Zobrazeno 1 - 10
of 2 496
pro vyhledávání: '"Yun, Min"'
Autor:
Long, Arianna S., Casey, Caitlin M., McKinney, Jed, Zavala, Jorge A., Akins, Hollis B., Cooper, Olivia R., Lambrides, Matthieu Bethermin Erini L., Franco, Maximilien, Caputi, Karina, Champagne, Jaclyn B., Man, Allison W. S., Treister, Ezequiel, Manning, Sinclaire M., Sanders, David B., Talia, Margherita, Aravena, Manuel, Clements, D. L., da Cunha, Elisabete, Faisst, Andreas L., Gentile, Fabrizio, Hodge, Jacqueline, Brammer, Gabriel, Brusa, Marcella, Finkelstein, Steven L., Fujimoto, Seiji, Hayward, Christopher C., Ilbert, Olivier, Jolly, Jean-Baptiste, Kartaltepe, Jeyhan S., Knudsen, Kirsten, Koekemoer, Anton M., Liu, Daizhong, Magdis, Georgios, McCracken, Henry Joy, Rhodes, Jason, Robertson, Brant E., Scoville, Nick, Sheth, Kartik, Smolcic, Vernesa, Spilker, Justin, Taniguchi, Yoshiaki, Toft, Sune, Urry, C. Megan, Yun, Min
One of the greatest challenges in galaxy evolution over the last decade has been constraining the prevalence of heavily dust-obscured galaxies in the early Universe. At $z>3$, these galaxies are increasingly rare, and difficult to identify as they ar
Externí odkaz:
http://arxiv.org/abs/2408.14546
Autor:
Tamura, Yoichi, Sakai, Takeshi, Kawabe, Ryohei, Kojima, Takafumi, Taniguchi, Akio, Takekoshi, Tatsuya, Kang, Haoran, Shan, Wenlei, Hagimoto, Masato, Okauchi, Norika, Tetsuka, Airi, Inoue, Akio K., Kohno, Kotaro, Tanaka, Kunihiko, Bakx, Tom J. L. C., Fudamoto, Yoshinobu, Fujita, Kazuyuki, Harikane, Yuichi, Hashimoto, Takuya, Hatsukade, Bunyo, Hughes, David H., Iino, Takahiro, Kimura, Yuki, Maezawa, Hiroyuki, Matsuda, Yuichi, Mawatari, Ken, Nakajima, Taku, Nakatsubo, Shunichi, Oshima, Tai, Sagawa, Hideo, Schloerb, F. Peter, Takahashi, Shigeru, Taniguchi, Kotomi, Tsujita, Akiyoshi, Umehata, Hideki, Yonetsu, Teppei, Yun, Min S.
Unveiling the emergence and prevalence of massive/bright galaxies during the epoch of reionization and beyond, within the first 600 million years of the Universe, stands as a pivotal pursuit in astronomy. Remarkable progress has been made by JWST in
Externí odkaz:
http://arxiv.org/abs/2406.07975
Autor:
Ortiz III, Rafael, Windhorst, Rogier A., Cohen, Seth H., Willner, S. P., Jansen, Rolf A., Carleton, Timothy, Kamieneski, Patrick S., Rutkowski, Michael J., Smith, Brent, Summers, Jake, McCabe, Tyler J., O'Brien, Rosalia, Diego, Jose M., Yun, Min S., D'Silva, Jordan C. J., Li, Juno, Gim, Hansung B., Hathi, Nimish P., Holwerda, Benne W., Zitrin, Adi, Cheng, Cheng, McLeod, Noah J., Conselice, Christopher J., Driver, Simon P., Yan, Haojing, Coe, Dan, Frye, Brenda, Grogin, Norman, Koekemoer, Anton, Marshall, Madeline A., Pirzkal, Nor, Robotham, Aaron, Ryan, Jr., Russell E., Willmer, Christopher N. A., Keel, William, Hammel, H. B., Hyun, M., Im, M., Milam, S. N.
