Zobrazeno 1 - 10
of 52
pro vyhledávání: '"Claeyssens, Adélaïde"'
Autor:
Claeyssens, Adélaïde, Adamo, Angela, Messa, Matteo, Dessauges-Zavadsky, Miroslava, Richard, Johan, Kramarenko, Ivan, Matthee, Jorryt, Naidu, Rohan P.
We present a sample of 1956 individual stellar clumps at redshift 0.7
Externí odkaz:
http://arxiv.org/abs/2410.10974
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:
Richard, Johan, Giroud, Rémi, Laurent, Florence, Krajnović, Davor, Jeanneau, Alexandre, Bacon, Roland, Abreu, Manuel, Adamo, Angela, Araujo, Ricardo, Bouché, Nicolas, Brinchmann, Jarle, Cai, Zhemin, Castro, Norberto, Calcines, Ariadna, Chapuis, Diane, Claeyssens, Adélaïde, Cortese, Luca, Daddi, Emanuele, Davison, Christopher, Goodwin, Michael, Harris, Robert, Hayes, Matthew, Jauzac, Mathilde, Kelz, Andreas, Kneib, Jean-Paul, Lanotte, Audrey A., Lawrence, Jon, Bouteiller, Vianney Le, Breton, Rémy Le, Lehnert, Matthew, Sanchez, Angel Lopez, McGregor, Helen, McLeod, Anna F., Monteiro, Manuel, Morris, Simon, Opitom, Cyrielle, Pécontal, Arlette, Robertson, David, Roth, Martin M., van de Sande, Jesse, Smith, Russell, Steinmetz, Matthias, Swinbank, Mark, Urrutia, Tanya, Verhamme, Anne, Weilbacher, Peter M., Wendt, Martin, Wildi, François, Zheng, Jessica, consortium, The BlueMUSE
BlueMUSE is a blue-optimised, medium spectral resolution, panoramic integral field spectrograph under development for the Very Large Telescope (VLT). With an optimised transmission down to 350 nm, spectral resolution of R$\sim$3500 on average across
Externí odkaz:
http://arxiv.org/abs/2406.13914
Autor:
Kusakabe, Haruka, Mauerhofer, Valentin, Verhamme, Anne, Garel, Thibault, Blaizot, Jeremy, Wisotzki, Lutz, Richard, Johan, Boogaard, Leindert A., Leclercq, Floriane, Guo, Yucheng, Claeyssens, Adelaide, Contini, Thierry, Herenz, Edmund Christian, Kerutt, Josephine, Maseda, Michael V., Michel-Dansac, Leo, Nanayakkara, Themiya, Ouchi, Masami, Pessa, Ismael, Schaye, Joop
Publikováno v:
A&A 691, A255 (2024)
The circumgalactic medium (CGM) serves as a baryon reservoir that connects galaxies to the intergalactic medium and fuels star formation. The spatial distribution of the metal-enriched cool CGM has not yet been directly revealed at cosmic noon (z~2-4
Externí odkaz:
http://arxiv.org/abs/2406.04399
Autor:
Messa, Matteo, Dessauges-Zavadsky, Miroslava, Adamo, Angela, Richard, Johan, Claeyssens, Adélaïde
We study the populations of stellar clumps in three high-redshift galaxies, at z=4.92, 4.88 and 4.03, gravitationally lensed by the foreground galaxy clusters MS1358, RCS0224 and MACS0940, respectively. The lensed galaxies consist of multiple counter
Externí odkaz:
http://arxiv.org/abs/2402.14920
Autor:
Adamo, Angela, Bradley, Larry D., Vanzella, Eros, Claeyssens, Adélaïde, Welch, Brian, Diego, Jose M, Mahler, Guillaume, Oguri, Masamune, Sharon, Keren, Abdurro'uf, Hsiao, Tiger Yu-Yang, Xu, Xinfeng, Messa, Matteo, Lassen, Augusto E., Zackrisson, Erik, Brammer, Gabriel, Coe, Dan, Kokorev, Vasily, Ricotti, Massimo, Zitrin, Adi, Fujimoto, Seiji, Inoue, Akio K., Resseguier, Tom, Rigby, Jane R., Jiménez-Teja, Yolanda, Windhorst, Rogier A., Hashimoto, Takuya, Tamura, Yoichi
The Cosmic Gems arc is among the brightest and highly magnified galaxies observed at redshift $z\sim10.2$. However, it is an intrinsically UV faint galaxy, in the range of those now thought to drive the reionization of the Universe. Hitherto the smal
Externí odkaz:
http://arxiv.org/abs/2401.03224
Autor:
Thai, Tran Thi, Tuan-Anh, Pham, Pello, Roser, Goovaerts, Ilias, Richard, Johan, Claeyssens, Adélaïde, Mahler, Guillaume, Lagattuta, David J., de la Vieuville, Geoffroy, Salvador-Solé, Eduard, Garel, Thibault, Bauer, Franz E., Jeanneau, Alexandre, Clément, Benjamin, Matthee, Jorryt
Publikováno v:
A&A 678, A139 (2023)
We present a study of the galaxy Lyman-alpha luminosity function (LF) using a sample of 17 lensing clusters observed by the MUSE/VLT. Magnification from strong gravitational lensing by clusters of galaxies and MUSE apabilities allow us to blindly det
Externí odkaz:
http://arxiv.org/abs/2308.08685
Autor:
Goovaerts, Ilias, Pello, Roser, Thai, Tran Thi, Tuan-Anh, Pham, Richard, Johan, Claeyssens, Adélaïde, Carinos, Emile, de la Vieuville, Geoffroy, Matthee, Jorryt
Publikováno v:
A&A 678, A174 (2023)
Faint galaxies are theorised to have played a major role in reionising the Universe. Their properties as well as the Lyman-{\alpha} emitter fraction, could provide useful insight into this epoch. We use four galaxy clusters from the Lensed Lyman-alph
Externí odkaz:
http://arxiv.org/abs/2307.15559
JWST observations of the strongly lensed galaxy The Sparkler have revealed a population of gravitationally bound globular cluster (GC) candidates. Different analyses have resulted in broadly similar ages but significantly different metallicities, que
Externí odkaz:
http://arxiv.org/abs/2306.11814
Autor:
Beauchesne, Benjamin, Clément, Benjamin, Hibon, Pascale, Limousin, Marceau, Eckert, Dominique, Kneib, Jean-Paul, Richard, Johan, Natarajan, Priyamvada, Jauzac, Mathilde, Montes, Mireia, Mahler, Guillaume, Claeyssens, Adélaïde, Jeanneau, Alexandre, Koekemoer, Anton M., Lagattuta, David, Pagul, Amanda, Sánchez, Javier
We present a new method to simultaneously/self-consistently model the mass distribution of galaxy clusters that combines constraints from strong lensing features, X-ray emission and galaxy kinematics measurements. We are able to successfully decompos
Externí odkaz:
http://arxiv.org/abs/2301.10907