Zobrazeno 41 - 50
of 564
pro vyhledávání: '"Holwerda, Benne"'
Autor:
Holwerda, Benne W., Bigiel, Frank, Bosma, Albert, Courtois, Helene M., Deg, Nathan, Dénes, Helga, Elagali, Ahmed, For, Bi-Qing, Koribalski, Baerbel, Leahy, Denis A., Lee-Waddell, Karen, López-Sánchez, Ángel R., Oh, Se-Heon, Reynolds, Tristan N., Rhee, Jonghwan, Spekkens, Kristine, Wang, Jing, Westmeier, Tobias, Wong, O. Ivy
Galaxy morphology in atomic hydrogen (HI) and in the ultra-violet (UV) are closely linked. This has motivated their combined use to quantify morphology over the full H i disk for both H i and UV imaging. We apply galaxy morphometrics: Concentration,
Externí odkaz:
http://arxiv.org/abs/2302.07963
Autor:
Shen, Lu, Papovich, Casey, Yang, Guang, Matharu, Jasleen, Wang, Xin, Magnelli, Benjamin, Elbaz, David, Jogee, Shardha, Alavi, Anahita, Haro, Pablo Arrabal, Backhaus, Bren E., Bagley, Micaela B., Bell, Eric F., Bisigello, Laura, Calabrò, Antonello, Cooper, M. C., Costantin, Luca, Daddi, Emanuele, Dickinson, Mark, Finkelstein, Steven L., Fujimoto, Seiji, Giavalisco, Mauro, Grogin, Norman A., Guo, Yuchen, Holwerda, Benne W., Kartaltepe, Jeyhan S., Koekemoer, Anton M., Kurczynski, Peter, Lucas, Ray A., Peŕez-Gonzaĺez, Pablo G., Pirzkal, Nor, Prichard, Laura, Rafelski, Marc, Ronayne, Kaila, Simons, Raymond C., Sunnquist, Ben, Teplitz, Harry I., Trump, Jonathan R., Weiner, Benjamin J., Windhorst, Rogier A., Yung, L. Y. Aaron
We present the mid-IR (MIR) morphologies for 64 star-forming galaxies at $0.210^{9}~M_\odot}$ using JWST MIRI observations from the Cosmic Evolution Early Release Science survey (CEERS). The MIRI bands span the MIR
Externí odkaz:
http://arxiv.org/abs/2301.05727
Autor:
Papovich, Casey, Cole, Justin, Yang, Guang, Finkelstein, Steven L., Barro, Guillermo, Buat, Véronique, Burgarella, Denis, Pérez-González, Pablo G., Santini, Paola, Seillé, Lise-Marie, Shen, Lu, Haro, Pablo Arrabal, Bagley, Micaela B., Bell, Eric F., Bisigello, Laura, Calabrò, Antonello, Casey, Caitlin M., Castellano, Marco, Chworowsky, Katherine, Cleri, Nikko J., Cooper, M. C., Costantin, Luca, Dickinson, Mark, Ferguson, Henry C., Fontana, Adriano, Giavalisco, Mauro, Grazian, Andrea, Grogin, Norman A., Hathi, Nimish P., Holwerda, Benne W., Hutchison, Taylor A., Kartaltepe, Jeyhan S., Kewley, Lisa J., Kirkpatrick, Allison, Kocevski, Dale D., Koekemoer, Anton M., Larson, Rebecca L., Long, Arianna S., Lucas, Ray A., Pentericci, Laura, Pirzkal, Nor, Ravindranath, Swara, Somerville, Rachel S., Trump, Jonathan R., Stawinski, Stephanie M. Urbano, Weiner, Benjamin J., Wilkins, Stephen M., Yung, L. Y. Aaron, Zavala, Jorge A.
We present results from the Cosmic Evolution Early Release Survey (CEERS) on the stellar-population parameters for 28 galaxies with redshifts $4
Externí odkaz:
http://arxiv.org/abs/2301.00027
Autor:
Jung, Intae, Finkelstein, Steven L., Larson, Rebecca L., Hutchison, Taylor A., Straughn, Amber N., Bagley, Micaela B., Castellano, Marco, Cleri, Nikko J., Cooper, M. C., Dickinson, Mark, Ferguson, Henry C., Holwerda, Benne W., Kartaltepe, Jeyhan S., Kim, Seonwoo, Koekemoer, Anton M., Papovich, Casey, Park, Hyunbae, Pentericci, Laura, Perez-Gonzalez, Pablo G., Song, Mimi, Tacchella, Sandro, Weiner, Benjamin J., Willmer, Christopher N. A., Zavala, Jorge A.
We perform a ground-based near-infrared spectroscopic survey using the Keck/MOSFIRE spectrograph to target Ly$\alpha$ emission at $7.0
Externí odkaz:
http://arxiv.org/abs/2212.09850
Autor:
Duncan, Kenneth J., Windhorst, Rogier A., Koekemoer, Anton M., Röttgering, Huub J. A., Cohen, Seth H., Jansen, Rolf A., Summers, Jake, Tompkins, Scott, Hutchison, Taylor A., Conselice, Christopher J., Driver, Simon P., Yan, Haojing, Adams, Nathan J., Cheng, Cheng, Coe, Dan, Diego, Jose M., Dole, Hervé, Frye, Brenda, Gim, Hansung B., Grogin, Norman A., Holwerda, Benne W., Lim, Jeremy, Marshall, Madeline A., Nonino, Mario, Pirzkal, Nor, Robotham, Aaron, Ryan, Jr., Russell E., Willmer, Christopher N. A.
