Zobrazeno 1 - 10
of 818
pro vyhledávání: '"Reddy, Naveen A"'
Autor:
Sanjaripour, Sogol, Hemmati, Shoubaneh, Mobasher, Bahram, Canalizo, Gabriela, Barish, Barry, Shivaei, Irene, Coil, Alison L., Chartab, Nima, Jafariyazani, Marziye, Reddy, Naveen A., Azadi, Mojegan
The growing volume of data produced by large astronomical surveys necessitates the development of efficient analysis techniques capable of effectively managing high-dimensional datasets. This study addresses this need by demonstrating some applicatio
Externí odkaz:
http://arxiv.org/abs/2410.07354
Autor:
Shapley, Alice E., Sanders, Ryan L., Topping, Michael W., Reddy, Naveen A., Pahl, Anthony J., Oesch, Pascal A., Berg, Danielle A., Bouwens, Rychard J., Brammer, Gabriel, Carnall, Adam C., Cullen, Fergus, Davé, Romeel, Dunlop, James S., Ellis, Richard S., Schreiber, N. M. Förster, Furlanetto, Steven R ., Glazebrook, Karl, Illingworth, Garth D., Jones, Tucker, Kriek, Mariska, McLeod, Derek J., McLure, Ross J., Narayanan, Desika, Pettini, Max, Schaerer, Daniel, Stark, Daniel P., Steidel, Charles C., Tang, Mengtao, Clarke, Leonardo, Donnan, Callum T., Kehoe, Emily
We present the properties of a massive, large, dusty, metal-rich, star-forming galaxy at z_spec=6.73. GOODSN-100182 was observed with JWST/NIRSpec as part of the AURORA survey, and is also covered by public multi-wavelength HST and JWST imaging. Whil
Externí odkaz:
http://arxiv.org/abs/2410.00110
Autor:
Lorenz, Brian, Kriek, Mariska, Shapley, Alice E., Sanders, Ryan L., Coil, Alison L., Leja, Joel, Mobasher, Bahram, Nelson, Erica, Price, Sedona H., Reddy, Naveen A., Runco, Jordan N., Suess, Katherine A., Shivaei, Irene, Siana, Brian, Weisz, Daniel R.
We examine star-formation and dust properties for a sample of 660 galaxies at $1.37\leq z\leq 2.61$ in the MOSDEF survey by dividing them into groups with similarly-shaped spectral energy distributions (SEDs). For each group, we combine the galaxy ph
Externí odkaz:
http://arxiv.org/abs/2409.18179
Autor:
Covelo-Paz, Alba, Giovinazzo, Emma, Oesch, Pascal A., Meyer, Romain A., Weibel, Andrea, Brammer, Gabriel, Fudamoto, Yoshinobu, Kerutt, Josephine, Lin, Jamie, Matharu, Jasleen, Naidu, Rohan P., Velichko, Anna, Bollo, Victoria, Bouwens, Rychard, Chisholm, John, Illingworth, Garth D., Kramarenko, Ivan, Magee, Daniel, Maseda, Michael, Matthee, Jorryt, Nelson, Erica, Reddy, Naveen, Schaerer, Daniel, Stefanon, Mauro, Xiao, Mengyuan
The H{\alpha} nebular emission line is an optimal tracer for recent star formation in galaxies. With the advent of JWST, this line has recently become observable at z>3 for the first time. We present a catalog of 1013 H{\alpha} emitters at 3.7
Externí odkaz:
http://arxiv.org/abs/2409.17241
Autor:
Sanders, Ryan L., Shapley, Alice E., Topping, Michael W., Reddy, Naveen A., Berg, Danielle A., Bouwens, Rychard J., Brammer, Gabriel, Carnall, Adam C., Cullen, Fergus, Davé, Romeel, Dunlop, James S., Ellis, Richard S., Schreiber, N. M. Förster, Furlanetto, Steven R., Glazebrook, Karl, Illingworth, Garth D., Jones, Tucker, Kriek, Mariska, McLeod, Derek J., McLure, Ross J., Narayanan, Desika, Oesch, Pascal A., Pahl, Anthony J., Pettini, Max, Schaerer, Daniel, Stark, Daniel P., Steidel, Charles C., Tang, Mengtao, Clarke, Leonardo, Donnan, Callum T., Kehoe, Emily
