Zobrazeno 1 - 10
of 71
pro vyhledávání: '"Leethochawalit, N."'
Autor:
Zhuang, Zhuyun, Kirby, Evan N., Steidel, Charles C., Reyes, Mithi A. C. de los, Prusinski, Nikolaus Z., Leethochawalit, N., Park, Minjung, Conroy, Charlie, Nuñez, Evan H.
Understanding the chemical enrichment of different elements is crucial to gaining a complete picture of galaxy chemical evolution. In this study, we present a new sample of 46 low-redshift, low-mass star-forming galaxies at $M_*\sim 10^{8-10}M_{\odot
Externí odkaz:
http://arxiv.org/abs/2407.04782
Autor:
Dressler, A., Vulcani, B., Treu, T., Rieke, M., Burns, C., Calabro', A., Bonchi, A., Castellano, M., Fontana, A., Leethochawalit, N., Mason, C., Merlin, E., Morishita, T., Paris, D., Mercurio, A., Nanayakkara, T., Poggianti, B. M., Santini, P., Wang, X., Misselt, K., Stark, D. P., Willmer, C.
JWST observations of high redshift galaxies are used to measure their star formation histories - the buildup of stellar mass in the earliest galaxies. Here we use a novel analysis program, SEDz*, to compare near-IR spectral energy distributions for g
Externí odkaz:
http://arxiv.org/abs/2208.04292
Autor:
Glazebrook, Karl, Nanayakkara, T., Jacobs, C., Leethochawalit, N., Calabrò, A., Bonchi, A., Castellano, M., Fontana, A., Mason, C., Merlin, E., Morishita, T., Paris, D., Trenti, M., Treu, T., Santini, P., Wang, X., Boyett, K., Bradac, Marusa, Brammer, G., Jones, T., Marchesini, D., Nonino, M., Vulcani, B.
We present a first look at the reddest 2-5$\mu\rm m$ sources found in deep images from the GLASS Early Release Science program. We undertake a general search, i.e. not looking for any particular spectral signatures, for sources detected only in bands
Externí odkaz:
http://arxiv.org/abs/2208.03468
Autor:
Treu, T., Calabro, A., Castellano, M., Leethochawalit, N., Merlin, E., Fontana, A., Yang, L., Morishita, T., Trenti, M., Dressler, A., Mason, C., Paris, D., Pentericci, L., Roberts-Borsani, G., Vulcani, B., Boyett, K., Bradac, M., Glazebrook, K., Jones, T., Marchesini, D., Mascia, S., Nanayakkara, T., Santini, P., Strait, V., Vanzella, E., Wang, X.
Star-forming galaxies can exhibit strong morphological differences between the rest-frame far-UV and optical, reflecting inhomogeneities in star-formation and dust attenuation. We exploit deep, high resolution NIRCAM 7-band observations to take a fir
Externí odkaz:
http://arxiv.org/abs/2207.13527
Autor:
Boyett, K., Mascia, S., Pentericci, L., Leethochawalit, N., Trenti, M., Brammer, G., Roberts-Borsani, G., Strait, V., Treu, T., Bradac, M., Glazebrook, K., Acebron, A., Bergamini, P., Calabro`, A., Castellano, M., Fontana, A., Grillo, C., Henry, A., Jones, T., Marchesini, D., Mason, C., Mercurio, A., Morishita, T., Nanayakkara, T., Rosati, P., Scarlata, C., Vanzella, E., Vulcani, B., Wang, X., Willott, C.
