Zobrazeno 1 - 10
of 14 390
pro vyhledávání: '"Miller, A B"'
With upcoming wide field surveys from the ground and space the number of known dwarf galaxies at $\lesssim 25$ Mpc is expected to dramatically increase. Insight into their nature and analyses of these systems' intrinsic properties will rely on reliab
Externí odkaz:
http://arxiv.org/abs/2407.04091
Autor:
Suess, Katherine A., Weaver, John R., Price, Sedona H., Pan, Richard, Wang, Bingjie, Bezanson, Rachel, Brammer, Gabriel, Cutler, Sam E., Labbe, Ivo, Leja, Joel, Williams, Christina C., Whitaker, Katherine E., Dayal, Pratika, de Graaff, Anna, Feldmann, Robert, Franx, Marijn, Fudamoto, Yoshinobu, Fujimoto, Seiji, Furtak, Lukas J., Goulding, Andy D., Greene, Jenny E., Khullar, Gourav, Kokorev, Vasily, Kriek, Mariska, Lorenz, Brian, Marchesini, Danilo, Maseda, Michael V., Matthee, Jorryt, Miller, Tim B., Mitsuhashi, Ikki, Mowla, Lamiya A., Muzzin, Adam, Naidu, Rohan P., Nanayakkara, Themiya, Nelson, Erica J., Oesch, Pascal A., Setton, David J., Shipley, Heath, Smit, Renske, Spilker, Justin S., van Dokkum, Pieter, Zitrin, Adi
In this paper, we describe the "Medium Bands, Mega Science" JWST Cycle 2 survey (JWST-GO-4111) and demonstrate the power of these data to reveal both the spatially-integrated and spatially-resolved properties of galaxies from the local universe to th
Externí odkaz:
http://arxiv.org/abs/2404.13132
Autor:
Cramer, William J., Noble, A. G., Rudnick, G., Pigarelli, A., Wilson, G., Bahé, Y. M., Cooper, M. C., Demarco, R., Matharu, J., Miller, T. B., Muzzin, A., Nantais, J., Sportsman, W., van Kampen, E., Webb, T. M. A., Yee, H. K. C.
The changes in colors across a galaxy are intimately connected to the galaxy's formation, growth, quenching history, and dust content. A particularly important epoch in the growth of galaxies is near $z \sim 2$ often referred to as 'cosmic noon', whe
Externí odkaz:
http://arxiv.org/abs/2404.07355
Autor:
Setton, David J., Khullar, Gourav, Miller, Tim B., Bezanson, Rachel, Greene, Jenny E., Suess, Katherine A., Whitaker, Katherine E., Antwi-Danso, Jacqueline, Atek, Hakim, Brammer, Gabriel, Cutler, Sam E., Dayal, Pratika, Feldmann, Robert, Furtak, Lukas J., Fujimoto, Seiji, Glazebrook, Karl, Goulding, Andy D., Kokorev, Vasily, Labbe, Ivo, Leja, Joel, Ma, Yilun, Marchesini, Danilo, Nanayakkara, Themiya, Pan, Richard, Price, Sedona H., Siegel, Jared C., Shipley, Heath, Weaver, John R., van Dokkum, Pieter, Wang, Bingjie, Williams, Christina C.
We report the spectroscopic confirmation of a massive ($\log(M_\star/M_\odot)=10.34 \pm_{0.07}^{0.06}$), HST-dark ($m_\mathrm{F150W} - m_\mathrm{F444W} = 3.6$) quiescent galaxy at $z_{spec}=3.97$ in the UNCOVER survey. NIRSpec/PRISM spectroscopy and
Externí odkaz:
http://arxiv.org/abs/2402.05664
Autor:
Kokorev, Vasily, Caputi, Karina I., Greene, Jenny E., Dayal, Pratika, Trebitsch, Maxime, Cutler, Sam E., Fujimoto, Seiji, Labbé, Ivo, Miller, Tim B., Iani, Edoardo, Navarro-Carrera, Rafael, Rinaldi, Pierluigi
Observations with the James Webb Space Telescope (JWST) have uncovered numerous faint active galactic nuclei (AGN) at $z\sim5$ and beyond. These objects are key to our understanding of the formation of supermassive black holes (SMBHs), their co-evolu
Externí odkaz:
http://arxiv.org/abs/2401.09981
Autor:
Cutler, Sam E., Whitaker, Katherine E., Weaver, John R., Wang, Bingjie, Pan, Richard, Bezanson, Rachel, Furtak, Lukas J., Labbe, Ivo, Leja, Joel, Price, Sedona H., Cheng, Yingjie, Clausen, Maike, Cullen, Fergus, Dayal, Pratika, de Graaff, Anna, Dickinson, Mark, Dunlop, James S., Feldmann, Robert, Franx, Marijn, Giavalisco, Mauro, Glazebrook, Karl, Greene, Jenny E., Grogin, Norman A., Illingworth, Garth, Koekemoer, Anton M., Kokorev, Vasily, Marchesini, Danilo, Maseda, Michael V., Miller, Tim B., Nanayakkara, Themiya, Nelson, Erica J., Setton, David J., Shipley, Heath, Suess, Katherine A.
