43 results on '"Tamburri S."'
Search Results
2. PCGF6 controls murine Tuft cell differentiation via H3K9me2 modification independently of Polycomb repression
- Author
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Del Vecchio, A, Mule, P, Fernandez-Perez, D, Amato, S, Lattanzi, G, Zanotti, M, Rustichelli, S, Pivetti, S, Oldani, P, Mariani, A, Iommazzo, F, Koseki, H, Facciotti, F, Tamburri, S, Ferrari, K, Pasini, D, Del Vecchio A., Mule P., Fernandez-Perez D., Amato S., Lattanzi G., Zanotti M., Rustichelli S., Pivetti S., Oldani P., Mariani A., Iommazzo F., Koseki H., Facciotti F., Tamburri S., Ferrari K. J., Pasini D., Del Vecchio, A, Mule, P, Fernandez-Perez, D, Amato, S, Lattanzi, G, Zanotti, M, Rustichelli, S, Pivetti, S, Oldani, P, Mariani, A, Iommazzo, F, Koseki, H, Facciotti, F, Tamburri, S, Ferrari, K, Pasini, D, Del Vecchio A., Mule P., Fernandez-Perez D., Amato S., Lattanzi G., Zanotti M., Rustichelli S., Pivetti S., Oldani P., Mariani A., Iommazzo F., Koseki H., Facciotti F., Tamburri S., Ferrari K. J., and Pasini D.
- Abstract
Cell fate is determined by specific transcription programs that are essential for tissue homeostasis and regeneration. The E3-ligases RING1A and B represent the core activity of the Polycomb repressive complex 1 (PRC1) that deposits repressive histone H2AK119 mono-ubiquitination (H2AK119ub1), which is essential for mouse intestinal homeostasis by preserving stem cell functions. However, the specific role of different PRC1 forms, which are defined by the six distinct PCGF1–6 paralogs, remains largely unexplored in vivo. We report that PCGF6 regulates mouse intestinal Tuft cell differentiation independently of H2AK119ub1 deposition. We show that PCGF6 chromatin occupancy expands outside Polycomb repressive domains, associating with unique promoter and distal regulatory elements. This occurs in the absence of RING1A/B and involves MGA-mediated E-BOX recognition and specific H3K9me2 promoter deposition. PCGF6 inactivation induces an epithelial autonomous accumulation of Tuft cells that was not phenocopied by RING1A/B loss. This involves direct PCGF6 association with a Tuft cell differentiation program that identified Polycomb-independent properties of PCGF6 in adult tissues homeostasis.
- Published
- 2024
3. Ultramassive dense early-type galaxies: velocity dispersions and number density evolution since z=1.6
- Author
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Gargiulo, A., Saracco, P., Tamburri, S., Lonoce, I., and Ciocca, F.
- Subjects
Astrophysics - Astrophysics of Galaxies - Abstract
In this paper we investigate the mass assembly history of ultramassive (Mstar > 10^11Msun) dense (Sigma = Mstar/(2*pi*Re^2) > 2500 Msun/pc^2) early-type galaxies (ETGs) over the last 9 Gyr. We have traced the evolution of the number density rho of ultramassive dense ETGs and have compared their structural (effective radius Re and stellar mass Mstar) and dynamical (velocity dispersion sigma_e) parameters over the redshift range 0 < z < 1.6. We have derived the number density at 1.6 < z < 1 from the MUNICS and GOODS-South surveys, while we have used the COSMOS and SDSS spectroscopic surveys to probe the intermediate and local redshift range. For the comparison of the dynamical and structural parameters, we have collected the ultramassive dense ETGs at 1.2 < z < 1.6 for which velocity dispersion measurements are available (11 ETGs). For 4 of them we present unpublished estimates of sigma_e. We probe the intermediate redshift range, and the local universe using the samples of ETGs by Saglia et al. (2010), Zahid et al. (2015), and by Thomas et al. (2010). We find that the number density of ultramassive dense ETGs evolves as rho(z) = K*(1 + z)^(0.3\pm0.8) implying a decrease of ~ 25% of the population since z = 1.6. By comparing the values of Re, Mstar, and sigma_e of ultramassive dense ETGs over the range 0 < z < 1.6 we find that all the high-z ETGs have a counterpart in the local universe. This implies either that the majority (~70%) of ultramassive dense ETGs has already completed its assembly and its shaping at
= 1.4, or that, if a significant fraction of them evolves in size, new ultramassive dense ETGs must form at z < 1.5 to maintain their number density almost constant. The difficulty into identify good progenitors for these new dense ETGs at z < 1.5, and the stellar populations properties of local ultramassive dense ETGs point toward the first hypothesis., Comment: 22 pages, 16 figures, accepted for publication in A&A - Published
- 2016
- Full Text
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4. Lower mass normalization of the stellar initial mass function for dense massive early-type galaxies at z ~ 1.4
- Author
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Gargiulo, A., Saracco, P., Longhetti, M., Tamburri, S., Lonoce, I., and Ciocca, F.
- Subjects
Astrophysics - Astrophysics of Galaxies - Abstract
This paper aims at understanding if the normalization of the stellar initial mass function (IMF) of massive early-type galaxies (ETGs) varies with cosmic time and/or with mean stellar mass density Sigma (M*/2\pi Re^2). For this purpose we collected a sample of 18 dense (Sigma>2500 M_sun/pc^2) ETGs at 1.2
= 1.4 follow the same IMF-sigma_e trend of typical local ETGs, but with a lower mass-normalization. Nonetheless, once the IMF-sigma_e trend we have found for high-z dense ETGs is compared with that of local ETGs with similar Sigma and sigma_e, they turn out to be consistent. The similarity between the IMF-sigma_e trends of dense high-z and low-z ETGs over 9 Gyr of evolution and their lower mass-normalization with respect to the mean value of local ETGs suggest that, independently on formation redshift, the physical conditions characterizing the formation of a dense spheroid lead to a mass spectrum of new formed stars with an higher ratio of high- to low-mass stars with respect to the IMF of normal local ETGs., Comment: 9 pages, 4 figures, accepted for pubblication in A&A, updated to match final journal version - Published
- 2014
- Full Text
- View/download PDF
5. Spectral detection of multiple stellar populations in z~1 early-type galaxies
- Author
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Lonoce, I., Longhetti, M., Saracco, P., Gargiulo, A., and Tamburri, S.
- Subjects
Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present a spectroscopic analysis based on measurements of two mainly age-dependent spectrophotometric indices in the 4000A rest frame region, i.e. H+K(CaII) and Delta4000, for a sample of 15 early-type galaxies (ETGs) at 0.7 < z_{spec} < 1.1, morphologically selected in the GOODS-South field. Ages derived from the two different indices by means of the comparison with stellar population synthesis models, are not consistent with each other for at least nine galaxies (60 per cent of the sample), while for the remaining six galaxies, the ages derived from their global spectral energy distribution (SED) fitting are not consistent with those derived from the two indices. We then hypothesized that the stellar content of many galaxies is made of two stellar components with different ages. The double-component analysis, performed by taking into account both the index values and the observed SED, fully explains the observational data and improves the results of the standard one-component SED fitting in 9 out of the 15 objects, i.e. those for which the two indices point towards two different ages. In all of them, the bulk of the mass belongs to rather evolved stars, while a small mass fraction is many Gyr younger. In some cases, thanks to the sensitivity of the H+K(CaII) index, we find that the minor younger component reveals signs of recent star formation. The distribution of the ages of the younger stellar components appears uniformly in time and this suggests that small amounts of star formation could be common during the evolution of high-z ETGs. We argue the possibility that these new star formation episodes could be frequently triggered by internal causes due to the presence of small gas reservoir., Comment: 18 pages, 12 figures. Accepted for publication in MNRAS
- Published
- 2014
- Full Text
- View/download PDF
6. The population of early-type galaxies: how it evolves with time and how it differs from passive and late-type galaxies
- Author
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Tamburri, S., Saracco, P., Longhetti, M., Gargiulo, A., Lonoce, I., and Ciocca, F.
