Zobrazeno 1 - 10
of 677
pro vyhledávání: '"Frayer, D."'
Autor:
Michałowski, Michał J., Gall, C., Hjorth, J., Frayer, D. T., Tsai, A. -L., Rowlands, K., Takeuchi, T. T., Leśniewska, A., Behrendt, D., Bourne, N., Hughes, D. H., Koprowski, M. P., Nadolny, J., Ryzhov, O., Solar, M., Spring, E., Zavala, J., Bartczak, P.
Publikováno v:
2024, ApJ, 964, 129
Understanding how galaxies quench their star formation is crucial for studies of galaxy evolution. Quenching is related to the cold gas decrease. In the first paper we showed that the dust removal timescale in early-type galaxies (ETGs) is about 2.5
Externí odkaz:
http://arxiv.org/abs/2401.04774
Autor:
Su, T., Marriage, T. A., Asboth, V., Baker, A. J., Bond, J. R., Crichton, D., Devlin, M. J., Dünner, R., Farrah, D., Frayer, D. T., Gralla, M. B., Hall, K., Halpern, M., Harris, A. I., Hilton, M., Hincks, A. D., Hughes, J. P., Niemack, M. D., Page, L. A., Partridge, B., Rivera, J., Scott, D., Sievers, J. L., Thornton, R. J., Viero, M. P., Wang, L., Wollack, E. J., Zemcov, M.
We present multi-wavelength detections of nine candidate gravitationally lensed dusty starforming galaxies (DSFGs) selected at 218 GHz (1.4 mm) from the Atacama Cosmology Telescope (ACT) equatorial survey. Among the brightest ACT sources, these repre
Externí odkaz:
http://hdl.handle.net/10150/623115
http://arizona.openrepository.com/arizona/handle/10150/623115
http://arizona.openrepository.com/arizona/handle/10150/623115
Autor:
White, E., Ghigo, F. D., Prestage, R. M., Frayer, D. T., Maddalena, R. J., Wallace, P. T., Brandt, J. J., Egan, D., Nelson, J. D., Ray, J.
Publikováno v:
A&A 659, A113 (2022)
With a 100mx110m off-axis paraboloid dish, the Green Bank Telescope (GBT) is the largest fully steerable radio telescope on Earth. A major challenge facing large ground-based radio telescopes is achieving sufficient pointing accuracy for observing at
Externí odkaz:
http://arxiv.org/abs/2111.12636
Autor:
Vidal-García, A., Falgarone, E., Battaia, F. Arrigoni, Godard, B., Ivison, R. J., Zwaan, M. A., Herrera, C., Frayer, D., Andreani, P., Li, Q., Gavazzi, R.
We present a comparative analysis of the $\rm CH^+$(1-0) and $\rm Ly \alpha$ lines, observed with the Atacama Large Millimeter Array (ALMA) and Keck telescope respectively, in the field of the submillimetre-selected galaxy (SMG) SMM\,J02399$-$0136 at
Externí odkaz:
http://arxiv.org/abs/2105.10202
Autor:
Harrington, Kevin C., Weiss, Axel, Yun, Min S., Magnelli, Benjamin, Sharon, C. E., Leung, T. K. D., Vishwas, A., Wang, Q. D., Jimenez-Andrade, E. F., Frayer, D. T., Liu, D., Garcia, P., Romano-Diaz, E., Frye, B. L., Jarugula, S., Badescu, T., Berman, D., Dannerbauer, H., Diaz-Sanchez, A., Grassitelli, L., Kamieneski, P., Kim, W. J., Kirkpatrick, A., Lowenthal, J. D., Messias, H., Puschnig, J., Stacey, G. J., Torne, P., Bertoldi, F.
Dusty star-forming galaxies at high redshift (1 < z < 3) represent the most intense star-forming regions in the Universe. Key aspects to these processes are the gas heating and cooling mechanisms. Although it is well known that these galaxies are gas
Externí odkaz:
http://arxiv.org/abs/2010.16231
Autor:
Bakx, T. J. L. C., Dannerbauer, H., Frayer, D., Eales, S. A., Pérez-Fournon, I., Cai, Z. -Y., Clements, D. L., De Zotti, G., González-Nuevo, J., Ivison, R. J., Lapi, A., Michałowski, M. J., Negrello, M., Serjeant, S., Smith, M. W. L., Temi, P., Urquhart, S., van der Werf, P.
Using the EMIR instrument on the IRAM 30m telescope, we conducted a spectroscopic redshift search of seven z$_{\rm phot}$ $\sim$ 4 sub-millimetre bright galaxies selected from the Herschel Bright Sources (HerBS) sample with fluxes at 500 $\mu$m great
Externí odkaz:
http://arxiv.org/abs/2006.05992
Autor:
Michałowski, Michał J., Hjorth, J., Gall, C., Frayer, D. T., Tsai, A. -L., Hirashita, H., Rowlands, K., Takeuchi, T. T., Leśniewska, A., Behrendt, D., Bourne, N., Hughes, D. H., Spring, E., Zavala, J., Bartczak, P.
Publikováno v:
A&A 632, A43 (2019)
An important aspect of quenching star formation is the removal of the cold interstellar medium (ISM; non-ionised gas and dust) from a galaxy. In addition, dust grains can be destroyed in a hot or turbulent medium. The adopted timescale of dust remova
Externí odkaz:
http://arxiv.org/abs/1910.06327
Autor:
Herrero-Illana, R., Privon, G. C., Evans, A. S., Díaz-Santos, T., Pérez-Torres, M. Á., U, V., Alberdi, A., Iwasawa, K., Armus, L., Aalto, S., Mazzarella, J., Chu, J., Sanders, D. B., Barcos-Muñoz, L., Charmandaris, V., Linden, S. T., Yoon, I., Frayer, D. T., Inami, H., Kim, D. -C., Borish, H. J., Conway, J., Murphy, E. J, Song, Y., Stierwalt, S., Surace, J.
Publikováno v:
A&A 628, A71 (2019)
We present IRAM-30m Telescope $^{12}$CO and $^{13}$CO observations of a sample of 55 luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) in the local universe. This sample is a subset of the Great Observatory All-Sky LIRG Survey (GOALS),
Externí odkaz:
http://arxiv.org/abs/1907.03854
Autor:
Harrington, K. C., Vishwas, A., Weiss, A., Magnelli, B., Grassitelli, L., Zajacek, M., Jimenez-Andrade, E. F., Leung, T. K. D., Bertoldi, F., Romano-Diaz, E., Frayer, D. T., Kamieneski, P., Riechers, D., Stacey, G. J., Yun, M. S., Wang, Q. D.
We report the detection of the far-infrared (FIR) fine-structure line of singly ionised nitrogen, \Nplusa, within the peak epoch of galaxy assembly, from a strongly lensed galaxy, hereafter ``The Red Radio Ring''; the RRR, at z = 2.55. We combine new
Externí odkaz:
http://arxiv.org/abs/1906.09656
High-redshift ($z$) proto-clusters will serve as testing grounds to probe the gas supply furnishing the emerging metals, stars, and large-scale structures we see at the current epoch. This work focuses on the major role large radio/millimeter (mm) si
Externí odkaz:
http://arxiv.org/abs/1903.11345