Zobrazeno 1 - 10
of 58
pro vyhledávání: '"Canning, Rebecca E. A."'
Autor:
Khederlarian, Ashod, Newman, Jeffrey A., Andrews, Brett H., Dey, Biprateep, Moustakas, John, Hearin, Andrew, Juneau, Stéphanie, Tortorelli, Luca, Gruen, Daniel, Hahn, ChangHoon, Canning, Rebecca E. A., Aguilar, Jessica Nicole, Ahlen, Steven, Brooks, David, Claybaugh, Todd, de la Macorra, Axel, Doel, Peter, Fanning, Kevin, Ferraro, Simone, Forero-Romero, Jaime, Gaztañaga, Enrique, Gontcho, Satya Gontcho A, Kehoe, Robert, Kisner, Theodore, Kremin, Anthony, Lambert, Andrew, Landriau, Martin, Manera, Marc, Meisner, Aaron, Miquel, Ramon, Mueller, Eva-Maria, Muñoz-Gutiérrez, Andrea, Myers, Adam, Nie, Jundan, Poppett, Claire, Prada, Francisco, Rezaie, Mehdi, Rossi, Graziano, Sanchez, Eusebio, Schubnell, Michael, Silber, Joseph Harry, Sprayberry, David, Tarlé, Gregory, Weaver, Benjamin Alan, Zhou, Zhimin, Zou, Hu
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 531, Issue 1, June 2024, Pages 1454 - 1470
We present a simple, differentiable method for predicting emission line strengths from rest-frame optical continua using an empirically-determined mapping. Extensive work has been done to develop mock galaxy catalogues that include robust predictions
Externí odkaz:
http://arxiv.org/abs/2404.03055
Autor:
Chapman, Scott C., Hill, Ryley, Aravena, Manuel, Archipley, Melanie, Babul, Arif, Burgoyne, James, Canning, Rebecca E. A., De Breuck, Carlos, Gonzalez, Anthony H., Hayward, Christopher C., Kim, Seon Woo, Malkan, Matt, Marrone, Dan P., McIntyre, Vincent, Murphy, Eric, Pass, Emily, Perry, Ryan W., Phadke, Kedar A., Rennehan, Douglas, Reuter, Cassie, Rotermund, Kaja M., Scott, Douglas, Seymour, Nick, Solimano, Manuel, Spilker, Justin, Stark, Anthony A., Sulzenauer, Nikolaus, Tothill, Nick, Vieira, Joaquin D., Vizgan, David, Wang, George, Weiss, Axel
We have observed the z=4.3 protocluster SPT2349-56 with ATCA with the aim of detecting radio-loud active galactic nuclei (AGN) amongst the ~30 submillimeter galaxies identified in the structure. We detect the central complex of SMGs at 2.2\,GHz with
Externí odkaz:
http://arxiv.org/abs/2301.01375
Autor:
Hahn, ChangHoon, Kwon, K. J., Tojeiro, Rita, Siudek, Malgorzata, Canning, Rebecca E. A., Mezcua, Mar, Tinker, Jeremy L., Brooks, David, Doel, Peter, Fanning, Kevin, Gaztañaga, Enrique, Kehoe, Robert, Landriau, Martin, Meisner, Aaron, Moustakas, John, Poppett, Claire, Tarle, Gregory, Weiner, Benjamin, Zou, Hu
The PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) catalog will provide measurements of galaxy properties, such as stellar mass ($M_*$), star formation rate (${\rm SFR}$), stellar metallicity ($Z_{\rm MW}$), and stellar age ($t_{\rm age, M
Externí odkaz:
http://arxiv.org/abs/2202.01809
Autor:
Mantz, Adam B., Allen, Steven W., Canning, Rebecca E. A., Baumont, Lucie, Benson, Bradford, Bleem, Lindsey E., Ehlert, Steven R., Floyd, Benjamin, Herbonnet, Ricardo, Kelly, Patrick L., Liang, Shuang, von der Linden, Anja, McDonald, Michael, Rapetti, David A., Schmidt, Robert W., Werner, Norbert, Wright, Adam
We present updated cosmological constraints from measurements of the gas mass fractions ($f_{gas}$) of massive, dynamically relaxed galaxy clusters. Our new data set has greater leverage on models of dark energy, thanks to the addition of the Perseus
Externí odkaz:
http://arxiv.org/abs/2111.09343
Autor:
