Zobrazeno 1 - 10
of 580
pro vyhledávání: '"Bèthermin, M."'
Autor:
Strandet, M. L., Weiss, A., Breuck, C. De, Marrone, D. P., Vieira, J. D., Aravena, M., Ashby, M. L. N., Béthermin, M., Bothwell, M. S., Bradford, C. M., Carlstrom, J. E., Chapman, S. C., Cunningham, D. J. M., Chen, Chian-Chou, Fassnacht, C. D., Gonzalez, A. H., Greve, T. R., Gullberg, B., Hayward, C. C., Hezaveh, Y., Litke, K., Ma, J., Malkan, M., Menten, K. M., Miller, T., Murphy, E. J., Narayanan, D., Phadke, K. A., Rotermund, K. M., Spilker, J. S., Sreevani, J.
We report the discovery and constrain the physical conditions of the interstellar medium of the highest-redshift millimeter-selected dusty star-forming galaxy to date, SPT-S J031132-5823.4 (hereafter SPT0311-58), at z = 6.900 +/- 0.002. SPT0311-58 wa
Externí odkaz:
http://hdl.handle.net/10150/627112
http://arizona.openrepository.com/arizona/handle/10150/627112
http://arizona.openrepository.com/arizona/handle/10150/627112
Autor:
Bothwell, M. S., Aguirre, J. E., Aravena, M., Bethermin, M., Bisbas, T. G., Chapman, S. C., De Breuck, C., Gonzalez, A. H., Greve, T. R., Hezaveh, Y., Ma, J., Malkan, M., Marrone, D. P., Murphy, E. J., Spilker, J. S., Strandet, M., Vieira, J. D., Weiß, A.
We present Atacama Large Millimeter Array [C-I](1 - 0) (rest frequency 492 GHz) observations for a sample of 13 strongly lensed dusty star-forming galaxies (DSFGs) originally discovered at 1.4 mm in a blank-field survey by the South Pole Telescope (S
Externí odkaz:
http://hdl.handle.net/10150/623935
http://arizona.openrepository.com/arizona/handle/10150/623935
http://arizona.openrepository.com/arizona/handle/10150/623935
Autor:
Ma, Jingzhe, Gonzalez, Anthony. H., Vieira, J. D., Aravena, M., Ashby, M. L. N., Béthermin, M., Bothwell, M. S., Brandt, W. N., Breuck, C. de, Carlstrom, J. E., Chapman, S. C., Gullberg, B., Hezaveh, Y., Litke, K., Malkan, M., Marrone, D. P., McDonald, M., Murphy, E. J., Spilker, J. S., Sreevani, J., Stark, A. A., Strandet, M., Wang, S. X.
We present Chandra ACIS-S and Australia Telescope Compact Array (ATCA) radio continuum observations of the strongly lensed dusty, star-forming galaxy SPT-S J034640-5204.9 (hereafter SPT0346-52) at z = 5.656. This galaxy has also been observed with AL
Externí odkaz:
http://hdl.handle.net/10150/622449
http://arizona.openrepository.com/arizona/handle/10150/622449
http://arizona.openrepository.com/arizona/handle/10150/622449
Autor:
Spilker, J. S., Marrone, D. P., Aravena, M., Béthermin, M., Bothwell, M. S., Carlstrom, J. E., Chapman, S. C., Crawford, T. M., Breuck, C. de, Fassnacht, C. D., Gonzalez, A. H., Greve, T. R., Hezaveh, Y., Litke, K., Ma, J., Malkan, M., Rotermund, K. M., Strandet, M., Vieira, J. D., Weiss, A., Welikala, N.
The South Pole Telescope has discovered 100 gravitationally lensed, high-redshift, dusty, star-forming galaxies (DSFGs). We present 0."5 resolution 870 mu m. Atacama Large Millimeter/submillimeter Array imaging of a sample of 47 DSFGs spanning z = 1.
Externí odkaz:
http://hdl.handle.net/10150/621394
http://arizona.openrepository.com/arizona/handle/10150/621394
http://arizona.openrepository.com/arizona/handle/10150/621394
Autor:
Strandet, M. L., Weiss, A., Vieira, J. D., de Breuck, C., Aguirre, J. E., Aravena, M., Ashby, M. L. N., Béthermin, M., Bradford, C. M., Carlstrom, J. E., Chapman, S. C., Crawford, T. M., Everett, W., Fassnacht, C. D., Furstenau, R. M., Gonzalez, A. H., Greve, T. R., Gullberg, B., Hezaveh, Y., Kamenetzky, J. R., Litke, K., Ma, J., Malkan, M., Marrone, D. P., Menten, K. M., Murphy, E. J., Nadolski, A., Rotermund, K. M., Spilker, J. S., Stark, A. A., Welikala, N.
