[PDF] Top 20 Spatially Resolved Spectroscopy of Submillimeter Galaxies at z ≃ 2
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Spatially Resolved Spectroscopy of Submillimeter Galaxies at z ≃ 2
... nature of the large energy output in SMGs is now commonly assumed to be associated with their vigorous star formation ...fraction of the ...75% of the radio-selected spectro- scopically identi fi ed ... See full document
14
Reliable Identification of Compton thick Quasars at at z ? 2: Spitzer Mid Infrared Spectroscopy of HDF Omd49
... Selection of distant Compton-thick AGNs. (a) Ratio of mid-IR-based to UV-based SFR ...the z 2 galaxies studied by Daddi et ...Fig. 2 of Daddi et ...the galaxies ... See full document
13
A detailed gravitational lens model based on submillimeter array and keck adaptive optics imaging of a Herschel atlas submillimeter galaxy AT z = 4 243
... sample of ∼1000 lensed ...selection at 1.4 mm, the SPT sample of lensed SMGs will be complementary to the Herschel sample in the sense that it will be biased towards higher redshift or cooler dust ... See full document
11
Ly alpha EMITTING GALAXIES AT z=2 1 IN ECDF S: BUILDING BLOCKS OF TYPICAL PRESENT DAY GALAXIES?
... term at small scales and to avoid sampling noise at big ...hints of a large-scale inhomogeneity in the spatial distribution of the LAE candidates at δ > ...process of ... See full document
15
Multiwavelength Study of Massive Galaxies at z~2 I Star Formation and Galaxy Growth
... aim of this paper is to verify to what extent this agreement among the various star formation tracers persists in- dividually for distant massive galaxies, hence to what extent SFRs can be unambiguously ... See full document
17
HIGH RESOLUTION NEAR INFRARED IMAGING OF SUBMILLIMETER GALAXIES
... obscuration at short ...use of radio maps and blind optical spectroscopy that can be confirmed with CO detections (Chapman et ...2005), of mid-IR spectroscopy of polycyclic ... See full document
17
SDSS IV MaNGA: Dependence of Global and Spatially Resolved SFR M ∗ Relations on Galaxy Properties
... source of H α ...nature of the SFR – M * relation would require spatially resolved data to understand what processes drive the connection between SFR and M * ...Using spatially ... See full document
8
HST WFC3/IR Observations of Active Galactic Nucleus Host Galaxies at z ~ 2 : Supermassive Black Holes Grow in Disk Galaxies
... Table 2, we report the results for all 20 AGN host galaxies 11 that are well ...difference of the host galaxy to the AGN from the S´ersic + PSF ...is at least 1 mag brighter than the point ... See full document
6
Measurements of co redshifts with Z spec for lensed submillimeter galaxies discovered in the H atlas survey
... nature of these galaxies, in particular whether they represent a previously undiscovered population of intrinsically bright sources ...starburst galaxies lensed by fore- ground structures ... See full document
27
Weighhing the black holes in z 2 submillimeter emitting galaxies hosting active galactic nuclei
... presence of absorption in the X-ray-obscured SMGs hinders direct black- hole mass measurements, the identification of broad Paα in a small number of nearby obscured ULIRGs provides the poten- tial to ... See full document
14
Magellan/MMIRS near infrared multi object spectroscopy of nebular emission from star forming galaxies at 2 < z < 3
... the at- mospheric sky ...bulk of the constant and variable IR backgrounds, obtain- ing background-subtracted (A-B) or (B-A) ...variation at a specific moment of the night and air- mass, in the ... See full document
21
Nondestructive quality evaluation and monitoring of Braeburn apples by Spatially Resolved Spectroscopy.
... aperture of 0.22 and a core diameter of 200 ...placed at center-to- center distances ranging from ...means of a data acquisition card and a custom written LabView program (National ... See full document
6
Submillimeter galaxies behind the Bullet cluster (1E 0657 56)
... 0657-56) at z 0.3 is one of the most massive galaxy clusters known to date (see Markevitch et ...image of a background galaxy at a redshift of about ...line of the lens, ... See full document
14
Spatially resolved analysis of superluminous supernovae PTF 11hrq and PTF 12dam host galaxies
... 0.5 Z ) and a high rate of star formation (SFR) for their low mass (Neill et ...rate of star formation is not required, since there are many counterexamples of SLSNe with low SFRs, based on ... See full document
13
The Evolution of Lyα emitting Galaxies between z = 2 1 and z = 3 1
... DENSITY OF LAEs Narrowband imaging (Ouchi et ...2011) spectroscopy now yield a coherent picture of the evolution of the LAE population and their SFR ...luminosities of the z = ... See full document
11
The composite nature of Dust Obscured Galaxies (DOGs) at z ∼ 2–3 in the COSMOS field – I A far infrared view
... intensity of the field is responsible for the bluer colour of these bright DOGs, by comparing to the 100 /24 μ m colours de- rived from the templates of Magdis et ...ensembles at different ... See full document
16
A PROTOCLUSTER AT z=2 45
... shows at times contradictory examples for environmental in fl uences in protoclusters at z > ...three z > 2 protoclusters, suggesting the appearance of massive elliptical ... See full document
8
ALMA Observations of Gas rich Galaxies in z ~ 1 6 Galaxy Clusters: Evidence for Higher Gas Fractions in High density Environments
... eld galaxies from the Genzel et ...mass of our cluster galaxies. The gas fraction in cluster galaxies mimics the strong evolution in the fi ...the z > 1 cluster galaxies lie ... See full document
6
Heavily obscured quasar host galaxies at z ∼ 2 are discs, not major mergers
... question of whether fea- tures indicative of a major merger would be apparent given the quality of the ...images of red quasars hosted by major mergers at z < 1 (Urrutia et ... See full document
5
Spatio-temporal characterization of laser pulses by spatially resolved spectral interferometry
... difference of delay Δτ=1671 fs introduced by the plate is calculated from (n−1)L=c⋅Δτ where ...thickness of the plate and n=1.454 is the refractive index of the fused silica at wavelength ... See full document
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