We present the first JWST observations of the $z=4.11$ luminous radio galaxy TN J1338-1942, obtained as part of the ``Prime Extragalactic Areas for Reionization and Lensing Science'' (``PEARLS'') project. Our NIRCam observations, designed to probe th
Externí odkaz:
http://arxiv.org/abs/2212.09769
Autor:
Kim, Shin-Jeong, Oh, Se-Heon, Wang, Jing, Staveley-Smith, Lister, Koribalski, Bärbel S., Kim, Minsu, Park, Hye-Jin, Kim, Shinna, Spekkens, Kristine, Westmeier, Tobias, Wong, O. Ivy, Meurer, Gerhardt R., Kamphuis., Peter, Catinella, Barbara, McQuinn, Kristen B. W., Bigiel, Frank, Holwerda, Benne W., Rhee, Jonghwan, Lee-Waddell, Karen, Deg, Nathan, Verdes-Montenegro, Lourdes, For, Bi-Qing, Madrid, Juan P., Dénes, Helga, Elagali, Ahmed
We examine the HI gas kinematics of galaxy pairs in two clusters and a group using Australian Square Kilometre Array Pathfinder (ASKAP) WALLABY pilot survey observations. We compare the HI properties of galaxy pair candidates in the Hydra I and Norma
Externí odkaz:
http://arxiv.org/abs/2211.15123
Autor:
Martinez-Lombilla, Cristina, Brough, Sarah, Montes, Mireia, Baena-Galle, Roberto, Akhlaghi, Mohammad, Infante-Sainz, Raul, Driver, Simon P., Holwerda, Benne W., Pimbblet, Kevin A., Robotham, Aaron S. G.
We present a pilot study to assess the potential of Hyper Suprime-Cam Public Data Release 2 (HSC-PDR2) images for the analysis of extended faint structures within groups of galaxies. We examine the intra-group light (IGL) of the group 400138 ($M_{\rm
Externí odkaz:
http://arxiv.org/abs/2211.12749
Autor:
Larson, Rebecca L., Hutchison, Taylor A., Bagley, Micaela, Finkelstein, Steven L., Yung, L. Y. Aaron, Somerville, Rachel S., Hirschmann, Michaela, Brammer, Gabriel, Holwerda, Benne W., Papovich, Casey, Morales, Alexa M., Wilkins, Stephen M.
Publikováno v:
2023 ApJ 958 141
The selection of high-redshift galaxies often involves spectral energy distribution (SED) fitting to photometric data, an expectation for contamination levels, and measurement of sample completeness -- all vetted through comparison to spectroscopic r
Externí odkaz:
http://arxiv.org/abs/2211.10035
Autor:
Smith, Dominic, Haberzettl, Lutz, Porter, L. E., Porter-Temple, Ren, Henry, Christopher P. A., Holwerda, Benne, Lopez-Sanchez, A. R., Phillipps, Steven, Graham, Alister W., Brough, Sarah, Pimbblet, Kevin A., Liske, Jochen, Kelvin, Lee S., Robertson, Clayton D., Roemer, Wade, Walmsley, Michael, O'Ryan, David, Geron, Tobias
Galaxies broadly fall into two categories: star-forming (blue) galaxies and quiescent (red) galaxies. In between, one finds the less populated ``green valley". Some of these galaxies are suspected to be in the process of ceasing their star-formation
Externí odkaz:
http://arxiv.org/abs/2211.08355
Autor:
Finkelstein, Steven L., Bagley, Micaela B., Ferguson, Henry C., Wilkins, Stephen M., Kartaltepe, Jeyhan S., Papovich, Casey, Yung, L. Y. Aaron, Haro, Pablo Arrabal, Behroozi, Peter, Dickinson, Mark, Kocevski, Dale D., Koekemoer, Anton M., Larson, Rebecca L., Bail, Aurelien Le, Morales, Alexa M., Perez-Gonzalez, Pablo G., Burgarella, Denis, Dave, Romeel, Hirschmann, Michaela, Somerville, Rachel S., Wuyts, Stijn, Bromm, Volker, Casey, Caitlin M., Fontana, Adriano, Fujimoto, Seiji, Gardner, Jonathan P., Giavalisco, Mauro, Grazian, Andrea, Grogin, Norman A., Hathi, Nimish P., Hutchison, Taylor A., Jha, Saurabh W., Jogee, Shardha, Kewley, Lisa J., Kirkpatrick, Allison, Long, Arianna S., Lotz, Jennifer M., Pentericci, Laura, Pierel, Justin D. R., Pirzkal, Nor, Ravindranath, Swara, Ryan Jr, Russell E., Trump, Jonathan R., Yang, Guang, Bhatawdekar, Rachana, Bisigello, Laura, Buat, Veronique, Calabro, Antonello, Castellano, Marco, Cleri, Nikko J., Cooper, M. C., Croton, Darren, Daddi, Emanuele, Dekel, Avishai, Elbaz, David, Franco, Maximilien, Gawiser, Eric, Holwerda, Benne W., Huertas-Company, Marc, Jaskot, Anne E., Leung, Gene C. K., Lucas, Ray A., Mobasher, Bahram, Pandya, Viraj, Tacchella, Sandro, Weiner, Benjamin J., Zavala, Jorge A.
We present an investigation into the first 500 Myr of galaxy evolution from the Cosmic Evolution Early Release Science (CEERS) survey. CEERS, one of 13 JWST ERS programs, targets galaxy formation from z~0.5 to z>10 using several imaging and spectrosc
Externí odkaz:
http://arxiv.org/abs/2211.05792