Zobrazeno 1 - 10
of 56
pro vyhledávání: '"Romero, Charles E."'
Autor:
Zhou, Dazhi, Greve, Thomas R., Gullberg, Bitten, Lee, Minju M., Di Mascolo, Luca, Dicker, Simon R., Romero, Charles E., Chapman, Scott C., Chen, Chian-Chou, Cornish, Thomas, Devlin, Mark J., Ho, Luis C., Kohno, Kotaro, Lagos, Claudia D. P., Mason, Brian S., Mroczkowski, Tony, Wagg, Jeff F. W., Wang, Q. Daniel, Wang, Ran, Brinch, Malte., Dannerbauer, Helmut, Jiang, Xue-Jian, Lauritsen, Lynge R. B., Vijayan, Aswin P., Vizgan, David, Wardlow, Julie L., Sarazin, Craig L., Sarmiento, Karen P., Serjeant, Stephen, Bhandarkar, Tanay A., Haridas, Saianeesh K., Moravec, Emily, Orlowski-Scherer, John, Sievers, Jonathan L. R., Tanaka, Ichi, Wang, Yu-Jan, Zeballos, Milagros, Laza-Ramos, Andres, Liu, Yuanqi, Hassan, Mohd Shaiful Rizal, Jwel, Abdul Kadir Md, Nazri, Affan Adly, Lim, Ming-Kang, Ibrahim, Ungku Ferwani Salwa Ungku
High-redshift radio(-loud) galaxies (H$z$RGs) are massive galaxies with powerful radio-loud active galactic nuclei (AGNs) and serve as beacons for protocluster identification. However, the interplay between H$z$RGs and the large-scale environment rem
Externí odkaz:
http://arxiv.org/abs/2408.02177
Autor:
Romero, Charles E., Gaspari, Massimo, Schellenberger, Gerrit, Benson, Bradford A., Bleem, Lindsey E., Bulbul, Esra, Klein, Matthias, Kraft, Ralph, Nulsen, Paul, Reichardt, Christian L., Salvati, Laura, Somboonpanyakul, Taweewat, Su, Yuanyuan
Studies of surface brightness fluctuations in the intracluster medium (ICM) present an indirect probe of turbulent properties such as the turbulent velocities, injection scales, and the slope of the power spectrum of fluctuations towards smaller scal
Externí odkaz:
http://arxiv.org/abs/2404.04373
Autor:
Calzadilla, Michael S., McDonald, Michael, Benson, Bradford A., Bleem, Lindsey E., Croston, Judith H., Donahue, Megan, Edge, Alastair C., Floyd, Benjamin, Garmire, Gordon P., Hlavacek-Larrondo, Julie, Huynh, Minh T., Khullar, Gourav, Kraft, Ralph P., McNamara, Brian R., Noble, Allison G., Romero, Charles E., Ruppin, Florian, Somboonpanyakul, Taweewat, Voit, G. Mark
We present a multi-wavelength study of the brightest cluster galaxies (BCGs) in a sample of the 95 most massive galaxy clusters selected from South Pole Telescope (SPT) Sunyaev-Zeldovich (SZ) survey. Our sample spans a redshift range of 0.3 < z < 1.7
Externí odkaz:
http://arxiv.org/abs/2311.00396
Autor:
Romero, Charles E., Gaspari, Massimo, Schellenberger, Gerrit, Bhandarkar, Tanay, Devlin, Mark, Dicker, Simon R., Forman, William, Khatri, Rishi, Kraft, Ralph, Di Mascolo, Luca, Mason, Brian S., Moravec, Emily, Mroczkowski, Tony, Nulsen, Paul, Orlowski-Scherer, John, Sarmiento, Karen Perez, Sarazin, Craig, Sievers, Jonathan, Su, Yuanyuan
The galaxy cluster Zwicky 3146 is a sloshing cool core cluster at $z{=}0.291$ that in SZ imaging does not appear to exhibit significant pressure substructure in the intracluster medium (ICM). We perform a surface brightness fluctuation analysis via F
Externí odkaz:
http://arxiv.org/abs/2305.05790
Autor:
Orlowski-Scherer, John, Haridas, Saianeesh K., Di Mascolo, Luca, Sarmiento, Karen Perez, Romero, Charles E., Dicker, Simon, Mroczkowski, Tony, Bhandarkar, Tanay, Churazov, Eugene, Clarke, Tracy E, Devlin, Mark, Gaspari, Massimo, Lowe, Ian, Mason, Brian, Sarazin, Craig L, Sievers, Jonathon, Sunyaev, Rashid
