Zobrazeno 1 - 10
of 47
pro vyhledávání: '"Kammoun, Elias"'
Autor:
Boorman, Peter G., Gandhi, Poshak, Buchner, Johannes, Stern, Daniel, Ricci, Claudio, Baloković, Mislav, Asmus, Daniel, Harrison, Fiona A., Svoboda, Jiří, Greenwell, Claire, Koss, Michael, Alexander, David M., Annuar, Adlyka, Bauer, Franz, Brandt, William N., Brightman, Murray, Panessa, Francesca, Chen, Chien-Ting J., Farrah, Duncan, Forster, Karl, Grefenstette, Brian, Hönig, Sebastian F., Hill, Adam B., Kammoun, Elias, Lansbury, George, Lanz, Lauranne, LaMassa, Stephanie, Madsen, Kristin, Marchesi, Stefano, Middleton, Matthew, Mingo, Beatriz, Parker, Michael L., Treister, Ezequiel, Ueda, Yoshihiro, Urry, C. Megan, Zappacosta, Luca
Hard X-ray-selected samples of Active Galactic Nuclei (AGN) provide one of the cleanest views of supermassive black hole accretion, but are biased against objects obscured by Compton-thick gas column densities of $N_{\rm H}$ $>$ 10$^{24}$ cm$^{-2}$.
Externí odkaz:
http://arxiv.org/abs/2410.07339
Autor:
Bogensberger, David, Miller, Jon M., Mushotzky, Richard, Brandt, W. N., Kammoun, Elias, Zoghbi, Abderahmen, Behar, Ehud
The structure of the jet in Cen A is likely better revealed in X-rays than in the radio band, which is usually used to investigate jet proper motions. In this paper, we analyze Chandra ACIS observations of Cen A from 2000 to 2022 and develop an algor
Externí odkaz:
http://arxiv.org/abs/2408.14078
Autor:
Serafinelli, Roberto, De Rosa, Alessandra, Tortosa, Alessia, Stella, Luigi, Vagnetti, Fausto, Bianchi, Stefano, Ricci, Claudio, Kammoun, Elias, Petrucci, Pierre-Olivier, Middei, Riccardo, Lanzuisi, Giorgio, Marinucci, Andrea, Ursini, Francesco, Matt, Giorgio
Publikováno v:
A&A 690, A145 (2024)
Active galactic nuclei (AGN) are extremely variable in the X-ray band down to very short timescales. However, the driver behind the X-ray variability is still poorly understood. Previous results suggest that the hot corona responsible for the primary
Externí odkaz:
http://arxiv.org/abs/2407.06769
Autor:
Greenwell, Claire L., Klindt, Lizelke, Lansbury, George B., Rosario, David J., Alexander, David M., Aird, James, Stern, Daniel, Forster, Karl, Koss, Michael J., Bauer, Franz E., Ricci, Claudio, Tomsick, John, Brandt, William N., Connor, Thomas, Boorman, Peter G., Annuar, Adlyka, Ballantyne, David R., Chen, Chien-Ting, Civano, Francesca, Comastri, Andrea, Fawcett, Victoria A., Fornasini, Francesca M., Gandhi, Poshak, Harrison, Fiona, Heida, Marianne, Hickox, Ryan, Kammoun, Elias S., Lanz, Lauranne, Marchesi, Stefano, Noirot, Gaël, Romero-Colmenero, Encarni, Treister, Ezequiel, Urry, C. Megan, Väisänen, Petri, van Soelen, Brian
We present a catalog of hard X-ray serendipitous sources detected in the first 80 months of observations by the Nuclear Spectroscopic Telescope Array (NuSTAR). The NuSTAR serendipitous survey 80-month (NSS80) catalog has an unprecedented $\sim$ 62 Ms
Externí odkaz:
http://arxiv.org/abs/2404.17637
Autor:
Zak, Miranda K., Miller, Jon M., Behar, Ehud, Brandt, William N., Brenneman, Laura, Draghis, Paul A., Kammoun, Elias, Koss, Michael J., Reynolds, Mark T., Zoghbi, Abderahmen
