Zobrazeno 1 - 10
of 1 324
pro vyhledávání: '"Vito F"'
Autor:
Saeid Ebrahimzadeh, Sakib Adnan, Yishen Li, Vito F Pecile, Jakob Fellinger, Sarper Salman, Christoph M Heyl, Ingmar Hartl, Oliver H Heckl, Gil Porat
Publikováno v:
JPhys Photonics, Vol 6, Iss 2, p 02LT01 (2024)
Applications of mode-locked fiber lasers benefit from robust and self-starting mode-locking, spectral tuning, high pulse energy and high average power. All-polarization-maintaining (PM) fiber lasers mode-locked with a phase-biased nonlinear amplifyin
Externí odkaz:
https://doaj.org/article/2210aa9949374bfa9e9ef4c7584e785a
Autor:
Soehartati Gondhowiardjo, Nadia Christina, Ngakan P.D. Ganapati, Salik Hawariy, Fahmi Radityamurti, Vito F. Jayalie, Steven Octavianus, Andre Prawira Putra, Sri M. Sekarutami, Gregorius B. Prajogi, Angela Giselvania, Marlinda Adham, Agus R.A.H. Hamid, Endang Widyastuti, Yogi Prabowo, Tiara Aninditha, Gatot Purwoto, Renindra A. Aman, Trifona P. Siregar, Alvita Dewi Siswoyo, Diah R. Handjari, Djumhana Atmakusuma, Wulyo Rajabto, Nadia A. Mulansari, Nurul Ratna, Ceva W. Pitoyo, Sonar Soni Panigoro, Diani Kartini, Erwin D. Yulian, Rossalyn S. Andrisa, Wifanto S. Jeo, Rizky K. Wardhani, Tresia F.U. Tambunan, Feranindhya Agianda
Publikováno v:
JCO Global Oncology, Vol , Iss 7, Pp 190-203 (2021)
PURPOSEIn 2016, there were 1,308,061 cases of cancer being treated in Indonesia, with 2.2 trillion rupiahs spent, amounting to $486,960,633 in US dollars (purchasing power parity 2016). The high burden of cancers in Indonesia requires a valid data co
Externí odkaz:
https://doaj.org/article/c53c3720c382406baa7df81ec75f4702
Autor:
Mazzolari, G., Gilli, R., Maiolino, R., Prandoni, I., Delvecchio, I., Norman, C., Jimenez-Andrade, E. F., Belladitta, S., Vito, F., Momjian, E., Chiaberge, M., Trefoloni, B., Signorini, M., Ji, X., D'Amato, Q., Risaliti, G., Baldi, R. D., Fabian, A., Übler, H., D'Eugenio, F., Scholtz, J., Juodžbalis, I., Mignoli, M., Brusa, M., Murphy, E., Muxlow, T. W. B.
We explore the radio emission of spectroscopically confirmed, X-ray weak, Broad Line AGN (BLAGN, or type 1) selected with JWST in the GOODS-N field, one of the fields with the best combination of deep radio observations and statistics of JWST-selecte
Externí odkaz:
http://arxiv.org/abs/2412.04224
Autor:
Saccheo, I., Bongiorno, A., Piconcelli, E., Zappacosta, L., Bischetti, M., D'Odorico, V., Done, C., Temple, M. J., Testa, V., Tortosa, A., Brusa, M., Carniani, S., Civano, F., Comastri, A., Cristiani, S., De Cicco, D., Elvis, M., Fan, X., Feruglio, C., Fiore, F., Gallerani, S., Giallongo, E., Gilli, R., Grazian, A., Guainazzi, M., Haardt, F., Maiolino, R., Menci, N., Miniutti, G., Nicastro, F., Paolillo, M., Puccetti, S., Salvestrini, F., Schneider, R., Tombesi, F., Tripodi, R., Valiante, R., Vallini, L., Vanzella, E., Vietri, G., Vignali, C., Vito, F., Volonteri, M., La Franca, F.
