==================================================================== we have recently observed several gravitationally lensed objects with scuba on the jcmt. one of them shows very strong submm flux, comparable to iras f10214+4724 and the cloverleaf quasar. the object is very likely a dusty high redshift infrared galaxy or quasar, but its redshift has not yet been measured because of an extremely red optical spectrum. hst observations in the near-ir reveal a 1 diameter einstein ring. we wish to obtain a full, broadband spectrum across the ir to determine this objects spectral energy distribution and possibly get a rough estimate of its redshift. this appears to be a member of a rare class of observable high-redshift ir-galaxies/quasars which warrants follow-up with iso before the mission ends.
Instrument
CAM01 , PHT03 , PHT22
Temporal Coverage
1998-03-28T14:48:04Z/1998-04-04T13:32:49Z
Version
1.0
Mission Description
The Infrared Space Observatory (ISO) was the worlds first true orbiting infrared observatory. Equipped with four highly-sophisticated and versatile scientific instruments, it was launched by Ariane in November 1995 and provided astronomers world-wide with a facility of unprecedented sensitivity and capabilities for a detailed exploration of the Universe at infrared wavelengths.
European Space Agency, BARVAINIS et al., 1999, 'AN EINSTEIN RING WITH STRONG SUBMILLIMETER EMISSION', 1.0, European Space Agency, https://doi.org/10.5270/esa-zu97z53
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.