Wide Field Slitless Spectroscopy (WFSS) provides a powerful tool for detecting strong line emission in star forming galaxies (SFGs) without the need for target pre-selection. As part of the GLASS-JWST-ERS program, we leverage the near-infrared wavele
Externí odkaz:
http://arxiv.org/abs/2207.13459
Autor:
Yang, Lilan, Morishita, T., Leethochawalit, N., Castellano, M., Calabro, A., Treu, T., Bonchi, A., Fontana, A., Mason, C., Merlin, E., Paris, D., Trenti, M., Roberts-Borsani, G., Bradac, M., Vanzella, E., Vulcani, B., Marchesini, D., Ding, X., Nanayakkara, Themiya, Birrer, Simon, Glazebrook, K., Jones, T., Boyett, K., Santini, P., Strait, Victoria, Wang, Xin
We present the first rest-frame optical size-luminosity relation of galaxies at $z>7$, using the NIRCam imaging data obtained by the GLASS James Webb Space Telescope Early Release Science (GLASS-JWST-ERS) program, providing the deepest extragalactic
Externí odkaz:
http://arxiv.org/abs/2207.13101
Autor:
Santini, P., Fontana, A., Castellano, M., Leethochawalit, N., Trenti, M., Treu, T., Belfiori, D., Birrer, S., Bonchi, A., Merlin, E., Mason, C., Morishita, T., Nonino, M., Paris, D., Polenta, G., Rosati, P., Yang, L., Bradac, M., Calabrò, A., Dressler, A., Glazebrook, K., Marchesini, D., Mascia, S., Nanayakkara, T., Pentericci, L., Roberts-Borsani, G., Scarlata, C., Vulcani, B., Wang, Xin
We exploit James Webb Space Telescope (JWST) NIRCam observations from the GLASS-JWST-Early Release Science program to investigate galaxy stellar masses at z>7. We first show that JWST observations reduce the uncertainties on the stellar mass by a fac
Externí odkaz:
http://arxiv.org/abs/2207.11379
Autor:
Leethochawalit, N., Trenti, M., Santini, P., Yang, L., Merlin, E., Castellano, M., Fontana, A., Treu, T., Mason, C., Glazebrook, K., Jones, T., Vulcani, B., Nanayakkara, T., Marchesini, D., Mascia, S., Morishita, T., Roberts-Borsani, G., Bonchi, A., Paris, D., Boyett, K., Strait, V., Calabro`, A., Pentericci, L., Bradac, M., Wang, X., Scarlata, C.
We present the first James Webb Space Telescope/NIRCam-led determination of $7
Externí odkaz:
http://arxiv.org/abs/2207.11135
Autor:
Treu, T., Roberts-Borsani, G., Bradac, M., Brammer, G., Fontana, A., Henry, A., Mason, C., Morishita, T., Pentericci, L., Wang, X., Acebron, A., Bagley, M., Bergamini, P., Belfiori, D., Bonchi, A., Boyett, K., Boutsia, K., Calabro, A., Caminha, G. B., Castellano, M., Dressler, A., Glazebrook, K., Grillo, C., Jacobs, C., Jones, T., Kelly, P., Leethochawalit, N., Malkan, M., Marchesini, D., Mascia, S., Mercurio, A., Merlin, E., Nanayakkara, T., Nonino, M., Paris, D., Poggianti, B., Rosati, P., Santini, P., Scarlata, C., Shipley, H., Strait, V., Trenti, M., Tubthong, C., Vanzella, E., Vulcani, B., Yang, L.
The GLASS James Webb Space Telescope Early Release Science (hereafter GLASS-JWST-ERS) Program will obtain and make publicly available the deepest extragalactic data of the ERS campaign. It is primarily designed to address two key science questions, n
Externí odkaz:
http://arxiv.org/abs/2206.07978
Autor:
High, F. W., Hoekstra, H., Leethochawalit, N., de Haan, T., Abramson, L., Aird, K. A., Armstrong, R., Ashby, M. L. N., Bautz, M., Bayliss, M., Bazin, G., Benson, B. A., Bleem, L. E., Brodwin, M., Carlstrom, J. E., Chang, C. L., Cho, H. M., Clocchiatti, A., Conroy, M., Crawford, T. M., Crites, A. T., Desai, S., Dobbs, M. A., Dudley, J. P., Foley, R. J., Forman, W. R., George, E. M., Gladders, M. D., Gonzalez, A. H., Halverson, N. W., Harrington, N. L., Holder, G. P., Holzapfel, W. L., Hoover, S., Hrubes, J. D., Jones, C., Joy, M., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Liu, J., Lueker, M., Luong-Van, D., Mantz, A., Marrone, D. P., McDonald, M., McMahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Mohr, J. J., Montroy, T. E., Murray, S. S., Natoli, T., Nurgaliev, D., Padin, S., Plagge, T., Pryke, C., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Saliwanchik, B. R., Saro, A., Sayre, J. T., Schaffer, K. K., Shaw, L., Schrabback, T., Shirokoff, E., Song, J., Spieler, H. G., Stalder, B., Staniszewski, Z., Stark, A. A., Story, K., Stubbs, C. W., Suhada, R., Tokarz, S., van Engelen, A., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zahn, O., Zenteno, A.
We use weak gravitational lensing to measure the masses of five galaxy clusters selected from the South Pole Telescope (SPT) survey, with the primary goal of comparing these with the SPT Sunyaev--Zel'dovich (SZ) and X-ray based mass estimates. The cl
Externí odkaz:
http://arxiv.org/abs/1205.3103