Zobrazeno 1 - 10
of 21 673
pro vyhledávání: '"Labbé A"'
Autor:
Lenschen, Jakob, Labbe, Rosalie, Drotleff, Nils, Fuhrmann, Markus, Lisenfeld, Jürgen, Rotzinger, Hannes, Ustinov, Alexey V.
We proposed and tested a cryogenic setup comprising dielectric waveguides for mm-wave frequencies in the range of 75-110 GHz and temperatures down to 10 mK. The targeted applications are quantum technologies at millimeter-wave frequencies, which requ
Externí odkaz:
http://arxiv.org/abs/2411.15058
Autor:
Kokorev, Vasily, Atek, Hakim, Chisholm, John, Endsley, Ryan, Chemerynska, Iryna, Muñoz, Julian B., Furtak, Lukas J., Pan, Richard, Berg, Danielle, Fujimoto, Seiji, Oesch, Pascal A., Weibel, Andrea, Adamo, Angela, Blaizot, Jeremy, Bouwens, Rychard, Dessauges-Zavadsky, Miroslava, Khullar, Gourav, Korber, Damien, Goovaerts, Ilias, Jecmen, Michelle, Labbé, Ivo, Leclercq, Floriane, Marques-Chaves, Rui, Mason, Charlotte, McQuinn, Kristen B. W., Naidu, Rohan, Natarajan, Priyamvada, Nelson, Erica, Rosdahl, Joki, Saldana-Lopez, Alberto, Schaerer, Daniel, Trebitsch, Maxime, Volonteri, Marta, Zitrin, Adi
We report the discovery of five galaxy candidates at redshifts between $15.9
Externí odkaz:
http://arxiv.org/abs/2411.13640
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:
Setton, David J., Greene, Jenny E., de Graaff, Anna, Ma, Yilun, Leja, Joel, Matthee, Jorryt, Bezanson, Rachel, Boogaard, Leindert A., Cleri, Nikko J., Katz, Harley, Labbe, Ivo, Maseda, Michael V., McConachie, Ian, Miller, Tim B., Price, Sedona H., Suess, Katherine A., van Dokkum, Pieter, Wang, Bingjie, Weibel, Andrea, Whitaker, Katherine E., Williams, Christina C.
Among the most puzzling early discoveries of JWST are "Little Red Dots" -- compact red sources that host broad Balmer emission lines and, in many cases, exhibit a "V shaped" change in slope in the rest-optical. The physical properties of Little Red D
Externí odkaz:
http://arxiv.org/abs/2411.03424
Autor:
Ma, Yilun, Greene, Jenny E., Setton, David J., Volonteri, Marta, Leja, Joel, Wang, Bingjie, Bezanson, Rachel, Brammer, Gabriel, Cutler, Sam E., Dayal, Pratika, van Dokkum, Pieter, Furtak, Lukas J., Glazebrook, Karl, Goulding, Andy D., de Graaff, Anna, Kokorev, Vasily, Labbe, Ivo, Pan, Richard, Price, Sedona H., Weaver, John R., Williams, Christina C., Whitaker, Katherine E., Zitrin, Adi
JWST has revealed an abundance of compact, red objects at $z\approx5-8$ dubbed "little red dots" (LRDs), whose SEDs display a faint blue UV continuum followed by a steep rise in the optical. Despite extensive study of their characteristic V-shaped SE
Externí odkaz:
http://arxiv.org/abs/2410.06257
Autor:
Nanayakkara, Themiya, Glazebrook, Karl, Schreiber, Corentin, Chittenden, Harry, Brammer, Gabriel, Esdaile, James, Jacobs, Colin, Kacprzak, Glenn G., Kawinwanichakij, Lalitwadee, Kimmig, Lucas C., Labbe, Ivo, Lagos, Claudia, Marchesini, Danilo, Martìnez-Marìn, M., Marsan, Z. Cemile, Oesch, Pascal A., Papovich, Casey, Remus, Rhea-Silvia, Tran, Kim-Vy H.
We present the formation histories of 19 massive ($\gtrsim3\times10^{10}\text{M}_\odot$) quiescent galaxy candidates at $z\sim3.0-4.5$ observed using JWST/NIRSpec. This completes the spectroscopic confirmation of the 24 $K$-selected quiescent galaxy
Externí odkaz:
http://arxiv.org/abs/2410.02076
Autor:
Williams, Christina C., Oesch, Pascal A., Weibel, Andrea, Brammer, Gabriel, Cloonan, Aidan P., Whitaker, Katherine E., Barrufet, Laia, Bezanson, Rachel, Bowler, Rebecca A. A., Dayal, Pratika, Franx, Marijn, Greene, Jenny E., Hutter, Anne, Ji, Zhiyuan, Labbé, Ivo, Manning, Sinclaire M., Maseda, Michael V., Xiao, Mengyuan
We present the PANORAMIC survey, a pure parallel extragalactic imaging program with NIRCam observed during JWST Cycle 1. The survey obtained $\sim$530 sq arcmin of NIRCam imaging from 1-5$\mu$m, totaling $\sim$192 hours of science integration time. T
Externí odkaz:
http://arxiv.org/abs/2410.01875
Autor:
Naidu, Rohan P., Matthee, Jorryt, Kramarenko, Ivan, Weibel, Andrea, Brammer, Gabriel, Oesch, Pascal A., Lechner, Peter, Furtak, Lukas J., Di Cesare, Claudia, Torralba, Alberto, Kotiwale, Gauri, Bezanson, Rachel, Bouwens, Rychard J., Chandra, Vedant, Claeyssens, Adélaïde, Danhaive, A. Lola, Frebel, Anna, de Graaff, Anna, Greene, Jenny E., Heintz, Kasper E., Ji, Alexander P., Kashino, Daichi, Katz, Harley, Labbe, Ivo, Leja, Joel, Li, Yijia, Maseda, Michael V., Richard, Johan, Shivaei, Irene, Simcoe, Robert A., Sobral, David, Suess, Katherine A., Tacchella, Sandro, Williams, Christina C.
Dwarf galaxies hold the key to crucial frontiers of astrophysics, however, their faintness renders spectroscopy challenging. Here we present the JWST Cycle 2 survey, All the Little Things (ALT, PID 3516), which is designed to seek late-forming Pop II
Externí odkaz:
http://arxiv.org/abs/2410.01874
Autor:
Treiber, Helena, Greene, Jenny, Weaver, John R., Miller, Tim B., Furtak, Lukas J., Setton, David J., Wang, Bingjie, de Graaff, Anna, Bezanson, Rachel, Brammer, Gabriel, Cutler, Sam E., Dayal, Pratika, Feldmann, Robert, Fujimoto, Seiji, Goulding, Andy D., Kokorev, Vasily, Labbe, Ivo, Leja, Joel, Marchesini, Danilo, Nanayakkara, Themiya, Nelson, Erica, Pan, Richard, Price, Sedona H., Siegel, Jared, Suess, Katherine, Whitaker, Katherine
JWST has revealed diverse new populations of high-redshift ($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:
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