Zobrazeno 1 - 10
of 110
pro vyhledávání: '"Hainline, L."'
Autor:
Hainline, L. J., Blain, A. W., Smail, I., Alexander, D. M., Armus, L., Chapman, S. C., Ivison, R. J.
We present a new study of the stellar mass in a sample of ~ 70 submillimeter-selected galaxies (SMGs) with accurate spectroscopic redshifts. We fit combinations of stellar population synthesis models and power laws to the galaxies' observed-frame opt
Externí odkaz:
http://arxiv.org/abs/1006.0238
Autor:
Casey, C. M., Chapman, S. C., Beswick, R. J., Biggs, A. D., Blain, A. W., Hainline, L. J., Ivison, R. J., Muxlow, T., Smail, I.
We identify eight z>1 radio sources undetected at 850um but robustly detected at 70um, confirming that they represent ultraluminous infrared galaxies (ULIRGs) with hotter dust temperatures (T_dust=52+-10 K) than Submillimetre Galaxies (SMGs) at simil
Externí odkaz:
http://arxiv.org/abs/0906.5346
Autor:
Sasaki, S. S., Taniguchi, Y., Scoville, N., Mobasher, B., Aussel, H., Sanders, D. B., Koekemoer, A., Ajiki, M., Komiyama, Y., Miyazaki, S., Kaifu, N., Karoji, H., Okamura, S., Arimoto, N., Ohta, K., Shioya, Y., Murayama, T., Nagao, T., Koda, J., Hainline, L., Renzini, A., Giavalisco, M., LeFevre, O., Impey, C., Elvis, M., Lilly, S., Rich, M., Schinnerer, E., Sheth, K.
We report on the discovery of a new potential galaxy threshing system in the COSMOS 2 square degree field using the prime-focus camera, Suprime-Cam, on the 8.2 m Subaru Telescope. This system consists of a giant elliptical galaxy with $M_V \approx -2
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612351
Publikováno v:
Astron.J.132:1938-1943,2006
We report deep K-band (18-27GHz) observations with the 100-m Green Bank Telescope of HCN(1-0) line emission towards the two submillimeter-selected galaxies (SMGs) SMMJ02399-0136 (z=2.81) and SMMJ16359+6612 (z=2.52). For both sources we have obtained
Externí odkaz:
http://arxiv.org/abs/astro-ph/0607365
Publikováno v:
Astrophys.J.650:614-623,2006
We report the first detection of CO(1-0) emission from a submillimeter-selected galaxy, using the Green Bank Telescope. We identify the line in the spectrum of SMM J13120+4242 as a broad emission feature at z=3.408, with Delta(V_FWHM)=1040 +/- 190 km
Externí odkaz:
http://arxiv.org/abs/astro-ph/0607089
Publikováno v:
Astrophys.J. 609 (2004) 61
Searches for CO emission in high-redshift objects have traditionally suffered from the accuracy of optically-derived redshifts due to lack of bandwidth in correlators at radio observatories. This problem has motivated the creation of the new COBRA co
Externí odkaz:
http://arxiv.org/abs/astro-ph/0403194
Autor:
HAINLINE, L. J.
Publikováno v:
Human Biology, 1965 May 01. 37(2), 174-177.
Externí odkaz:
https://www.jstor.org/stable/41448720
Publikováno v:
Europe PubMed Central
The Hirschberg ratio has been defined as the ratio of the change in angular position of the line of sight to the change in location of the first Purkinje image relative to the pupil center. This study was designed to determine empirically whether the
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