Zobrazeno 1 - 10
of 29
pro vyhledávání: '"Bout, P. Vanden"'
Autor:
Scoville, Nick, Faisst, Andreas, Weaver, John, Toft, Sune, McCracken, Henry, Ilbert, Olivier, Diaz-Santos, Tanio, Staguhn, Johannes, Koda, Jin, Casey, Caitlin, Sanders, David, Mobasher, Bahram, Chartab, Nima, Sattari, Zahra, Capak, Peter, Bout, Paul Vanden, Bongiorno, Angela, Vlahakis, Catherine, Sheth, Kartik, Yun, Min, Aussel, Herve, Laigle, Clotilde, Masters, Dan
ALMA observations of the long wavelength dust continuum are used to estimate the gas masses in a sample of 708 star-forming (SF) galaxies at z = 0.3 to 4.5. We determine the dependence of gas masses and star formation efficiencies (SFE=SFR per unit g
Externí odkaz:
http://arxiv.org/abs/2211.07836
Autor:
Frayer, David T., Maddalena, Ronald J., Ivison, R. J., Smail, Ian, Blain, Andrew W., Bout, Paul Vanden
We present CO(1-0), CO(3-2), and CO(7-6) observations using the Green Bank Telescope (GBT) and the Atacama Large Millimeter Array (ALMA) of the z=2.8 sub-millimeter galaxy SMM J02399-0136. This was the first submillimeter-selected galaxy discovered a
Externí odkaz:
http://arxiv.org/abs/1805.07212
Autor:
Scoville, N., Lee, N., Bout, P. Vanden, Diaz-Santos, T., Sanders, D., Darvish, B., Bongiorno, A., Casey, C. M., Murchikova, L., Koda, J., Capak, P., Vlahakis, Catherine, Ilbert, O., Sheth, K., Morokuma-Matsui, K., Ivison, R. J., Aussel, H., Laigle, C., McCracken, H. J., Armus, L., Pope, A., Toft, S., Masters, D.
ALMA observations of the long wavelength dust continuum are used to estimate the interstellar medium (ISM) masses in a sample of 708 galaxies at z = 0.3 to 4.5 in the COSMOS field. The galaxy sample has known far-infrared luminosities and, hence, sta
Externí odkaz:
http://arxiv.org/abs/1702.04729
Autor:
Scoville, Nick, Murchikova, Lena, Walter, Fabian, Vlahakis, Catherine, Koda, Jin, Bout, Paul Vanden, Barnes, Joshua, Hernquist, Lars, Sheth, Kartik, Yun, Min, Sanders, David, Armus, Lee, Cox, Pierre, Thompson, Todd, Robertson, Brant, Zschaechner, Laura, Tacconi, Linda, Torrey, Paul, Hayward, Christopher C., Genzel, Reinhard, Hopkins, Phil, van der Werf, Paul, Decarli, Roberto
We present 90 mas (37 pc) resolution ALMA imaging of Arp 220 in the CO (1-0) line and continuum at $\lambda = 2.6$ mm. The internal gas distribution and kinematics of both galactic nuclei are well-resolved for the first time. In the West nucleus, the
Externí odkaz:
http://arxiv.org/abs/1605.09381
Autor:
Scoville, N., Sheth, K., Aussel, H., Bout, P. Vanden, Capak, P., Bongiorno, A., Casey, C. M., Murchikova, L., Koda, J., 'Alvarez-M'arquez, J., Lee, N., Laigle, C., McCracken, H. J., Ilbert, O., Pope, A., Sanders, D., Chu, J., Toft, S., Ivison, R. J., Manohar, S.
Publikováno v:
2016ApJ,820,83
ALMA Cycle 2 observations of the long wavelength dust emission in 145 star-forming galaxies are used to probe the evolution of star-forming ISM. We also develop the physical basis and empirical calibration (with 72 low-z and z ~ 2 galaxies) for using
Externí odkaz:
http://arxiv.org/abs/1511.05149
Autor:
Thiessen, Alexander, Vogelsang, Jan, Adachi, Takuji, Steiner, Florian, Bout, David Vanden, Lupton, John M.
The spectral breadth of conjugated polymers gives these materials a clear advantage over other molecular compounds for organic photovoltaic applications and is a key factor in recent efficiencies topping 10%. But why do excitonic transitions, which a
Externí odkaz:
http://arxiv.org/abs/1507.06531
Autor:
Scoville, N., Sheth, K., Aussel, H., Bout, P. Vanden, Capak, P., Bongiorno, A., Casey, C. M., Murchikova, L., Koda, J., Pope, A., Toft, S., Ivison, R., Sanders, D., Manohar, S., Lee, N.
ALMA Cycle 2 observations of the long wavelength dust emission in 180 star-forming (SF) galaxies are used to investigate the evolution of ISM masses at z = 1 to 6.4. The ISM masses exhibit strong increases from z = 0 to $\rm $ = 1.15 and further t
Externí odkaz:
http://arxiv.org/abs/1505.02159
Autor:
Scoville, N., Aussel, H., Sheth, K., Scott, K. S., Sanders, D., Ivison, R., Pope, A., Capak, P., Bout, P. Vanden, Manohar, S., Kartaltepe, J., Lilly, S.
Publikováno v:
2014, ApJ, 783, 84
The use of submm dust continuum emission to probe the mass of interstellar dust and gas in galaxies is empirically calibrated using samples of local star forming galaxies, Planck observations of the Milky Way and high redshift submm galaxies (SMGs).
Externí odkaz:
http://arxiv.org/abs/1401.2987
Publikováno v:
Astrophys.J.707:988-999,2009
We report observations of 15 high redshift (z = 1-5) galaxies at 350 microns using the Caltech Submillimeter Observatory and SHARC-II array detector. Emission was detected from eight galaxies, for which far-infrared luminosities, star formation rates
Externí odkaz:
http://arxiv.org/abs/0910.5267
Autor:
Guelin, M., Salome, P., Neri, R., Garcia-Burillo, S., Gracia-Carpio, J., Cernicharo, J., Cox, P., Planesas, P., Solomon, P. M., Tacconi, L. J., Bout, P. Vanden
Molecular line emission from high-redshift galaxies holds great promise for the study of galaxy formation and evolution. The weak signals can only be detected with the largest mm-wave telescopes, such as the IRAM interferometer. We report the detecti
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612345