Zobrazeno 1 - 10
of 203
pro vyhledávání: '"Goulding, Andy D"'
Autor:
Treiber, Helena, Greene, Jenny, Weaver, John R., Miller, Tim B., Furtak, Lukas J., Setton, David J., Wang, Bingjie, de Graaff, Anna, Bezanson, Rachel, Brammer, Gabriel, Cutler, Sam E., Dayal, Pratika, Feldmann, Robert, Fujimoto, Seiji, Goulding, Andy D., Kokorev, Vasily, Labbe, Ivo, Leja, Joel, Marchesini, Danilo, Nanayakkara, Themiya, Nelson, Erica, Pan, Richard, Price, Sedona H., Siegel, Jared, Suess, Katherine, Whitaker, Katherine
JWST has revealed diverse new populations of high-redshift ($z\sim4-11$) AGN and extreme star-forming galaxies that challenge current models. In this paper, we use rest-frame UV emission-line diagnostics to identify AGN candidates and other exception
Externí odkaz:
http://arxiv.org/abs/2409.12232
Autor:
Rosado, Rodrigo Córdova, Goulding, Andy D., Greene, Jenny E., Petter, Grayson C., Hickox, Ryan C., Kokron, Nickolas, Strauss, Michael A., Givans, Jahmour J., Toba, Yoshiki, Henderson, Cassandra Starr
Active galactic nuclei (AGN) are the signposts of black hole growth, and likely play an important role in galaxy evolution. An outstanding question is whether AGN of different spectral types indicate different evolutionary stages in the coevolution o
Externí odkaz:
http://arxiv.org/abs/2409.08314
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:
Casey-Clyde, J. Andrew, Mingarelli, Chiara M. F., Greene, Jenny E., Goulding, Andy D., Chen, Siyuan, Trump, Jonathan R.
Supermassive black holes (SMBHs) are found in the centers of massive galaxies, and galaxy mergers should eventually lead to SMBH mergers. Quasar activity has long been associated with galaxy mergers, so here we investigate if supermassive black hole
Externí odkaz:
http://arxiv.org/abs/2405.19406
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:
La Torre, Valentina, Sajina, Anna, Goulding, Andy D., Marchesini, Danilo, Bezanson, Rachel, Pearl, Alan N., Sodré Jr, Laerte
The current and upcoming large data volume galaxy surveys require the use of machine learning techniques to maximize their scientific return. This study explores the use of Self-Organizing Maps (SOMs) to estimate galaxy parameters with a focus on han
Externí odkaz:
http://arxiv.org/abs/2403.18888
Autor:
Wang, Bingjie, de Graaff, Anna, Davies, Rebecca L., Greene, Jenny E., Leja, Joel, Goulding, Andy D., Williams, Christina C., Brammer, Gabriel B., Suess, Katherine A., Weibel, Andrea, Bezanson, Rachel, Boogaard, Leindert A., Cleri, Nikko J., Hirschmann, Michaela, Katz, Harley, Labbe, Ivo, Maseda, Michael V., Matthee, Jorryt, McConachie, Ian, Naidu, Rohan P., Oesch, Pascal A., Rix, Hans-Walter, Setton, David J., Whitaker, Katherine E.
The JWST discovery of ``little red dots'' (LRDs) is reshaping our picture of the early Universe, yet the physical mechanisms driving their compact size and UV-optical colors remain elusive. Here we report an unusually bright LRD ($z=3.1$) observed as
Externí odkaz:
http://arxiv.org/abs/2403.02304
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
We present the result of a spectroscopic campaign targeting Active Galactic Nucleus (AGN) candidates selected using a novel unsupervised machine-learning (ML) algorithm trained on optical and mid-infrared (mid-IR) photometry. AGN candidates are chose
Externí odkaz:
http://arxiv.org/abs/2402.05169
Drawing from the Chandra archive and using a carefully selected set of nearby dwarf galaxies, we present a calibrated high-mass X-ray binary (HMXB) luminosity function in the low-mass galaxy regime and search for an already hinted at dependence on me
Externí odkaz:
http://arxiv.org/abs/2401.14477