Zobrazeno 1 - 10
of 639
pro vyhledávání: '"Grogin, Norman A"'
Autor:
Barro, Guillermo, Perez-Gonzalez, Pablo G., Kocevski, Dale D., McGrath, Elizabeth J., Leung, Gene C. K., Cullen, Fergus, Dunlop, James S., Ellis, Richard S., Finkelstein, Steven L., Grogin, Norman A., Illingworth, Garth, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Lucas, Ray A., McLure, Ross J., Yang, Guang
JWST has revealed a population of compact `Little Red Dots' (LRDs) at $z\gtrsim4$, with red rest-frame optical and blue UV colors. These objects are likely compact dusty starbursts or heavily reddened AGNs, playing a pivotal role in early black hole
Externí odkaz:
http://arxiv.org/abs/2412.01887
Autor:
Leung, Gene C. K., Finkelstein, Steven L., Pérez-González, Pablo G., Morales, Alexa M., Taylor, Anthony J., Barro, Guillermo, Kocevski, Dale D., Akins, Hollis B., Carnall, Adam C., Ortiz, Óscar A. Chávez, Cleri, Nikko J., Cullen, Fergus, Donnan, Callum T., Dunlop, James S., Ellis, Richard S., Grogin, Norman A., Hirschmann, Michaela, Koekemoer, Anton M., Kokorev, Vasily, Lucas, Ray A., McLeod, Derek J., Papovich, Casey, Yung, L. Y. Aaron
JWST has revealed a large population of compact, red galaxies at $z>4$ known as Little Red Dots (LRDs). We analyze the spectral energy distributions (SEDs) of 95 LRDs from the JWST PRIMER survey with complete photometric coverage from $1-18\ \mu$m us
Externí odkaz:
http://arxiv.org/abs/2411.12005
Autor:
Duan, Qiao, Li, Qiong, Conselice, Christopher J., Harvey, Thomas, Austin, Duncan, Adams, Nathan J., Ferreira, Leonardo, Duncan, Kenneth J., Trussler, James, Pascalau, Robert G., Windhorst, Rogier A., Holwerda, Benne W., Broadhurst, Thomas J., Coe, Dan, Cohen, Seth H., Du, Xiaojing, Driver, Simon P., Frye, Brenda, Grogin, Norman A., Hathi, Nimish P., Jansen, Rolf A., Koekemoer, Anton M., Marshall, Madeline A., Nonino, Mario, Ortiz III, Rafael, Pirzkal, Nor, Robotham, Aaron, Ryan Jr, Russell E., Summers, Jake, D'Silva, Jordan C. J., Willmer, Christopher N. A., Yan, Haojing
Galaxy mergers are a key driver of galaxy formation and evolution, including the triggering of AGN and star formation to a still unknown degree. We thus investigate the impact of galaxy mergers on star formation and AGN activity using a sample of 3,3
Externí odkaz:
http://arxiv.org/abs/2411.04944
Autor:
Burgarella, Denis, Buat, Véronique, Theulé, Patrice, Zavala, Jorge, Haro, Pablo Arrabal, Bagley, Micaela B., Boquien, Médéric, Cleri, Nikko, Dewachter, Tim, Dickinson, Mark, Ferguson, Henry C., Fernández, Vital, Finkelstein, Steven L., Fontana, Adriano, Gawiser, Eric, Grazian, Andrea, Grogin, Norman, Holwerda, Benne W., Kartaltepe, Jeyhan S., Kewley, Lisa, Kirkpatrick, Allison, Kocevski, Dale, Koekemoer, Anton M., Long, Arianna, Lotz, Jennifer, Lucas, Ray A., Mobasher, Bahram, Papovich, Casey, Pérez-González, Pablo G., Pirzkal, Nor, Ravindranath, Swara, Rodighiero, Giulia, Roehlly, Yannick, Rose, Caitlin, Seillé, Lise-Marie, Somerville, Rachel, Wilkins, Steve, Yang, Guang, Yung, L. Y. Aaron
We investigate the coevolution of metals and dust for 173 galaxies at 4.0
Externí odkaz:
http://arxiv.org/abs/2410.23959
Autor:
Shen, Lu, Papovich, Casey, Matharu, Jasleen, Pirzkal, Nor, Hu, Weida, Berg, Danielle A., Bagley, Micaela B., Backhaus, Bren E., Cleri, Nikko J., Dickinson, Mark, Finkelstein, Steven L., Hathi, Nimish P., Huertas-Company, Marc, Hutchison, Taylor A., Giavalisco, Mauro, Grogin, Norman A., Jaskot, Anne E., Jung, Intae, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Lotz, Jennifer M., Pérez-González, Pablo G., Rothberg, Barry, Simons, Raymond C., Vanderhoof, Brittany N., Yung, L. Y. Aaron
We use JWST/NIRISS slitless spectroscopy from the Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey to investigate the physical condition of star-forming galaxies at $1.7 < z < 3.4$. At these redshifts, the deep NGDEEP NIRISS slit
Externí odkaz:
http://arxiv.org/abs/2410.23349
Autor:
