FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3101148258> ?p ?o ?g. }

• W3101148258 endingPage "L16" @default.
• W3101148258 startingPage "L16" @default.
• W3101148258 abstract "We derive the stacked 1.4 GHz flux from the FIRST survey for 811 K+A galaxies selected from the Sloan Digital Sky Survey Data Release 7. For these objects we find a mean flux density of 56 ± 9 μJy. A similar stack of radio-quiet white dwarfs yields an upper limit of 43 μJy at a 5σ significance to the flux in blank regions of the sky. This implies an average star formation rate of 1.6 ± 0.3 M☉ yr−1 for K+A galaxies. However, the majority of the signal comes from ∼4% of K+A fields that have aperture fluxes above the 5σ noise level of the FIRST survey. A stack of the remaining galaxies shows little residual flux consistent with an upper limit on star formation of 1.3 M☉ yr−1. Even for a subset of 456 young (spectral ages <250 Myr) K+A galaxies, we find that the stacked 1.4 GHz flux is consistent with no current star formation. Our data suggest that the original starburst has been terminated in the majority of K+A galaxies, but that this may represent part of a duty cycle where a fraction of these galaxies may be active at a given moment with dusty starbursts and active galactic nuclei being present." @default.
• W3101148258 created "2020-11-23" @default.
• W3101148258 creator A5021292157 @default.
• W3101148258 creator A5050485401 @default.
• W3101148258 creator A5077847742 @default.
• W3101148258 creator A5080603188 @default.
• W3101148258 date "2012-11-29" @default.
• W3101148258 modified "2023-09-29" @default.
• W3101148258 title "THE CURRENT STAR FORMATION RATE OF K+A GALAXIES" @default.
• W3101148258 cites W1927790219 @default.
• W3101148258 cites W1969512945 @default.
• W3101148258 cites W1971146348 @default.
• W3101148258 cites W1987664245 @default.
• W3101148258 cites W1990146662 @default.
• W3101148258 cites W1991633896 @default.
• W3101148258 cites W1994671833 @default.
• W3101148258 cites W1997529816 @default.
• W3101148258 cites W1998032974 @default.
• W3101148258 cites W2002482748 @default.
• W3101148258 cites W2005539785 @default.
• W3101148258 cites W2006749766 @default.
• W3101148258 cites W2008603454 @default.
• W3101148258 cites W2013465449 @default.
• W3101148258 cites W2036934554 @default.
• W3101148258 cites W2042181581 @default.
• W3101148258 cites W2047002529 @default.
• W3101148258 cites W2055548073 @default.
• W3101148258 cites W2056356419 @default.
• W3101148258 cites W2058969567 @default.
• W3101148258 cites W2066644685 @default.
• W3101148258 cites W2067853161 @default.
• W3101148258 cites W2070073823 @default.
• W3101148258 cites W2074675121 @default.
• W3101148258 cites W2077326407 @default.
• W3101148258 cites W2094710844 @default.
• W3101148258 cites W2110294314 @default.
• W3101148258 cites W2124199755 @default.
• W3101148258 cites W2124380423 @default.
• W3101148258 cites W2134601765 @default.
• W3101148258 cites W2135894620 @default.
• W3101148258 cites W2142059889 @default.
• W3101148258 cites W2157917411 @default.
• W3101148258 cites W2963518027 @default.
• W3101148258 cites W3098241704 @default.
• W3101148258 cites W3098705452 @default.
• W3101148258 cites W3099700849 @default.
• W3101148258 cites W3100711035 @default.
• W3101148258 cites W3100745146 @default.
• W3101148258 cites W3102540473 @default.
• W3101148258 cites W3103868583 @default.
• W3101148258 cites W3104027651 @default.
• W3101148258 cites W3104182824 @default.
• W3101148258 cites W3104491675 @default.
• W3101148258 cites W3104973015 @default.
• W3101148258 cites W3105232245 @default.
• W3101148258 doi "https://doi.org/10.1088/2041-8205/761/2/l16" @default.
• W3101148258 hasPublicationYear "2012" @default.
• W3101148258 type Work @default.
• W3101148258 sameAs 3101148258 @default.
• W3101148258 citedByCount "20" @default.
• W3101148258 countsByYear W31011482582013 @default.
• W3101148258 countsByYear W31011482582014 @default.
• W3101148258 countsByYear W31011482582016 @default.
• W3101148258 countsByYear W31011482582017 @default.
• W3101148258 countsByYear W31011482582018 @default.
• W3101148258 countsByYear W31011482582021 @default.
• W3101148258 countsByYear W31011482582022 @default.
• W3101148258 countsByYear W31011482582023 @default.
• W3101148258 crossrefType "journal-article" @default.
• W3101148258 hasAuthorship W3101148258A5021292157 @default.
• W3101148258 hasAuthorship W3101148258A5050485401 @default.
• W3101148258 hasAuthorship W3101148258A5077847742 @default.
• W3101148258 hasAuthorship W3101148258A5080603188 @default.
• W3101148258 hasBestOaLocation W31011482581 @default.
• W3101148258 hasConcept C121332964 @default.
• W3101148258 hasConcept C125857072 @default.
• W3101148258 hasConcept C1276947 @default.
• W3101148258 hasConcept C139809296 @default.
• W3101148258 hasConcept C191897082 @default.
• W3101148258 hasConcept C192562407 @default.
• W3101148258 hasConcept C20249676 @default.
• W3101148258 hasConcept C43481613 @default.
• W3101148258 hasConcept C44870925 @default.
• W3101148258 hasConcept C68709404 @default.
• W3101148258 hasConcept C73329638 @default.
• W3101148258 hasConcept C89108925 @default.
• W3101148258 hasConcept C98444146 @default.
• W3101148258 hasConceptScore W3101148258C121332964 @default.
• W3101148258 hasConceptScore W3101148258C125857072 @default.
• W3101148258 hasConceptScore W3101148258C1276947 @default.
• W3101148258 hasConceptScore W3101148258C139809296 @default.
• W3101148258 hasConceptScore W3101148258C191897082 @default.
• W3101148258 hasConceptScore W3101148258C192562407 @default.
• W3101148258 hasConceptScore W3101148258C20249676 @default.
• W3101148258 hasConceptScore W3101148258C43481613 @default.
• W3101148258 hasConceptScore W3101148258C44870925 @default.
• W3101148258 hasConceptScore W3101148258C68709404 @default.
• W3101148258 hasConceptScore W3101148258C73329638 @default.

• next