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Autor:
Ming SWY, Haughney J, Ryan D, Small I, Lavorini F, Papi A, Singh D, Halpin DMG, Hurst JR, Patel S, Ochel M, Kocks J, Carter V, Hardjojo A, Price DB
Publikováno v:
International Journal of COPD, Vol Volume 15, Pp 3093-3103 (2020)
Simon Wan Yau Ming,1 John Haughney,2 Dermot Ryan,3 Iain Small,4 Federico Lavorini,5 Alberto Papi,6 Dave Singh,7 David MG Halpin,8 John R Hurst,9 Shishir Patel,10 Matthias Ochel,10 Janwillem Kocks,1,11,12 Victoria Carter,1 Antony Hardjojo,1 David B Pr
Externí odkaz:
https://doaj.org/article/7e2c9cdcdb4a4751aa5c98be1aff229e
Autor:
Project, The Supernova Cosmology, Kim, A. G., Gabi, S., Goldhaber, G., Groom, D. E., Hook, I. M., Kim, M. Y., Lee, J. C., Pennypacker, C. R., Perlmutter, S., Small, I. A., Goobar, A., Pain, R., Ellis, R. S., McMahon, R. G., Boyle, B. J., Bunclark, P. S., Carter, D., Irwin, M. J., Glazebrook, K., Newberg, H. J. M., Filippenko, A. V., Matheson, T., Dopita, M., Couch, W. J.
Publikováno v:
Astrophys.J.476:L63,1997
The Supernova Cosmology Project has discovered over twenty-eight supernovae (SNe) at 0.35
Externí odkaz:
http://arxiv.org/abs/astro-ph/9701188
Autor:
Perlmutter, S., Gabi, S., Goldhaber, G., Groom, D. E., Hook, I. M., Kim, A. G., Kim, M. Y., Lee, J. C., Pennypacker, C. R., Small, I. A., Goobar, A., Pain, R., Ellis, R. S., McMahon, R. G., Boyle, B. J., Bunclark, P. S., Carter, D., Irwin, M. J., Glazebrook, K., Newberg, H. J. M., Filippenko, A. V., Matheson, T., Dopita, M., Couch, W. J.
Publikováno v:
Astrophys.J.483:565,1997
We have developed a technique to systematically discover and study high-redshift supernovae that can be used to measure the cosmological parameters. We report here results based on the initial seven of >28 supernovae discovered to date in the high-re
Externí odkaz:
http://arxiv.org/abs/astro-ph/9608192
Autor:
Pain, R., Hook, I. M., Deustua, S., Gabi, S., Goldhaber, G., Goobar, A., Groom, D., Kim, A. G., Kim, M. Y., Lee, J. C., Pennypacker, C. R., Perlmutter, S., Small, I. A., Ellis, R. S., McMahon, R. G., Glazebrook, K., Boyle, B. J., Bunclark, P. S., Carter, D., Irwin, M. J.
Publikováno v:
Astrophys.J.473:356,1996
We present the first measurement of the rate of Type Ia supernovae at high redshift. The result is derived using a large subset of data from the Supernova Cosmology Project. Three supernovae were discovered in a surveyed area of 1.7 square degrees. T
Externí odkaz:
http://arxiv.org/abs/astro-ph/9607034
Autor:
Perlmutter, S., Deustua, S., Gabi, S., Goldhaber, G., Groom, D., Hook, I., Kim, A., Kim, M., Lee, J., Pain, R., Pennypacker, C., Small, I., Goobar, A., Ellis, R., Glazebrook, K., McMahon, R., Boyle, B., Bunclark, P., Carter, D., Irwin, M., Newberg, H., Filippenko, A. V., Matheson, T., Dopita, M., Mould, J., Couch, W.
Our search for high-redshift Type Ia supernovae discovered, in its first years, a sample of seven supernovae. Using a "batch" search strategy, almost all were discovered before maximum light and were observed over the peak of their light curves. The
Externí odkaz:
http://arxiv.org/abs/astro-ph/9602122
Autor:
Kim, A., Deustua, S., Gabi, S., Goldhaber, G., Groom, D., Hook, I., Kim, M., Lee, J., Pain, R., Pennypacker, C., Perlmutter, S., Small, I., Goobar, A., Ellis, R., Glazebrook, K., McMahon, R., Boyle, B., Bunclark, P., Carter, D., Irwin, M., Newberg, H., Filippenko, A. V., Matheson, T., Dopita, M., Mould, J., Couch, W.
Cross-filter K corrections for a sample of "normal" Type Ia supernovae (SNe) have been calculated for a range of epochs. With appropriate filter choices, the combined statistical and systematic K correction dispersion of the full sample lies within 0
Externí odkaz:
http://arxiv.org/abs/astro-ph/9602123
Autor:
Pain, R., Hook, I., Perlmutter, S., Deustua, S., Gabi, S., Goldhaber, G., Groom, D., Kim, A., Kim, M., Lee, J., Pennypacker, C., Small, I., Goobar, A., Ellis, R., Glazebrook, K., McMahon, R., Boyle, B., Bunclark, P., Carter, D., Irwin, M., Newberg, H., Filippenko, A. V., Matheson, T., Dopita, M., Mould, J., Couch, W.
We present the first measurement of the rate of Type Ia supernovae at high redshift. The result is derived using a large subset of data from the Supernova Cosmology Project as described in more detail at this meeting by Perlmutter et al. (1996). We p
Externí odkaz:
http://arxiv.org/abs/astro-ph/9602125
Autor:
Goldhaber, G., Deustua, S., Gabi, S., Groom, D., Hook, I., Kim, A., Kim, M., Lee, J., Pain, R., Pennypacker, C., Perlmutter, S., Small, I., Goobar, A., Ellis, R., Glazebrook, K., McMahon, R., Boyle, B., Bunclark, P., Carter, D., Irwin, M., Newberg, H., Filippenko, A. V., Matheson, T., Dopita, M., Mould, J., Couch, W.
This work is based on the first results from a systematic search for high redshift Type Ia supernovae. Using filters in the R-band we discovered seven such SNe, with redshift z = 0.3 - 0.5, before or at maximum light. Type Ia SNe are known to be a ho
Externí odkaz:
http://arxiv.org/abs/astro-ph/9602124
Autor:
Perlmutter, S., Pennypacker, C. R., Goldhaber, G., Goobar, A., Muller, R. A., Newberg, H. J. M., Desai, J., Kim, A. G., Kim, M. Y., Small, I. A., Boyle, B. J., Crawford, C. S., McMahon, R. G., Bunclark, P. S., Carter, D., Irwin, M. J., Terlevich, R. J., Ellis, R. S., Glazebrook, K., Couch, W. J., Mould, J. R., Small, T. A., Abraham, R. G.
Publikováno v:
Astrophys.J.440:L41-L44,1995
We have begun a program to discover high-redshift supernovae ($z \approx$ 0.25--0.5), and study them with follow-up photometry and spectroscopy. We report here our first discovery, a supernova at $z = 0.458$. The photometry for this supernova closely
Externí odkaz:
http://arxiv.org/abs/astro-ph/9505023