
ARS305 is placed asymmetrically (
Fig. SI2). If the 305R fork pauses long enough, then large bubble intermediates should be visualized, analogously to what shown for subtelomeric regions (
Makovets et al., 2004). We failed to detect large bubbles in the
HO strain (
Fig. SI2), thus suggesting that, if there is any 305R fork pausing, it does not persist long enough to be detected. Therefore, the 305R fork is rapidly resolved in proximity of the DSB giving rise to linear ends. The previous result leaves open the possibility that the accumulation of replication intermediates in the
HO strain may reflect a DSB-induced
ARS305 activation also in those cells that were not ready yet to fire it at that particular time. To address whether DSB formation can induce origin activation, we analyzed two dormant origins,
ARS313 and
ARS314, which are located at 6 and 3 kb respectively from the physiological HO cut site at the
MATa locus in strain CY6914. In the absence of the DSB, the genomic locus carrying
ARS313 and
ARS314 is replicated passively as only Y intermediates are detected, starting from 45 min. () (
Poloumienko et al., 2001). Following DSB formation at
MATa, however, Y structures appear 20 min earlier than in the strain lacking the cleavage site. (25 min. in ) and bubble-shaped intermediates accumulate at 45 min. Hence, DSB formation accelerates replication of the fragment containing
ARS313 and
ARS314 and triggers the firing of one or both origins. The digestion strategy described in does not allow us to visualize bubbles arising from
ARS314, as potential initiation events from this origin would generate Y intermediates. Moreover, the observation that intermediates resembling termination structures (
Greenfeder and Newlon, 1992;
Zhu et al., 1992) appear (arrow in ), also suggests that both
ARS313 and
ARS314 can fire within the same cell. The analysis of smaller restriction fragments containing either
ARS313 or
ARS314 indeed shows that both origins fire in response to DSB formation (
Fig. SI3). Hence, DSB formation triggers the firing of both dormant origins, despite the short inter-origin spacing that, in principle, should cause origin interference (
Brewer and Fangman, 1993). The DSB unlikely has a global effect on dormant origin firing as we did not observe a faster completion of S phase following DSB formation, as expected if all dormant origins were fired. These results suggest that origin activity is positively influenced by DSB formation. This could also account for the increased intensity of replication intermediates observed at
ARS305 in response to DSB formation.