Zobrazeno 1 - 10
of 79
pro vyhledávání: '"Pascale, Massimo"'
Autor:
Pascale, Massimo, Dai, Liang
We suggest that "Godzilla" of the lensed Sunburst galaxy ($z=2.37$) is a young super star cluster powering a nebula of gravitationally trapped stellar ejecta. Employing HST photometry and spectroscopy from VLT/MUSE and VLT/X-Shooter, we infer physica
Externí odkaz:
http://arxiv.org/abs/2404.10755
Autor:
Kamieneski, Patrick S., Frye, Brenda L., Windhorst, Rogier A., Harrington, Kevin C., Yun, Min S., Noble, Allison, Pascale, Massimo, Foo, Nicholas, Cohen, Seth H., Jansen, Rolf A., Carleton, Timothy, Koekemoer, Anton M., Willmer, Christopher N. A., Summers, Jake S., Garuda, Nikhil, Leimbach, Reagen, Holwerda, Benne W., Pierel, Justin D. R., Jimenez-Andrade, Eric F., Willner, S. P., Pampliega, Belen Alcalde, Vishwas, Amit, Keel, William C., Wang, Q. Daniel, Cheng, Cheng, Coe, Dan, Conselice, Christopher J., D'Silva, Jordan C. J., Driver, Simon P., Grogin, Norman A., Hinrichs, Tyler, Lowenthal, James D., Marshall, Madeline A., Nonino, Mario, Ortiz III, Rafael, Pigarelli, Alex, Pirzkal, Nor, Polletta, Maria del Carmen, Robotham, Aaron S. G., Ryan Jr., Russell E., Yan, Haojing
We present a new parametric lens model for the G165.7+67.0 galaxy cluster, which was discovered with $Planck$ through its bright submillimeter flux, originating from a pair of extraordinary dusty star-forming galaxies (DSFGs) at $z\approx 2.2$. Using
Externí odkaz:
http://arxiv.org/abs/2404.08058
Autor:
Chen, Wenlei, Kelly, Patrick L., Frye, Brenda L., Pierel, Justin, Willner, S. P., Pascale, Massimo, Cohen, Seth H., Conselice, Christopher J., Engesser, Michael, Furtak, Lukas J., Gilman, Daniel, Grogin, Norman A., Huber, Simon, Jha, Saurabh W., Johansson, Joel, Koekemoer, Anton M., Larison, Conor, Meena, Ashish K., Siebert, Matthew R., Windhorst, Rogier A., Yan, Haojing, Zitrin, Adi
SN H0pe is a triply imaged supernova (SN) at redshift $z=1.78$ discovered using the James Webb Space Telescope (JWST). In order to classify the SN spectroscopically and measure the relative time delays of its three images (designated A, B, and C), we
Externí odkaz:
http://arxiv.org/abs/2403.19029
SN H0pe: The First Measurement of $H_0$ from a Multiply-Imaged Type Ia Supernova, Discovered by JWST
Autor:
Pascale, Massimo, Frye, Brenda L., Pierel, Justin D. R., Chen, Wenlei, Kelly, Patrick L., Cohen, Seth H., Windhorst, Rogier A., Riess, Adam G., Kamieneski, Patrick S., Diego, Jose M., Meena, Ashish K., Cha, Sangjun, Oguri, Masamune, Zitrin, Adi, Jee, M. James, Foo, Nicholas, Leimbach, Reagen, Koekemoer, Anton M., Conselice, C. J., Dai, Liang, Goobar, Ariel, Siebert, Matthew R., Strolger, Lou, Willner, S. P.
The first James Webb Space Telescope ({\it JWST}) Near InfraRed Camera (NIRCam) imaging in the field of the galaxy cluster PLCK G165.7+67.0 ($z=0.35$) uncovered a Type Ia supernova (SN~Ia) at $z=1.78$, called ``SN H0pe." Three different images of thi
Externí odkaz:
http://arxiv.org/abs/2403.18902
Autor:
Wang, Q. Daniel, Diaz, Carlos Garcia, Kamieneski, Patrick S., Harrington, Kevin C., Yun, Min S., Foo, Nicholas, Frye, Brenda L., Jimenez-Andrade, Eric F., Liu, Daizhong, Lowenthal, James D., Pampliega, Belen Alcalde, Pascale, Massimo, Vishwas, Amit, Gurwell, Mark A.
