Carnegie-Spitzer-IMACS Survey

E183929

The Carnegie-Spitzer-IMACS Survey is an astronomical research project that combines infrared observations from the Spitzer Space Telescope with optical spectroscopy from the IMACS instrument to study the formation and evolution of galaxies across cosmic time.

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Carnegie-Spitzer-IMACS Survey canonical 1

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Predicate Object
instanceOf astronomical survey
galaxy survey
observational cosmology project
aimsToStudy galaxy evolution
galaxy formation
galaxy properties across cosmic time
stellar mass assembly in galaxies
collaborationType international collaboration
combines ground-based optical spectroscopy
space-based infrared imaging
dataProduct galaxy redshift catalogues
spectroscopic measurements of galaxy properties
stellar mass estimates for galaxies
dataSource IMACS multi-object spectroscopy
Spitzer IRAC observations
field astronomy
astrophysics
extragalactic astronomy
focusesOn distant galaxies
intermediate-redshift galaxies
low-redshift galaxies
goal to constrain the buildup of stellar mass in the universe
to obtain a mass-selected sample of galaxies
to trace galaxy evolution over a wide redshift range
hostInstitution Carnegie Observatories
instrumentLocation Magellan Telescopes
surface form: Magellan telescopes
measures galaxy redshifts
galaxy spectral features
galaxy stellar masses
star-formation rates
observatory Las Campanas Observatory
observesBand 3.6 micron band
near-infrared continuum
relatedTo cosmic star-formation history
galaxy luminosity functions
galaxy stellar mass functions
mass-to-light ratios of galaxies
studies environmental dependence of galaxy evolution
relationship between stellar mass and star-formation rate
usesDataType infrared imaging
optical spectroscopy
usesInstrument IMACS
usesMethod multi-object spectroscopy
photometric and spectroscopic redshift estimation
spectral energy distribution fitting
usesTelescope Spitzer Space Telescope
usesWavelengthRange infrared
optical

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Carnegie Observatories notableProject Carnegie-Spitzer-IMACS Survey