Zobrazeno 1 - 10
of 13 917
pro vyhledávání: '"Edward, N."'
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
Autor:
D'Eugenio, Francesco, Colless, Matthew, van der Wel, Arjen, Vaughan, Sam P., Said, Khaled, van de Sande, Jesse, Bland-Hawthorn, Joss, Bryant, Julia J., Croom, Scott M., Lopez-Sanchez, Angel R., Lorente, Nuria P. F., Maiolino, Roberto, Taylor, Edward N.
We use deep spectroscopy from the SAMI Galaxy Survey to explore the precision of the fundamental plane of early-type galaxies (FP) as a distance indicator for future single-fibre spectroscopy surveys. We study the optimal trade-off between sample siz
Externí odkaz:
http://arxiv.org/abs/2406.17842
Autor:
Mun, Marcie, Wisnioski, Emily, Battisti, Andrew J., Mendel, J. Trevor, Ellison, Sara L., Taylor, Edward N., Lagos, Claudia D. P., Harborne, Katherine E., Foster, Caroline, Croom, Scott M., Bellstedt, Sabine, Barsanti, Stefania, Gupta, Anshu, Valenzuela, Lucas M., Chen, Qian-Hui, Grasha, Kathryn, Mukherjee, Tamal, Park, Hye-Jin, Sharda, Piyush, Sweet, Sarah M., Remus, Rhea-Silvia, Zafar, Tayyaba
Using adaptive optics with the Multi-Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope (VLT), the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey allows us to study the spatially resolved Universe at a cruci
Externí odkaz:
http://arxiv.org/abs/2404.16319
Autor:
Ward, Edward N., McClelland, Rebecca M., Lamb, Jacob R., Rubio-Sánchez, Roger, Christensen, Charles N., Mazumder, Bismoy, Kapsiani, Sofia, Mascheroni, Luca, Di Michele, Lorenzo, Schierle, Gabriele S. Kaminski, Kaminski, Clemens F.
Structured illumination can reject out-of-focus signal from a sample, enabling high-speed and high-contrast imaging over large areas with widefield detection optics. Currently, this optical-sectioning technique is limited by image reconstruction arte
Externí odkaz:
http://arxiv.org/abs/2311.00089
Autor:
Wang, Bingjie, Leja, Joel, Labbé, Ivo, Bezanson, Rachel, Whitaker, Katherine E., Brammer, Gabriel, Furtak, Lukas J., Weaver, John R., Price, Sedona H., Zitrin, Adi, Atek, Hakim, Coe, Dan, Cutler, Sam E., Dayal, Pratika, van Dokkum, Pieter, Feldmann, Robert, Marchesini, Danilo, Franx, Marijn, Schreiber, Natascha Förster, Fujimoto, Seiji, Geha, Marla, Glazebrook, Karl, de Graaff, Anna, Greene, Jenny E., Juneau, Stéphanie, Kassin, Susan, Kriek, Mariska, Khullar, Gourav, Maseda, Michael, Mowla, Lamiya A., Muzzin, Adam, Nanayakkara, Themiya, Nelson, Erica J., Oesch, Pascal A., Pacifici, Camilla, Pan, Richard, Papovich, Casey, Setton, David J., Shapley, Alice E., Smit, Renske, Stefanon, Mauro, Suess, Katherine A., Taylor, Edward N., Williams, Christina C.
Publikováno v:
The Astrophysical Journal Supplement Series, 270, 12 (2024)
The recent UNCOVER survey with the James Webb Space Telescope (JWST) exploits the nearby cluster Abell 2744 to create the deepest view of our universe to date by leveraging strong gravitational lensing. In this work, we perform photometric fitting of
Externí odkaz:
http://arxiv.org/abs/2310.01276
Autor:
Dogruel, M. Burak, Taylor, Edward N., Cluver, Michelle, D'Eugenio, Francesco, de Graaff, Anna, Colless, Matthew, Sonnenfeld, Alessandro
In this empirical work, we aim to quantify the systematic uncertainties in stellar mass $(M_\star)$ estimates made from spectral energy distribution (SED) fitting through stellar population synthesis (SPS), for galaxies in the local Universe, by usin
Externí odkaz:
http://arxiv.org/abs/2306.10693