Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Herard-Demanche, Thomas"'
Autor:
Rowland, Lucie E., Hodge, Jacqueline, Bouwens, Rychard, Piña, Pavel Mancera, Hygate, Alexander, Algera, Hiddo, Aravena, Manuel, Bowler, Rebecca, da Cunha, Elisabete, Dayal, Pratika, Ferrara, Andrea, Herard-Demanche, Thomas, Inami, Hanae, van Leeuwen, Ivana, de Looze, Ilse, Oesch, Pascal, Pallottini, Andrea, Phillips, Siân, Rybak, Matus, Schouws, Sander, Smit, Renske, Sommovigo, Laura, Stefanon, Mauro, van der Werf, Paul
We present high resolution ($\sim0.14$" = 710 pc) ALMA [CII] 158$\mu$m and dust continuum follow-up observations of REBELS-25, a [CII]-luminous ($L_{\mathrm{[CII]}}=(1.7\pm0.2)\times 10^9 \mathrm{L_{\odot}}$) galaxy at redshift $z=7.3065\pm0.0001$. T
Externí odkaz:
http://arxiv.org/abs/2405.06025
Autor:
Matharu, Jasleen, Nelson, Erica J., Brammer, Gabriel, Oesch, Pascal A., Allen, Natalie, Shivaei, Irene, Naidu, Rohan P., Chisholm, John, Covelo-Paz, Alba, Fudamoto, Yoshinobu, Giovinazzo, Emma, Herard-Demanche, Thomas, Kerutt, Josephine, Kramarenko, Ivan, Marchesini, Danilo, Meyer, Romain A., Prieto-Lyon, Gonzalo, Reddy, Naveen, Shuntov, Marko, Weibel, Andrea, Wuyts, Stijn, Xiao, Mengyuan
We present the first results on the spatial distribution of star formation in 454 star-forming galaxies at $4.8
Externí odkaz:
http://arxiv.org/abs/2404.17629
Autor:
Herard-Demanche, Thomas, Bouwens, Rychard J., Oesch, Pascal A., Naidu, Rohan P., Decarli, Roberto, Nelson, Erica J., Brammer, Gabriel, Weibel, Andrea, Xiao, Mengyuan, Stefanon, Mauro, Walter, Fabian, Matthee, Jorryt, Meyer, Romain A., Wuyts, Stijn, Reddy, Naveen, Haro, Pablo Arrabal, Dannerbauer, Helmut, Shapley, Alice E., Chisholm, John, van Dokkum, Pieter, Labbe, Ivo, Illingworth, Garth, Schaerer, Daniel, Shivaei, Irene
We report the detection of a 13$\sigma$ H$\alpha$ emission line from HDF850.1 at $z=5.188\pm0.001$ using the FRESCO NIRCam F444W grism observations. Detection of H$\alpha$ in HDF850.1 is noteworthy, given its high far-IR luminosity, substantial dust
Externí odkaz:
http://arxiv.org/abs/2309.04525
Autor:
Xiao, Mengyuan, Oesch, Pascal, Elbaz, David, Bing, Longji, Nelson, Erica, Weibel, Andrea, Naidu, Rohan, Daddi, Emanuele, Bouwens, Rychard, Matthee, Jorryt, Wuyts, Stijn, Chisholm, John, Brammer, Gabriel, Dickinson, Mark, Magnelli, Benjamin, Leroy, Lucas, van Dokkum, Pieter, Schaerer, Daniel, Herard-Demanche, Thomas, Barrufet, Laia, Endsley, Ryan, Fudamoto, Yoshinobu, Gómez-Guijarro, Carlos, Gottumukkala, Rashmi, Illingworth, Garth, Labbe, Ivo, Magee, Daniel, Marchesini, Danilo, Maseda, Michael, Qin, Yuxiang, Reddy, Naveen, Shapley, Alice, Shivaei, Irene, Shuntov, Marko, Stefanon, Mauro, Whitaker, Katherine, Wyithe, J. Stuart
Over the past decade, the existence of a substantial population of optically invisible, massive galaxies at $z\gtrsim3$ has been implied from mid-infrared to millimeter observations. With the unprecedented sensitivity of the JWST, such extremely mass
Externí odkaz:
http://arxiv.org/abs/2309.02492
Autor:
Bouwens, Rychard J., Stefanon, Mauro, Brammer, Gabriel, Oesch, Pascal A., Herard-Demanche, Thomas, Illingworth, Garth D., Matthee, Jorryt, Naidu, Rohan P., van Dokkum, Pieter G., van Leeuwen, Ivana F.
We present the first constraints on the prevalence of z>10 galaxies in the Hubble Ultra Deep Field (HUDF) leveraging new NIRCam observations from JEMS (JWST Extragalactic Medium-band Survey). These NIRCam observations probe redward of 1.6$\mu$m, beyo
Externí odkaz:
http://arxiv.org/abs/2211.02607