Zobrazeno 1 - 10
of 161
pro vyhledávání: '"Kocevski, D. D."'
Autor:
Yang, G., Caputi, K. I., Papovich, C., Haro, P. Arrabal, Bagley, M. B., Behroozi, P., Bell, E. F., Bisigello, L., Buat, V., Burgarella, D., Cheng, Y., Cleri, N. J., Dave, R., Dickinson, M., Elbaz, D., Ferguson, H. C., Finkelstein, S. L., Grogin, N. A., Hathi, N. P., Hirschmann, M., Holwerda, B. W., Huertas-Company, M., Hutchison, T., Iani, E., Kartaltepe, J. S., Kirkpatrick, A., Kocevski, D. D., Koekemoer, A. M., Kokorev, V., Larson, R. L., Lucas, R. A., Perez-Gonzalez, P. G., Rinaldi, P., Shen, L., Trump, J. R., de la Vega, A., Yung, L. Y. A., Zavala, J. A.
Mid-infrared observations are powerful in identifying heavily obscured Active Galactic Nuclei (AGN) which have weak emission in other wavelengths. Data from the Mid-Infrared Instrument (MIRI) onboard JWST provides an excellent opportunity to perform
Externí odkaz:
http://arxiv.org/abs/2303.11736
Autor:
Grazian, A., Giallongo, E., Paris, D., Boutsia, K., Dickinson, M., Santini, P., Windhorst, R. A., Jansen, R. A., Cohen, S. H., Ashcraft, T. A., Scarlata, C., Rutkowski, M. J., Vanzella, E., Cusano, F., Cristiani, S., Giavalisco, M., Ferguson, H. C., Koekemoer, A., Grogin, N. A., Castellano, M., Fiore, F., Fontana, A., Marchi, F., Pedichini, F., Pentericci, L., Amorín, R., Barro, G., Bonchi, A., Bongiorno, A., Faber, S. M., Fumana, M., Galametz, A., Guaita, L., Kocevski, D. D., Merlin, E., Nonino, M., O’Connell, R. W., Pilo, S., Ryan, R. E., Sani, E., Speziali, R., Testa, V., Weiner, B., Yan, H.
Context. The reionization of the Universe is one of the most important topics of present-day astrophysical research. The most plausible candidates for the reionization process are star-forming galaxies, which according to the predictions of the major
Externí odkaz:
http://hdl.handle.net/10150/625832
http://arizona.openrepository.com/arizona/handle/10150/625832
http://arizona.openrepository.com/arizona/handle/10150/625832
Autor:
Hung, D., Lemaux, B. C., Gal, R. R., Tomczak, A. R., Lubin, L. M., Cucciati, O., Pelliccia, D., Shen, L., Fèvre, O. Le, Zamorani, G., Wu, P-F., Kocevski, D. D., Fassnacht, C. D., Squires, G. K.
We present a new mass function of galaxy clusters and groups using optical/near-infrared wavelength spectroscopic and photometric data from the Observations of Redshift Evolution in Large-Scale Environments (ORELSE) survey. At $z\sim1$, cluster mass
Externí odkaz:
http://arxiv.org/abs/2101.02215
Autor:
Hung, D., Lemaux, B. C., Gal, R. R., Tomczak, A. R., Lubin, L. M., Cucciati, O., Pelliccia, D., Shen, L., Fèvre, O. Le, Wu, P-F., Kocevski, D. D., Mei, S., Squires, G. K.
The Observations of Redshift Evolution in Large Scale Environments (ORELSE) survey is an ongoing imaging and spectroscopic campaign initially designed to study the effects of environment on galaxy evolution in high-redshift ($z\sim1$) large-scale str
Externí odkaz:
http://arxiv.org/abs/1905.09298
Autor:
Rumbaugh, N., Lemaux, B. C., Tomczak, A. R., Shen, L., Pelliccia, D., Lubin, L. M., Kocevski, D. D., Wu, P. -F., Gal, R. R., Mei, S., Fassnacht, C. D., Squires, G. K.