- Subjects
Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
The aim of our analysis is twofold. On the one hand we are interested in addressing whether a sample of ETGs morphologically selected differs from a sample of passive galaxies in terms of galaxy statistics. On the other hand we study how the relative abundance of galaxies, the number density and the stellar mass density for different morphological types change over the redshift range 0.6
=10^(11) M_sol) galaxies, with the fraction of massive ETGs rising up to 40% and the fraction of massive LTGs decreasing down to 60%. Moreover, we find that the number density and the stellar mass density of the whole population of massive galaxies increase almost by a factor of ~10 between 0.6 3-4x10^(11) M_sol) both ETGs and LTGs do not increase since z~2.5, contrary to the lower mass galaxies. This suggests that the population of the most massive galaxies formed at z>2.5-3 and that the assembly of such high-mass galaxies is not effective at lower redshift., Comment: 15 pages, 14 figures. Published in A&A - Published
- 2014
- Full Text
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7. Scaling relations of cluster elliptical galaxies at z~1.3. Distinguishing luminosity and structural evolution
- Author
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Saracco, P., Casati, A., Gargiulo, A., Longhetti, M., Lonoce, I., Tamburri, S., Bettoni, D., D'Onofrio, M., Fasano, G., Poggianti, B. M., Boutsia, K., Fumana, M., and Sani, E.
- Subjects
Astrophysics - Astrophysics of Galaxies - Abstract
[Abridged] We studied the size-surface brightness and the size-mass relations of a sample of 16 cluster elliptical galaxies in the mass range 10^{10}-2x10^{11} M_sun which were morphologically selected in the cluster RDCS J0848+4453 at z=1.27. Our aim is to assess whether they have completed their mass growth at their redshift or significant mass and/or size growth can or must take place until z=0 in order to understand whether elliptical galaxies of clusters follow the observed size evolution of passive galaxies. To compare our data with the local universe we considered the Kormendy relation derived from the early-type galaxies of a local Coma Cluster reference sample and the WINGS survey sample. The comparison with the local Kormendy relation shows that the luminosity evolution due to the aging of the stellar content already assembled at z=1.27 brings them on the local relation. Moreover, this stellar content places them on the size-mass relation of the local cluster ellipticals. These results imply that for a given mass, the stellar mass at z~1.3 is distributed within these ellipticals according to the same stellar mass profile of local ellipticals. We find that a pure size evolution, even mild, is ruled out for our galaxies since it would lead them away from both the Kormendy and the size-mass relation. If an evolution of the effective radius takes place, this must be compensated by an increase in the luminosity, hence of the stellar mass of the galaxies, to keep them on the local relations. We show that to follow the Kormendy relation, the stellar mass must increase as the effective radius. However, this mass growth is not sufficient to keep the galaxies on the size-mass relation for the same variation in effective radius. Thus, if we want to preserve the Kormendy relation, we fail to satisfy the size-mass relation and vice versa., Comment: Accepted for publication in A&A, updated to match final journal version
- Published
- 2014
- Full Text
- View/download PDF
8. Exploring the bulk of the BL Lac object population:1. parsec-scale radio structures
- Author
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Liuzzo, E., Giroletti, M., Giovannini, G., Boccardi, B., Tamburri, S., Taylor, G. B., Casadio, C., Kadler, M., Tosti, G., and Mignano, A.
- Subjects
Astrophysics - High Energy Astrophysical Phenomena - Abstract
Context. The advent of Fermi is changing our understanding on the radio and gamma-ray emission in Active Galactic Nuclei. Contrary to pre-Fermi ideas, BL Lac objects are found to be the most abundant emitters in the gamma-ray band. However, since they are relatively weak radio sources, most of their parsec-scale structure and their multi-frequency properties are poorly understood and/or have not been investigated in a systematically fashion. Aims. Our main goal is to analyze the radio and gamma-ray emission properties of a sample of 42 BL Lacs selected, for the first time in the literature, with no constraint on their radio and gamma-ray flux densities/emission. Methods. Thanks to new Very Long Baseline Array observations at 8 and 15 GHz for the whole sample, we present here fundamental parameters such as radio flux densities, spectral index information, and parsec-scale structure. Moreover, we search for gamma-ray counterparts using data reported in the Second Catalog of Fermi Gamma-ray sources. Results. Parsec-scale radio emission is observed in the majority of the sources at both frequencies. Gamma-ray counterparts are found for 14/42 sources. Conclusions. The comparison between our results in radio and gamma-ray bands points out the presence of a large number of faint BL Lacs showing "non classical" properties such as low source compactness, core dominance, no gamma-ray emission and steep radio spectral indexes. A deeper multiwavelength analysis will be needed., Comment: 19 pages, 6 figures, 6 tables, accepted for publication in A&A
- Published
- 2013
- Full Text
- View/download PDF
9. Spatially Resolved Colors and Stellar Population Properties in Early-Type Galaxies at z ~ 1.5
- Author
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Gargiulo, A., Saracco, P., Longhetti, M., La Barbera, F., and Tamburri, S.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present F850LP-F160W color gradients for 11 early-type galaxies (ETGs) at 1.0
R_e we have found that the fraction of high-z ETGs with negative F850LP-F160W color gradients rises up to 100%. For each galaxy, we investigate the origin of the radial color variation with a technique based on the matching of both the spatially resolved color and the global spectral energy distribution (SED) to predictions of composite stellar population models. In fact, we find that the age of the stellar populations is the only parameter whose radial variation alone can fully account for the observed color gradients and global SEDs for half of the galaxies in our sample (6 ETGs), without the need of radial variation of any other stellar population property. For four out of these six ETGs, a pure metallicity variation can also reproduce the detected color gradients. Nonetheless, a minor contribution to the observed color gradients from radial variation of star-formation time scale, abundance of low-to-high mass stars and dust cannot be completely ruled out. For the remaining half of the sample, our analysis suggests a more complex scenario whereby more properties of the stellar populations need to simultaneously vary to generate the observed color gradients and global SED. Our results show that, despite the young mean age of our galaxies (<3-4 Gyr), they already exhibit significant differences among their stellar content. We have discussed our results within the framework of the widest accepted scenarios of galaxy formation and conclude that none of them can satisfactorily account for the observed distribution of color gradients and for the spatially resolved content of high-z ETGs., Comment: 19 pages, 13 figures, 3 tables, accepted for publication in MNRAS - Published
- 2012
- Full Text
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10. Seyfert's Sextet: where is the gas?
