Search Results - "TOZZI, P"

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    Radio-faint AGN: a tale of two populations by Padovani, P., Bonzini, M., Kellermann, K. I., Miller, N., Mainieri, V., Tozzi, P.

    “…We study the Extended Chandra Deep Field-South Very Large Array sample, which reaches a flux density limit at 1.4 GHz of 32.5 μJy at the field centre and…”
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    The X-Ray Halo Scaling Relations of Supermassive Black Holes by Gaspari, M., Eckert, D., Ettori, S., Tozzi, P., Bassini, L., Rasia, E., Brighenti, F., Sun, M., Borgani, S., Johnson, S. D., Tremblay, G. R., Stone, J. M., Temi, P., Yang, H.-Y. K., Tombesi, F., Cappi, M.

    Published in The Astrophysical journal (20-10-2019)
    “…We carry out a comprehensive Bayesian correlation analysis between hot halos and direct masses of supermassive black holes (SMBHs), by retrieving the X-ray…”
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    The sub-mJy radio sky in the Extended Chandra Deep Field-South: source population by Bonzini, M., Padovani, P., Mainieri, V., Kellermann, K. I., Miller, N., Rosati, P., Tozzi, P., Vattakunnel, S.

    “…The sub-mJy radio population is a mixture of active systems, that is star-forming galaxies (SFGs) and active galactic nuclei (AGNs). We study a sample of 883…”
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    Star formation properties of sub-mJy radio sources by Bonzini, M., Mainieri, V., Padovani, P., Andreani, P., Berta, S., Bethermin, M., Lutz, D., Rodighiero, G., Rosario, D., Tozzi, P., Vattakunnel, S.

    “…We investigate the star formation properties of ∼800 sources detected in one of the deepest radio surveys at 1.4 GHz. Our sample spans a wide redshift range…”
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    Paving the way for the JWST: witnessing globular cluster formation at z > 3 by Vanzella, E., Calura, F., Meneghetti, M., Mercurio, A., Castellano, M., Caminha, G. B., Balestra, I., Rosati, P., Tozzi, P., De Barros, S., Grazian, A., D'Ercole, A., Ciotti, L., Caputi, K., Grillo, C., Merlin, E., Pentericci, L., Fontana, A., Cristiani, S., Coe, D.

    “…Abstract We report on five compact, extremely young (<10 Myr) and blue (βUV < −2.5, Fλ = λβ) objects observed with VLT/Multi Unit Spectroscopic Explorer at…”
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    Constraints on the Lyman continuum escape fraction for faint star-forming galaxies by Japelj, J., Vanzella, E., Fontanot, F., Cristiani, S., Caminha, G. B., Tozzi, P., Balestra, I., Rosati, P., Meneghetti, M.

    “…Abstract Star-forming galaxies have long been considered the dominant sources of the cosmic ultraviolet background radiation at early epochs. However,…”
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    Candidate Population III stellar complex at z = 6.629 in the MUSE Deep Lensed Field by Vanzella, E, Meneghetti, M, Caminha, G B, Castellano, M, Calura, F, Rosati, P, Grillo, C, Dijkstra, M, Gronke, M, Sani, E, Mercurio, A, Tozzi, P, Nonino, M, Cristiani, S, Mignoli, M, Pentericci, L, Gilli, R, Treu, T, Caputi, K, Cupani, G, Fontana, A, Grazian, A, Balestra, I

    “…ABSTRACT We discovered a strongly lensed (μ ≳ 40) Ly α emission at z = 6.629 (S/N ≃ 18) in the MUSE Deep Lensed Field (MDLF) targeting the Hubble Frontier…”
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    A New Photometric Technique for the Joint Selection of Star-forming and Passive Galaxies at 1.4 z 2.5 by Daddi, E, Cimatti, A, Renzini, A, Fontana, A, Mignoli, M, Pozzetti, L, Tozzi, P, Zamorani, G

    Published in The Astrophysical journal (20-12-2004)
    “…A simple two-color selection based on B-, z-, and K-band photometry is proposed for culling galaxies at 1.4 z 2.5 in K-selected samples and classifying them as…”
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    Illuminating gas inflows/outflows in the MUSE deepest fields: Lyα nebulae around forming galaxies at z ≃ 3.3 by Vanzella, E., Balestra, I., Gronke, M., Karman, W., Caminha, G. B., Dijkstra, M., Rosati, P., De Barros, S., Caputi, K., Grillo, C., Tozzi, P., Meneghetti, M., Mercurio, A., Gilli, R.