Mehta, Vihang, Rafelski, Marc, Sunnquist, Ben, Teplitz, Harry I., Scarlata, Claudia, Wang, Xin, Fontana, Adriano, Hathi, Nimish P., Iyer, Kartheik G., Alavi, Anahita, Colbert, James, Grogin, Norman, Koekemoer, Anton, Nedkova, Kalina V., Hayes, Matthew, Prichard, Laura, Siana, Brian, Smith, Brent M., Windhorst, Rogier, Ashcraft, Teresa, Bagley, Micaela, Baronchelli, Ivano, Barro, Guillermo, Blanche, Alex, Broussard, Adam, Carleton, Timothy, Chartab, Nima, Codoreanu, Alex, Cohen, Seth, Conselice, Christopher, Dai, Y. Sophia, Darvish, Behnam, Dave, Romeel, DeGroot, Laura, De Mello, Duilia, Dickinson, Mark, Emami, Najmeh, Ferguson, Henry, Ferreira, Leonardo, Finkelstein, Keely, Finkelstein, Steven, Gardner, Jonathan P., Gawiser, Eric, Gburek, Timothy, Giavalisco, Mauro, Grazian, Andrea, Gronwall, Caryl, Guo, Yicheng, Haro, Pablo Arrabal, Hemmati, Shoubaneh, Howell, Justin, Jansen, Rolf A., Ji, Zhiyuan, Kaviraj, Sugata, Kim, Keunho J., Kurczynski, Peter, Lazar, Ilin, Lucas, Ray A., MacKenty, John, Mantha, Kameswara Bharadwaj, Martin, Alec, Martin, Garreth, McCabe, Tyler, Mobasher, Bahram, Morales, Alexa M., O'Connell, Robert, Olsen, Charlotte, Otteson, Lillian, Ravindranath, Swara, Redshaw, Caleb, Rutkowski, Michael, Robertson, Brant, Sattari, Zahra, Soto, Emmaris, Sun, Lei, Taamoli, Sina, Vanzella, Eros, Yung, L. Y. Aaron, Zabelle, Bonnabelle
The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) program provides deep HST F275W and F435W imaging over four CANDELS fields (GOODS-N, GOODS-S, COSMOS, and EGS). We combine this newly acq
Externí odkaz:
http://arxiv.org/abs/2410.16404
Autor:
Gupta, Ansh R., Kirkpatrick, Allison, Fernandez, Vital, Haro, Pablo Arrabal, Backhaus, Bren E., Cleri, Nikko J., Grogin, Norman A., Koekemoer, Anton M.
Galaxy emission-line fluxes can be analyzed to determine star formation rates (SFR) and ISM ionization. Here, we investigate rest-frame optical emission lines of 71 star-forming galaxies at redshift 0.7 < z < 7 from the Cosmic Evolution Early Release
Externí odkaz:
http://arxiv.org/abs/2410.03784
Autor:
Rose, Caitlin, Kartaltepe, Jeyhan S., Snyder, Gregory F., Huertas-Company, Marc, Yung, L. Y. Aaron, Haro, Pablo Arrabal, Bagley, Micaela B., Bisigello, Laura, Calabrò, Antonello, Cleri, Nikko J., Dickinson, Mark, Ferguson, Henry C., Finkelstein, Steven L., Fontana, Adriano, Grazian, Andrea, Grogin, Norman A., Holwerda, Benne W., Iyer, Kartheik G., Kewley, Lisa J., Kirkpatrick, Allison, Kocevski, Dale D., Koekemoer, Anton M., Lotz, Jennifer M., Lucas, Ray A., Napolitan, Lorenzo, Papovich, Casey, Pentericci, Laura, Pérez-González, Pablo G., Pirzkal, Nor, Ravindranath, Swara, Somerville, Rachel S., Straughn, Amber N., Trump, Jonathan R., Wilkins, Stephen M., Yang, Guang
A crucial yet challenging task in galaxy evolution studies is the identification of distant merging galaxies, a task which suffers from a variety of issues ranging from telescope sensitivities and limitations to the inherently chaotic morphologies of
Externí odkaz:
http://arxiv.org/abs/2407.21279
Autor:
Pandya, Viraj, Loeb, Abraham, McGrath, Elizabeth J., Barro, Guillermo, Finkelstein, Steven L., Ferguson, Henry C., Grogin, Norman A., Kartaltepe, Jeyhan S., Koekemoer, Anton M., Papovich, Casey, Pirzkal, Nor, Yung, L. Y. Aaron
The majority of low-mass ($\log_{10} M_*/M_{\odot}=9-10$) galaxies at high redshift ($z>1$) appear elongated in projection. We use JWST-CEERS observations to explore the role of gravitational lensing in this puzzle. The typical galaxy-galaxy lensing
Externí odkaz:
http://arxiv.org/abs/2407.17552
Autor:
Conselice, Christopher J., Adams, Nathan, Harvey, Thomas, Austin, Duncan, Ferreira, Leonardo, Ormerod, Katherine, Duan, Qiao, Trussler, James, Li, Qiong, Juodzbalis, Ignas, Westcott, Lewi, Harris, Honor, Seeyave, Louise T. C., Bluck, Asa F. L., Windhorst, Rogier A., Bhatawdekar, Rachana, Coe, Dan, Cohen, Seth H., Cheng, Cheng, Driver, Simon P., Frye, Brenda, Furtak, Lukas J., Grogin, Norman A., Hathi, Nimish P., Holwerda, Benne W., Jansen, Rolf A., Koekemoer, Anton M., Marshall, Madeline A., Nonino, Mario, Robotham, Aaron, Summers, Jake, Wilkins, Stephen M., Willmer, Christopher N. A., Yan, Haojing, Zitrin, Adi
We present in this paper the discovery, properties, and a catalog of 1165 high redshift $6.5 < z < 18$ galaxies found in deep JWST NIRCam imaging from the GTO PEARLS survey combined with data from JWST public fields. We describe our bespoke homogeneo
Externí odkaz:
http://arxiv.org/abs/2407.14973