- Author
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Tamburri, S., Trinchieri, G., Wolter, A., Sulentic, J., Durbala, A., and Rosado, M.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Seyfert's Sextet (a.k.a HCG 79) is one of the most compact and isolated galaxy groups in the local Universe. It shows a prominent diffuse light component that accounts for ~50% of the total observed light. This likely indicates that the group is in an advanced evolutionary phase, which would predict a significant hot gaseous component. Previous X-ray observations had suggested a low luminosity for this system, but with large uncertainties and poor resolution. We present the results from a deep (70 ks), high resolution Chandra observation of Seyfert's Sextet, requested with the aim of separating the X-ray emission associated with the individual galaxies from that of a more extended inter-galactic component. We discuss the spatial and spectral characteristics of this group we derive with those of a few similar systems also studied in the X-ray band. The high resolution X-ray image indicates that the majority of the detected emission does not arise in the compact group but is concentrated towards the NW and corresponds to what appears to be a background galaxy cluster. The emission from the group alone has a total luminosity of ~1x10^40 erg/s in the (0.5-5) keV band. Most of the luminosity can be attributed to the individual sources in the galaxies, and only ~2x10^39 erg/s is due to a gaseous component. However, we find that this component is also mostly associated with the individual galaxies of the Sextet, leaving little or no residual in a truly IGM component. The extremely low luminosity of the diffuse emission in Seyfert's Sextet might be related to its small total mass., Comment: 8 pages, 7 figures. Accepted on A&A
- Published
- 2012
- Full Text
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11. Radio-faint BL Lac objects and their impact on the radio/gamma-ray connection
- Author
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Giroletti, Marcello, Pavlidou, V., Reimer, A., Taylor, G.B., Tosti, G., Giovannini, G., Casadio, C., Liuzzo, E., and Tamburri, S.
- Published
- 2012
- Full Text
- View/download PDF
12. Ultramassive dense early-type galaxies: Velocity dispersions and number density evolution sincez= 1.6
- Author
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Gargiulo, A., primary, Saracco, P., additional, Tamburri, S., additional, Lonoce, I., additional, and Ciocca, F., additional
- Published
- 2016
- Full Text
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13. GIS methodology applied to proposals for geotourism in the area of Ascoli Piceno Province. Metodologie G.I.S. applicate a proposte di geoturismo nel territorio della Provincia di Ascoli Piceno
- Author
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Scalella, G., Tamburri, S., Pignoloni, I., Farabollini, P., Bonifazi, B., Veccia, L., and Latini, E.
- Published
- 2008
14. Lower mass normalization of the stellar initial mass function for dense massive early-type galaxies atz~ 1.4
- Author
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Gargiulo, A., primary, Saracco, P., additional, Longhetti, M., additional, Tamburri, S., additional, Lonoce, I., additional, and Ciocca, F., additional
- Published
- 2015
- Full Text
- View/download PDF
15. The population of early-type galaxies: how it evolves with time and how it differs from passive and late-type galaxies
- Author
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Tamburri, S., primary, Saracco, P., additional, Longhetti, M., additional, Gargiulo, A., additional, Lonoce, I., additional, and Ciocca, F., additional
- Published
- 2014
- Full Text
- View/download PDF
16. Spectral detection of multiple stellar populations in z ∼ 1 early-type galaxies
- Author
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Lonoce, I., primary, Longhetti, M., additional, Saracco, P., additional, Gargiulo, A., additional, and Tamburri, S., additional
- Published
- 2014
- Full Text
- View/download PDF
17. Scaling relations of cluster elliptical galaxies atz~ 1.3
- Author
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Saracco, P., primary, Casati, A., additional, Gargiulo, A., additional, Longhetti, M., additional, Lonoce, I., additional, Tamburri, S., additional, Bettoni, D., additional, D’Onofrio, M. D’Onofrio, additional, Fasano, G., additional, Poggianti, B. M., additional, Boutsia, K., additional, Fumana, M., additional, and Sani, E., additional
- Published
- 2014
- Full Text
- View/download PDF
18. Large Binocular Telescope/LUCIFER spectroscopy: kinematics of a compact early-type galaxy at z ≃ 1.4★
- Author
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Longhetti, M., primary, Saracco, P., additional, Gargiulo, A., additional, Tamburri, S., additional, and Lonoce, I., additional
- Published
- 2014
- Full Text
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19. Exploring the bulk of the BL Lacertae object population
- Author
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Liuzzo, E., primary, Giroletti, M., additional, Giovannini, G., additional, Boccardi, B., additional, Tamburri, S., additional, Taylor, G. B., additional, Casadio, C., additional, Kadler, M., additional, Tosti, G., additional, and Mignano, A., additional
- Published
- 2013
- Full Text
- View/download PDF
20. Ultramassive dense early-type galaxies: Velocity dispersions and number density evolution since z = 1.6.
- Author
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Gargiulo, A., Saracco, P., Tamburri, S., Lonoce, I., and Ciocca, F.
- Abstract
Aims. We investigate the stellar mass assembly history of ultramassive (M
⋆ ≳ 1011 M⊙ ) dense (Σ = M⋆ /2πRe 2 > 2500M⊙ pc-2 ) early-type galaxies (ETGs, elliptical and spheroidal galaxies) selected on basis of visual classification over the last 9 Gyr. Methods. We traced the evolution of the comoving number density ρ of ultramassive dense ETGs and compared their structural (effective radius Re and stellar mass M⋆ ) and dynamical (velocity dispersion σe ) parameters over the redshift range 0 < z < 1.6. We derived the number density ρ at 1.60.3 ± 0.8 implying a decrease of ~25% of the population of ultramassive dense ETGs since z = 1.6. By comparing the structural and dynamical properties of high-z ultramassive dense ETGs over the range 0 ≲ z < 1.6 in the [R e , M⋆ , σe ] plane, we find that all of the ETGs of the high-z sample have counterparts with similar properties in the local Universe. This implies either that the majority (~70%) of ultramassive dense ETGs already completed the assembly and shaping at ⟨ z ⟩ = 1.4, or that, if a significant portion of dense ETGs evolves in size, new ultramassive dense ETGs must form at z < 1.5 to maintain their number density at almost constant. The difficulty in identify good progenitors for these new dense ETGs at z ≲ 1.5 and the stellar populations properties of local ultramassive dense ETGs point towards the first hypothesis. In this case, the ultramassive dense galaxies missing in the local Universe could have joined, in the last 9 Gyr, the so colled non-dense ETGs population through minor mergers, thus contributing to mean size growth. In any case, the comparison between their number density and the number density of the whole population of ultramassive ETGs relegates their contribution to the mean size evolution to a secondary process. [ABSTRACT FROM AUTHOR]- Published
- 2016
- Full Text
- View/download PDF
21. Spatially resolved colours and stellar population properties in early-type galaxies at z ∼ 1.5
- Author
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Gargiulo, A., primary, Saracco, P., additional, Longhetti, M., additional, La Barbera, F., additional, and Tamburri, S., additional
- Published
- 2012
- Full Text
- View/download PDF
22. Seyfert’s Sextet: where is the gas?
- Author
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Tamburri, S., primary, Trinchieri, G., additional, Wolter, A., additional, Sulentic, J., additional, Durbala, A., additional, and Rosado, M., additional
- Published
- 2012
- Full Text
- View/download PDF
23. Lower mass normalization of the stellar initial mass function for dense massive early-type galaxies at z ~ 1.4.
- Author
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Gargiulo, A., Saracco, P., Longhetti, M., Tamburri, S., Lonoce, I., and Ciocca, F.
