Zobrazeno 1 - 10
of 56
pro vyhledávání: '"Fornasini F"'
Autor:
Zhao, X., Civano, F., Fornasini, F. M., Alexander, D. M., Cappelluti, N., Chen, C. T., Cohen, S. H., Elvis, M., Gandhi, P., Grogin, N. A., Hickox, R. C., Jansen, R. A., Koekemoer, A., Lanzuisi, G., Maksym, W. P., Masini, A., Rosario, D. J., Ward, M. J., Willmer, C. N. A., Windhorst, R. A.
We present the $NuSTAR$ extragalactic survey of the $James$ $Webb$ $Space$ $Telescope$ ($JWST$) North Ecliptic Pole (NEP) Time-Domain Field. The survey covers a $\sim$0.16 deg$^2$ area with a total exposure of 681 ks acquired in a total of nine obser
Externí odkaz:
http://arxiv.org/abs/2109.13839
Autor:
Lazzarini, M., Williams, B. F., Hornschemeier, A. E., Antoniou, V., Vasilopoulos, G., Haberl, F., Vulic, N., Yukita, M., Zezas, A., Bodaghee, A., Lehmer, B. D., Maccarone, T. J., Ptak, A., Wik, D., Fornasini, F. M., Hong, Jaesub, Kennea, J. A., Tomsick, J. A., Venters, T., Udalski, A., Cassity, A.
We present a source catalog from the first deep hard X-ray ($E>10$ keV) survey of the Small Magellanic Cloud (SMC), the NuSTAR Legacy Survey of the SMC. We observed three fields, for a total exposure time of 1 Ms, along the bar of this nearby star-fo
Externí odkaz:
http://arxiv.org/abs/1909.11110
Autor:
Hickox, R. C., Civano, F., Ballantyne, D. R., Balokovic, M., Boorman, P. G., Brandt, W. N., Canning, R. E. A., Fornasini, F., Gandhi, P., Jones, M. L., Lansbury, G. B., Lanz, L., Lanzuisi, G., Madsen, K. K., Marchesi, S., Masini, A., Ananna, T., Stern, D., Ricci, C.
The cosmic X-ray background (CXB), which peaks at an energy of ~30 keV, is produced primarily by emission from accreting supermassive black holes (SMBHs). The CXB therefore serves as a constraint on the integrated SMBH growth in the Universe and the
Externí odkaz:
http://arxiv.org/abs/1905.11439
Autor:
Vulic, N., Hornschemeier, A. E., Antoniou, V., Basu-Zych, A. R., Binder, B., Fornasini, F. M., Furst, F., Haberl, F., Heida, M., Lehmer, B. D., Maccarone, T. J., Ptak, A. F., Sivakoff, G. R., Tzanavaris, P., Wik, D. R., Williams, B. F., Wilms, J., Yukita, M., Zezas, A.
What are the most important conditions and processes governing the growth of stellar-origin compact objects? The identification of compact object type as either black hole (BH) or neutron star (NS) is fundamental to understanding their formation and
Externí odkaz:
http://arxiv.org/abs/1903.09858
Autor:
Fabbiano, G., Elvis, M., Accomazzi, A., Berriman, G. B., Brickhouse, N., Bose, S., Carrera, D., Chilingarian, I., Civano, F., Czerny, B., D'Abrusco, R., Diemer, B., Drake, J., Meibody, R. Emami, Farah, J. R., Fazio, G. G., Feigelson, E., Fornasini, F., Gallagher, Jay, Grindlay, J., Hernquist, L., James, D. J., Karovska, M., Kashyap, V., Kim, D. -W., Lacy, G. M., Lazio, J., Lusso, E., Maksym, W. P., Galarza, R. Martinez, Mazzarella, J., Ntampaka, M., Risaliti, G., Sanders, D., Scoville, N., Shapiro, I., Siemiginowska, A., Smth, A., Smith, S., Szentgyorgyi, A., Tacchella, S., Thakar, A., Tolls, V., Vrtilek, S., Wilkes, B., Wilner, D., Willner, S. P., Wolk, S. J., Zhao, J. -H.
We write in response to the call from the 2020 Decadal Survey to submit white papers illustrating the most pressing scientific questions in astrophysics for the coming decade. We propose exploration as the central question for the Decadal Committee's
Externí odkaz:
http://arxiv.org/abs/1903.06634
Autor:
Masini, A., Civano, F., Comastri, A., Fornasini, F., Ballantyne, D. R., Lansbury, G. B., Treister, E., Alexander, D. M., Boorman, P. G., Brandt, W. N., Farrah, D., Gandhi, P., Harrison, F. A., Hickox, R. C., Kocevski, D. D., Lanz, L., Marchesi, S., Puccetti, S., Ricci, C., Saez, C., Stern, D., Zappacosta, L.
We present the results and the source catalog of the NuSTAR survey in the UKIDSS Ultra Deep Survey (UDS) field, bridging the gap in depth and area between NuSTAR's ECDFS and COSMOS surveys. The survey covers a $\sim 0.6$ deg$^2$ area of the field for
Externí odkaz:
http://arxiv.org/abs/1801.01881
Autor:
Clavel, Maïca, Tomsick, J. A., Bodaghee, A., Chiu, J. -L., Fornasini, F. M., Hong, J., Krivonos, R., Ponti, G., Rahoui, F., Stern, D.
Studying the population of faint hard X-ray sources along the plane of the Galaxy is challenging because of high-extinction and crowding, which make the identification of individual sources more difficult. IGR J18293-1213 is part of the population of
Externí odkaz:
http://arxiv.org/abs/1605.08802
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