    “…We report the identification of extended Lyα nebulae at z ≃ 3.3 in the Hubble Ultra Deep Field (HUDF, ≃40 kpc × 80 kpc) and behind the Hubble Frontier Field…”
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    The Great Observatories Origins Deep Survey: Constraints on the Lyman Continuum Escape Fraction Distribution of Lyman-break Galaxies at 3.4 < z < 4.5 by Vanzella, E, Giavalisco, M, Inoue, A. K, Nonino, M, Fontanot, F, Cristiani, S, Grazian, A, Dickinson, M, Stern, D, Tozzi, P, Giallongo, E, Ferguson, H, Spinrad, H, Boutsia, K, Fontana, A, Rosati, P, Pentericci, L

    Published in The Astrophysical journal (10-12-2010)
    “…We use ultra-deep ultraviolet VLT/VIMOS intermediate-band and VLT/FORS1 narrowband imaging in the GOODS Southern field to derive limits on the distribution of…”
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    The reversal of the SF–density relation in a massive, X-ray-selected galaxy cluster at z  = 1.58: results from Herschel by Santos, J. S., Altieri, B., Valtchanov, I., Nastasi, A., Böhringer, H., Cresci, G., Elbaz, D., Fassbender, R., Rosati, P., Tozzi, P., Verdugo, M.

    “…Abstract Dusty, star-forming galaxies have a critical role in the formation and evolution of massive galaxies in the Universe. Using deep far-infrared imaging…”
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    X-Ray Unveiling Events in a z ≈ 1.6 Active Galactic Nucleus in the 7 Ms Chandra Deep Field-South by Yu, Li-Ming, Luo, Bin, Brandt, W. N., Bauer, Franz E., De Cicco, D., Fabian, A., Gilli, R., Koekemoer, A., Paolillo, M., Schneider, D. P., Shemmer, O., Tozzi, P., Trump, Jonathan R., Vignali, C., Vito, F., Wang, J.-X., Xue, Y. Q.

    Published in The Astrophysical journal (01-05-2023)
    “…Abstract We investigate the extreme X-ray variability of a z = 1.608 active galactic nucleus in the 7 Ms Chandra Deep Field-South (XID 403), which showed two…”
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    X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation by Borgani, S., Murante, G., Springel, V., Diaferio, A., Dolag, K., Moscardini, L., Tormen, G., Tornatore, L., Tozzi, P.

    “…We present results on the X-ray properties of clusters and groups of galaxies, extracted from a large cosmological hydrodynamical simulation. We used the…”
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    THE 4 Ms CHANDRA DEEP FIELD-SOUTH NUMBER COUNTS APPORTIONED BY SOURCE CLASS: PERVASIVE ACTIVE GALACTIC NUCLEI AND THE ASCENT OF NORMAL GALAXIES by LEHMER, B. D, XUE, Y. Q, PAOLILLO, M, PTAK, A, SHEMMER, O, SCHNEIDER, D. P, TOZZI, P, VIGNALI, C, BRANDT, W. N, ALEXANDER, D. M, BAUER, F. E, BRUSA, M, COMASTRI, A, GILLI, R, HORNSCHEMEIER, A. E, LUO, B

    Published in The Astrophysical journal (10-06-2012)
    “…We present 0.5-2 keV, 2-8 keV, 4-8 keV, and 0.5-8 keV (hereafter soft, hard, ultra-hard, and full bands, respectively) cumulative and differential number-count…”
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    The Evolution of AGN Host Galaxies: From Blue to Red and the Influence of Large-Scale Structures by Silverman, J. D, Mainieri, V, Lehmer, B. D, Alexander, D. M, Bauer, F. E, Bergeron, J, Brandt, W. N, Gilli, R, Hasinger, G, Schneider, D. P, Tozzi, P, Vignali, C, Koekemoer, A. M, Miyaji, T, Popesso, P, Rosati, P, Szokoly, G

    Published in The Astrophysical journal (10-03-2008)
    “…We present an analysis of 109 moderate-luminosity AGNs in the Extended Chandra Deep Field-South survey, which is drawn from 5549 galaxies from the COMBO-17 and…”
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    CHANDRA DEEP OBSERVATION OF XDCP J0044.0-2033, A MASSIVE GALAXY CLUSTER AT z > 1.5 by Tozzi, P, Santos, J S, Jee, M J, Fassbender, R, Rosati, P, Nastasi, A, man, W, Sartoris, B, Borgani, S, Boehringer, H, Altieri, B, Pratt, G W, Nonino, M, Jones, C

    Published in The Astrophysical journal (20-01-2015)
    “…We report the analysis of the Chandra observation of XDCP J0044.0-2033, a massive, distant galaxy cluster discovered in the XDCP survey. The total exposure…”
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