- Subjects
GALAXY formation ,GALACTIC evolution ,MASS density gradients ,STELLAR initial mass function ,ELLIPTICAL galaxies ,PHOTOMETRY - Abstract
Aims. This paper aims at understanding whether the normalization of the stellar initial mass function (IMF) of massive galaxies varies with cosmic time and/or with mean stellar mass density Σ = M
* /(2πRe 5 ). Methods. We have tackled this question by taking advantage of a spectroscopic sample of 18 dense (Σ > 2500 Mʘ pc-2 ) massive early-type galaxies (ETGs) that we collected at 1.2 ≲ z ≲ 1.6. Each galaxy in the sample was selected in order to have available: i) a high-resolution deep HST-F160W image to visually classify it as an ETG; ii) an accurate velocity dispersion estimate; iii) stellar mass derived through the fit of multiband photometry; and iv) structural parameters (i.e. effective radius Re and Sersic index n) derived in the F160W-band. We have constrained the mass-normalization of the IMF of dense high-z ETGs by comparing the true stellar masses of the ETGs in the sample (Mtrue ) derived through virial theorem, hence IMF independent, with those inferred through the fit of the photometry which assume a reference IMF (Mref ). Adopting the virial estimator as proxy of the true stellar mass, we have implicitly assumed that these systems have zero dark matter. However, recent dynamical analysis of massive local ETGs have shown that the dark matter fraction within Re in dense ETGs is negligible (<5-10%) and simulations of dissipationless mergers of spheroidal galaxies have shown that this fraction decreases going back with time. Accurate dynamical models of local ETGs performed by the ATLAS3D team have shown that the virial estimator is prone to underestimating or overestimating the total masses. We have considered this, and based on the results of ATLAS3D we have shown that for dense ETGs the mean value of total masses derived through the virial estimator with a non-homologous virial coefficient and Sersic-Re are perfectly in agreement with the mean value of those derived through more sophisticated dynamical models, although, of course, the estimates show higher uncertainties. Results. Tracing the variation of the parameter Γ = Mtrue /Mref with velocity dispersion σe , we have found that, on average, dense ETGs at 〈z〉 = 1.4 follow the same IMF-σe trend of typical local ETGs, but with a lower mass-normalization. The observed lower normalization could be evidence of i) an evolution of the IMF with time or ii) a correlation with σ. To discriminate between the two possibilities, we have compared the IMF-σe trend that we have found for high-z dense ETGs with that of local ETGs with similar mean stellar mass density and velocity dispersion and we have found that the IMF of massive dense ETGs does not depend on redshift. The similarity between the IMF-σe trends observed both in dense high-z and low-z ETGs over 9 Gyr of evolution and their lower massnormalization with respect to the mean value of local ETGs suggests that, independently of formation redshift, the physical conditions which characterized the formation of a dense spheroid on average lead to a mass spectrum of newly formed stars with a higher ratio of high- to low-mass stars with respect to the IMF of normal local ETGs. In the direction of our findings, recent hydrodynamical simulations show that the higher star-formation rate that should have characterized the early stage of star formation of dense ETGs is expected to inhibit the formation of low-mass stars. Hence, compact ETGs should have higher ratio of high- to low-mass stars than normal spheroids, as we observe. [ABSTRACT FROM AUTHOR]- Published
- 2015
- Full Text
- View/download PDF
24. Self-assembling of n-diamond nanocrystals into supercrystals
- Author
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Terranova, M. L., Daniela Manno, Rossi, M., Antonio Serra, Filippo, Emanuela, Tamburri, S. Orlanducci And E., M. L., Terranova, Manno, Daniela Erminia, M., Rossi, Serra, Antonio, Filippo, Emanuela, and S. ORLANDUCCI AND E., Tamburri
- Subjects
Self-Assembly ,electron diffraction ,n-Diamond Nanocrystal - Abstract
Face-centered cubic n-diamond (sg F4 j3m) is a carbon allotrope relatively new and, similar to the others (graphite, diamond, fullerenes, and nanotubes are the most relevant ones), is currently a focus of great interest for potential advanced applications, with a particular emphasis in the field of nanotechnologies. The presence of n-diamond has been in general revealed as a byproduct of several diamond synthesis techniques. In the case of detonation nanodiamond, self-assembly mechanisms can be used in order to selectively separate n-diamond from other carbon nanomaterials. In particular, we show the possibility to achieve single crystal-like organized three-dimensional particles (with a size of some hundreds of nanometers), using as building blocks n-diamond nanocrystals (with a size of a few nanometers).
25. Exploring the bulk of the BL Lacertae object population. I. Parsec-scale radio structures
- Author
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S. Tamburri, G. Giovannini, G. B. Taylor, Marcello Giroletti, Carolina Casadio, G. Tosti, B. Boccardi, A. Mignano, Matthias Kadler, Elisabetta Liuzzo, Liuzzo E., Giroletti M., Giovannini G., Boccardi B., Tamburri S., Taylor G. B., Casadio C., Kadler M., Tosti G., and Mignano A.
- Subjects
Physics ,radio continuum: galaxies ,education.field_of_study ,Spectral index ,Active galactic nucleus ,Astrophysics::High Energy Astrophysical Phenomena ,Population ,galaxies: active ,Flux ,Astronomy and Astrophysics ,Context (language use) ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,galaxies: jets ,Space and Planetary Science ,radio continuum: galaxie ,education ,Astrophysics::Galaxy Astrophysics ,Very Long Baseline Array ,Fermi Gamma-ray Space Telescope ,BL Lac object - Abstract
Context. The advent of Fermi is changing our understanding on the radio and gamma-ray emission in Active Galactic Nuclei. Contrary to pre-Fermi ideas, BL Lac objects are found to be the most abundant emitters in the gamma-ray band. However, since they are relatively weak radio sources, most of their parsec-scale structure and their multi-frequency properties are poorly understood and/or have not been investigated in a systematically fashion. Aims. Our main goal is to analyze the radio and gamma-ray emission properties of a sample of 42 BL Lacs selected, for the first time in the literature, with no constraint on their radio and gamma-ray flux densities/emission. Methods. Thanks to new Very Long Baseline Array observations at 8 and 15 GHz for the whole sample, we present here fundamental parameters such as radio flux densities, spectral index information, and parsec-scale structure. Moreover, we search for gamma-ray counterparts using data reported in the Second Catalog of Fermi Gamma-ray sources. Results. Parsec-scale radio emission is observed in the majority of the sources at both frequencies. Gamma-ray counterparts are found for 14/42 sources. Conclusions. The comparison between our results in radio and gamma-ray bands points out the presence of a large number of faint BL Lacs showing "non classical" properties such as low source compactness, core dominance, no gamma-ray emission and steep radio spectral indexes. A deeper multiwavelength analysis will be needed.
- Published
- 2013
26. Intervention development of the resiliency in stressful events (RISE) curriculum: A trauma-informed reentry approach for men.
