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Full-Text Articles in Physical Sciences and Mathematics
Deep 1.1 Mm-Wavelength Imaging Of The Goods-S Field By Aztec/Aste – I. Source Catalogue And Number Counts, Thushara Perera, K. Scott, M. Yun, G. Wilson, J. Austermann, E. Aguilar, I. Aretxaga, H. Ezawa, D. Ferrusca, B. Hatsukade, D. Hughes, D. Iono, M. Giavalisco, R. Kawabe, K. Khono, P. Mauskopf, T. Oshima, J. Rand, Y. Tamura, T. Tosaki, M. Velazquez, C. Williams, M. Zeballos
Deep 1.1 Mm-Wavelength Imaging Of The Goods-S Field By Aztec/Aste – I. Source Catalogue And Number Counts, Thushara Perera, K. Scott, M. Yun, G. Wilson, J. Austermann, E. Aguilar, I. Aretxaga, H. Ezawa, D. Ferrusca, B. Hatsukade, D. Hughes, D. Iono, M. Giavalisco, R. Kawabe, K. Khono, P. Mauskopf, T. Oshima, J. Rand, Y. Tamura, T. Tosaki, M. Velazquez, C. Williams, M. Zeballos
Thushara A. Perera
No abstract provided.
Origins Of The Extragalactic Background At 1mm From A Combined Analysis Of The Aztec And Mambo Data In Goods-N, Kyle Penner, Alexandra Pope, Edward L. Chapin, Thomas R. Greve, Frank Bertoldi, Mark Brodwin, Ranga-Ram Chary, Christopher J, Conselice, Kristen Coppin, Mauro Giavalisco, David H. Hughes, Rob J. Ivison, Thushara Perera, Douglas Scott, Kimberly Scott, Grant Wilson
Origins Of The Extragalactic Background At 1mm From A Combined Analysis Of The Aztec And Mambo Data In Goods-N, Kyle Penner, Alexandra Pope, Edward L. Chapin, Thomas R. Greve, Frank Bertoldi, Mark Brodwin, Ranga-Ram Chary, Christopher J, Conselice, Kristen Coppin, Mauro Giavalisco, David H. Hughes, Rob J. Ivison, Thushara Perera, Douglas Scott, Kimberly Scott, Grant Wilson
Thushara A. Perera
We present a study of the cosmic infrared background, which is a measure of the dust obscured activity in all galaxies in the Universe. We venture to isolate the galaxies responsible for the background at 1mm; with spectroscopic and photometric redshifts we constrain the redshift distribution of these galaxies. We create a deep 1.16mm map (sigma ~ 0.5mJy) by combining the AzTEC 1.1mm and MAMBO 1.2mm datasets in GOODS-N. This combined map contains 41 secure detections, 13 of which are new. By averaging the 1.16mm flux densities of individually undetected galaxies with 24um flux densities > 25uJy, we resolve 31--45 per …