Inhibition of type IA topoisomerase by a monoclonal antibody through perturbation of DNA cleavage-religation equilibrium

Type IA DNA topoisomerases, typically found in bacteria, are essential enzymes that catalyse the DNA relaxation of negative supercoils. DNA gyrase is the only type II topoisomerase that can carry out the opposite reaction (i.e. the introduction of the DNA supercoils). A number of diverse molecules target DNA gyrase. However, inhibitors that arrest the activity of bacterial topoisomerase I at low concentrations remain to be identified. Towards this end, as a proof of principle, monoclonal antibodies that inhibit Mycobacterium smegmatis topoisomerase I have been characterized and the specific inhibition of Mycobacterium smegmatis topoisomerase I by a monoclonal antibody, 2F3G4, at a nanomolar concentration is described. The enzyme-bound monoclonal antibody stimulated the first transesterification reaction leading to enhanced DNA cleavage, without significantly altering the religation activity of the enzyme. The stimulated DNA cleavage resulted in perturbation of the cleavagereligation equilibrium, increasing single-strand nicks and proteinDNA covalent adducts. Monoclonal antibodies with such a mechanism of inhibition can serve as invaluable tools for probing the structure and mechanism of the enzyme, as well as in the design of novel inhibitors that arrest enzyme activity.

Type IA topoisomerase inhibition by clamp closure

Bacterial DNA topoisomerase I (topoI) catalyzes relaxation of negatively supercoiled DNA. The enzyme alters DNA topology through protein-operated DNA gate, switching between open and closed conformations during its reaction. We describe the mechanism of inhibition of Mycobacterium smegmatis and Mycobacterium tuberculosis topoI by monoclonal antibodies (mAbs) that bind with high affinity and inhibit at 10-50 nM concentration. Unlike other inhibitors of topoisomerases, the mAbs inhibited several steps of relaxation reaction, namely DNA binding, cleavage, strand passage, and enzyme-DNA dissociation. The enhanced religation of the cleaved DNA in presence of the mAb indicated closing of the enzyme DNA gate. The formation of enzyme-DNA heterocatenane in the presence of the mAbs as a result of closing the gate could be inferred by the salt resistance of the complex, visualized by atomic force microscopy and confirmed by fluorescence measurements. Locking the enzyme-DNA complex as a closed clamp restricted the movements of the DNA gate, affecting all of the major steps of the relaxation reaction. Enzyme trapped on DNA in closed clamp conformation formed roadblock for the elongating DNA polymerase. The unusual multistep inhibition of mycobacterial topoisomerases may facilitate lead molecule development, and the mAbs would also serve as valuable tools to probe the enzyme mechanism.

Rôle des topoisomérases de type IA dans la ségrégation des chromosomes chez Escherichia coli

Les topoisomérases I (topA) et III (topB) sont les deux topoisomérases (topos) de type IA d’Escherichia coli. La fonction principale de la topo I est la relaxation de l’excès de surenroulement négatif, tandis que peu d’information est disponible sur le rôle de la topo III. Les cellules pour lesquelles les deux topoisomérases de type IA sont manquantes souffrent d’une croissance difficile ainsi que de défauts de ségrégation sévères. Nous démontrons que ces problèmes sont majoritairement attribuables à des mutations dans la gyrase qui empêchent l’accumulation d’excès de surenroulement négatif chez les mutants sans topA. L’augmentation de l’activité de la gyrase réalisée par le remplacement de l’allèle gyrB(Ts) par le gène de type sauvage ou par l’exposition des souches gyrB(Ts) à une température permissive, permet la correction significative de la croissance et de la ségrégation des cellules topos de type IA. Nous démontrons également que les mutants topB sont hypersensibles à l’inhibition de la gyrase par la novobiocine. La réplication non-régulée en l’absence de topA et de rnhA (RNase HI) augmente la nécessité de l’activité de la topoisomérase III. De plus, en l’absence de topA et de rnhA, la surproduction de la topoisomérase III permet de réduire la dégradation importante d’ADN qui est observée en l’absence de recA (RecA). Nous proposons un rôle pour la topoisomérase III dans la ségrégation des chromosomes lorsque l’activité de la gyrase n’est pas optimale, par la réduction des collisions fourches de réplication s’observant particulièrement en l’absence de la topo I et de la RNase HI.