- Author
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Renn T, Tamburri S, Pettus C, and Tripodi SJ
- Abstract
This article addresses the demand for trauma-based interventions tailored to the distinctive challenges confronting young men during the reentry phase, approximately 4-6 months prior to release and a year postrelease. We introduce the Resiliency in Stressful Experiences (RISE) program as a response to this need, drawing on two foundational conceptual frameworks: the trauma-based reentry framework and the well-being development model. These frameworks guide RISE in addressing lifetime traumatic experiences and trauma symptoms within the broader reentry context. In the article, the process of developing the RISE curriculum is delineated, which involved a literature review, adaptation of pertinent interventions, and collaborative engagement with a community advisory board consisting of formerly incarcerated individuals. The resulting curriculum seamlessly integrates trauma-informed cognitive-behavioral principles with well-being-oriented reentry programming, with a primary objective of augmenting emotion regulation, coping skills, and community stabilization. Finally, we discuss the ongoing randomized controlled trial of the RISE intervention that aims to evaluate the impact of RISE on community stability, posttraumatic stress disorder symptom management, and recidivism rates among individuals in a southeastern state. The potential for successful implementation and dissemination of the RISE curriculum is considered, emphasizing accessibility, ease of implementation, and acceptability. (PsycInfo Database Record (c) 2025 APA, all rights reserved).
- Published
- 2025
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27. SP140 represses specific loci by recruiting polycomb repressive complex 2 and NuRD complex.
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Tamburri S, Zucchelli C, Matafora V, Zapparoli E, Jevtic Z, Farris F, Iannelli F, Musco G, and Bachi A
- Abstract
SP140, a lymphocytic-restricted protein, is an epigenetic reader working as a corepressor of genes implicated in inflammation and orchestrating macrophage transcriptional programs to maintain cellular identity. Reduced SP140 expression is associated both to autoimmune diseases and blood cancers. However, the molecular mechanisms that link SP140 altered protein levels to detrimental effects on the immune response and cellular growth, as well as the interactors through which SP140 promotes gene silencing, remain elusive. In this work, we have applied a multi-omics approach (i.e. interactomics, ChIP-seq and proteomics) in two Burkitt lymphoma cell lines to identify both interactors and target genes of endogenous SP140. We found that SP140 interacts with the PRC2 and NuRD complexes, and we showed that these interactions are functional as SP140 directs H3K27me3 deposition and NuRD binding on a set of target genes implicated in cellular growth and leukemia progression., (© The Author(s) 2024. Published by Oxford University Press on behalf of Nucleic Acids Research.)
- Published
- 2024
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28. Navigating the complexity of Polycomb repression: Enzymatic cores and regulatory modules.
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Tamburri S, Rustichelli S, Amato S, and Pasini D
- Subjects
- Humans, Animals, Methylation, Transcription, Genetic, Polycomb-Group Proteins metabolism, Polycomb-Group Proteins genetics, Histones metabolism, Histones genetics, Protein Processing, Post-Translational
- Abstract
Polycomb proteins are a fundamental repressive system that plays crucial developmental roles by orchestrating cell-type-specific transcription programs that govern cell identity. Direct alterations of Polycomb activity are indeed implicated in human pathologies, including developmental disorders and cancer. General Polycomb repression is coordinated by three distinct activities that regulate the deposition of two histone post-translational modifications: tri-methylation of histone H3 lysine 27 (H3K27me3) and histone H2A at lysine 119 (H2AK119ub1). These activities exist in large and heterogeneous multiprotein ensembles consisting of common enzymatic cores regulated by heterogeneous non-catalytic modules composed of a large number of accessory proteins with diverse biochemical properties. Here, we have analyzed the current molecular knowledge, focusing on the functional interaction between the core enzymatic activities and their regulation mediated by distinct accessory modules. This provides a comprehensive analysis of the molecular details that control the establishment and maintenance of Polycomb repression, examining their underlying coordination and highlighting missing information and emerging new features of Polycomb-mediated transcriptional control., Competing Interests: Declaration of interests The authors declare no competing interests., (Copyright © 2024 Elsevier Inc. All rights reserved.)
- Published
- 2024
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29. Editorial: Polycomb group (PcG) proteins in development and disease.
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Pethe P, Rao SMR, Tamburri S, and Tomar RS
- Abstract
Competing Interests: The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest. The author(s) declared that they were an editorial board member of Frontiers, at the time of submission. This had no impact on the peer review process and the final decision
- Published
- 2024
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30. PCGF6 controls murine Tuft cell differentiation via H3K9me2 modification independently of Polycomb repression.
- Author
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Del Vecchio A, Mulé P, Fernández-Pérez D, Amato S, Lattanzi G, Zanotti M, Rustichelli S, Pivetti S, Oldani P, Mariani A, Iommazzo F, Koseki H, Facciotti F, Tamburri S, Ferrari KJ, and Pasini D
- Subjects
- Animals, Mice, Cell Differentiation physiology, Polycomb-Group Proteins, Ubiquitin-Protein Ligases, Polycomb Repressive Complex 1, Tuft Cells
- Abstract
Cell fate is determined by specific transcription programs that are essential for tissue homeostasis and regeneration. The E3-ligases RING1A and B represent the core activity of the Polycomb repressive complex 1 (PRC1) that deposits repressive histone H2AK119 mono-ubiquitination (H2AK119ub1), which is essential for mouse intestinal homeostasis by preserving stem cell functions. However, the specific role of different PRC1 forms, which are defined by the six distinct PCGF1-6 paralogs, remains largely unexplored in vivo. We report that PCGF6 regulates mouse intestinal Tuft cell differentiation independently of H2AK119ub1 deposition. We show that PCGF6 chromatin occupancy expands outside Polycomb repressive domains, associating with unique promoter and distal regulatory elements. This occurs in the absence of RING1A/B and involves MGA-mediated E-BOX recognition and specific H3K9me2 promoter deposition. PCGF6 inactivation induces an epithelial autonomous accumulation of Tuft cells that was not phenocopied by RING1A/B loss. This involves direct PCGF6 association with a Tuft cell differentiation program that identified Polycomb-independent properties of PCGF6 in adult tissues homeostasis., Competing Interests: Declaration of interests The authors declare no competing interests., (Copyright © 2023 Elsevier Inc. All rights reserved.)
- Published
- 2024
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31. Structural basis of histone H2A lysine 119 deubiquitination by Polycomb repressive deubiquitinase BAP1/ASXL1.
- Author
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Thomas JF, Valencia-Sánchez MI, Tamburri S, Gloor SL, Rustichelli S, Godínez-López V, De Ioannes P, Lee R, Abini-Agbomson S, Gretarsson K, Burg JM, Hickman AR, Sun L, Gopinath S, Taylor HF, Sun ZW, Ezell RJ, Vaidya A, Meiners MJ, Cheek MA, Rice WJ, Svetlov V, Nudler E, Lu C, Keogh MC, Pasini D, and Armache KJ
- Subjects
- Humans, Histones genetics, Nucleosomes, Lysine, Ubiquitin Thiolesterase genetics, Ubiquitin Thiolesterase metabolism, Polycomb-Group Proteins genetics, Repressor Proteins genetics, Tumor Suppressor Proteins genetics, Tumor Suppressor Proteins metabolism, Drosophila Proteins genetics, Neoplasms genetics
- Abstract
Histone H2A lysine 119 (H2AK119Ub) is monoubiquitinated by Polycomb repressive complex 1 and deubiquitinated by Polycomb repressive deubiquitinase complex (PR-DUB). PR-DUB cleaves H2AK119Ub to restrict focal H2AK119Ub at Polycomb target sites and to protect active genes from aberrant silencing. The PR-DUB subunits (BAP1 and ASXL1) are among the most frequently mutated epigenetic factors in human cancers. How PR-DUB establishes specificity for H2AK119Ub over other nucleosomal ubiquitination sites and how disease-associated mutations of the enzyme affect activity are unclear. Here, we determine a cryo-EM structure of human BAP1 and the ASXL1 DEUBAD in complex with a H2AK119Ub nucleosome. Our structural, biochemical, and cellular data reveal the molecular interactions of BAP1 and ASXL1 with histones and DNA that are critical for restructuring the nucleosome and thus establishing specificity for H2AK119Ub. These results further provide a molecular explanation for how >50 mutations in BAP1 and ASXL1 found in cancer can dysregulate H2AK119Ub deubiquitination, providing insight into understanding cancer etiology.
