Zobrazeno 1 - 10
of 176
pro vyhledávání: '"Simons, Raymond"'
Autor:
Acharyya, Ayan, Peeples, Molly S., Tumlinson, Jason, Shea, Brian W. O, Lochhaas, Cassandra, Wright, Anna C., Simons, Raymond C., Augustin, Ramona, Smith, Britton D., Lee, Eugene Hyeonmin
Gas-phase metallicity gradients are a crucial element in understanding the chemical evolution of galaxies. We use the FOGGIE simulations to study the metallicity gradients ($\nabla Z$) of six Milky Way-like galaxies throughout their evolution. FOGGIE
Externí odkaz:
http://arxiv.org/abs/2404.06613
Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES
Autor:
Zheng, Yong, Tchernyshyov, Kirill, Olsen, Knut, Choi, Yumi, Bustard, Chad, Roman-Duval, Julia, Zhu, Robert, Di Teodoro, Enrico M., Werk, Jessica, Putman, Mary, McLeod, Anna F., Faerman, Yakov, Simons, Raymond C., Peek, Joshua
The Large Magellanic Cloud (LMC) is home to many HII regions, which may lead to significant outflows. We examine the LMC's multiphase gas ($T\sim10^{4-5}$ K) in HI, SII, SiIV, and CIV using 110 stellar sight lines from the HST's Ultraviolet Legacy Li
Externí odkaz:
http://arxiv.org/abs/2402.04313
Autor:
Cheng, Yingjie, Giavalisco, Mauro, Simons, Raymond C., Ji, Zhiyuan, Stroupe, Darren, Cleri, Nikko J.
Publikováno v:
The Astrophysical Journal, 2024, Volume 964, Issue 1, id.94, 17 pp
We explore the relationships between the [O/H] gas-phase metallicity radial gradients and multiple galaxy properties for 238 star-forming galaxies at 0.6
Externí odkaz:
http://arxiv.org/abs/2401.12319
Autor:
Pirzkal, Nor, Rothberg, Barry, Papovich, Casey, Shen, Lu, Leung, Gene C. K., Bagley, Micaela B., Finkelstein, Steven L., Vanderhoof, Brittany N., Lotz, Jennifer M., Koekemoer, Anton M., Hathi, Nimish P., Cheng, Yingjie, Cleri, Nikko J., Grogin, Norman A., Yung, L. Y. Aaron, Dickinson, Mark, Ferguson, Henry C., Gardner, Jonathan P., Jung, Intae, Kartaltepe, Jeyhan S., Ryan, Russell, Simons, Raymond C., Ravindranath, Swara, Berg, Danielle A., Backhaus, Bren E., Casey, Caitlin M., Castellano, Marco, Ortiz, Óscar A. Chávez, Chworowsky, Katherine, Cox, Isabella G., Davé, Romeel, Davis, Kelcey, Estrada-Carpenter, Vicente, Fontana, Adriano, Fujimoto, Seiji, Giavalisco, Mauro, Grazian, Andrea, Hutchison, Taylor A., Jaskot, Anne E., Kewley, Lisa J., Kirkpatrick, Allison, Kocevski, Dale D., Larson, Rebecca L., Matharu, Jasleen, Natarajan, Priyamvada, Pentericci, Laura, Pérez-González, Pablo G., Snyder, Gregory F., Somerville, Rachel S., Trump, Jonathan R., Wilkins, Stephen M.
The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) survey program was designed specifically to include Near Infrared Slitless Spectroscopic observations (NGDEEP-NISS) to detect multiple emission lines in as many galaxies as possible a
Externí odkaz:
http://arxiv.org/abs/2312.09972
Autor:
Davis, Kelcey, Trump, Jonathan R., Simons, Raymond C., Mcgrath, Elizabeth J., Wilkins, Stephen M., Haro, Pablo Arrabal, Bagley, Micaela B., Dickinson, Mark, FernÁndez, Vital, AmorÍn, Ricardo O., Backhaus, Bren E., Cleri, Nikko J., Llerena, Mario, Brunker, Samantha W., Barro, Guillermo, Bisigello, Laura, Brooks, Madisyn, Costantin, Luca, De La Vega, Alexander, Dekel, Avishai, Finkelstein, Steven L., Hathi, Nimish P., Hirschmann, Michaela, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Lucas, Ray A., Papovich, Casey, PÉrez-GonzÁlez, Pablo G., Pirzkal, Nor, Rodighiero, Giulia, Rose, Caitlin, Yung, L. Y. Aaron
We present a sample of 1165 extreme emission-line galaxies (EELGs) at 4
Externí odkaz:
http://arxiv.org/abs/2312.07799
Autor:
Pandya, Viraj, Zhang, Haowen, Huertas-Company, Marc, Iyer, Kartheik G., McGrath, Elizabeth, Barro, Guillermo, Finkelstein, Steven L., Kuemmel, Martin, Hartley, William G., Ferguson, Henry C., Kartaltepe, Jeyhan S., Primack, Joel, Dekel, Avishai, Faber, Sandra M., Koo, David C., Bryan, Greg L., Somerville, Rachel S., Amorin, Ricardo O., Haro, Pablo Arrabal, Bagley, Micaela B., Bell, Eric F., Bertin, Emmanuel, Costantin, Luca, Dave, Romeel, Dickinson, Mark, Feldmann, Robert, Fontana, Adriano, Gavazzi, Raphael, Giavalisco, Mauro, Grazian, Andrea, Grogin, Norman A., Guo, Yuchen, Hahn, ChangHoon, Holwerda, Benne W., Kewley, Lisa J., Kirkpatrick, Allison, Koekemoer, Anton M., Lotz, Jennifer M., Lucas, Ray A., Pentericci, Laura, Perez-Gonzalez, Pablo G., Pirzkal, Nor, Kocevski, Dale D., Papovich, Casey, Ravindranath, Swara, Rose, Caitlin, Schefer, Marc, Simons, Raymond C., Straughn, Amber N., Tacchella, Sandro, Trump, Jonathan R., de la Vega, Alexander, Wilkins, Stephen M., Wuyts, Stijn, Yang, Guang, Yung, L. Y. Aaron
The 3D geometry of high-redshift galaxies remains poorly understood. We build a differentiable Bayesian model and use Hamiltonian Monte Carlo to efficiently and robustly infer the 3D shapes of star-forming galaxies in JWST-CEERS observations with $\l
Externí odkaz:
http://arxiv.org/abs/2310.15232
Autor:
Shen, Lu, Papovich, Casey, Matharu, Jasleen, Pirzkal, Nor, Hu, Weida, Backhaus, Bren E., Bagley, Micaela B., Cheng, Yingjie, Cleri, Nikko J., Finkelstein, Steven L., Huertas-Company, Marc, Giavalisco, Mauro, Grogin, Norman A., Jung, Intae, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Lotz, Jennifer M., Maseda, Michael V., Pérez-González, Pablo G., Rothberg, Barry, Simons, Raymond C., Tacchella, Sandro, Williams, Christina C., Yung, L. Y. Aaron
We study the H$\alpha$ equivalent width, EW(H$\alpha$), maps of 19 galaxies at $0.6 < z < 2.2$ in the Hubble Ultra Deep Field (HUDF) derived from NIRISS slitless spectroscopy as part of the Next Generation Deep Extragalactic Exploratory Public (NGDEE
Externí odkaz:
http://arxiv.org/abs/2310.13745
Autor:
Wright, Anna C., Tumlinson, Jason, Peeples, Molly S., O'Shea, Brian W., Lochhaas, Cassandra, Corlies, Lauren, Smith, Britton D., Binh, Nguyen, Augustin, Ramona, Simons, Raymond C.
Over the next decade, the astronomical community will be commissioning multiple wide-field observatories well-suited for studying stellar halos in both integrated light and resolved stars. In preparation for this, we use five high-resolution cosmolog
Externí odkaz:
http://arxiv.org/abs/2309.10039
Autor:
Backhaus, Bren E., Trump, Jonathan R., Pirzkal, Nor, Barro, Guillermo, Finkelstein, Steven L., Haro, Pablo Arrabal, Simons, Raymond C., Wessner, Jessica, Cleri, Nikko J., Hirschmann, Michaela, Bagley, Micaela B., Nicholls, David C., Dickinson, Mark, Kartaltepe, Jeyhan S., Papovich, Casey, Kocevski, Dale D., Koekemoer, Anton M., Bisigello, Laura, Jaskot, Anne E., Lucas, Ray A., Jung, Intae, Wilkins, Stephen M., Yung, L. Y. Aaron, Ferguson, Henry C., Fontana, Adriano, Grazian, Andrea, Grogin, Norman A., Kewley, Lisa J., Kirkpatrick, Allison, Lotz, Jennifer M., Pentericci, Laura, Perez-Gonzalez, Pablo G., Ravindranath, Swara, Somerville, Rachel S., Yang, Guang, Holwerda, Benne W., Kurczynski, Peter, Hathi, Nimish P., Rose, Caitlin, Davis, Kelcey
We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey (CEERS) to measure rest-frame optical emission-line of 155 gal
Externí odkaz:
http://arxiv.org/abs/2307.09503
Autor:
Barro, Guillermo, Perez-Gonzalez, Pablo G., Kocevski, Dale D., McGrath, Elizabeth J., Trump, Jonathan R., Simons, Raymond C., Somerville, Rachel S., Yung, L. Y. Aaron, Haro, Pablo Arrabal, Bagley, Michaela B., Cleri, Nikko J., Costantin, Luca, Davis, Kelcey, Dickinson, Mark, Finkelstein, Steve L., Giavalisco, Mauro, Gomez-Guijarro, Carlos, Hathi, Nimish P., Hirschmann, Michaela, Akins, Hollis B., Holwerda, Benne W., Huertas-Company, Marc, Lucas, Ray A., Papovich, Casey, Seille, Lise-Marie, Tacchella, Sandro, Wilkins, Stephen M., de la Vega, Alexander, Yang, Guang, Zavala, Jorge A.
We study a new population of extremely red objects (EROs) recently discovered by JWST based on their NIRCam colors F277W$-$F444W $>1.5$ mag. We find 37 EROs in the CEERS field with F444W $<28$ mag and photometric redshifts between $5
Externí odkaz:
http://arxiv.org/abs/2305.14418