Genetic studies on the role of type IA DNA topoisomerases in DNA metabolism and genome maintenance in Escherichia coli

Le surenroulement de l’ADN est important pour tous les processus cellulaires qui requièrent la séparation des brins de l’ADN. Il est régulé par l’activité enzymatique des topoisomérases. La gyrase (gyrA et gyrB) utilise l’ATP pour introduire des supertours négatifs dans l’ADN, alors que la topoisomérase I (topA) et la topoisomérase IV (parC et parE) les éliminent. Les cellules déficientes pour la topoisomérase I sont viables si elles ont des mutations compensatoires dans un des gènes codant pour une sous-unité de la gyrase. Ces mutations réduisent le niveau de surenroulement négatif du chromosome et permettent la croissance bactérienne. Une de ces mutations engendre la production d'une gyrase thermosensible. L’activité de surenroulement de la gyrase en absence de la topoisomérase I cause l’accumulation d’ADN hyper-surenroulé négativement à cause de la formation de R-loops. La surproduction de la RNase HI (rnhA), une enzyme qui dégrade l’ARN des R-loops, permet de prévenir l’accumulation d’un excès de surenroulement négatif. En absence de RNase HI, des R-loops sont aussi formés et peuvent être utilisés pour déclencher la réplication de l’ADN indépendamment du système normal oriC/DnaA, un phénomène connu sous le nom de « constitutive stable DNA replication » (cSDR). Pour mieux comprendre le lien entre la formation de R-loops et l’excès de surenroulement négatif, nous avons construit un mutant conditionnel topA rnhA gyrB(Ts) avec l’expression inductible de la RNase HI à partir d’un plasmide. Nous avons trouvé que l’ADN des cellules de ce mutant était excessivement relâché au lieu d'être hypersurenroulé négativement en conditions de pénurie de RNase HI. La relaxation de l’ADN a été montrée comme étant indépendante de l'activité de la topoisomérase IV. Les cellules du triple mutant topA rnhA gyrB(Ts) forment de très longs filaments remplis d’ADN, montrant ainsi un défaut de ségrégation des chromosomes. La surproduction de la topoisomérase III (topB), une enzyme qui peut effectuer la décaténation de l’ADN, a corrigé les problèmes de ségrégation sans toutefois restaurer le niveau de surenroulement de l’ADN. Nous avons constaté que des extraits protéiques du mutant topA rnhA gyrB(Ts) pouvaient inhiber l’activité de surenroulement négatif de la gyrase dans des extraits d’une souche sauvage, suggérant ainsi que la pénurie de RNase HI avait déclenché une réponse cellulaire d’inhibition de cette activité de la gyrase. De plus, des expériences in vivo et in vitro ont montré qu’en absence de RNase HI, l’activité ATP-dépendante de surenroulement négatif de la gyrase était inhibée, alors que l’activité ATP-indépendante de cette enzyme demeurait intacte. Des suppresseurs extragéniques du défaut de croissance du triple mutant topA rnhA gyrB(Ts) qui corrigent également les problèmes de surenroulement et de ségrégation des chromosomes ont pour la plupart été cartographiés dans des gènes impliqués dans la réplication de l’ADN, le métabolisme des R-loops, ou la formation de fimbriae. La deuxième partie de ce projet avait pour but de comprendre les rôles des topoisomérases de type IA (topoisomérase I et topoisomérase III) dans la ségrégation et la stabilité du génome de Escherichia coli. Pour étudier ces rôles, nous avons utilisé des approches de génétique combinées avec la cytométrie en flux, l’analyse de type Western blot et la microscopie. Nous avons constaté que le phénotype Par- et les défauts de ségrégation des chromosomes d’un mutant gyrB(Ts) avaient été corrigés en inactivant topA, mais uniquement en présence du gène topB. En outre, nous avons démontré que la surproduction de la topoisomérase III pouvait corriger le phénotype Par- du mutant gyrB(Ts) sans toutefois corriger les défauts de croissance de ce dernier. La surproduction de topoisomérase IV, enzyme responsable de la décaténation des chromosomes chez E. coli, ne pouvait pas remplacer la topoisomérase III. Nos résultats suggèrent que les topoisomérases de type IA jouent un rôle important dans la ségrégation des chromosomes lorsque la gyrase est inefficace. Pour étudier le rôle des topoisomérases de type IA dans la stabilité du génome, la troisième partie du projet, nous avons utilisé des approches génétiques combinées avec des tests de « spot » et la microscopie. Nous avons constaté que les cellules déficientes en topoisomérase I avaient des défauts de ségrégation de chromosomes et de croissance liés à un excès de surenroulement négatif, et que ces défauts pouvaient être corrigés en inactivant recQ, recA ou par la surproduction de la topoisomérase III. Le suppresseur extragénique oriC15::aph isolé dans la première partie du projet pouvait également corriger ces problèmes. Les cellules déficientes en topoisomérases de type IA formaient des très longs filaments remplis d’ADN d’apparence diffuse et réparti inégalement dans la cellule. Ces phénotypes pouvaient être partiellement corrigés par la surproduction de la RNase HI ou en inactivant recA, ou encore par des suppresseurs isolés dans la première partie du projet et impliques dans le cSDR (dnaT18::aph et rne59::aph). Donc, dans E. coli, les topoisomérases de type IA jouent un rôle dans la stabilité du génome en inhibant la réplication inappropriée à partir de oriC et de R-loops, et en empêchant les défauts de ségrégation liés à la recombinaison RecA-dépendante, par leur action avec RecQ. Les travaux rapportés ici révèlent que la réplication inappropriée et dérégulée est une source majeure de l’instabilité génomique. Empêcher la réplication inappropriée permet la ségrégation des chromosomes et le maintien d’un génome stable. La RNase HI et les topoisomérases de type IA jouent un rôle majeur dans la prévention de la réplication inappropriée. La RNase HI réalise cette tâche en modulant l’activité de surenroulement ATP-dependante de la gyrase, et en empêchant la réplication à partir des R-loops. Les topoisomérases de type IA assurent le maintien de la stabilité du génome en empêchant la réplication inappropriée à partir de oriC et des R-loops et en agissant avec RecQ pour résoudre des intermédiaires de recombinaison RecA-dépendants afin de permettre la ségrégation des chromosomes.