- Published
- 2023
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32. Study protocol paper for the multisite randomized controlled trial of comprehensive trauma informed reentry services for moderate to high-risk young males releasing from state prisons.
- Author
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Pettus C, Renn T, Tripodi S, and Tamburri S
- Subjects
- Adaptation, Psychological, Adolescent, Adult, Employment, Female, Housing, Humans, Male, Randomized Controlled Trials as Topic, Young Adult, Prisoners, Prisons
- Abstract
Introduction: Nearly half of the individuals who release from state prisons each year are under the age of 35; 89% are men. These young men are highly likely to be re-incarcerated. Research suggests untreated trauma symptoms contribute to high rates of incarceration and re-incarceration. As trauma symptomatology can increase during reentry, implementing trauma treatment during this time is critical. The current study fills an important gap by implementing an evidence-driven trauma intervention with young, incarcerated men and extending treatment post-release in the community., Methods: This study evaluates the impact of the Resiliency in Stressful Experiences (RISE) program for 18-35-year-old incarcerated males releasing to participating counties. RISE is a multi-phased comprehensive trauma-based reentry program designed according to the transitional nature of reentry. The researchers will assess the influence of RISE on post-release housing and employment stability and recidivism and identify key mechanisms of change. Participants (n = 400) are randomly assigned 1:1 to RISE or a Treatment as Usual control group., Discussion: This study will provide critical information about how trauma-informed reentry programming impacts traditional reentry outcomes (e.g., recidivism, housing, employment) and identify key mechanisms of action (e.g., reduced impulsivity and aggression). Coping with trauma symptomatology is a largely untapped area of scientific inquiry for criminal justice-involved populations, despite the significant role trauma plays in individuals' lives. Results advance identification of critical components of trauma-informed reentry interventions for moderate- to high-risk young men. This study provides critical data to support policymakers and corrections professionals eager for innovative approaches to improve post-release outcomes., (Copyright © 2022. Published by Elsevier Inc.)
- Published
- 2022
- Full Text
- View/download PDF
33. Polycomb-dependent histone H2A ubiquitination links developmental disorders with cancer.
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Tamburri S, Conway E, and Pasini D
- Subjects
- Child, Chromatin genetics, Humans, Developmental Disabilities genetics, Histones genetics, Histones metabolism, Neoplasms genetics, Polycomb Repressive Complex 1 genetics, Polycomb Repressive Complex 1 metabolism, Polycomb-Group Proteins genetics, Polycomb-Group Proteins metabolism, Ubiquitination
- Abstract
Cell identity is tightly controlled by specific transcriptional programs which require post-translational modifications of histones. These histone modifications allow the establishment and maintenance of active and repressed chromatin domains. Histone H2A lysine 119 ubiquitination (H2AK119ub1) has an essential role in building repressive chromatin domains during development. It is regulated by the counteracting activities of the Polycomb repressive complex 1 (PRC1) and the Polycomb repressive-deubiquitinase (PR-DUB) complexes, two multi-subunit ensembles that write and erase this modification, respectively. We have catalogued the recurrent genetic alterations in subunits of the PRC1 and PR-DUB complexes in both neurodevelopmental disorders and cancer. These genetic lesions are often shared across disorders, and we highlight common mechanisms of H2AK119ub1 dysregulation and how they affect development in multiple disease contexts., Competing Interests: Declaration of interests The authors declare no conflicts of interest., (Copyright © 2021 Elsevier Ltd. All rights reserved.)
- Published
- 2022
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34. BAP1 enhances Polycomb repression by counteracting widespread H2AK119ub1 deposition and chromatin condensation.
- Author
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Conway E, Rossi F, Fernandez-Perez D, Ponzo E, Ferrari KJ, Zanotti M, Manganaro D, Rodighiero S, Tamburri S, and Pasini D
- Subjects
- Animals, Cell Line metabolism, Chromatin genetics, Chromatin physiology, Embryonic Stem Cells metabolism, Heterochromatin, Histones metabolism, Humans, Mice, Mouse Embryonic Stem Cells metabolism, Polycomb Repressive Complex 1 metabolism, Polycomb Repressive Complex 2 metabolism, Polycomb-Group Proteins genetics, Tumor Suppressor Proteins genetics, Tumor Suppressor Proteins physiology, Ubiquitin Thiolesterase genetics, Ubiquitin Thiolesterase physiology, Ubiquitination, Chromatin metabolism, Polycomb-Group Proteins metabolism, Tumor Suppressor Proteins metabolism, Ubiquitin Thiolesterase metabolism
- Abstract
BAP1 is mutated or deleted in many cancer types, including mesothelioma, uveal melanoma, and cholangiocarcinoma. It is the catalytic subunit of the PR-DUB complex, which removes PRC1-mediated H2AK119ub1, essential for maintaining transcriptional repression. However, the precise relationship between BAP1 and Polycombs remains elusive. Using embryonic stem cells, we show that BAP1 restricts H2AK119ub1 deposition to Polycomb target sites. This increases the stability of Polycomb with their targets and prevents diffuse accumulation of H2AK119ub1 and H3K27me3. Loss of BAP1 results in a broad increase in H2AK119ub1 levels that is primarily dependent on PCGF3/5-PRC1 complexes. This titrates PRC2 away from its targets and stimulates H3K27me3 accumulation across the genome, leading to a general chromatin compaction. This provides evidence for a unifying model that resolves the apparent contradiction between BAP1 catalytic activity and its role in vivo, uncovering molecular vulnerabilities that could be useful for BAP1-related pathologies., Competing Interests: Declarations of interests The authors declare no competing interests., (Copyright © 2021 The Authors. Published by Elsevier Inc. All rights reserved.)
- Published
- 2021
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- View/download PDF
35. Intestinal differentiation involves cleavage of histone H3 N-terminal tails by multiple proteases.
- Author
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Ferrari KJ, Amato S, Noberini R, Toscani C, Fernández-Pérez D, Rossi A, Conforti P, Zanotti M, Bonaldi T, Tamburri S, and Pasini D
- Subjects
- Animals, Cathepsin L metabolism, Cell Differentiation, Homeostasis, Intestinal Mucosa cytology, Mice, Microvilli ultrastructure, Nucleosomes metabolism, Nucleosomes ultrastructure, Organoids, Protein Domains, Trypsin metabolism, Enterocytes metabolism, Histones metabolism, Intestine, Small cytology, Paneth Cells metabolism, Peptide Hydrolases metabolism, Protein Processing, Post-Translational, Stem Cells metabolism
- Abstract
The proteolytic cleavage of histone tails, also termed histone clipping, has been described as a mechanism for permanent removal of post-translational modifications (PTMs) from histone proteins. Such activity has been ascribed to ensure regulatory function in key cellular processes such as differentiation, senescence and transcriptional control, for which different histone-specific proteases have been described. However, all these studies were exclusively performed using cell lines cultured in vitro and no clear evidence that histone clipping is regulated in vivo has been reported. Here we show that histone H3 N-terminal tails undergo extensive cleavage in the differentiated cells of the villi in mouse intestinal epithelium. Combining biochemical methods, 3D organoid cultures and in vivo approaches, we demonstrate that intestinal H3 clipping is the result of multiple proteolytic activities. We identified Trypsins and Cathepsin L as specific H3 tail proteases active in small intestinal differentiated cells and showed that their proteolytic activity is differentially affected by the PTM pattern of histone H3 tails. Together, our findings provide in vivo evidence of H3 tail proteolysis in mammalian tissues, directly linking H3 clipping to cell differentiation., (© The Author(s) 2021. Published by Oxford University Press on behalf of Nucleic Acids Research.)
