Hubble Diagrams of Type Ia Supernovae in the Near-Infrared
Author(s) -
K. Krisciunas,
M. M. Phillips,
N. B. Suntzeff
Publication year - 2004
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/382731
Subject(s) - supernova , physics , astrophysics , brightness , cosmic distance ladder , infrared , hubble's law , redshift , absolute magnitude , type (biology) , astronomy , galaxy , geology , paleontology
From observations of 7 Type Ia supernovae obtained during the last four yearsat the Las Campanas and Cerro Tololo Inter-American Observatories, along withprevious published data for 9 supernovae, we present JHK Hubble diagrams andderive absolute magnitudes at maximum light of 16 objects out to a redshift of0.038. On the scale of H_0 = 72 km/s/Mpc we find mean absolute magnitudes atmaximum of -18.57, -18.24, and -18.42 for J, H, and K, respectively, with1-sigma uncertainties of the distributions of values of +/- 0.14, 0.18, and0.12 mag. The data indicate no significant decline rate relations for theinfrared. Thus, Type Ia SNe at maximum brightness appear to be standard candlesin the infrared at the +/- 0.20 mag level or better. The minimum requirementsfor obtaining the distance to a Type Ia SN are: reasonably accurate values ofDelta m_15(B) and T(B_max), and one night of infrared data in the -12 to +10 dwindow with respect to T(B_max).Comment: 15 pages, 3 figures, published in the Astrophysical Journal, vol. 602, pp. L81-L84 (20 February 2004). This version gives more credit where credit is du
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