Hyper-luminous infrared galaxies (HyLIRGs) are the most extreme star-forming systems observed in the early Universe, and their properties still elude comprehensive understanding. We have undertaken a large XMM-Newton observing program to probe the to
Externí odkaz:
http://arxiv.org/abs/2312.05442
Autor:
Frye, Brenda L., Pascale, Massimo, Pierel, Justin, Chen, Wenlei, Foo, Nicholas, Leimbach, Reagen, Garuda, Nikhil, Cohen, Seth, Kamieneski, Patrick, Windhorst, Rogier, Koekemoer, Anton M., Kelly, Pat, Summers, Jake, Engesser, Michael, Liu, Daizhong, Furtak, Lukas, Polletta, Maria, Harrington, Kevin, Willner, Steve, Diego, Jose M., Jansen, Rolf, Coe, Dan, Conselice, Christopher J., Dai, Liang, Dole, Herve, D'Silva, Jordan C. J., Driver, Simon, Grogin, Norman, Marshall, Madeline A., Meena, Ashish, Nonino, Mario, Ortiz III, Rafael, Pirzkal, Nor, Robotham, Aaron, Ryan, Russell E., Strolger, Lou, Tompkins, Scott, Trussler, James, Willmer, Christopher, Yan, Haojing, Yun, Min S., Zitrin, Adi
A Type Ia supernova (SN) at $z=1.78$ was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; $z = 0.35$). The SN is situated 1.5-2 kpc from the host-galaxy nucleus and appears in three d
Externí odkaz:
http://arxiv.org/abs/2309.07326
Autor:
Diego, Jose M., Li, Sung Kei, Meena, Ashish K., Niemiec, Anna, Acebron, Ana, Jauzac, Mathilde, Struble, Mitchell F., Amruth, Alfred, Broadhurst, Tom J., Cerny, Catherine, Ebeling, Harald, Filippenko, Alexei V., Jullo, Eric, Kelly, Patrick, Koekemoer, Anton M., Lagatutta, David, Lim, Jeremy, Limousin, Marceau, Mahler, Guillaume, Patel, Nency, Remolina, Juan, Richard, Johan, Sharon, Keren, Steinhardt, Charles, Umetsu, Keichii, Williams, Liliya, Zitrin, Adi, Palencia, J. M., Ji, Liang Dai. Lingyuan, Pascale, Massimo
We present a constraint on the abundance of supergiant (SG) stars at redshift z approx. 1, based on recent observations of a strongly lensed arc at this redshift. First we derive a free-form model of MACS J0416.1-2403 using data from the BUFFALO prog
Externí odkaz:
http://arxiv.org/abs/2304.09222
Autor:
Kamieneski, Patrick S., Frye, Brenda L., Pascale, Massimo, Cohen, Seth H., Windhorst, Rogier A., Jansen, Rolf A., Yun, Min S., Cheng, Cheng, Summers, Jake S., Carleton, Timothy, Harrington, Kevin C., Diego, Jose M., Yan, Haojing, Koekemoer, Anton M., Willmer, Christopher N. A., Petric, Andreea, Furtak, Lukas J., Foo, Nicholas, Conselice, Christopher J., Coe, Dan, Driver, Simon P., Grogin, Norman A., Marshall, Madeline A., Pirzkal, Nor, Robotham, Aaron S. G., Ryan Jr., Russell E., Tompkins, Scott
Gradients in the mass-to-light ratio of distant galaxies impede our ability to characterize their size and compactness. The long-wavelength filters of $JWST$'s NIRCam offer a significant step forward. For galaxies at Cosmic Noon ($z\sim2$), this regi
Externí odkaz:
http://arxiv.org/abs/2303.05054
Autor:
Frye, Brenda L., Pascale, Massimo, Foo, Nicholas, Leimbach, Reagen, Garuda, Nikhil, Robles, Paulina Soto, Summers, Jake, Diaz, Carlos, Kamieneski, Patrick, Furtak, Lukas, Cohen, Seth, Diego, Jose, Beauchesne, Benjamin, Windhorst, Rogier, Willner, Steve, Koekemoer, Anton M., Zitrin, Adi, Caminha, Gabriel, Caputi, Karina, Coe, Dan, Conselice, Christopher J., Dai, Liang, Dole, Herve, Driver, Simon, Grogin, Norman, Harrington, Kevin, Jansen, Rolf A., Kneib, Jean-Paul, Lehnert, Matt, Lowenthal, James, Marshall, Madeline A., Menanteau, Felipe, Pampleiga, Belen Alcalde, Pirzkal, Nor, Polletta, Mari, Richard, Johan, Robotham, Aaron, Ryan, Russell E., Rutkowski, Michael J., Sifon, Christobal, Tompkins, Scott, Wang, Daniel, Yan, Haojing, Yun, Min S.
The massive galaxy cluster El Gordo (z=0.87) imprints multitudes of gravitationally lensed arcs onto James Webb Space Telescope (JWST) Near-Infrared Camera (NIRCam) images. Eight bands of NIRCam imaging were obtained in the ``Prime Extragalactic Area
Externí odkaz:
http://arxiv.org/abs/2303.03556
Nitrogen-enriched, highly-pressurized nebular clouds surrounding a super star cluster at cosmic noon
Publikováno v:
ApJ 957 77 (2023)
Strong lensing offers a precious opportunity for studying the formation and early evolution of super star clusters that are rare in our cosmic backyard. The Sunburst Arc, a lensed Cosmic Noon galaxy, hosts a young super star cluster with escaping Lym
Externí odkaz:
http://arxiv.org/abs/2301.10790