Zobrazeno 1 - 10
of 58
pro vyhledávání: '"Drakos, Nicole E."'
Autor:
Akins, Hollis B., Casey, Caitlin M., Lambrides, Erini, Allen, Natalie, Andika, Irham T., Brinch, Malte, Champagne, Jaclyn B., Cooper, Olivia, Ding, Xuheng, Drakos, Nicole E., Faisst, Andreas, Finkelstein, Steven L., Franco, Maximilien, Fujimoto, Seiji, Gentile, Fabrizio, Gillman, Steven, Gozaliasl, Ghassem, Harish, Santosh, Hayward, Christopher C., Hirschmann, Michaela, Ilbert, Olivier, Kartaltepe, Jeyhan S., Kocevski, Dale D., Koekemoer, Anton M., Kokorev, Vasily, Liu, Daizhong, Long, Arianna S., McCracken, Henry Joy, McKinney, Jed, Onoue, Masafusa, Paquereau, Louise, Renzini, Alvio, Rhodes, Jason, Robertson, Brant E., Shuntov, Marko, Silverman, John D., Tanaka, Takumi S., Toft, Sune, Trakhtenbrot, Benny, Valentino, Francesco, Zavala, Jorge
JWST has revealed a population of compact and extremely red galaxies at $z>4$, which likely host active galactic nuclei (AGN). We present a sample of 434 ``little red dots'' (LRDs), selected from the 0.54 deg$^2$ COSMOS-Web survey. We fit galaxy and
Externí odkaz:
http://arxiv.org/abs/2406.10341
Autor:
Tanaka, Takumi S., Silverman, John D., Ding, Xuheng, Jahnke, Knud, Trakhtenbrot, Benny, Lambrides, Erini, Onoue, Masafusa, Andika, Irham Taufik, Bongiorno, Angela, Faisst, Andreas L., Gillman, Steven, Hayward, Christopher C., Hirschmann, Michaela, Koekemoer, Anton, Kokorev, Vasily, Liu, Zhaoxuan, Magdis, Georgios E., Renzini, Alvio, Casey, Caitlin, Drakos, Nicole E., Franco, Maximilien, Gozaliasl, Ghassem, Kartaltepe, Jeyhan, Liu, Daizhong, McCracken, Henry Joy, Rhodes, Jason, Robertson, Brant, Toft, Sune
Our knowledge of relations between supermassive black holes and their host galaxies at $z\gtrsim1$ is still limited, even though being actively sought out to $z\sim6$. Here, we use the high resolution and sensitivity of JWST to measure the host galax
Externí odkaz:
http://arxiv.org/abs/2401.13742
Autor:
Berman, Edward, McCleary, Jacqueline, Koekemoer, Anton M., Franco, Maximilien, Drakos, Nicole E., Liu, Daizhong, Nightingale, James W., Shuntov, Marko, Scognamiglio, Diana, Massey, Richard, Mahler, Guillaume, McCracken, Henry Joy, Robertson, Brant E., Faisst, Andreas L., Casey, Caitlin M., Kartaltepe, Jeyhan S.
With their high angular resolutions of 30--100 mas, large fields of view, and complex optical systems, imagers on next-generation optical/near-infrared space observatories, such as the Near-Infrared Camera (NIRCam) on the James Webb Space Telescope (
Externí odkaz:
http://arxiv.org/abs/2401.11625
Autor:
Wilkins, Stephen M., Turner, Jack C., Bagley, Micaela B., Finkelstein, Steven L., Amorín, Ricardo O., Hautefort, Adrien Aufan Stoffels D, Behroozi, Peter, Bhatawdekar, Rachana, Dekel, Avishai, Donnellan, James, Drakos, Nicole E., Fortuni, Flaminia, Hathi, Nimish P., Hirschmann, Michaela, Holwerda, Benne W., Irodotou, Dimitrios, Koekemoer, Anton M., Lovell, Christopher C., Merlin, Emiliano, Roper, Will J., Seeyave, Louise T. C., Vijayan, Aswin P., Yung, L. Y. Aaron
The wavelength-coverage and sensitivity of JWST now enables us to probe the rest-frame UV - optical spectral energy distributions (SEDs) of galaxies at high-redshift ($z>4$). From these SEDs it is, in principle, through SED fitting possible to infer
Externí odkaz:
http://arxiv.org/abs/2311.08065
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 527, Issue 2, January 2024, Pages 3459-3473
Dark matter haloes grow at a rate that depends on the value of the cosmological parameters $\sigma_8$ and $\Omega_{\rm m}$ through the initial power spectrum and the linear growth factor. While halo abundance is routinely used to constrain these para
Externí odkaz:
http://arxiv.org/abs/2311.03580
Autor:
Casey, Caitlin M., Akins, Hollis B., Shuntov, Marko, Ilbert, Olivier, Paquereau, Louise, Franco, Maximilien, Hayward, Christopher C., Finkelstein, Steven L., Boylan-Kolchin, Michael, Robertson, Brant E., Allen, Natalie, Brinch, Malte, Cooper, Olivia R., Ding, Xuheng, Drakos, Nicole E., Faisst, Andreas L., Fujimoto, Seiji, Gillman, Steven, Harish, Santosh, Hirschmann, Michaela, Jin, Shuowen, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Kokorev, Vasily, Liu, Daizhong, Long, Arianna S., Magdis, Georgios, Maraston, Claudia, Martin, Crystal L., McCracken, Henry Joy, McKinney, Jed, Mobasher, Bahram, Rhodes, Jason, Rich, R. Michael, Sanders, David B., Silverman, John D., Toft, Sune, Vijayan, Aswin P., Weaver, John R., Wilkins, Stephen M., Yang, Lilan, Zavala, Jorge A.
