[PDF] Top 20 The Interstellar Medium in [O III] selected Star forming Galaxies at z similar to 3 2
Has 10000 "The Interstellar Medium in [O III] selected Star forming Galaxies at z similar to 3 2" found on our website. Below are the top 20 most common "The Interstellar Medium in [O III] selected Star forming Galaxies at z similar to 3 2".
![The Interstellar Medium in [O III] selected Star forming Galaxies at z similar to 3 2](data:image/gif;base64,R0lGODlhAQABAIAAAP///wAAACH5BAEAAAAALAAAAAABAAEAAAICRAEAOw==)
The Interstellar Medium in [O III] selected Star forming Galaxies at z similar to 3 2
... that star-forming galaxies at high redshifts (z > 1) typically have different interstellar medium (ISM) conditions from those found in local star-forming ... See full document
20
Spitzer catalog of Herschel selected ultrared dusty, star forming galaxies
... photo- z and fixed-z versions are generally consistent with each other although the SFRs from the fixed-z version are higher, which is mostly driven by the higher FIR-derived photo-z than the ... See full document
33
The Hα luminosity dependent clustering of star forming galaxies from z ∼ 0 8 to z ∼ 2 2 with HiZELS
... are selected based on their NB-BB colour excess, with a signal-to-noise cut of S/N > 3 and an equivalent width selection corre- sponding to EW > 25 for ...being selected for each emitter, and ... See full document
21
GLACE survey: OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster ZwCl 0024 0+1652 at z=0 395
... SF galaxies using the ratio between the [N ] and the Hα ...LINER galaxies, the so-called “EWαn2 di- agram” as depicted in the left-hand panel of ...Seyfert galaxies tend to have a higher power for ... See full document
22
The production and escape of Lyman Continuum radiation from star forming galaxies at z~2 and their redshift evolution
... of galaxies in the COSMOS field (Scoville et al. 2007) out to z ∼ ...∼ 2 deg 2 ) for the effects of the large- scale structure to be discernible, with a minimal cosmic ...is selected in ... See full document
17
Strong Far ultraviolet Fields Drive the [C II]/Far infrared Deficit in z ∼ 3 Dusty, Star forming Galaxies
... detectable, while the [C II ] line remains relatively unaf- fected (da Cunha et al. 2013; Vallini et al. 2015; Lagache et al. 2018). Indeed, with the advent of Atacama Large Millimeter/submillimeter Array (ALMA), [C II ] ... See full document
24
Starburst galaxies in the COSMOS field : clumpy star formation at redshift 0 < z <0 5
... four galaxies and 12 knots), our results are backed up by previous findings in the ...starburst galaxies, claims that no di ff erence in color is found between the disk and clump regions when the clumps are ... See full document
17
The production and escape of Lyman Continuum radiation from star forming galaxies at z~2 and their redshift evolution
... are similar to that of Rutkowski et ...higher star formation rate (SFR). This is be- cause our galaxies are selected from wide-field surveys and the typical SFR of galaxies at z ... See full document
19
The SCUBA 2 Cosmology Legacy Survey : the clustering of submillimetre galaxies in the UKIDSS UDS field
... these galaxies were assembled at high redshifts (z ∼ 3–5), with the preceding starburst event taking place on short timescales of ∼ 500 Myr (Thomas et ...passive galaxies cluster more strongly ... See full document
14
The KMOS Deep Survey (KDS) I:Dynamical measurements of typical star forming galaxies at z $\simeq$ 3 5
... spatially-resolved galaxies in the KDS, divided into rotation-dominated (13/38), dispersion-dominated (19/38) and merger categories ...[O III ]λ5007 intensity map and velocity dispersion ... See full document
44
An enhanced fraction of starbursting galaxies among high Eddington ratio AGNs
... the 3 σ upper-limits on their Herschel ...positions selected at random around the source ...(2011) star-forming galaxies templates to convert the monochromatic 3 σ upper-limits ... See full document
15
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
... the galaxies; see Stott et ...those galaxies with Hα fluxes brighter than 5 × 10 −17 erg s −1 cm −2 ...a star to monitor the PSF and one IFU on blank sky to measure OH ...a similar ... See full document
21
The evolution of the cold interstellar medium in galaxies following a starburst
... is selected purely based on the properties of the stellar population of the galaxies, ...Section 2, we describe the method used to select a com- plete sample of starburst to PSB ...Section 3, ... See full document
22
The LOFAR window on star forming galaxies and AGNs – curved radio SEDs and IR–radio correlation at 0<z<2 5
... SF galaxies and AGN are 49 and 51 per cent, respectively, given our LOFAR–I-band-selected sam- ...a similar LOFAR-selected sample presented by Hardcastle et ...SF galaxies to AGN of ... See full document
21
Multi Wavelength Properties of Submillimeter Selected Galaxies
... bins: z < 1 . 0, 1 . 0 < z < 2 . 0, and z > 2 ...lower-luminosity star-forming galaxies nearby ...luminous galaxies frequently used as “cold” and ... See full document
241
The properties of star forming galaxies at z~2 : kinematics, stellar populations, and metallicities
... [O III ] because of higher surface brightness; but Pettini et ...[O III ]λ5007/Hβ ∼ 3, and Hα/Hβ ∼ 3 as well, so Hα and [O III ]λ5007 should have roughly comparable ... See full document
228
The Intergalactic and Circumgalactic Medium Surrounding Star-Forming Galaxies at Redshifts 2<z<3
... The often-invoked solution to this problem is feedback: the injection of energy or momentum into the ISM of a galaxy from the combined effects of star formation, supernovae, and AGN. Clearly, the large discrepancy ... See full document
221
The dynamics and distribution of angular momentum in HiZELS star forming galaxies at z = 0 8–3 3
... 34 star–forming galaxies at z = 0.8–3.3 selected from the HiZELS narrow-band ...ionised interstellar medium on ∼1 kpc scales, and show that the galaxies are ... See full document
31
VALES: III The calibration between the dust continuum and interstellar gas content of star forming galaxies
... FIR from numerous facilities, currently including: GALaxy Evolu- tion eXplorer (GALEX), Sloan Digital Sky Survey (SDSS), Visible and Infrared Telescope for Astronomy (VISTA), Wide-field Infrared Survey Explorer (WISE), ... See full document
5
An Empirically Calibrated Model for Interpreting the Evolution of Galaxies during the Reionization Era
... simple star formation model whose goal is to interpret the emerging body of observational data of star-forming galaxies at z k ...the star formation activity within dark matter ... See full document
17
Related subjects