Grossová, Romana, Werner, Norbert, Massaro, Francesco, Lakhchaura, Kiran, Plšek, Tomáš, Gabányi, Krizstina, Rajpurohit, Kamlesh, Canning, Rebecca E. A., Nulsen, Paul, O'Sullivan, Ewan, Allen, Steven W., Fabian, Andrew
Many massive early-type galaxies host central radio sources and hot X-ray atmospheres indicating the presence of radio-mechanical active galactic nucleus (AGN) feedback. The duty cycle and detailed physics of the radio-mode AGN feedback is still a ma
Externí odkaz:
http://arxiv.org/abs/2111.02430
Autor:
Hill, Ryley, Chapman, Scott, Phadke, Kedar A., Aravena, Manuel, Archipley, Melanie, Ashby, Matthew L. N., Bethermin, Matthieu, Canning, Rebecca E. A., Gonzalez, Anthony, Greve, Thomas R., Gururajan, Gayathri, Hayward, Christopher C., Hezaveh, Yashar, Jarugula, Sreevani, MacIntyre, Duncan, Marrone, Daniel P., Miller, Tim, Rennehan, Douglas, Reuter, Cassie, Rotermund, Kaja, Scott, Douglas, Spilker, Justin, Vieira, Joaquin D., Wang, George, Weiss, Axel
Publikováno v:
MNRAS 512(3), 4352, 2022
The protocluster SPT2349$-$56 at $z\,{=}\,4.3$ contains one of the most actively star-forming cores known, yet constraints on the total stellar mass of this system are highly uncertain. We have therefore carried out deep optical and infrared observat
Externí odkaz:
http://arxiv.org/abs/2109.04534
Autor:
Flores, Anthony M., Mantz, Adam B., Allen, Steven W., Morris, R. Glenn, Canning, Rebecca E. A., Bleem, Lindsey E., Calzadilla, Michael S., Floyd, Benjamin T., McDonald, Michael, Ruppin, Florian
We present the analysis of deep X-ray observations of 10 massive galaxy clusters at redshifts $1.05 < z < 1.71$, with the primary goal of measuring the metallicity of the intracluster medium (ICM) at intermediate radii, to better constrain models of
Externí odkaz:
http://arxiv.org/abs/2108.12051
Autor:
Mantz, Adam B., Allen, Steven W., Morris, R. Glenn, Canning, Rebecca E. A., Bayliss, Matthew, Bleem, Lindsey E., Floyd, Benjamin T., McDonald, Michael
Publikováno v:
Mon. Not. Roy. Astron. Soc. 496:1554-1564,2020
We present results from a 577 ks XMM-Newton observation of SPT-CL J0459-4947, the most distant cluster detected in the South Pole Telescope 2500 square degree (SPT-SZ) survey, and currently the most distant cluster discovered through its Sunyaev-Zel'
Externí odkaz:
http://arxiv.org/abs/2006.02009
Ultra-diffuse galaxies (UDGs) exhibit low surface brightness, but their optical extent is comparable to Milky Way-type galaxies. Due to their peculiar properties, it remains ambiguous whether UDGs are the descendants of massive galaxies or they are p
Externí odkaz:
http://arxiv.org/abs/2004.11388
Autor:
Hill, Ryley, Chapman, Scott, Scott, Douglas, Apostolovski, Yordanka, Aravena, Manuel, Bethermin, Matthieu, Bradford, C. M., de Breuck, Carlos, Canning, Rebecca E. A., Dong, Chenxing, Gonzalez, Anthony, Greve, Thomas R., Hayward, Christopher C., Hezaveh, Yashar, Litke, Katrina, Malkan, Matt, Marrone, Daniel P., Phadke, Kedar, Reuter, Cassie, Rotermund, Kaja, Spilker, Justin, Vieira, Joaquin D., Weiss, Axel
Publikováno v:
MNRAS, 495, 3124 (2020)
We present an extensive ALMA spectroscopic follow-up programme of the $z\,{=}\,4.3$ structure SPT2349$-$56, one of the most actively star-forming proto-cluster cores known, to identify additional members using their [C{\sc ii}] 158\,$\mu$m and \mbox{
Externí odkaz:
http://arxiv.org/abs/2002.11600