Zobrazeno 1 - 10
of 986
pro vyhledávání: '"Miller, Tim"'
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
Goal recognition (GR) involves inferring an agent's unobserved goal from a sequence of observations. This is a critical problem in AI with diverse applications. Traditionally, GR has been addressed using 'inference to the best explanation' or abducti
Externí odkaz:
http://arxiv.org/abs/2409.11675
Autor:
Siegel, Jared, Setton, David, Greene, Jenny, Suess, Katherine, Whitaker, Katherine, Bezanson, Rachel, Leja, Joel, Furtak, Lukas, Cutler, Sam, de Graaff, Anna, Feldmann, Robert, Khullar, Gourav, Labbé, Ivo, Marchesini, Danilo, Miller, Tim, Nanayakkara, Themiya, Pan, Richard, Price, Sedona, Treiber, Helena, van Dokkum, Pieter, Wang, Bingjie, Weaver, John
We explore the physical properties of five massive quiescent galaxies at $z\sim2.5$, revealing the presence of non-negligible dust reservoirs. JWST NIRSpec observations were obtained for each target, finding no significant line emission; multiple sta
Externí odkaz:
http://arxiv.org/abs/2409.11457
Autor:
Benton, Chloë E., Nelson, Erica J., Miller, Tim B., Bezanson, Rachel, Gibson, Justus, Hartley, Abigail I, Martorano, Marco, Price, Sedona H., Suess, Katherine A., van der Wel, Arjen, van Dokkum, Pieter, Weaver, John R., Whitaker, Katherine E.
Hubble Space Telescope imaging shows that most star-forming galaxies at cosmic noon -- the peak of cosmic star formation history -- appear disk-dominated, leaving the origin of the dense cores in their quiescent descendants unclear. With the James We
Externí odkaz:
http://arxiv.org/abs/2409.08328
Autor:
de Graaff, Anna, Brammer, Gabriel, Weibel, Andrea, Lewis, Zach, Maseda, Michael V., Oesch, Pascal A., Bezanson, Rachel, Boogaard, Leindert A., Cleri, Nikko J., Cooper, Olivia R., Gottumukkala, Rashmi, Greene, Jenny E., Hirschmann, Michaela, Hviding, Raphael E., Katz, Harley, Labbé, Ivo, Leja, Joel, Matthee, Jorryt, McConachie, Ian, Miller, Tim B., Naidu, Rohan P., Price, Sedona H., Rix, Hans-Walter, Setton, David J., Suess, Katherine A., Wang, Bingjie, Whitaker, Katherine E., Williams, Christina C.
We present the Red Unknowns: Bright Infrared Extragalactic Survey (RUBIES), providing JWST/NIRSpec spectroscopy of red sources selected across ~150 arcmin$^2$ from public JWST/NIRCam imaging in the UDS and EGS fields. RUBIES novel observing strategy
Externí odkaz:
http://arxiv.org/abs/2409.05948
Autor:
Weibel, Andrea, de Graaff, Anna, Setton, David J., Miller, Tim B., Oesch, Pascal A., Brammer, Gabriel, Lagos, Claudia D. P., Whitaker, Katherine E., Williams, Christina C., Baggen, Josephine F. W., Bezanson, Rachel, Boogaard, Leindert A., Cleri, Nikko J., Greene, Jenny E., Hirschmann, Michaela, Hviding, Raphael E., Kuruvanthodi, Adarsh, Labbé, Ivo, Leja, Joel, Maseda, Michael V., Matthee, Jorryt, McConachie, Ian, Naidu, Rohan P., Roberts-Borsani, Guido, Schaerer, Daniel, Suess, Katherine A., Valentino, Francesco, van Dokkum, Pieter, Wang, Bingjie
We report the spectroscopic discovery of a massive quiescent galaxy at $z_{\rm spec}=7.29\pm0.01$, just $\sim700\,$Myr after the Big Bang. RUBIES-UDS-QG-z7 was selected from public JWST/NIRCam and MIRI imaging from the PRIMER survey and observed with
Externí odkaz:
http://arxiv.org/abs/2409.03829
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
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:
Singh, Ronal, Miller, Tim, Sonenberg, Liz, Velloso, Eduardo, Vetere, Frank, Howe, Piers, Dourish, Paul
In this paper, we introduce and evaluate a tool for researchers and practitioners to assess the actionability of information provided to users to support algorithmic recourse. While there are clear benefits of recourse from the user's perspective, th
Externí odkaz:
http://arxiv.org/abs/2407.09516
Autor:
Clausen, Maike, Whitaker, Katherine E., Momcheva, Ivelina, Cutler, Sam E., Suess, Katherine A., Weaver, John R., Miller, Tim, van der Wel, Arjen, Wuyts, Stijn, Wake, David, van Dokkum, Pieter, Bezanson, Rachel S., Brammer, Gabriel, Franx, Marijn, Nelson, Erica J., Schreiber, Natasha M. Foerster
We present a study of the growth of the quiescent galaxy population between 0.5 < z < 3 by tracing the number density and structural evolution of a sample of 4518 old and 583 young quiescent galaxies with log($M_*$/$M_{\odot}$)>10.4, selected from th
Externí odkaz:
http://arxiv.org/abs/2405.09354