FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2325296095> ?p ?o ?g. }

• W2325296095 endingPage "453" @default.
• W2325296095 startingPage "443" @default.
• W2325296095 abstract "We present spectroscopic observations obtained with the ESO Very Large Telecope (VLT) of seven candidate Lyα emitting galaxies in the field of the radio quiet Q1205-30 at previously detected with deep narrow band imaging. Based on equivalent widths and limits on line ratios we confirm that all seven objects are Lyα emitting galaxies. Deep images also obtained with the VLT in the B and I bands show that five of the seven galaxies have very faint continuum fluxes ( and ). The star formation rates of these seven galaxies estimated from the rest-frame UV continuum around 2000 Å, as probed by the I-band detections, as well as from the Lyα luminosities, are 1-4 yr-1 assuming a Hubble constant of 65 km s-1 Mpc-1, , and . This is 1-3 orders of magnitude lower than for other known populations of star-forming galaxies at similar redshifts (the Lyman-Break galaxies and the sub-mm selected sources). The inferred density of the objects is high, per arcmin2 per unit redshift. This is consistent with the integrated luminosity function for Lyman-Break galaxies down to if the fraction of Lyα emitting galaxies is ≈70% at the faint end of the luminosity function. However, if this fraction is 20% as reported for the bright end of the luminosity function then the space density in this field is significantly larger (by a factor of 3.5) than expected from the luminosity function for Lyman-Break galaxies in the HDF-North. This would be an indication that at least some radio quiet QSOs at high redshift reside in overdense environments or that the faint end slope of the high redshift luminosity function has been underestimated. We find evidence that the faint Lyα galaxies are essentially dust-free. These observations show that Lyα emission is an efficient method by which to probe the faint end of the luminosity function at high redshifts." @default.
• W2325296095 created "2016-06-24" @default.
• W2325296095 creator A5028778207 @default.
• W2325296095 creator A5029396897 @default.
• W2325296095 creator A5039053686 @default.
• W2325296095 date "2001-08-01" @default.
• W2325296095 modified "2023-10-03" @default.
• W2325296095 title "Probing the faint end of the Galaxy luminosity function at $vec{z}=$ 3 with Ly<i>α</i>emission" @default.
• W2325296095 cites W1507586867 @default.
• W2325296095 cites W1665422179 @default.
• W2325296095 cites W1801581886 @default.
• W2325296095 cites W1968438730 @default.
• W2325296095 cites W1971204277 @default.
• W2325296095 cites W1988697524 @default.
• W2325296095 cites W1993856735 @default.
• W2325296095 cites W1994454575 @default.
• W2325296095 cites W1995711731 @default.
• W2325296095 cites W2007596869 @default.
• W2325296095 cites W2008481098 @default.
• W2325296095 cites W2017219295 @default.
• W2325296095 cites W2020548367 @default.
• W2325296095 cites W2028062388 @default.
• W2325296095 cites W2040006211 @default.
• W2325296095 cites W2041574552 @default.
• W2325296095 cites W2057672934 @default.
• W2325296095 cites W2077504681 @default.
• W2325296095 cites W2084040570 @default.
• W2325296095 cites W2121015243 @default.
• W2325296095 cites W2137896835 @default.
• W2325296095 cites W2138801852 @default.
• W2325296095 cites W2161219732 @default.
• W2325296095 cites W2165659164 @default.
• W2325296095 cites W2168204758 @default.
• W2325296095 cites W2170344725 @default.
• W2325296095 cites W2329717823 @default.
• W2325296095 cites W2951752678 @default.
• W2325296095 cites W3098422281 @default.
• W2325296095 cites W3101173890 @default.
• W2325296095 cites W3101642300 @default.
• W2325296095 cites W3102176150 @default.
• W2325296095 cites W3103632742 @default.
• W2325296095 cites W3103868583 @default.
• W2325296095 cites W3104219087 @default.
• W2325296095 cites W3121630487 @default.
• W2325296095 cites W3171996771 @default.
• W2325296095 cites W4292241054 @default.
• W2325296095 doi "https://doi.org/10.1051/0004-6361:20010739" @default.
• W2325296095 hasPublicationYear "2001" @default.
• W2325296095 type Work @default.
• W2325296095 sameAs 2325296095 @default.
• W2325296095 citedByCount "83" @default.
• W2325296095 countsByYear W23252960952012 @default.
• W2325296095 countsByYear W23252960952013 @default.
• W2325296095 countsByYear W23252960952014 @default.
• W2325296095 countsByYear W23252960952015 @default.
• W2325296095 countsByYear W23252960952016 @default.
• W2325296095 countsByYear W23252960952017 @default.
• W2325296095 countsByYear W23252960952018 @default.
• W2325296095 countsByYear W23252960952019 @default.
• W2325296095 countsByYear W23252960952020 @default.
• W2325296095 countsByYear W23252960952021 @default.
• W2325296095 countsByYear W23252960952022 @default.
• W2325296095 countsByYear W23252960952023 @default.
• W2325296095 crossrefType "journal-article" @default.
• W2325296095 hasAuthorship W2325296095A5028778207 @default.
• W2325296095 hasAuthorship W2325296095A5029396897 @default.
• W2325296095 hasAuthorship W2325296095A5039053686 @default.
• W2325296095 hasBestOaLocation W23252960951 @default.
• W2325296095 hasConcept C116367930 @default.
• W2325296095 hasConcept C121332964 @default.
• W2325296095 hasConcept C12287442 @default.
• W2325296095 hasConcept C125857072 @default.
• W2325296095 hasConcept C1276947 @default.
• W2325296095 hasConcept C133971210 @default.
• W2325296095 hasConcept C17959413 @default.
• W2325296095 hasConcept C20249676 @default.
• W2325296095 hasConcept C33024259 @default.
• W2325296095 hasConcept C44870925 @default.
• W2325296095 hasConcept C89108925 @default.
• W2325296095 hasConcept C98444146 @default.
• W2325296095 hasConceptScore W2325296095C116367930 @default.
• W2325296095 hasConceptScore W2325296095C121332964 @default.
• W2325296095 hasConceptScore W2325296095C12287442 @default.
• W2325296095 hasConceptScore W2325296095C125857072 @default.
• W2325296095 hasConceptScore W2325296095C1276947 @default.
• W2325296095 hasConceptScore W2325296095C133971210 @default.
• W2325296095 hasConceptScore W2325296095C17959413 @default.
• W2325296095 hasConceptScore W2325296095C20249676 @default.
• W2325296095 hasConceptScore W2325296095C33024259 @default.
• W2325296095 hasConceptScore W2325296095C44870925 @default.
• W2325296095 hasConceptScore W2325296095C89108925 @default.
• W2325296095 hasConceptScore W2325296095C98444146 @default.
• W2325296095 hasIssue "2" @default.
• W2325296095 hasLocation W23252960951 @default.
• W2325296095 hasOpenAccess W2325296095 @default.
• W2325296095 hasPrimaryLocation W23252960951 @default.
• W2325296095 hasRelatedWork W1647088338 @default.
• W2325296095 hasRelatedWork W1672876861 @default.

• next