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Paper: Supernova Search at Intermediate-redshift.
II. Host Galaxy Morphology
Volume: 342, 1604-2004: Supernovae as Cosmological Lighthouses
Page: 488
Authors: Mendez, J.; Ruiz-Lapuente, P.; Altavilla, G.; Balastegui, A.; Irwin, M.; Schamanache, K.; Balland, C.; Pain, R.; Walton, N.
Abstract: We discuss the host galaxy morphology of the 8 supernovae (SNe) discovered as a part of the International Time Programme (ITP) project “Ω and Λ from Supernovae, and the physics of Supernovae Explosions” at the European Northern Observatory (ENO). Identification of the SN host galaxies was performed exploiting both imaging and spectroscopic facilities at the Isaac Newton Group of Telescopes (ING) which comprises the 4.2m William Hershel Telescope (WHT), the 2.5m Isaac Newton Telescope (INT) and the 1.0m Jacobus Kapteyn Telescope (JKT). Also the 3.6m Telescopio onale Galileo (TNG) and the 2.5m Nordic Optical Telescope (NOT) were used for the optical photometric follow-up of the supernovae.
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