We report the discovery of 15 exceptionally luminous $10\lesssim z\lesssim14$ candidate galaxies discovered in the first 0.28 deg$^2$ of JWST/NIRCam imaging from the COSMOS-Web Survey. These sources span rest-frame UV magnitudes of $-20.5>M_{\rm UV}>
Externí odkaz:
http://arxiv.org/abs/2308.10932
A growing body of evidence suggests that the central density of cuspy dark matter subhaloes is conserved in minor mergers. However, empirical models of subhalo evolution, calibrated from simulations, often assume a drop in the central density. Since
Externí odkaz:
http://arxiv.org/abs/2308.00830
Autor:
Franco, Maximilien, Akins, Hollis B., Casey, Caitlin M., Finkelstein, Steven L., Shuntov, Marko, Chworowsky, Katherine, Faisst, Andreas L., Fujimoto, Seiji, Ilbert, Olivier, Koekemoer, Anton M., Liu, Daizhong, Lovell, Christopher C., Maraston, Claudia, McCracken, Henry Joy, McKinney, Jed, Robertson, Brant E., Bagley, Micaela B., Champagne, Jaclyn B., Cooper, Olivia R., Ding, Xuheng, Drakos, Nicole E., Enia, Andrea, Gillman, Steven, Hayward, Christopher C., Hirschmann, Michaela, Kokorev, Vasily, Laigle, Clotilde, Long, Arianna S., Gozaliasl, Ghassem, Harish, Santosh, Jin, Shuowen, Kartaltepe, Jeyhan S., Magdis, Georgios, Mahler, Guillaume, Martin, Crystal L., Rich, R. Michael, Trakhtenbrot, Benny, Mobasher, Bahram, Paquereau, Louise, Renzini, Alvio, Rhodes, Jason, Sheth, Kartik, Silverman, John D., Sparre, Martin, Talia, Margherita, Valentino, Francesco, Vijayan, Aswin P., Wilkins, Stephen M., Yang, Lilan, Zavala, Jorge A.
We report the identification of 15 galaxy candidates at $z\ge9$ using the initial COSMOS-Web JWST observations over 77 arcmin$^2$ through four NIRCam filters (F115W, F150W, F277W, F444W) with an overlap with MIRI (F770W) of 8.7 arcmin$^2$. We fit the
Externí odkaz:
http://arxiv.org/abs/2308.00751
Autor:
Akins, Hollis B., Casey, Caitlin M., Allen, Natalie, Bagley, Micaela B., Dickinson, Mark, Finkelstein, Steven L., Franco, Maximilien, Harish, Santosh, Haro, Pablo Arrabal, Ilbert, Olivier, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Liu, Daizhong, Long, Arianna S., McCracken, Henry Joy, Paquereau, Louise, Papovich, Casey, Pirzkal, Nor, Rhodes, Jason, Robertson, Brant E., Shuntov, Marko, Toft, Sune, Yang, Guang, Barro, Guillermo, Bisigello, Laura, Buat, Véronique, Champagne, Jaclyn B., Cooper, Olivia, Costantin, Luca, de la Vega, Alexander, Drakos, Nicole E., Faisst, Andreas, Fontana, Adriano, Fujimoto, Seiji, Gillman, Steven, Gómez-Guijarro, Carlos, Gozaliasl, Ghassem, Hathi, Nimish P., Hayward, Christopher C., Hirschmann, Michaela, Holwerda, Benne W., Jin, Shuowen, Kocevski, Dale D., Kokorev, Vasily, Lambrides, Erini, Lucas, Ray A., Magdis, Georgios E., Magnelli, Benjamin, McKinney, Jed, Mobasher, Bahram, Pérez-González, Pablo G., Rich, R. Michael, Seillé, Lise-Marie, Talia, Margherita, Urry, C. Megan, Valentino, Francesco, Whitaker, Katherine E., Yung, L. Y. Aaron, Zavala, Jorge
We present a search for extremely red, dust-obscured, $z>7$ galaxies with $\textit{JWST}$/NIRCam+MIRI imaging over the first 20 arcmin$^2$ of publicly-available Cycle 1 data from the COSMOS-Web, CEERS, and PRIMER surveys. Based on their red color in
Externí odkaz:
http://arxiv.org/abs/2304.12347
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