We use JWST/NIRSpec observations from the Assembly of Ultradeep Rest-optical Observations Revealing Astrophysics (AURORA) survey to constrain the shape of the nebular attenuation curve of a star-forming galaxy at z=4.41, GOODSN-17940. We utilize 11 u
Externí odkaz:
http://arxiv.org/abs/2408.05273
Autor:
Pahl, Anthony J., Topping, Michael W., Shapley, Alice, Sanders, Ryan, Reddy, Naveen A., Clarke, Leonardo, Kehoe, Emily, Bento, Trinity, Brammer, Gabe
We have used a combined sample of JADES and CEERS objects in order to constrain ionizing photon production efficiency ($\xi_{\rm ion}$) from JWST/NIRSpec and JWST/NIRCam data. We examine 163 objects at 1.06 < z < 6.71 with significant (3$\sigma$) spe
Externí odkaz:
http://arxiv.org/abs/2407.03399
Autor:
Shapley, Alice E., Sanders, Ryan L., Topping, Michael W., Reddy, Naveen A., Berg, Danielle A., Bouwens, Rychard J., Brammer, Gabriel, Carnall, Adam C., Cullen, Fergus, Davé, Romeel, Dunlop, James S., Ellis, Richard S., Schreiber, N. M. Förster, Furlanetto, Steven R ., Glazebrook, Karl, Illingworth, Garth D., Jones, Tucker, Kriek, Mariska, McLeod, Derek J., McLure, Ross J., Narayanan, Desika, Oesch, Pascal, Pahl, Anthony J., Pettini, Max, Schaerer, Daniel, Stark, Daniel P., Steidel, Charles C., Tang, Mengtao, Clarke, Leonardo, Donnan, Callum T., Kehoe, Emily
We present results on the emission-line properties of z=1.4-7.5 star-forming galaxies in the Assembly of Ultradeep Rest-optical Observations Revealing Astrophysics (AURORA) Cycle 1 JWST/NIRSpec program. Based on its depth, continuous wavelength cover
Externí odkaz:
http://arxiv.org/abs/2407.00157
Autor:
Kehoe, Emily, Shapley, Alice E., Schreiber, N. M Forster, Pahl, Anthony J., Topping, Michael W., Reddy, Naveen A., Genzel, Reinhard, Price, Sedona H., Tacconi, L. J.
We investigate the multi-phase structure of gas flows in galaxies. We study 80 galaxies during the epoch of peak star formation ($1.4\leq z\leq2.7$) using data from Keck/LRIS and VLT/KMOS. Our analysis provides a simultaneous probe of outflows using
Externí odkaz:
http://arxiv.org/abs/2406.07621
Autor:
Clarke, Leonardo, Shapley, Alice E., Sanders, Ryan L., Topping, Michael W., Brammer, Gabriel B., Bento, Trinity, Reddy, Naveen A., Kehoe, Emily
We have used public JWST/NIRSpec and JWST/NIRCam observations from the CEERS and JADES surveys in order to analyze the star-forming main sequence (SFMS) over the redshift range $1.4 \leq z < 7$. We calculate the star-formation rates (SFRs) of the gal
Externí odkaz:
http://arxiv.org/abs/2406.05178
Ly$\alpha$ Halo Properties and Dust in the Circumgalactic Medium of $z \sim 2$ Star-forming Galaxies
Autor:
Song, Zhiyuan, Reddy, Naveen A., Chen, Yuguang, Shapley, Alice E., Rezaee, Saeed, Weldon, Andrew, Fetherolf, Tara, Coil, Alison L., Mobasher, Bahram, Steidel, Charles C.
We present Keck Cosmic Web Imager IFU observations around extended Ly$\alpha$ halos of 27 typical star-forming galaxies with redshifts $2.0 < z < 3.2$ drawn from the MOSFIRE Deep Evolution Field survey. We examine the average Ly$\alpha$ surface-brigh
Externí odkaz:
http://arxiv.org/abs/2405.13122