Zobrazeno 1 - 10
of 838
pro vyhledávání: '"Muzzin, P."'
Autor:
McConachie, Ian, Wilson, Gillian, Forrest, Ben, Marsan, Z. Cemile, Muzzin, Adam, Cooper, M. C., Annunziatella, Marianna, Marchesini, Danilo, Gomez, Percy, Chang, Wenjun, Stawinski, Stephanie M. Urbano, McDonald, Michael, Webb, Tracy, Noble, Allison, Lemaux, Brian C., Shah, Ekta A., Staab, Priti, Lubin, Lori M., Gal, Roy R.
We examine the quiescent fractions of massive galaxies in six $z\gtrsim3$ spectroscopically-confirmed protoclusters in the COSMOS field, one of which is newly confirmed and presented here. We report the spectroscopic confirmation of MAGAZ3NE~J100143+
Externí odkaz:
http://arxiv.org/abs/2411.14641
Autor:
Zaidi, Kumail, Wake, David A., Marchesini, Danilo, Iyer, Kartheik, Muzzin, Adam, Papovich, Casey, Antwi-Danso, Jacqueline, Glazebrook, Karl, Labbé, Ivo
We present a comprehensive analysis of the observed Stellar-to-Halo mass relationship (SHMR) spanning redshifts from 0.2 to 4.5. This was enabled through galaxy clustering and abundance measurements from two large (effective area ~ 1.61 deg^2) and ho
Externí odkaz:
http://arxiv.org/abs/2411.04256
Autor:
Asada, Yoshihisa, Desprez, Guillaume, Willott, Chris J., Sawicki, Marcin, Bradač, Maruša, Brammer, Gabriel, Dubath, Florian, Iyer, Kartheik G., Martis, Nicholas S., Muzzin, Adam, Noirot, Gaël, Paltani, Stéphane, Sarrouh, Ghassan T. E., Harshan, Anishya, Markov, Vladan
We present a new analytical model for the attenuation to Epoch of Reionization (EoR) galaxies by proximate neutral hydrogen gas. Many galaxy spectra in the EoR taken by JWST have shown a flux deficit at wavelengths just redward of the Lyman break, an
Externí odkaz:
http://arxiv.org/abs/2410.21543
Autor:
Sok, Visal, Muzzin, Adam, Jablonka, Pascale, Tan, Vivian Yun Yan, Marsan, Z. Cemile, Marchesini, Danilo, Wilson, Gillian, Alcorn, Leo Y.
Despite the ubiquity of clumpy star-forming galaxies at high-redshift, the origin of clumps are still largely unconstrained due to the limited observations that can validate the mechanisms for clump formation. We postulate that if clumps form due to
Externí odkaz:
http://arxiv.org/abs/2410.21370
Autor:
Harshan, Anishya, Tripodi, Roberta, Martis, Nicholas S., Rihtaršič, Gregor, Bradač, Maruša, Asada, Yoshihisa, Brammer, Gabe, Desprez, Guillaume, Estrada-Carpenter, Vince, Matharu, Jasleen, Markov, Vladan, Muzzin, Adam, Mowla, Lamiya, Noirot, Gaël, Sarrouh, Ghassan T. E., Sawicki, Marcin, Strait, Victoria, Willot, Chris
We present galaxy MACS0416-Y1 at z$_{\rm{spec}} = 8.312$ as observed by the CAnadian NIRISS Unbiased Cluster Survey (CANUCS). MACS0416-Y1 has been shown to have extreme dust properties, thus, we study the physical properties and star formation histor
Externí odkaz:
http://arxiv.org/abs/2408.12310
Autor:
Price, Sedona H., Bezanson, Rachel, Labbe, Ivo, Furtak, Lukas J., de Graaff, Anna, Greene, Jenny E., Kokorev, Vasily, Setton, David J., Suess, Katherine A., Brammer, Gabriel, Cutler, Sam E., Leja, Joel, Pan, Richard, Wang, Bingjie, Weaver, John R., Whitaker, Katherine E., Atek, Hakim, Burgasser, Adam J., Chemerynska, Iryna, Dayal, Pratika, Feldmann, Robert, Schreiber, Natascha M. Förster, Fudamoto, Yoshinobu, Fujimoto, Seiji, Glazebrook, Karl, Goulding, Andy D., Khullar, Gourav, Kriek, Mariska, Marchesini, Danilo, Maseda, Michael V., Miller, Tim B., Muzzin, Adam, Nanayakkara, Themiya, Nelson, Erica, Oesch, Pascal A., Shipley, Heath, Smit, Renske, Taylor, Edward N., van Dokkum, Pieter, Williams, Christina C., Zitrin, Adi
