@article{oai:jaxa.repo.nii.ac.jp:00036668,
 author = {OYABU, Shinki and KAWARA, Kimiaki and TSUZUKI, Yumihiko and SOFUE, Yoshiaki and SATO, Yasunori and OKUDA, Haruyuki and TANIGUCHI, Yoshiaki and SHIBAI, Hiroshi and GABRIEL, Carlos and HASEGAWA, Takashi and NISHIHARA, Eiji},
 journal = {The Institute of Space and Astronautical Science report. S.P. : Mid- and Far-Infrared Astronomy and Future Space Mission},
 month = {Dec},
 note = {Eight luminous quasars with -30 < MB < -27 at z = 1.4 - 3.7 have been observedin the mid- and far-infrared with ISO. To obtain spectral energy distributions (SEDs) from theUV to far-infrared, additional optical and near-infrared observations were made from the ground.The observed SEDs are compared with the mean-SED of low-redshift quasars with less luminosity(-27 < MB < -22) given by Elvis et al. (1994). There is no evidence of excess in the mid- andfar-infrared in our quasar sample., 資料番号: SA4590593000},
 pages = {139--146},
 title = {ISO Continuum Observations of Quasars at z=1-4},
 volume = {14},
 year = {2000}
}