We evaluated the effectiveness of different indicators of cluster virialization using 12 large-scale structures in the ORELSE survey spanning from $0.7
Externí odkaz:
http://arxiv.org/abs/1805.00488
Autor:
Masini, A., Civano, F., Comastri, A., Fornasini, F., Ballantyne, D. R., Lansbury, G. B., Treister, E., Alexander, D. M., Boorman, P. G., Brandt, W. N., Farrah, D., Gandhi, P., Harrison, F. A., Hickox, R. C., Kocevski, D. D., Lanz, L., Marchesi, S., Puccetti, S., Ricci, C., Saez, C., Stern, D., Zappacosta, L.
We present the results and the source catalog of the NuSTAR survey in the UKIDSS Ultra Deep Survey (UDS) field, bridging the gap in depth and area between NuSTAR's ECDFS and COSMOS surveys. The survey covers a $\sim 0.6$ deg$^2$ area of the field for
Externí odkaz:
http://arxiv.org/abs/1801.01881
Autor:
Barro, G., Kriek, M., Perez-Gonzalez, P. G., Diaz-Santos, T., Price, S. H., Rujopakarn, W., Pandya, V., Koo, D. C., Faber, S. M., Dekel, A., Primack, J. R., Kocevski, D. D.
We present high spatial resolution (FWHM$\sim$0.14'') observations of the CO($8-7$) line in GDS-14876, a compact star-forming galaxy at $z=2.3$ with total stellar mass of $\log(M_{\star}/M_{\odot})=10.9$. The spatially resolved velocity map of the in
Externí odkaz:
http://arxiv.org/abs/1712.01283
Autor:
Grazian, A., Giallongo, E., Paris, D., Boutsia, K., Dickinson, M., Santini, P., Windhorst, R. A., Jansen, R. A., Cohen, S. H., Ashcraft, T. A., Scarlata, C., Rutkowski, M. J., Vanzella, E., Cusano, F., Cristiani, S., Giavalisco, M., Ferguson, H. C., Koekemoer, A., Grogin, N. A., Castellano, M., Fiore, F., Fontana, A., Marchi, F., Pedichini, F., Pentericci, L., Amorin, R., Barro, G., Bonchi, A., Bongiorno, A., Faber, S. M., Fumana, M., Galametz, A., Guaita, L., Kocevski, D. D., Merlin, E., Nonino, M., O'Connell, R. W., Pilo, S., Ryan, R. E., Sani, E., Speziali, R., Testa, V., Weiner, B., Yan, H.
Publikováno v:
A&A 602, A18 (2017)
The reionization of the Universe is one of the most important topics of present day astrophysical research. The most plausible candidates for the reionization process are star-forming galaxies, which according to the predictions of the majority of th
Externí odkaz:
http://arxiv.org/abs/1703.00354
Autor:
Barro, G., Kriek, M., Pérez-González, P. G., Trump, J. R., Koo, D. C., Faber, S. M., Dekel, A., Primack, J. R., Guo, Y., Kocevski, D. D., Muñoz-Mateos, J. C., Rujoparkarn, W., Sheth, K.
We present spatially-resolved Atacama Large Millimeter/sub-millimeter Array (ALMA) 870 $\mu$m dust continuum maps of six massive, compact, dusty star-forming galaxies (SFGs) at $z\sim2.5$. These galaxies are selected for their small rest-frame optica
Externí odkaz:
http://arxiv.org/abs/1607.01011
Autor:
Huertas-Company, M., Bernardi, M., Pérez-González, P. G., Ashby, M. L. N., Barro, G., Conselice, C., Daddi, E., Dekel, A., Dimauro, P., Faber, S. M., Grogin, N. A., Kartaltepe, J. S., Kocevski, D. D., Koekemoer, A. M., Koo, D. C., Mei, S., Shankar, F.
[abridged] We quantify the evolution of the stellar mass functions of star-forming and quiescent galaxies as a function of morphology from $z\sim 3$ to the present. Our sample consists of ~50,000 galaxies in the CANDELS fields ($\sim880$ $arcmin^2$),
Externí odkaz:
http://arxiv.org/abs/1606.04952