We aim at characterizing the X-ray-to-optical/near-infrared broad-band emission of luminous QSOs in the first Gyr of cosmic evolution to understand whether they exhibit differences compared to the lower-\textit{z} QSO population. Our goal is also to
Externí odkaz:
http://arxiv.org/abs/2411.02105
Autor:
Tortosa, A., Zappacosta, L., Piconcelli, E., Bischetti, M., Done, C., Miniutti, G., Saccheo, I., Vietri, G., Bongiorno, A., Brusa, M., Carniani, S., Chilingarian, I. V., Civano, F., Cristiani, S., D'Odorico, V., Elvis, M., Fan, X., Feruglio, C., Fiore, F., Gallerani, S., Giallongo, E., Gilli, R., Grazian, A., Guainazzi, M., Haardt, F., Luminari, A., Maiolino, R., Menci, N., Nicastro, F., Petrucci, P. O., Puccetti, S., Salvestrini, F., Schneider, R., Testa, V., Tombesi, F., Tripodi, R., Valiante, R., Vallini, L., Vanzella, E., Vasylenko, A., Vignali, C., Vito, F., Volonteri, M., La Franca, F.
One of the main open questions in the field of luminous ($L_{\rm bol}>10^{47}\,\rm erg\,s^{-1}$) quasars (QSOs) at $z \gtrsim 6$ is the rapid formation ($< 1\,$Gyr) of their supermassive black holes (SMBHs). For this work we analysed the relation bet
Externí odkaz:
http://arxiv.org/abs/2410.12786
Autor:
Travascio, A., Cantalupo, S., Tozzi, P., Vito, F., Paggi, A., Pezzulli, G., Elvis, M., Fabbiano, G., Fiore, F., Fossati, M., Fresco, A., Fumagalli, M., Galbiati, M., Lazeyras, T., Ledos, N., Pannella, M., Pensabene, A., Quadri, G., Wang, W.
Exploring SMBH population in protoclusters offers valuable insights into how environment affects SMBH growth. However, research on AGN within these areas is still limited by the small number of protoclusters known at high redshift and by the availabi
Externí odkaz:
http://arxiv.org/abs/2410.03933
Autor:
Pilat, Florian, Windischhofer, Andreas, Beiser, Maximilian, Pecile, Vito F., Gangrskaia, Elizaveta, Pugžlys, Audrius, Weih, Robert, Koeth, Johannes, Baltuška, Andrius, Heckl, Oliver H., Schwarz, Benedikt
Interband Cascade Lasers (ICL) have matured into a versatile technological platform in the mid-infrared spectral domain. To broaden their applicability even further, ongoing research pursues the emission of ultrashort pulses. The most promising appro
Externí odkaz:
http://arxiv.org/abs/2405.10203
Autor:
Pecile, Vito F., Leskowschek, Michael, Modsching, Norbert, Wittwer, Valentin J., Südmeyer, Thomas, Heckl, Oliver H.
Within the domain of optical frequency comb systems operating in the mid-infrared, extensive exploration has been undertaken regarding critical parameters such as stabilization, coherence, or spectral tunability. Despite this, certain essential param
Externí odkaz:
http://arxiv.org/abs/2403.19360
Autor:
Zuo, Zihao, Zhu, Shifu, Brandt, W. N., Garmire, Gordon P., Vito, F., Wu, Jianfeng, Xue, Yongquan
Highly radio-loud quasars (HRLQs; $\log R>2.5$) at $z\gtrsim 4$ show apparent enhanced X-ray emission compared to matched HRLQs at lower redshifts, perhaps due to a redshift-dependent fractional contribution to the X-ray luminosity from inverse-Compt
Externí odkaz:
http://arxiv.org/abs/2402.17828
Autor:
Pouliasis, E., Ruiz, A., Georgantopoulos, I., Vito, F., Gilli, R., Vignali, C., Ueda, Y., Koulouridis, E., Akiyama, M., Marchesi, S., Laloux, B., Nagao, T., Paltani, S., Pierre, M., Toba, Y., Habouzit, M., Vijarnwannaluk, B., Garrel, C.
Publikováno v:
A&A 685, A97 (2024)
The XLF of AGN offers a robust tool to study the evolution and the growth of SMBHs over cosmic time. Owing to the limited area probed by X-ray surveys, optical surveys are routinely used to probe the accretion in the high redshift Universe $z\geq 3$.
Externí odkaz:
http://arxiv.org/abs/2401.13515