We use the Atacama Large Millimeter/submillimeter Array (ALMA) in Cycle 1 to determine spectroscopic redshifts of high-redshift dusty star-forming galaxies (DSFGs) selected by their 1.4 mm continuum emission in the South Pole Telescope (SPT) survey.
Externí odkaz:
http://hdl.handle.net/10150/621235
http://arizona.openrepository.com/arizona/handle/10150/621235
http://arizona.openrepository.com/arizona/handle/10150/621235
Autor:
Ciesla, L., Adscheid, S., Magnelli, B., Boquien, M., Laporte, N., Bethermin, M., Carvajal, C., Schinnerer, E., Liu, D.
[Abridged] Our view of dust in primordial galaxies is limited towards a few tens of z~7 galaxies, pre-selected from UV-optical observations, and are thus not necessarily representative of the bulk of the sources at these redshifts. In this work, we a
Externí odkaz:
http://arxiv.org/abs/2412.02557
Autor:
Sawant, P., Nanni, A., Romano, M., Donevski, D., Bruzual, G., Ysard, N., Lemaux, B. C., Inami, H., Calura, F., Pozzi, F., Małek, K., Junais, Boquien, M., Faisst, A. L., Hamed, M., Ginolfi, M., Zamorani, G., Lorenzon, G., Molina, J., Bardelli, S., Ibar, E., Vergani, D., Di Cesare, C., Béthermin, M., Burgarella, D., Cassata, P., Dessauges-Zavadsky, M., D'Onghia, E., Dubois, Y., Magdis, G. E., Mendez-Hernandez, H.
Recent observations reveal a rapid dust build-up in high-redshift galaxies (z > 4), challenging current models of galaxy formation. While our understanding of dust production and destruction in the interstellar medium (ISM) is advancing, probing bary
Externí odkaz:
http://arxiv.org/abs/2412.02505
Autor:
Veraldi, E., Vallini, L., Pozzi, F., Esposito, F., Bethermin, M., Boquien, M., Faisst, A., Ginolfi, M., Gobat, R., Gruppioni, C., Hathi, N., Ibar, E., Molina, J., Rizzo, F., Romano, M., Zamorani, G.
In this work, we devise a model for estimating UV and optical line emission (i.e., CIII] $1909$A, H$\beta$, [OIII] $5007$A, H$\alpha$, [NII] $6583$A) tracing HII regions in the interstellar medium (ISM) of galaxies at $z\sim4-6$ from the ALMA Large P
Externí odkaz:
http://arxiv.org/abs/2411.08124
Autor:
Shuntov, M., Ilbert, O., Toft, S., Arango-Toro, R. C., Akins, H. B., Casey, C. M., Franco, M., Harish, S., Kartaltepe, J. S., Koekemoer, A. M., McCracken, H. J., Paquereau, L., Laigle, C., Bethermin, M., Dubois, Y., Drakos, N. E., Faisst, A., Gozaliasl, G., Gillman, S., Hayward, C. C., Hirschmann, M., Huertas-Company, M., Jespersen, C. K., Jin, S., Kokorev, V., Lambrides, E., Borgne, D. Le, Liu, D., Magdis, G., Massey, R., McPartland, C. J. R., Mercier, W., McCleary, J. E., McKinney, J., Oesch, P. A., Rhodes, J. D., Rich, R. M., Robertson, B. E., Sanders, D., Trebitsch, M., Tresse, L., Valentino, F., Vijayan, A. P., Weaver, J. R., Weibel, A., Wilkins, S. M.
We study the stellar mass function (SMF) and the co-evolution with dark matter halos via abundance matching in the largest redshift range to date $0.25$, we find increas
Externí odkaz:
http://arxiv.org/abs/2410.08290
Autor:
Arango-Toro, R. C., Ilbert, O., Ciesla, L., Shuntov, M., Aufort, G., Mercier, W., Laigle, C., Franco, M., Bethermin, M., Borgne, D. Le, Dubois, Y., McCracken, H. J., Paquereau, L., Huertas-Company, M., Kartaltepe, J., Casey, C. M., Akins, H., Allen, N., Andika, I., Brinch, M., Drakos, N. E., Faisst, A., Gozaliasl, G., Harish, S., Kaminsky, A., Koekemoer, A., Kokorev, V., Liu, D., Magdis, G., Martin, C. L., Moutard, T., Rhodes, J., Rich, R. M., Robertson, B., Sanders, D. B., Sheth, K., Talia, M., Toft, S., Tresse, L., Valentino, F., Vijayan, A., Weaver, J.
The stellar mass-star formation rate (M$_\star$ - SFR) plane is essential for distinguishing galaxy populations, but how galaxies move within this plane over cosmic time remains unclear. This study aims to describe galaxy migrations in the M$_\star$
Externí odkaz:
http://arxiv.org/abs/2410.05375