2004ApJS..154...25R

Query : 2004ApJS..154...25R

2004ApJS..154...25R - Astrophys. J., Suppl. Ser., 154, 25-29 (2004/September-0)

The multiband imaging photometer for Spitzer (MIPS).

RIEKE G.H., YOUNG E.T., ENGELBRACHT C.W., KELLY D.M., LOW F.J., HALLER E.E., BEEMAN J.W., GORDON K.D., STANSBERRY J.A., MISSELT K.A., CADIEN J., MORRISON J.E., RIVLIS G., LATTER W.B., NORIEGA-CRESPO A., PADGETT D.L., STAPELFELDT K.R., HINES D.C., EGAMI E., MUZEROLLE J., ALONSO-HERRERO A., BLAYLOCK M., DOLE H., HINZ J.L., LE FLOC'H E., PAPOVICH C., PEREZ-GONZALEZ P.G., SMITH P.S., SU K.Y.L., BENNETT L., FRAYER D.T., HENDERSON D., LU N., MASCI F., PESENSON M., REBULL L., RHO J., KEENE J., STOLOVY S., WACHTER S., WHEATON W., WERNER M.W. and RICHARDS P.L.

Abstract (from CDS):

The Multiband Imaging Photometer for Spitzer (MIPS) provides long-wavelength capability for the mission in imaging bands at 24, 70, and 160 µm and measurements of spectral energy distributions between 52 and 100 µm at a spectral resolution of about 7%. By using true detector arrays in each band, it provides both critical sampling of the Spitzer point-spread function and relatively large imaging fields of view, allowing for substantial advances in sensitivity, angular resolution, and efficiency of areal coverage compared with previous space far-infrared capabilities. The 24 µm array has excellent photometric properties, and measurements with rms relative errors of about 1% can be obtained. The two longer-wavelength arrays use detectors with poor photometric stability, but a system of onboard stimulators used for relative calibration, combined with a unique data pipeline, produce good photometry with rms relative errors of less than 10%.

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Journal keyword(s): Infrared: General - Space Vehicles: Instruments

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 NAME NOAO Deep Wide Field reg 14 32 05.75 +34 16 47.5           ~ 430 0

Query : 2004ApJS..154...25R

Basic data :
NAME NOAO Deep Wide Field -- Region defined in the Sky
Other object types: otypes_help 		reg ()
ICRS coord. (ep=J2000) : 		14 32 05.75 +34 16 47.5 [ ] D 2002AJ....123.1784D
FK4 coord. (ep=B1950 eq=1950) : 		14 29 59.98 +34 29 59.7 [ ]
Gal coord. (ep=J2000) : 		057.44983 +67.28315 [ ]
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Identifiers (4) :
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NAME NOAO Deep Wide Field NAME NDWF NAME Bootes Deep Field NAME Bootes Field

References (430 between 1850 and 2026) (Total 430)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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