The Wide-Field Infrared Explorer (Wire) Mission
The Wide-Field Infrared Explorer (WIRE) (Schember et al. 1996 and references within) is a small spaceborne telescope specifically designed to study the evolution of starburst galaxies. This powerful astronomical instrument will be capable of detecting typical starburst galaxies at z ∼ 0.5, ultralumi...
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| Veröffentlicht in: | Symposium - International Astronomical Union 1998, Vol.179, p.118-120 |
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| container_title | Symposium - International Astronomical Union |
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| creator | Shupe, D.L. Hacking, P.B. Herter, T. Gautier, T.N. Graf, P. Lonsdale, C.J. Stacey, G.J. Moseley, S.H. Soifer, B.T. Werner, M.W. Houck, J.R. |
| description | The Wide-Field Infrared Explorer (WIRE) (Schember
et al.
1996 and references within) is a small spaceborne telescope specifically designed to study the evolution of starburst galaxies. This powerful astronomical instrument will be capable of detecting typical starburst galaxies at
z
∼ 0.5, ultraluminous infrared galaxies beyond a
z
∼ 2, and luminous protogalaxies beyond
z
∼ 5. The WIRE survey, to be conducted during a four month period in 1998, will cover over 100 deg
2
of high Galactic latitude sky at 25
μ
m and 12
μ
m. |
| doi_str_mv | 10.1017/S0074180900128359 |
| format | Article |
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et al.
1996 and references within) is a small spaceborne telescope specifically designed to study the evolution of starburst galaxies. This powerful astronomical instrument will be capable of detecting typical starburst galaxies at
z
∼ 0.5, ultraluminous infrared galaxies beyond a
z
∼ 2, and luminous protogalaxies beyond
z
∼ 5. The WIRE survey, to be conducted during a four month period in 1998, will cover over 100 deg
2
of high Galactic latitude sky at 25
μ
m and 12
μ
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et al.
1996 and references within) is a small spaceborne telescope specifically designed to study the evolution of starburst galaxies. This powerful astronomical instrument will be capable of detecting typical starburst galaxies at
z
∼ 0.5, ultraluminous infrared galaxies beyond a
z
∼ 2, and luminous protogalaxies beyond
z
∼ 5. The WIRE survey, to be conducted during a four month period in 1998, will cover over 100 deg
2
of high Galactic latitude sky at 25
μ
m and 12
μ
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et al.
1996 and references within) is a small spaceborne telescope specifically designed to study the evolution of starburst galaxies. This powerful astronomical instrument will be capable of detecting typical starburst galaxies at
z
∼ 0.5, ultraluminous infrared galaxies beyond a
z
∼ 2, and luminous protogalaxies beyond
z
∼ 5. The WIRE survey, to be conducted during a four month period in 1998, will cover over 100 deg
2
of high Galactic latitude sky at 25
μ
m and 12
μ
m.</abstract><doi>10.1017/S0074180900128359</doi><tpages>3</tpages><oa>free_for_read</oa></addata></record> |
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| ispartof | Symposium - International Astronomical Union, 1998, Vol.179, p.118-120 |
| issn | 0074-1809 |
| language | eng |
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| source | Alma/SFX Local Collection |
| title | The Wide-Field Infrared Explorer (Wire) Mission |
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