MIPSGAL survey

E484841

The MIPSGAL survey is a Spitzer Space Telescope legacy program that mapped the inner Milky Way in mid-infrared wavelengths to study Galactic structure, star formation, and interstellar dust.

Try in SPARQL Jump to: Surface forms Statements Referenced by

All labels observed (1)

Label Occurrences
MIPSGAL survey canonical 1

Statements (47)

Predicate Object
instanceOf Spitzer Space Telescope legacy program
astronomical survey
infrared sky survey
acronym MIPSGAL NERFINISHED
dataArchive NASA/IPAC Infrared Science Archive NERFINISHED
dataFormat FITS images
dataProduct 24 micron images
70 micron images
extended emission maps
point source catalogues
dataReleasePolicy public
electromagneticSpectrumRegion infrared
focusesOn inner Galactic disk
fullName MIPS Galactic Plane Survey NERFINISHED
galacticLatitudeCoverage low galactic latitudes
hostGalaxy Milky Way NERFINISHED
observatory Spitzer Space Telescope NERFINISHED
observes H II regions
infrared bubbles
infrared dark clouds
interstellar dust emission
star-forming regions
supernova remnants
partOf Spitzer Legacy Program NERFINISHED
primaryWavelength 24 micrometres
70 micrometres
relatedSurvey CORNISH survey NERFINISHED
GLIMPSE survey NERFINISHED
Hi-GAL survey NERFINISHED
scienceGoal characterize infrared bubbles
identify young stellar objects
map dust emission in the Galactic plane
study Galactic structure
study H II regions
study interstellar dust
study star formation
study supernova remnants
surveyType imaging survey
target inner Milky Way
targetRegion Galactic plane
usedFor Galactic plane structure studies
interstellar medium studies
massive star formation studies
star formation rate estimates
usesInstrument MIPS NERFINISHED
usesTelescope Spitzer Space Telescope NERFINISHED
wavelengthBand mid-infrared

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.

W5 star-forming region surveyedIn MIPSGAL survey