K Corrections For Type Ia Supernovae and a Test for Spatial Variation of the Hubble Constant

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dc.creatorKim, A.
dc.creatorDeustua, S.
dc.creatorGabi, S.
dc.creatorGoldhaber, G.
dc.creatorGroom, D.
dc.creatorHook, I.
dc.creatorKim, M.
dc.creatorLee, J.
dc.creatorPain, R.
dc.creatorPennypacker, C.
dc.creatorPerlmutter, S.
dc.creatorSmall, I.
dc.creatorGoobar, A.
dc.creatorEllis, R.
dc.creatorGlazebrook, K.
dc.creatorMcMahon, R.
dc.creatorBoyle, B.
dc.creatorBunclark, P.
dc.creatorCarter, D.
dc.creatorIrwin, M.
dc.creatorNewberg, H.
dc.creatorFilippenko, A. V.
dc.creatorMatheson, T.
dc.creatorDopita, M.
dc.creatorMould, J.
dc.creatorCouch, W.
dc.date1996-02-23
dc.date.accessioned2026-07-07T02:20:55Z
dc.date.available2026-07-07T02:20:55Z
dc.descriptionCross-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 0.05 mag for redshifts z<0.7. This narrow dispersion of the calculated K correction allows the Type Ia to be used as a cosmological probe. We use the K corrections with observations of seven SNe at redshifts 0.3 < z <0.5 to bound the possible difference between the locally measured Hubble constant (H_L) and the true cosmological Hubble constant (H_0).
dc.description6 pages, 3 Postscript figures, uuencoded uses crckapb.sty and psfig.sty. To appear in Thermonuclear Supernovae (NATO ASI), eds. R. Canal, P. Ruiz-LaPuente, and J. Isern. Postscript version is also available at http://www-supernova.lbl.gov/
dc.identifierhttps://arxiv.org/abs/astro-ph/9602123
dc.identifierhttp://arxiv.org/abs/astro-ph/9602123
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10377
dc.subjectAstrophysics
dc.titleK Corrections For Type Ia Supernovae and a Test for Spatial Variation of the Hubble Constant
dc.typetext

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