New Mass Limit for White Dwarfs: Super-Chandrasekhar Type Ia Supernova as a New Standard Candle

Type Ia supernovae, sparked off by exploding white dwarfs of mass close to the Chandrasekhar limit, play the key role in understanding the expansion rate of the Universe. However, recent observations of several peculiar type Ia supernovae argue for its progenitor mass to be significantly super-Chandrasekhar. We show that strongly magnetized white dwarfs not only can violate the Chandrasekhar mass limit significantly, but exhibit a different mass limit. We establish from a foundational level that the generic mass limit of white dwarfs is 2.58 solar mass. This explains the origin of overluminous peculiar type Ia supernovae. Our finding further argues for a possible second standard candle, which has many far reaching implications, including a possible reconsideration of the expansion history of the Universe. DOI: 10.1103/PhysRevLett.110.071102

A POSSIBLE EVOLUTIONARY SCENARIO OF HIGHLY MAGNETIZED SUPER-CHANDRASEKHAR WHITE DWARFS: PROGENITORS OF PECULIAR TYPE Ia SUPERNOVAE

Several recently discovered peculiar Type Ia supernovae seem to demand an altogether new formation theory that might help explain the puzzling dissimilarities between them and the standard Type Ia supernovae. The most striking aspect of the observational analysis is the necessity of invoking super-Chandrasekhar white dwarfs having masses similar to 2.1-2.8 M-circle dot, M-circle dot being the mass of Sun, as their most probable progenitors. Strongly magnetized white dwarfs having super-Chandrasekhar masses have already been established as potential candidates for the progenitors of peculiar Type Ia supernovae. Owing to the Landau quantization of the underlying electron degenerate gas, theoretical results yielded the observationally inferred mass range. Here, we sketch a possible evolutionary scenario by which super-Chandrasekhar white dwarfs could be formed by accretion on to a commonly observed magnetized white dwarf, invoking the phenomenon of flux freezing. This opens multiple possible evolution scenarios ending in supernova explosions of super-Chandrasekhar white dwarfs having masses within the range stated above. We point out that our proposal has observational support, such as the recent discovery of a large number of magnetized white dwarfs by the Sloan Digital Sky Survey.

Conditional silencing of topoisomerase I gene of Mycobacterium tuberculosis validates its essentiality for cell survival

Topoisomerases are an important class of enzymes for regulating the DNA transaction processes. Mycobacterium tuberculosis (Mtb) is one of the most formidable pathogens also posing serious challenges for therapeutic interventions. The organism contains only one type IA topoisomerase (Rv3646c), offering an opportunity to test its potential as a candidate drug target. To validate the essentiality of M.tuberculosis topoisomerase I (TopoI(Mt)) for bacterial growth and survival, we have generated a conditionally regulated strain of topoI in Mtb. The conditional knockdown mutant exhibited delayed growth on agar plate. In liquid culture, the growth was drastically impaired when TopoI expression was suppressed. Additionally, novobiocin and isoniazid showed enhanced inhibitory potential against the conditional mutant. Analysis of the nucleoid revealed its altered architecture upon TopoI depletion. These studies establish the essentiality of TopoI for the M.tuberculosis growth and open up new avenues for targeting the enzyme.