Markarian 817 is a bright and variable Seyfert-1.2 active galactic nucleus (AGN). X-ray monitoring of Mrk 817 with the Neil Gehrels Swift Observatory in 2022 revealed that the source flux had declined to a lower level than recorded at any prior point
Externí odkaz:
http://arxiv.org/abs/2312.06487
Autor:
Pfeifle, Ryan W., Boorman, Peter G., Weaver, Kimberly A., Buchner, Johannes, Civano, Francesca, Madsen, Kristin, Stern, Daniel, Torres-Albà, Núria, Nardini, Emanuele, Ricci, Claudio, Marchesi, Stefano, Ballantyne, D. R., Sicilian, Dominic, Chen, Chien-Ting, Kammoun, Elias, Hickox, Ryan C., García, Javier A., Mallick, Labani
A fundamental goal of modern-day astrophysics is to understand the connection between supermassive black hole (SMBH) growth and galaxy evolution. Merging galaxies offer one of the most dramatic channels for galaxy evolution known, capable of driving
Externí odkaz:
http://arxiv.org/abs/2311.05154
Autor:
Brightman, Murray, Margutti, Raffaella, Polzin, Ava, Jaodand, Amruta, Hotokezaka, Kenta, Alford, Jason A. J., Hallinan, Gregg, Kammoun, Elias, Mooley, Kunal, Masterson, Megan, Marcotulli, Lea, Rau, Arne, Younes, George A., Stern, Daniel, García, Javier A., Madsen, Kristin
HEX-P will launch at a time when the sky is being routinely scanned for transient gravitational wave, electromagnetic and neutrino phenomena that will require the capabilities of a sensitive, broadband X-ray telescope for follow up studies. These inc
Externí odkaz:
http://arxiv.org/abs/2311.04856
Autor:
Civano, Francesca, Zhao, Xiurui, Boorman, Peter, Marchesi, Stefano, Ananna, Tonima, Creech, Samantha, Chen, Chien-Ting, Hickox, Ryan, Stern, Daniel, Madsen, Kristin, García, Javier A., Silver, Ross, Aird, James, Alexander, David M., Balokovíc, Mislav, Brandt, William N., Buchner, Johannes, Gandhi, Poshak, Kammoun, Elias, LaMassa, Stephanie, Lanzuisi, Giorgio, Merloni, Andrea, Moretti, Alberto, Nandra, Kirpal, Nardini, Emanuele, Pizzetti, Anrealuna, Puccetti, Simonetta, Pfeifle, Ryan, Ricci, Claudio, Spiga, Daniele, Torres-Albá, Nuria, Collaboration, the HEX-P
Since the discovery of the cosmic X-ray background (CXB), astronomers have strived to understand the accreting supermassive black holes (SMBHs) contributing to its peak in the 10-40 keV band. Existing soft X-ray telescopes could study this population
Externí odkaz:
http://arxiv.org/abs/2311.04832
Autor:
Gonzalez, Adam G., Gallo, Luigi C., Miller, Jon M., Kammoun, Elias S., Ghosh, Akshay, Pottie, Ben A.
We present the first results of a high-cadence Swift monitoring campaign ($3-4$ visits per day for $75$ days) of the Seyfert 1.5 galaxy NGC 6814 characterizing its variability throughout the X-ray and UV/optical wavebands. Structure function analysis
Externí odkaz:
http://arxiv.org/abs/2308.15543
Autor:
Saade, M. Lynne, Brightman, Murray, Stern, Daniel, Connor, Thomas, Djorgovski, S. G., D'Orazio, Daniel J., Ford, K. E. S., Graham, Matthew J., Haiman, Zoltan, Jun, Hyunsung D., Kammoun, Elias, Kraft, Ralph P., McKernan, Barry, Vikhlinin, Alexei, Walton, Dominic J.
We present analysis of NuSTAR X-ray observations of three AGN that were identified as candidate subparsec binary supermassive black hole (SMBH) systems in the Catalina Real-Time Transient Survey based on apparent periodicity in their optical light cu
Externí odkaz:
http://arxiv.org/abs/2304.06144