[PDF] Top 20 Evolution of Star forming Galaxies from z=0 7 to 1 2 with eBOSS Emission line Galaxies
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Evolution of Star forming Galaxies from z=0 7 to 1 2 with eBOSS Emission line Galaxies
... those from deeper imaging observa- tions (Leauthaud et ...ing galaxies selected with relaxed color cuts (Tinker et ...mates from other methods (see ... See full document
17
Boötes HiZELS:an optical to near infrared survey of emission line galaxies at z=0 4 4 7
... at z = 1.47, 3.3, 4.7 to the other published results. At z = ...fit from Ly et ...at z = 3.3 and z = ...hints from contamination in this sample is that some have relatively low ... See full document
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The Intergalactic and Circumgalactic Medium Surrounding Star-Forming Galaxies at Redshifts 2<z<3
... same line-fitting techniques used by previous authors on QSO spectra with improved wavelength coverage and signal-to-noise ratios, to revisit the statistics of the Lyman α forest in Chapters 3 and ...Chapter ... See full document
221
SINFONI HiZELS:the dynamics, merger rates & metallicity gradients of typical star forming galaxies at z = 0 8 2 2
... selected galaxies with IFU AO-aided observations – the ‘SHiZELS’ survey, with roughly equal number of galaxies per redshift slice, at z = ...that galaxies with higher velocity dispersions tend ... See full document
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The dynamics and distribution of angular momentum in HiZELS star forming galaxies at z = 0 8–3 3
... sky emission lines were removed using sky subtrac- tion techniques described in Davies ...measured from the telluric standard star in the NIFS data cubes is ...three galaxies in our sample ... See full document
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The properties of star forming galaxies at z~2 : kinematics, stellar populations, and metallicities
... of galaxies is not necessarily representative of the UV-selected sample as a whole, because objects were chosen for near-IR spectroscopy for a wide variety of ...the galaxies were selected because they lie ... See full document
228
The LOFAR window on star forming galaxies and AGNs – curved radio SEDs and IR–radio correlation at 0<z<2 5
... of star-forming (SF) galaxies and active galactic nuclei (AGNs) up to redshift z = ...continuum emission from 150 MHz to ...1542 galaxies in ∼7 deg 2 of the ... See full document
21
A multiwavelength exploration of the [C II]/IR ratio in H ATLAS/GAMA galaxies out to z = 0 2
... Nine galaxies present line ratios with large error bars ...dex). Galaxies to the left of the solid line (taken from Kauffmann et ...considered star forming (blue crosses); ... See full document
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The growth of the central region by acquisition of counterrotating gas in star forming galaxies
... blue star-forming galaxies, red quiescent galaxies with little star formation and green-valley galaxies between these two extremes ...of galaxies with nebular ... See full document
9
The SAMI Galaxy Survey : spatially resolving the environmental quenching of star formation in GAMA galaxies
... for galaxies with a range of stellar masses and star-forming morphologies in ...Fig. 7. Taking the inclination of the galaxy to our line of sight improves our estimate of the radial ... See full document
22
GLACE survey: OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster ZwCl 0024 0+1652 at z=0 395
... results from the Hα / [N ] survey performed in the galaxy cluster ZwCl 0024 + 1652 (here- after referred to as Cl0024) at z = ...Sect. 2, the GLACE survey is outlined, including its main ... See full document
22
Bulgeless galaxies in the COSMOS field:environment and star formation evolution at z
... redshifts z = 0.4 and z = 0.84 of the HiZELS survey, we selected ∼ 220 star-forming bulgeless systems (S´ersic index n ≤ ...their star formation properties and we investigate their ... See full document
14
Deviations from passive evolution – star formation and the ultraviolet excess in z ∼ 1 radio galaxies
... radio galaxies is that the radio power of sources in a flux-limited sample such as this increases with redshift, leading to a degeneracy between redshift and radio ...∼ 1) redshifts, and it is the ... See full document
17
Starburst galaxies in the COSMOS field : clumpy star formation at redshift 0 < z <0 5
... (obtained from the Sloan Digital Sky Survey; SDSS) massive clumps in local starbursts belonging to the Kiso Sur- vey (Miyauchi-Isobe et ...in galaxies at high redshift from the Hubble Ultra Deep ... See full document
17
The Hα luminosity dependent clustering of star forming galaxies from z ∼ 0 8 to z ∼ 2 2 with HiZELS
... derived from data spanning from optical to mid-IR wavelengths ...which emission line is being selected for each emitter, and thus select a clean sample of Hα ...emitting galaxies at ... See full document
21
The evolution of post starburst galaxies from z=2 to 0 5
... Fig. 2 we present the colour-colour distributions for the first two super-colours in six redshift ...of galaxies lie in different regions of super-colour space. Galaxies which have undergone no ... See full document
15
The production and escape of Lyman Continuum radiation from star forming galaxies at z~2 and their redshift evolution
... Darvish et al. (2015b) performed two sets of extensive simulations to check the performance of different den- sity estimators, including 5th and 10th nearest neigh- bors, Delaunay triangulation, adaptive kernel smooth- ... See full document
17
Angular momentum evolution of galaxies over the past 10 Gyr:a MUSE and KMOS dynamical survey of 400 star forming galaxies from z=0 3 to 1 7
... of GaLaxies and their Environments ( EAGLE ) simulations follows the evolution of dark matter, gas, stars and black-holes in cosmological (10 6 Mpc 3 ) volumes (Schaye et ...the z ∼ 0 galaxy ... See full document
21
The production and escape of Lyman Continuum radiation from star forming galaxies at z~2 and their redshift evolution
... fellowship from Leiden University. DS acknowledges financial support from the Netherlands Organisation for Scientific research (NWO) through a Veni fellowship and from FCT through a FCT Investigator ... See full document
19
The Interstellar Medium in [O III] selected Star forming Galaxies at z similar to 3 2
... of emission line galaxies in a particular narrow redshift slice ...At z > 3, the Hα emission line, which is one of the most reliable tracers of star-forming ... See full document
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