FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2078460887> ?p ?o ?g. }

• W2078460887 endingPage "1629" @default.
• W2078460887 startingPage "1618" @default.
• W2078460887 abstract "Dust extinction and stellar confusion by the Milky Way reduce the efficiency of detecting galaxies at low Galactic latitudes, creating the so-called Zone of Avoidance. This stands as a stumbling block in charting the distribution of galaxies and cosmic flow fields, and therewith our understanding of the local dynamics in the Universe (CMB dipole, convergence radius of bulk flows). For instance, ZoA galaxies are generally excluded from the whole-sky Tully-Fisher Surveys ($|b| leq 5^circ$) even if catalogued. We show here that by fine-tuning the near-infrared TF relation, there is no reason not to extend peculiar velocity surveys deeper into the ZoA. Accurate axial ratios ($b/a$) are crucial to both the TF sample selection and the resulting TF distances. We simulate the effect of dust extinction on the geometrical properties of galaxies. As expected, galaxies appear rounder with increasing obscuration level, even affecting existing TF samples. We derive correction models and demonstrate that we can reliably reproduce the intrinsic axial ratio from the observed value up to extinction level of about $A_Jsimeq3$ mag ($A_Vsim11$ mag), we also recover a fair fraction of galaxies that otherwise would fall out of an uncorrected inclination limited galaxy sample. We present a re-calibration of the 2MTF relation in the NIR $J$, $H$, and $K_s$-bands for isophotal rather than total magnitudes, using their same calibration sample. Both TF relations exhibit similar scatter at high Galactic latitudes. However, the isophotal TF relation results in a significant improvement in the scatter for galaxies in the ZoA, and low surface brightness galaxies in general, because isophotal apertures are more robust in the face of significant stellar confusion." @default.
• W2078460887 created "2016-06-24" @default.
• W2078460887 creator A5044483582 @default.
• W2078460887 creator A5080665198 @default.
• W2078460887 creator A5081882010 @default.
• W2078460887 date "2014-12-31" @default.
• W2078460887 modified "2023-10-18" @default.
• W2078460887 title "On how to extend the NIR Tully–Fisher relation to be truly all-sky" @default.
• W2078460887 cites W1505139343 @default.
• W2078460887 cites W1766019736 @default.
• W2078460887 cites W1853722646 @default.
• W2078460887 cites W1886868625 @default.
• W2078460887 cites W1900821594 @default.
• W2078460887 cites W1969141849 @default.
• W2078460887 cites W1969850707 @default.
• W2078460887 cites W1972504071 @default.
• W2078460887 cites W1982019562 @default.
• W2078460887 cites W1982735095 @default.
• W2078460887 cites W1996453689 @default.
• W2078460887 cites W2004071138 @default.
• W2078460887 cites W2006251234 @default.
• W2078460887 cites W2007925985 @default.
• W2078460887 cites W2011470589 @default.
• W2078460887 cites W2018083552 @default.
• W2078460887 cites W2020977594 @default.
• W2078460887 cites W2021620550 @default.
• W2078460887 cites W2021887861 @default.
• W2078460887 cites W2023590996 @default.
• W2078460887 cites W2023900725 @default.
• W2078460887 cites W2025796785 @default.
• W2078460887 cites W2029083557 @default.
• W2078460887 cites W2029343094 @default.
• W2078460887 cites W2029951163 @default.
• W2078460887 cites W2030503552 @default.
• W2078460887 cites W2031179275 @default.
• W2078460887 cites W2036806258 @default.
• W2078460887 cites W2036902403 @default.
• W2078460887 cites W2037548627 @default.
• W2078460887 cites W2038101582 @default.
• W2078460887 cites W2038935310 @default.
• W2078460887 cites W2041561966 @default.
• W2078460887 cites W2046380289 @default.
• W2078460887 cites W2053258667 @default.
• W2078460887 cites W2059814779 @default.
• W2078460887 cites W2063447809 @default.
• W2078460887 cites W2066990534 @default.
• W2078460887 cites W2068962850 @default.
• W2078460887 cites W2076494303 @default.
• W2078460887 cites W2079585743 @default.
• W2078460887 cites W2092434381 @default.
• W2078460887 cites W2101153440 @default.
• W2078460887 cites W2111817932 @default.
• W2078460887 cites W2113922560 @default.
• W2078460887 cites W2142220522 @default.
• W2078460887 cites W2142243016 @default.
• W2078460887 cites W2157604520 @default.
• W2078460887 cites W2162657839 @default.
• W2078460887 cites W2321762544 @default.
• W2078460887 cites W2617090628 @default.
• W2078460887 cites W2625830509 @default.
• W2078460887 cites W2950173210 @default.
• W2078460887 cites W3099430740 @default.
• W2078460887 cites W3101410207 @default.
• W2078460887 cites W3102531523 @default.
• W2078460887 cites W3102548583 @default.
• W2078460887 cites W3103788665 @default.
• W2078460887 cites W3104274208 @default.
• W2078460887 cites W3104914256 @default.
• W2078460887 cites W3122448116 @default.
• W2078460887 cites W3122799484 @default.
• W2078460887 cites W3124888198 @default.
• W2078460887 cites W4230099094 @default.
• W2078460887 cites W4296153596 @default.
• W2078460887 cites W4301195314 @default.
• W2078460887 doi "https://doi.org/10.1093/mnras/stu2496" @default.
• W2078460887 hasPublicationYear "2014" @default.
• W2078460887 type Work @default.
• W2078460887 sameAs 2078460887 @default.
• W2078460887 citedByCount "10" @default.
• W2078460887 countsByYear W20784608872015 @default.
• W2078460887 countsByYear W20784608872016 @default.
• W2078460887 countsByYear W20784608872018 @default.
• W2078460887 countsByYear W20784608872020 @default.
• W2078460887 countsByYear W20784608872021 @default.
• W2078460887 countsByYear W20784608872022 @default.
• W2078460887 crossrefType "journal-article" @default.
• W2078460887 hasAuthorship W2078460887A5044483582 @default.
• W2078460887 hasAuthorship W2078460887A5080665198 @default.
• W2078460887 hasAuthorship W2078460887A5081882010 @default.
• W2078460887 hasBestOaLocation W20784608872 @default.
• W2078460887 hasConcept C101991246 @default.
• W2078460887 hasConcept C120665830 @default.
• W2078460887 hasConcept C121332964 @default.
• W2078460887 hasConcept C1276947 @default.
• W2078460887 hasConcept C174802034 @default.
• W2078460887 hasConcept C178635117 @default.
• W2078460887 hasConcept C206564472 @default.
• W2078460887 hasConcept C207297109 @default.

• next