We present a measurement of the low-mass quiescent size-mass relation at Cosmic Noon (1
Externí odkaz:
http://arxiv.org/abs/2312.15012
Autor:
Wright, Lillian, Whitaker, Katherine E., Weaver, John R., Cutler, Sam E., Wang, Bingjie, Carnall, Adam, Suess, Katherine A., Bezanson, Rachel, Nelson, Erica, Miller, Tim B., Ito, Kei, Valentino, Francesco
In this letter, we measure the rest-frame optical and near-infrared sizes of ten quiescent candidates at $3
Externí odkaz:
http://arxiv.org/abs/2311.05394
Autor:
Price, Sedona H., Suess, Katherine A., Williams, Christina C., Bezanson, Rachel, Khullar, Gourav, Nelson, Erica J., Wang, Bingjie, Weaver, John R., Fujimoto, Seiji, Kokorev, Vasily, Greene, Jenny E., Brammer, Gabriel, Cutler, Sam E., Dayal, Pratika, Furtak, Lukas J., Labbe, Ivo, Leja, Joel, Miller, Tim B., Nanayakkara, Themiya, Pan, Richard, Whitaker, Katherine E.
With the wavelength coverage, sensitivity, and high spatial resolution of JWST, it is now possible to peer through the dust attenuation to probe the rest-frame near infrared (NIR) and stellar structures of extremely dusty galaxies at cosmic noon (z~1
Externí odkaz:
http://arxiv.org/abs/2310.02500
Autor:
Fujimoto, Seiji, Bezanson, Rachel, Labbe, Ivo, Brammer, Gabriel, Price, Sedona H., Wang, Bingjie, Weaver, John R., Fudamoto, Yoshinobu, Oesch, Pascal A., Williams, Christina C., Dayal, Pratika, Feldmann, Robert, Greene, Jenny E., Leja, Joel, Whitaker, Katherine E., Zitrin, Adi, Cutler, Sam E., Furtak, Lukas J., Pan, Richard, Chemerynska, Iryna, Kokorev, Vasily, Miller, Tim B., Atek, Hakim, van Dokkum, Pieter, Juneau, Stephanie, Kassin, Susan, Khullar, Gourav, Marchesini, Danilo, Maseda, Michael, Nelson, Erica J., Setton, David J., Smit, Renske
We present the survey design and initial results of the ALMA Cycle 9 program of DUALZ, which aims to establish a joint ALMA and JWST public legacy field targeting the massive galaxy cluster Abell 2744. DUALZ features a contiguous $4'\times6'$ ALMA 30
Externí odkaz:
http://arxiv.org/abs/2309.07834
Autor:
Greene, Jenny E., Labbe, Ivo, Goulding, Andy D., Furtak, Lukas J., Chemerynska, Iryna, Kokorev, Vasily, Dayal, Pratika, Williams, Christina C., Wang, Bingjie, Setton, David J., Burgasser, Adam J., Bezanson, Rachel, Atek, Hakim, Brammer, Gabriel, Cutler, Sam E., Feldmann, Robert, Fujimoto, Seiji, Glazebrook, Karl, de Graaff, Anna, Leja, Joel, Marchesini, Danilo, Maseda, Michael V., Matthee, Jorryt, Miller, Tim B., Naidu, Rohan P., Nanayakkara, Themiya, Oesch, Pascal A., Pan, Richard, Papovich, Casey, Price, Sedona H., van Dokkum, Pieter, Weaver, John R., Whitaker, Katherine E., Zitrin, Adi
JWST is revealing a new population of dust-reddened broad-line active galactic nuclei (AGN) at redshifts $z\gtrsim5$. Here we present deep NIRSpec/Prism spectroscopy from the Cycle 1 Treasury program UNCOVER of 15 AGN candidates selected to be compac
Externí odkaz:
http://arxiv.org/abs/2309.05714