The first public 0.9-4.4{\mu}m NIRCam images of the North Ecliptic Pole (NEP) Time Domain Field (TDF) uncovered galaxies displaying point-source features in their cores as seen in the longer wavelength filters. We visually identified a sample of 66 g
Externí odkaz:
http://arxiv.org/abs/2404.10709
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:
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:
Smail, Ian, Dudzeviciute, Ugne, Gurwell, Mark, Fazio, Giovanni G., Willner, S. P., Swinbank, A. M., Arumugam, Vinodiran, Summers, Jake, Cohen, Seth H., Jansen, Rolf A., Windhorst, Rogier A., Meena, Ashish, Zitrin, Adi, Keel, William C., Coe, Dan, Conselice, Christopher J., D'Silva, Jordan C. J., Driver, Simon P., Frye, Brenda, Grogin, Norman A., Koekemoer, Anton M., Marshall, Madeline A., Nonino, Mario, Pirzkal, Nor, Robotham, Aaron, Rutkowski, Michael J., Ryan Jr., Russell E., Tompkins, Scott, Willmer, Christopher N. A., Yan, Haojing, Broadhurst, Thomas J., Cheng, Cheng, Diego, Jose M., Kamieneski, Patrick, Yun, Min
We present a multi-wavelength analysis using SMA, JCMT, NOEMA, JWST, HST, and SST of two dusty strongly star-forming galaxies, 850.1 and 850.2, seen through the massive cluster lens A1489. These SMA-located sources both lie at z=4.26 and have bright
Externí odkaz:
http://arxiv.org/abs/2306.16039
Autor:
Pope, Alexandra, McKinney, Jed, Kamieneski, Patrick, Battisti, Andrew, Aretxaga, Itziar, Brammer, Gabriel, Diego, Jose M., Hughes, David H., Keller, Erica, Marchesini, Danilo, Mizener, Andrew, Montana, Alfredo, Murphy, Eric, Whitaker, Katherine E., Wilson, Grant, Yun, Min
We report ALMA detections of [CII] and dust continuum in Az9, a multiply-imaged galaxy behind the Frontier Field cluster MACSJ0717.5+3745. The bright [CII] emission line provides a spectroscopic redshift of z = 4.274. This strongly lensed (mu = 7 +/-
Externí odkaz:
http://arxiv.org/abs/2306.10450
Autor:
Pope, Alexandra, Montaña, Alfredo, Battisti, Andrew, Limousin, Marceau, Marchesini, Danilo, Wilson, Grant W., Alberts, Stacey, Aretxaga, Itziar, Avila-Reese, Vladimir, Bermejo-Climent, José Ramón, Brammer, Gabriel, Bravo-Alfaro, Hector, Calzetti, Daniela, Chary, Ranga-Ram, Cybulski, Ryan, Giavalisco, Mauro, Hughes, David, Kado-Fong, Erin, Keller, Erica, Kirkpatrick, Allison, Labbe, Ivo, Lange-Vagle, Daniel, Lowenthal, James, Murphy, Eric, Oesch, Pascal, Gonzalez, Daniel Rosa, Sánchez-Argüelles, David, Shipley, Heath, Stefanon, Mauro, Vega, Olga, Whitaker, Katherine, Williams, Christina C., Yun, Min, Zavala, Jorge A., Zeballos, Milagros
We directly detect dust emission in an optically detected, multiply imaged galaxy lensed by the Frontier Fields cluster MACSJ0717.5+3745. We detect two images of the same galaxy at 1.1 mm with the AzTEC camera on the Large Millimeter Telescope leavin
Externí odkaz:
http://hdl.handle.net/10150/623817
http://arizona.openrepository.com/arizona/handle/10150/623817
http://arizona.openrepository.com/arizona/handle/10150/623817
Autor:
McKinney, Jed, Manning, Sinclaire M., Cooper, Olivia R., Long, Arianna S., Akins, Hollis, Casey, Caitlin M., Faisst, Andreas L., Franco, Maximilien, Hayward, Christopher C., Lambrides, Erini, Magdis, Georgios, Whitaker, Katherine E., Yun, Min, Champagne, Jaclyn B., Drakos, Nicole E., Gentile, Fabrizio, Gillman, Steven, Gozaliasl, Ghassem, Ilbert, Olivier, Jin, Shuowen, Koekemoer, Anton M., Kokorev, Vasily, Liu, Daizhong, Rich, R. Michael, Robertson, Brant E., Valentino, Francesco, Weaver, John R., Zavala, Jorge A., Allen, Natalie, Kartaltepe, Jeyhan S., McCracken, Henry Joy, Paquereau, Louise, Rhodes, Jason, Shuntov, Marko, Toft, Sune
A growing number of far-infrared bright sources completely invisible in deep extragalactic optical surveys hint at an elusive population of z>4 dusty, star-forming galaxies. Cycle 1 JWST surveys are now detecting their rest-frame optical light, which
Externí odkaz:
http://arxiv.org/abs/2304.07316