FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100451852> ?p ?o ?g. }

• W3100451852 endingPage "37" @default.
• W3100451852 startingPage "37" @default.
• W3100451852 abstract "We provide an holistic view of galaxy evolution at high redshift z>4, that incorporates the constraints from various astrophysical/cosmological probes, including the estimate of the cosmic SFR density from UV/IR surveys and long GRB rates, the cosmic reionization history after the latest Planck measurements, and the missing satellites issue. We achieve this goal in a model-independent way by exploiting the SFR functions derived by Mancuso et al. (2016) on the basis of an educated extrapolation of the latest UV/far-IR data from HST/Herschel, and already tested against a number of independent observables. Our SFR functions integrated down to an UV magnitude limit M_UV<-13 (or SFR limit around 10^-2 M_sun/yr) produces a cosmic SFR density in excellent agreement with recent determinations from IR surveys and, taking into account a metallicity ceiling Z<Z_sun/2, with the estimates from long GRB rates. They also yield a cosmic reionization history consistent with that implied by the recent measurements of the Planck mission on the electron scattering optical depth tau_es~0.058; remarkably, this result is obtained under a conceivable assumption regarding the average value f_esc~0.1 of the escape fraction for ionizing photons. We demonstrate via the abundance matching technique that the above constraints concurrently imply galaxy formation to become inefficient within dark matter halos of mass below a few 10^8 M_sun; pleasingly, such a limit is also required not to run into the missing satellite issue. Finally, we predict a downturn of the galaxy luminosity function faintward of M_UV<-12, and stress that its detailed shape, as plausibly probed in the next future by the JWST, will be extremely informative on the astrophysics of galaxy formation in small halos, or even on the microscopic nature of the dark matter." @default.
• W3100451852 created "2020-11-23" @default.
• W3100451852 creator A5041560024 @default.
• W3100451852 creator A5051026292 @default.
• W3100451852 creator A5060557881 @default.
• W3100451852 creator A5061666272 @default.
• W3100451852 date "2017-01-17" @default.
• W3100451852 modified "2023-10-18" @default.
• W3100451852 title "GALAXY EVOLUTION AT HIGH REDSHIFT: OBSCURED STAR FORMATION, GRB RATES, COSMIC REIONIZATION, AND MISSING SATELLITES" @default.
• W3100451852 cites W1503787047 @default.
• W3100451852 cites W1908085087 @default.
• W3100451852 cites W1970058472 @default.
• W3100451852 cites W1970660289 @default.
• W3100451852 cites W1973808059 @default.
• W3100451852 cites W1984261945 @default.
• W3100451852 cites W1988066154 @default.
• W3100451852 cites W2000302520 @default.
• W3100451852 cites W2007099444 @default.
• W3100451852 cites W2020205763 @default.
• W3100451852 cites W2020266225 @default.
• W3100451852 cites W2033731878 @default.
• W3100451852 cites W2039879975 @default.
• W3100451852 cites W2041977406 @default.
• W3100451852 cites W2054857038 @default.
• W3100451852 cites W2063913239 @default.
• W3100451852 cites W2067649418 @default.
• W3100451852 cites W2070696493 @default.
• W3100451852 cites W2087936119 @default.
• W3100451852 cites W2093998251 @default.
• W3100451852 cites W2094181926 @default.
• W3100451852 cites W2096456403 @default.
• W3100451852 cites W2096624375 @default.
• W3100451852 cites W2103987722 @default.
• W3100451852 cites W2107245108 @default.
• W3100451852 cites W2109774665 @default.
• W3100451852 cites W2123267088 @default.
• W3100451852 cites W2141444993 @default.
• W3100451852 cites W2151274305 @default.
• W3100451852 cites W2158622701 @default.
• W3100451852 cites W2170769203 @default.
• W3100451852 cites W2171071003 @default.
• W3100451852 cites W2268149374 @default.
• W3100451852 cites W2363994444 @default.
• W3100451852 cites W2511105999 @default.
• W3100451852 cites W2963979336 @default.
• W3100451852 cites W2964219748 @default.
• W3100451852 cites W3098076155 @default.
• W3100451852 cites W3098361937 @default.
• W3100451852 cites W3098976132 @default.
• W3100451852 cites W3099774793 @default.
• W3100451852 cites W3099918481 @default.
• W3100451852 cites W3099994873 @default.
• W3100451852 cites W3100382286 @default.
• W3100451852 cites W3101501450 @default.
• W3100451852 cites W3101873082 @default.
• W3100451852 cites W3102416000 @default.
• W3100451852 cites W3102859222 @default.
• W3100451852 cites W3103050444 @default.
• W3100451852 cites W3103425094 @default.
• W3100451852 cites W3103591338 @default.
• W3100451852 cites W3104448025 @default.
• W3100451852 cites W3104728800 @default.
• W3100451852 cites W3105015425 @default.
• W3100451852 cites W3105177518 @default.
• W3100451852 cites W3105631369 @default.
• W3100451852 cites W3105808464 @default.
• W3100451852 cites W3106162244 @default.
• W3100451852 cites W3124333200 @default.
• W3100451852 cites W3124349042 @default.
• W3100451852 cites W3124371459 @default.
• W3100451852 cites W4291746798 @default.
• W3100451852 cites W4292875581 @default.
• W3100451852 doi "https://doi.org/10.3847/1538-4357/835/1/37" @default.
• W3100451852 hasPublicationYear "2017" @default.
• W3100451852 type Work @default.
• W3100451852 sameAs 3100451852 @default.
• W3100451852 citedByCount "18" @default.
• W3100451852 countsByYear W31004518522017 @default.
• W3100451852 countsByYear W31004518522018 @default.
• W3100451852 countsByYear W31004518522019 @default.
• W3100451852 countsByYear W31004518522020 @default.
• W3100451852 countsByYear W31004518522021 @default.
• W3100451852 countsByYear W31004518522022 @default.
• W3100451852 crossrefType "journal-article" @default.
• W3100451852 hasAuthorship W3100451852A5041560024 @default.
• W3100451852 hasAuthorship W3100451852A5051026292 @default.
• W3100451852 hasAuthorship W3100451852A5060557881 @default.
• W3100451852 hasAuthorship W3100451852A5061666272 @default.
• W3100451852 hasBestOaLocation W31004518521 @default.
• W3100451852 hasConcept C121332964 @default.
• W3100451852 hasConcept C125857072 @default.
• W3100451852 hasConcept C1276947 @default.
• W3100451852 hasConcept C166126730 @default.
• W3100451852 hasConcept C174802034 @default.
• W3100451852 hasConcept C33024259 @default.
• W3100451852 hasConcept C44870925 @default.
• W3100451852 hasConcept C59375849 @default.
• W3100451852 hasConcept C69672822 @default.

• next