Inhibition of Mycobacterium tuberculosis topoisomerase I by m-AMSA, a eukaryotic type II topoisomerase poison

m-AMSA, an established inhibitor of eukaryotic type II topoisomerases, exerts its cidal effect by binding to the enzyme-DNA complex thus inhibiting the DNA religation step. The molecule and its analogues have been successfully used as chemotherapeutic agents against different forms of cancer. After virtual screening using a homology model of the Mycobacterium tuberculosis topoisomerase I, we identified m-AMSA as a high scoring hit. We demonstrate that m-AMSA can inhibit the DNA relaxation activity of topoisomerase I from M. tuberculosis and Mycobacterium smegmatis. In a whole cell assay, m-AMSA inhibited the growth of both the mycobacteria. (C) 2014 Elsevier Inc. All rights reserved.

Direct control of type IIA topoisomerase activity by a chromosomally encoded regulatory protein

Precise control of supercoiling homeostasis is critical to DNA-dependent processes such as gene expression, replication, and damage response. Topoisomerases are central regulators of DNA supercoiling commonly thought to act independently in the recognition and modulation of chromosome superstructure; however, recent evidence has indicated that cells tightly regulate topoisomerase activity to support chromosome dynamics, transcriptional response, and replicative events. How topoisomerase control is executed and linked to the internal status of a cell is poorly understood. To investigate these connections, we determined the structure of Escherichia coil gyrase, a type HA topoisomerase bound to YacG, a recently identified chromosomally encoded inhibitor protein. Phylogenetic analyses indicate that YacG is frequently associated with coenzyme A (CoA) production enzymes, linking the protein to metabolism and stress. The structure, along with supporting solution studies, shows that YacG represses gyrase by sterically occluding the principal DNA-binding site of the enzyme. Unexpectedly, YacG acts by both engaging two spatially segregated regions associated with small-molecule inhibitor interactions (fluoroquinolone antibiotics and the newly reported antagonist GSK299423) and remodeling the gyrase holo enzyme into an inactive, ATP-trapped configuration. This study establishes a new mechanism for the protein-based control of topoisomerases, an approach that may be used to alter supercoiling levels for responding to changes in cellular state.

Modified Einstein's gravity as a possible missing link between sub- and super-Chandrasekhar type Ia supernovae

We explore the effect of modification to Einstein's gravity in white dwarfs for the first time in the literature, to the best of our knowledge. This leads to significantly sub- and super-Chandrasekhar limiting masses of white dwarfs, determined by a single model parameter. On the other hand, type Ia supernovae (SNeIa), a key to unravel the evolutionary history of the universe, are believed to be triggered in white dwarfs having mass close to the Chandrasekhar limit. However, observations of several peculiar, under- and over-luminous SNeIa argue for exploding masses widely different from this limit. We argue that explosions of the modified gravity induced sub- and super-Chandrasekhar limiting mass white dwarfs result in under- and over-luminous SNeIa respectively, thus unifying these two apparently disjoint sub-classes and, hence, serving as a missing link. Our discovery raises two fundamental questions. Is the Chandrasekhar limit unique? Is Einstein's gravity the ultimate theory for understanding astronomical phenomena? Both the answers appear to be no!

Imprint of modified Einstein's gravity on white dwarfs: Unifying Type Ia supernovae

We establish the importance of modified Einstein's gravity (MG) in white dwarfs (WDs) for the first time in the literature. We show that MG leads to significantly sub- and super-Chandrasekhar limiting mass WDs, depending on a single model parameter. However, conventional WDs on approaching Chandrasekhar's limit are expected to trigger Type Ia supernovae (SNeIa), a key to unravel the evolutionary history of the universe. Nevertheless, observations of several peculiar, under-and over-luminous SNeIa argue for the limiting mass widely different from Chandrasekhar's limit. Explosions of MG induced sub-and super-Chandrasekhar limiting mass WDs explain under-and over-luminous SNeIa respectively, thus unifying these two apparently disjoint sub-classes. Our discovery questions both the global validity of Einstein's gravity and the uniqueness of Chandrasekhar's limit.