Publikováno v:
A&A 667, L6 (2022)
Mechanical feedback from active galactic nuclei (AGN) is thought to be the dominant feedback mechanism quenching cooling flows and star formation in galaxy cluster cores. However, the mechanisms by which AGN couple to the intracluster medium (ICM) ar
Externí odkaz:
http://arxiv.org/abs/2207.07100
Autor:
Decker, Bandon, Brodwin, Mark, Saha, Ripon, Connor, Thomas, Eisenhardt, Peter R. M., Gonzalez, Anthony H., Moravec, Emily, Muhibullah, Mustafa, Stanford, S. Adam, Stern, Daniel, Thongkham, Khunanon, Wylezalek, Dominika, Dicker, Simon R., Mason, Brian, Mroczkowski, Tony, Romero, Charles E., Ruppin, Florian
We present stellar mass fractions and composite luminosity functions (LFs) for a sample of \Ncl\ clusters from the Massive and Distant Clusters of WISE Survey (MaDCoWS) at a redshift range of $0.951 \leq z \leq 1.43$. Using SED fitting of optical and
Externí odkaz:
http://arxiv.org/abs/2112.12239
Autor:
Dicker, Simon R., Romero, Charles E., Di Mascolo, Luca, Mroczkowski, Tony, Sievers, Jonathan, Moravec, Emily, Bhandarkar, Tanay, Brodwin, Mark, Connor, Thomas, Decker, Bandon, Devlin, Mark, Gonzalez, Anthony H., Lowe, Ian, Mason, Brian S., Sarazin, Craig, Stanford, Spencer A., Stern, Daniel, Thongkham, Khunanon, Wylezalek, Dominika, Zago, Fernando
Publikováno v:
2020 ApJ 902 2
The properties of galaxy clusters as a function of redshift can be utilized as an important cosmological tool. We present initial results from a program of follow-up observations of the Sunyaev-Zeldovich effect (SZE) in high redshift galaxy clusters
Externí odkaz:
http://arxiv.org/abs/2006.06703
Autor:
Okabe, Nobuhiro, Dicker, Simon, Eckert, Dominique, Mroczkowski, Tony, Gastaldello, Fabio, Lin, Yen-Ting, Devlin, Mark, Romero, Charles E., Birkinshaw, Mark, Sarazin, Craig, Horellou, Cathy, Kitayama, Tetsu, Umetsu, Keiichi, Sereno, Mauro, Mason, Brian S., ZuHone, John A., Honda, Ayaka, Akamatsu, Hiroki, Chiu, I-Non, Kohno, Kotaro, Lin, Kai-Yang, Medezinski, Elinor, Miyazaki, Satoshi, Mitsuishi, Ikuyuki, Nishizawa, Atsushi J., Oguri, Masamune, Ota, Naomi, Pacaud, Florian, Pierre, Marguerite, Sievers, Jonathan, Smolcic, Vernesa, Stanchfield, Sara, Tanaka, Keigo, Yamamoto, Ryoichi, Yang, Chong, Yoshida, Atsushi
We present results from simultaneous modeling of high angular resolution GBT/MUSTANG-2 90 GHz Sunyaev-Zel'dovich effect (SZE) measurements and XMM-XXL X-ray images of three rich galaxy clusters selected from the HSC-SSP Survey. The combination of hig
Externí odkaz:
http://arxiv.org/abs/1911.09236
Autor:
Romero, Charles E., Sievers, Jonathan, Ghirardini, Vittorio, Dicker, Simon, Giacintucci, Simona, Mroczkowski, Tony, Mason, Brian S., Sarazin, Craig, Devlin, Mark, Gaspari, Massimo, Battaglia, Nicholas, Hilton, Matthew, Bulbul, Esra, Lowe, Ian, Stanchfield, Sara
Publikováno v:
2020 ApJ, 891, 90
The galaxy cluster Zwicky 3146 is a sloshing cool core cluster at $z=0.291$ that in X-ray imaging does not appear to exhibit significant pressure substructure in the intracluster medium (ICM). The published $M_{500}$ values range between $3.88^{+0.62
Externí odkaz:
http://arxiv.org/abs/1908.09200
Akademický článek
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