- Published
- 2021
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36. Mapping the native interaction surfaces of PREP1 with PBX1 by cross-linking mass-spectrometry and mutagenesis.
- Author
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Bruckmann C, Tamburri S, De Lorenzi V, Doti N, Monti A, Mathiasen L, Cattaneo A, Ruvo M, Bachi A, and Blasi F
- Subjects
- A549 Cells, Binding Sites, Cloning, Molecular, Enzyme-Linked Immunosorbent Assay, Humans, Mass Spectrometry, Mutagenesis, Myeloid Ecotropic Viral Integration Site 1 Protein metabolism, Homeodomain Proteins metabolism, Pre-B-Cell Leukemia Transcription Factor 1 metabolism, Protein Interaction Mapping methods
- Abstract
Both onco-suppressor PREP1 and the oncogene MEIS1 bind to PBX1. This interaction stabilizes the two proteins and allows their translocation into the nucleus and thus their transcriptional activity. Here, we have combined cross-linking mass-spectrometry and systematic mutagenesis to detail the binding geometry of the PBX1-PREP1 (and PBX1-MEIS1) complexes, under native in vivo conditions. The data confirm the existence of two distinct interaction sites within the PBC domain of PBX1 and unravel differences among the highly similar binding sites of MEIS1 and PREP1. The HR2 domain has a fundamental role in binding the PBC-B domain of PBX1 in both PREP1 and MEIS1. The HR1 domain of MEIS1, however, seem to play a less stringent role in PBX1 interaction with respect to that of PREP1. This difference is also reflected by the different binding affinity of the two proteins to PBX1. Although partial, this analysis provides for the first time some ideas on the tertiary structure of the complexes not available before. Moreover, the extensive mutagenic analysis of PREP1 identifies the role of individual hydrophobic HR1 and HR2 residues, both in vitro and in vivo.
- Published
- 2020
- Full Text
- View/download PDF
37. Amyloid aggregates accumulate in melanoma metastasis modulating YAP activity.
- Author
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Matafora V, Farris F, Restuccia U, Tamburri S, Martano G, Bernardelli C, Sofia A, Pisati F, Casagrande F, Lazzari L, Marsoni S, Bonoldi E, and Bachi A
- Subjects
- Amyloidogenic Proteins, Humans, Mechanotransduction, Cellular, Transcription Factors genetics, Transcription Factors metabolism, Adaptor Proteins, Signal Transducing genetics, Adaptor Proteins, Signal Transducing metabolism, Melanoma drug therapy, Melanoma genetics
- Abstract
Melanoma progression is generally associated with increased transcriptional activity mediated by the Yes-associated protein (YAP). Mechanical signals from the extracellular matrix are sensed by YAP, which then activates the expression of proliferative genes, promoting melanoma progression and drug resistance. Which extracellular signals induce mechanotransduction, and how this is mediated, is not completely understood. Here, using secretome analyses, we reveal the extracellular accumulation of amyloidogenic proteins, i.e. premelanosome protein (PMEL), in metastatic melanoma, together with proteins that assist amyloid maturation into fibrils. We also confirm the accumulation of amyloid-like aggregates, similar to those detected in Alzheimer disease, in metastatic cell lines, as well as in human melanoma biopsies. Mechanistically, beta-secretase 2 (BACE2) regulates the maturation of these aggregates, which in turn induce YAP activity. We also demonstrate that recombinant PMEL fibrils are sufficient to induce mechanotransduction, triggering YAP signaling. Finally, we demonstrate that BACE inhibition affects cell proliferation and increases drug sensitivity, highlighting the importance of amyloids for melanoma survival, and the use of beta-secretase inhibitors as potential therapeutic approach for metastatic melanoma., (© 2020 The Authors. Published under the terms of the CC BY 4.0 license.)
- Published
- 2020
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- View/download PDF
38. Histone H2AK119 Mono-Ubiquitination Is Essential for Polycomb-Mediated Transcriptional Repression.
- Author
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Tamburri S, Lavarone E, Fernández-Pérez D, Conway E, Zanotti M, Manganaro D, and Pasini D
- Subjects
- Cell Line, Chromatin metabolism, Embryonic Stem Cells metabolism, Mutation, Missense, Polycomb Repressive Complex 1 genetics, Polycomb Repressive Complex 2 physiology, Ubiquitin-Protein Ligases genetics, Ubiquitin-Protein Ligases metabolism, Gene Expression Regulation, Histones metabolism, Polycomb Repressive Complex 1 metabolism, Polycomb Repressive Complex 2 metabolism, Transcription, Genetic, Ubiquitination
- Abstract
Polycomb group proteins (PcGs) maintain transcriptional repression to preserve cellular identity in two distinct repressive complexes, PRC1 and PRC2, that modify histones by depositing H2AK119ub1 and H3K27me3, respectively. PRC1 and PRC2 exist in different variants and show a complex regulatory cross-talk. However, the contribution that H2AK119ub1 plays in mediating PcG repressive functions remains largely controversial. Using a fully catalytic inactive RING1B mutant, we demonstrated that H2AK119ub1 deposition is essential to maintain PcG-target gene repression in embryonic stem cells (ESCs). Loss of H2AK119ub1 induced a rapid displacement of PRC2 activity and a loss of H3K27me3 deposition. This preferentially affected PRC2.2 variant with respect to PRC2.1, destabilizing canonical PRC1 activity. Finally, we found that variant PRC1 forms can sense H2AK119ub1 deposition, which contributes to their stabilization specifically at sites where this modification is highly enriched. Overall, our data place H2AK119ub1 deposition as a central hub that mounts PcG repressive machineries to preserve cell transcriptional identity., Competing Interests: Declarations of Interests The authors declare no competing interests., (Copyright © 2019 The Authors. Published by Elsevier Inc. All rights reserved.)
