about
A massive galaxy in its core formation phase three billion years after the Big BangThe detection of a population of submillimeter-bright, strongly lensed galaxies.The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large-area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large ArrayResolving the ISM at the Peak of Cosmic Star Formation with ALMA: The Distribution of CO and Dust Continuum in z ∼ 2.5 Submillimeter GalaxiesA Spatially Resolved Study of Cold Dust, Molecular Gas, H ii Regions, and Stars in the z = 2.12 Submillimeter Galaxy ALESS67.1An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Spectroscopic RedshiftsALMA spectroscopic survey in the Hubble Ultra Deep Field: survey descriptionThe ALMA spectroscopic survey in the Hubble Ultra Deep Field: molecular gas reservoirs in high-redshift galaxiesAn ALMA survey of sub-millimeter galaxies in the extended Chandra Deep Field-South: physical properties derived from ultraviolet-to-radio modelingCOLDz: KARL G. JANSKY VERY LARGE ARRAY DISCOVERY OF A GAS-RICH GALAXY IN COSMOSAn ALMA survey of submillimeter galaxies in the extended Chandra Deep Field-South: the redshift distribution and evolution of submillimeter galaxiesHerschel ★ -ATLAS: properties of dusty massive galaxies at low and high redshiftsEmpirical predictions for (Sub-)millimeter line and continuum deep fieldsOn the effect of the cosmic microwave background in high-redshift (sub-)millimeter observationsGalaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV–far-IR) and the low-zenergy budgetHerschel★-ATLAS: rapid evolution of dust in galaxies over the last 5 billion yearsSpitzer imaging of strongly lensed Herschel-selected dusty star-forming galaxiesCalibration of Ultraviolet, Mid-infrared, and Radio Star Formation Rate IndicatorsAn atlas of galaxy spectral energy distributions from the ultraviolet to the mid-infraredGalaxy spectra from the UV to the mid-IRHerschelobservations of Hickson compact groups of galaxies: Unveiling the properties of cold dustThe evolving interstellar medium of star-forming galaxies since z = 2 as probed by their infrared spectral energy distributionsA mid-IR study of Hickson compact groups. II. Multiwavelength analysis of the complete GALEX-Spitzer sampleHerschel-ATLAS: The dust energy balance in the edge-on spiral galaxy UGC 4754The dust budget crisis in high-redshift submillimetre galaxiesHerschel★-ATLAS/GAMA: dusty early-type galaxies and passive spiralsGAMA/H-ATLAS: the ultraviolet spectral slope and obscuration in galaxiesThe Survey of Lines in M31 (SLIM): The Drivers of the [C ii]/TIR VariationThe nature of extreme emission line galaxies at z = 1-2: kinematics and metallicities from near-infrared spectroscopyConfirmation of small dynamical and stellar masses for extreme emission line galaxies at z ~ 2ALMA spectroscopic survey in the Hubble Ultra Deep Field: the infrared excess of UV-selected z = 2-10 galaxies as a function of UV-continuum slope and stellar massThe ALMA spectroscopic survey in the Hubble Ultra Deep Field: continuum number counts, resolved 1.2 mm extragalactic background, and properties of the faintest dusty star-forming galaxiesThe ALMA spectroscopic survey in the Hubble Ultra Deep Field: search for [CII] line and dust emission in 6 < z < 8 galaxiesALMA spectroscopic survey in the Hubble Ultra Deep Field: CO luminosity functions and the evolution of the cosmic density of molecular gasDust and gas in luminous proto-cluster galaxies at z = 4.05: the case for different cosmic dust evolution in normal and starburst galaxiesRegularity underlying complexity: a redshift-independent description of the continuous variation of galaxy-scale molecular gas properties in the mass-star formation rate planeA molecular line scan in the Hubble Deep Field NorthA molecular line scan in the Hubble Deep Field North: constraints on the CO luminosity function and the cosmic H_2_DensityThe intense starburst HDF 850.1 in a galaxy overdensity at z ≈ 5.2 in the Hubble Deep FieldThe heating of dust by old stellar populations in the bulge of M31
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հետազոտող
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Elisabete da Cunha
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Elisabete da Cunha
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Elisabete da Cunha
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Elisabete da Cunha
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Elisabete da Cunha
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Elisabete da Cunha
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P1412
P19
P21
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P31
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0000-0001-9759-4797
P569
1983-07-02T00:00:00Z