The upstream enhancer elements of the G6PC promoter are critical for optimal G6PC expression in murine glycogen storage disease type Ia.

Glycogen storage disease type-Ia (GSD-Ia) patients deficient in glucose-6-phosphatase-α (G6Pase-α or G6PC) manifest impaired glucose homeostasis characterized by fasting hypoglycemia, growth retardation, hepatomegaly, nephromegaly, hyperlipidemia, hyperuricemia, and lactic acidemia. Two efficacious recombinant adeno-associated virus pseudotype 2/8 (rAAV8) vectors expressing human G6Pase-α have been independently developed. One is a single-stranded vector containing a 2864-bp of the G6PC promoter/enhancer (rAAV8-GPE) and the other is a double-stranded vector containing a shorter 382-bp minimal G6PC promoter/enhancer (rAAV8-miGPE). To identify the best construct, a direct comparison of the rAAV8-GPE and the rAAV8-miGPE vectors was initiated to determine the best vector to take forward into clinical trials. We show that the rAAV8-GPE vector directed significantly higher levels of hepatic G6Pase-α expression, achieved greater reduction in hepatic glycogen accumulation, and led to a better toleration of fasting in GSD-Ia mice than the rAAV8-miGPE vector. Our results indicated that additional control elements in the rAAV8-GPE vector outweigh the gains from the double-stranded rAAV8-miGPE transduction efficiency, and that the rAAV8-GPE vector is the current choice for clinical translation in human GSD-Ia.

On the nature of the circumstellar medium of the remarkable Type Ia/IIn supernova SN 2002ic

We present results from the first high-resolution, high signal-to-noise ratio spectrum of SN 2002ic. The resolved Ha line has a P Cygni-type profile, clearly demonstrating the presence of a dense, slow-moving (~100 km s-1) outflow. We have additionally found a huge near-infrared excess, hitherto unseen in Type Ia supernovae. We argue that this is due to an infrared light-echo arising from the pre-existing dusty circumstellar medium. We deduce a circumstellar medium mass probably exceeding 0.3 Msolar produced by a mass-loss rate greater than several times 10-4 Msolar yr-1. For the progenitor, we favour a single-degenerate system where the companion is a post-asymptotic giant branch star. As a by-product of our optical data, we are able to provide a firm identification of the host galaxy of SN 2002ic.

The Diversity of Type Ia Supernovae: Evidence for Systematics?

The photometric and spectroscopic properties of 26 well-observed Type Ia Supernovae (SNe Ia) were analyzed with the aim of exploring SN Ia diversity. The sample includes (Branch) normal SNe, as well as extreme events such as SN 1991T and SN 1991bg, while the truly peculiar SNe Ia, SN 2000cx and SN 2002cx, are not included in our sample. A statistical treatment reveals the existence of three different groups. The first group (FAINT) consists of faint SNe Ia similar to SN 1991bg, with low expansion velocities and rapid evolution of Si II velocity. A second group consists of normal SNe Ia, also with high temporal velocity gradient (HVG), but with brighter mean absolute magnitude =-19.3 and higher expansion velocities than the FAINT SNe. The third group includes both normal and SN 1991T-like SNe Ia: these SNe populate a narrow strip in the Si II velocity evolution plot, with a low-velocity gradient (LVG), but have absolute magnitudes similar to HVGs. While the FAINT and HVG SNe Ia together seem to define a relation between R(Si II) and ���m15(B), the LVG SNe either do not conform to that relation or define a new, looser one. The R(Si II) premaximum evolution of HVGs is strikingly different from that of LVGs. We discuss the impact of this evidence on the understanding of SN Ia diversity, in terms of explosion mechanisms, degree of ejecta mixing, and ejecta-circumstellar material interaction.

Spectroscopy of the type Ia supernova SN 2002er: Days-11 to+215

We present an extensive set of optical spectroscopy of the nearby type Ia supernova, SN 2002er, with 24 epochs spanning -11 to +34 days. Its spectral evolution is fairly typical of a type Ia supernova although it suffers high extinction. Nevertheless, there are differences in the spectral evolution when compared to coeval spectra of other normal type Ia supernova with comparable decline-rate parameters. Modelling of the photospheric phase spectra using a homogeneous abundance distribution in the atmosphere provides a fair match to the observations, but only by pushing the adopted distance and risetime close to the observational limits. Future improvements here will require models with a more realistic stratified abundance distribution. From simple modelling of a nebular spectrum obtained at +215 d, we infer a Ni-56 mass of 0.69 M-circle dot, consistent with that derived from the light curve.