- Published
- 2020
- Full Text
- View/download PDF
39. Functional Landscape of PCGF Proteins Reveals Both RING1A/B-Dependent-and RING1A/B-Independent-Specific Activities.
- Author
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Scelfo A, Fernández-Pérez D, Tamburri S, Zanotti M, Lavarone E, Soldi M, Bonaldi T, Ferrari KJ, and Pasini D
- Subjects
- Animals, Basic Helix-Loop-Helix Leucine Zipper Transcription Factors genetics, Basic Helix-Loop-Helix Transcription Factors, Chromatin genetics, DNA-Binding Proteins genetics, E2F6 Transcription Factor genetics, Heterochromatin genetics, Mice, Mouse Embryonic Stem Cells metabolism, Polycomb Repressive Complex 2 genetics, Polycomb-Group Proteins genetics, Repressor Proteins genetics, Transcription Factor DP1 genetics, Transcription Factors genetics, Upstream Stimulatory Factors genetics, Polycomb Repressive Complex 1 genetics, Transcription, Genetic, Ubiquitin-Protein Ligases genetics
- Abstract
Polycomb repressive complexes 1 and 2 (PRC1 and PRC2) control cell identity by establishing facultative heterochromatin repressive domains at common sets of target genes. PRC1, which deposits H2Aub1 through the E3 ligases RING1A/B, forms six biochemically distinct subcomplexes depending on the assembled PCGF protein (PCGF1-PCGF6); however, it is yet unclear whether these subcomplexes have also specific activities. Here we show that PCGF1 and PCGF2 largely compensate for each other, while other PCGF proteins have high levels of specificity for distinct target genes. PCGF2 associates with transcription repression, whereas PCGF3 and PCGF6 associate with actively transcribed genes. Notably, PCGF3 and PCGF6 complexes can assemble and be recruited to several active sites independently of RING1A/B activity (therefore, of PRC1). For chromatin recruitment, the PCGF6 complex requires the combinatorial activities of its MGA-MAX and E2F6-DP1 subunits, while PCGF3 requires an interaction with the USF1 DNA binding transcription factor., (Copyright © 2019 The Authors. Published by Elsevier Inc. All rights reserved.)
- Published
- 2019
- Full Text
- View/download PDF
40. Sp140 is a multi-SUMO-1 target and its PHD finger promotes SUMOylation of the adjacent Bromodomain.
- Author
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Zucchelli C, Tamburri S, Filosa G, Ghitti M, Quilici G, Bachi A, and Musco G
- Subjects
- HEK293 Cells, Humans, Protein Binding, Antigens, Nuclear chemistry, Antigens, Nuclear metabolism, PHD Zinc Fingers, Protein Domains, Sumoylation, Transcription Factors chemistry, Transcription Factors metabolism
- Abstract
Background: Human Sp140 protein is a leukocyte-specific member of the speckled protein (Sp) family (Sp100, Sp110, Sp140, Sp140L), a class of multi-domain nuclear proteins involved in intrinsic immunity and transcriptional regulation. Sp140 regulates macrophage transcriptional program and is implicated in several haematologic malignancies. Little is known about Sp140 structural domains and its post-translational modifications., Methods: We used mass spectrometry and biochemical experiments to investigate endogenous Sp140 SUMOylation in Burkitt's Lymphoma cells and Sp140 SUMOylation sites in HEK293T cells, FLAG-Sp140 transfected and His
6 -SUMO-1T95K infected. NMR spectroscopy and in vitro SUMOylation reactions were applied to investigate the role of Sp140 PHD finger in the SUMOylation of the adjacent BRD., Results: Endogenous Sp140 is a SUMO-1 target, whereby FLAG-Sp140 harbors at least 13 SUMOylation sites distributed along the protein sequence, including the BRD. NMR experiments prove direct binding of the SUMO E2 ligase Ubc9 and SUMO-1 to PHD-BRDSp140 . In vitro SUMOylation reactions show that the PHDSp140 behaves as SUMO E3 ligase, assisting intramolecular SUMOylation of the adjacent BRD., Conclusions: Sp140 is multi-SUMOylated and its PHD finger works as versatile protein-protein interaction platform promoting intramolecular SUMOylation of the adjacent BRD. Thus, combinatorial association of Sp140 chromatin binding domains generates a multifaceted interaction scaffold, whose function goes beyond the canonical histone recognition., General Significance: The addition of Sp140 to the increasing lists of multi-SUMOylated proteins opens new perspectives for molecular studies on Sp140 transcriptional activity, where SUMOylation could represent a regulatory route and a docking surface for the recruitment and assembly of leukocyte-specific transcription regulators., (Copyright © 2018 The Authors. Published by Elsevier B.V. All rights reserved.)- Published
- 2019
- Full Text
- View/download PDF
41. Structure of human Sp140 PHD finger: an atypical fold interacting with Pin1.
- Author
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Zucchelli C, Tamburri S, Quilici G, Palagano E, Berardi A, Saare M, Peterson P, Bachi A, and Musco G
- Subjects
- Amino Acid Sequence, Binding Sites, Blotting, Western, Chromatin genetics, HEK293 Cells, Humans, Immunoprecipitation, Magnetic Resonance Spectroscopy, Molecular Sequence Data, NIMA-Interacting Peptidylprolyl Isomerase, Phosphorylation, Protein Binding, Protein Conformation, Sequence Homology, Amino Acid, Antigens, Nuclear chemistry, Antigens, Nuclear metabolism, Histones metabolism, Peptidylprolyl Isomerase metabolism, Protein Folding, Transcription Factors chemistry, Transcription Factors metabolism
- Abstract
Sp140 is a nuclear leukocyte-specific protein involved in primary biliary cirrhosis and a risk factor in chronic lymphocytic leukemia. The presence of several chromatin related modules such as plant homeodomain (PHD), bromodomain and SAND domain suggests a role in chromatin-mediated regulation of gene expression; however, its real function is still elusive. Herein we present the solution structure of Sp140-PHD finger and investigate its role as epigenetic reader in vitro. Sp140-PHD presents an atypical PHD finger fold which does not bind to histone H3 tails but is recognized by peptidylprolyl isomerase Pin1. Pin1 specifically binds to a phosphopeptide corresponding to the L3 loop of Sp140-PHD and catalyzes cis-trans isomerization of a pThr-Pro bond. Moreover co-immunoprecipitation experiments demonstrate FLAG-Sp140 interaction with endogenous Pin1 in vivo. Overall these data include Sp140 in the list of the increasing number of Pin1 binders and expand the regulatory potential of PHD fingers as versatile structural platforms for diversified interactions., (© 2013 FEBS.)
- Published
- 2014
- Full Text
- View/download PDF
42. Skeletally metastatic malignant melanoma of the foot.
- Author
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Tamburri SA and Boberg JS
- Subjects
- Adult, Amputation, Surgical, Foot Diseases surgery, Humans, Male, Melanoma pathology, Melanoma surgery, Soft Tissue Neoplasms surgery, Toes surgery, Bone Neoplasms secondary, Foot Diseases pathology, Melanoma secondary, Soft Tissue Neoplasms pathology
- Abstract
Malignant melanoma involving the foot has typically been documented in cases whereby the primary lesion was subungually located. Characteristic clinical features usually assist the physician in diagnosing the suspicious lesion. The case study that follows illustrates an atypical presentation of skeletally metastatic malignant melanoma of the foot where the primary lesion was not identified.
- Published
- 1994
43. Hallux set angle. A new radiographic measurement for hallux valgus.
- Author
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Boberg JS, Menn JJ, Tamburri SA, and Chang TJ
- Subjects
- Hallux Valgus surgery, Humans, Radiography, Hallux Valgus diagnostic imaging
- Abstract
The authors introduce a unique and clinically oriented technique for evaluation of hallux abducto valgus deformity and its operative correction. A new concept in the application of the Austin osteotomy is also presented.
- Published
- 1994
- Full Text
- View/download PDF
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