We present the design and observations of low resolution JWST/NIRSpec PRISM spectroscopy from the Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization (UNCOVER) Cycle 1 JWST Treasury program. Targets are selected using JWST/NIRC
Externí odkaz:
http://arxiv.org/abs/2408.03920
Autor:
Beverage, Aliza G., Slob, Martje, Kriek, Mariska, Conroy, Charlie, Barro, Guillermo, Bezanson, Rachel, Brammer, Gabriel, Cheng, Chloe M., de Graaff, Anna, Schreiber, Natascha M. Förster, Franx, Marijn, Lorenz, Brian, Piña, Pavel E. Mancera, Marchesini, Danilo, Muzzin, Adam, Newman, Andrew B., Price, Sedona H., Shapley, Alice E., Stefanon, Mauro, Suess, Katherine A., van Dokkum, Pieter, Weinberg, David, Weisz, Daniel R.
We present the stellar metallicities and multi-element abundances (C, Mg, Si, Ca, Ti, Cr, and Fe) of 15 massive (log $M/M_\odot=10.2-11.2$) quiescent galaxies at z=1-3, derived from ultradeep JWST-SUSPENSE spectra. Compared to quiescent galaxies at z
Externí odkaz:
http://arxiv.org/abs/2407.02556
Autor:
Harshan, Anishya, Bradač, Maruša, Abraham, Roberto, Asada, Yoshihisa, Brammer, Gabriel, Desprez, Guillaume, Iyer, Karthiek, Martis, Nicholas S., Matharu, Jasleen, Mowla, Lamiya, Muzzin, Adam, Noirot, Gaël, Rihtaršič, Gregor, Sarrouh, Ghassan T. E., Sawicki, Marcin, Strait, Victoria, Willott, Chris J.
The epoch of reionisation progressed through the emission of ionising photons from galaxies to their local intergalactic medium. In this work, we characterise the dwarf star-forming galaxies as candidates for the source of ionising photons that drove
Externí odkaz:
http://arxiv.org/abs/2406.17128
Autor:
Estrada-Carpenter, Vicente, Sawicki, Marcin, Brammer, Gabe, Desprez, Guillaume, Abraham, Roberto, Asada, Yoshihisa, Bradač, Maruša, Iyer, Kartheik G., Martis, Nicholas S., Matharu, Jasleen, Mowla, Lamiya, Muzzin, Adam, Noirot, Gaël, Sarrouh, Ghassan T. E., Strait, Victoria, Willott, Chris J.
Spatially resolved studies are key to understanding when, where, and how stars form within galaxies. Using slitless grism spectra and broadband imaging from the CAnadian NIRISS Unbiased Cluster Survey (CANUCS) we study the spatially resolved properti
Externí odkaz:
http://arxiv.org/abs/2406.15551
Autor:
Nedkova, Kalina V., Häußler, Boris, Marchesini, Danilo, Brammer, Gabriel B., Feinstein, Adina D., Johnston, Evelyn J., Kartaltepe, Jeyhan S., Koekemoer, Anton M., Martis, Nicholas S., Muzzin, Adam, Rafelski, Marc, Shipley, Heath V., Skelton, Rosalind E., Stefanon, Mauro, van der Wel, Arjen, Whitaker, Katherine E.
Using deep imaging from the CANDELS and HFF surveys, we present bulge+disc decompositions with GalfitM for $\sim$17,000 galaxies over $0.2 \leq z\leq 1.5$. We use various model parameters to select reliable samples of discs and bulges, and derive the
Externí odkaz:
http://arxiv.org/abs/2406.14613