FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2146255680> ?p ?o ?g. }

• W2146255680 abstract "We present the work developed within the science team of the Very Large Telescope Interferometer Spectro-Imager (VSI) during the Phase A studies. VSI aims at delivering ~ 1 milliarcsecond resolution data cubes in the near-infrared, with several spectral resolutions up to 12 000, by combining up to 8 VLTI telescopes. In the design of an instrument, the science case plays a central role by supporting the instrument construction decision, defining the top-level requirements and balancing design options. The overall science philosophy of VSI was that of a general user instrument serving a broad community. The science team addressed themes which included several areas of astrophysics and illustrated specific modes of operation of the instrument: a) YSO disks and winds; b) Multiplicity of young stars; c) Exoplanets; d) Debris disks; e) Stellar surface imaging; f) The environments of evolved stars; g) AGN tori; h) AGN's Broad Line Region; i) Supermassive black-holes; and j) Microlensing. The main conclusions can be summarized as follows: a) The accessible targets and related science are extremely sensitive to the instrument limiting magnitude; the instrument should be optimized for sensitivity and have its own fringe tracker. b) Most of the science cases are readily achievable with on-axis fringe tracking, off-axis fringe tracking enabling extra science. c) In most targets (YSOs, evolved stars and AGNs), the interpretation and analysis of circumstellar/nuclear dust morphology requires direct access to the gas via spectral resolved studies of emission lines, requiring at least a spectral resolution of 2 500. d) To routinely deliver images at the required sensitivity, the number of telescopes in determinant, with 6 telescopes being favored. e) The factorial increase in the number of closure phases and visibilities, gained in a single observation, makes massive surveys of parameters and related science for the first time possible. f) High dynamic range imaging and very high dynamic range differential closure phase are possible allowing the study of debris disks and characterization of pegasides. g) Spectro-imaging in the near-infrared is highly complementary to ALMA, adaptive optics and interferometric imaging in the thermal infrared." @default.
• W2146255680 created "2016-06-24" @default.
• W2146255680 creator A5000384663 @default.
• W2146255680 creator A5001982498 @default.
• W2146255680 creator A5003972178 @default.
• W2146255680 creator A5008100631 @default.
• W2146255680 creator A5010821359 @default.
• W2146255680 creator A5011405198 @default.
• W2146255680 creator A5015544930 @default.
• W2146255680 creator A5020754900 @default.
• W2146255680 creator A5020853714 @default.
• W2146255680 creator A5022012017 @default.
• W2146255680 creator A5027255654 @default.
• W2146255680 creator A5029367093 @default.
• W2146255680 creator A5029595425 @default.
• W2146255680 creator A5030634186 @default.
• W2146255680 creator A5033009567 @default.
• W2146255680 creator A5034337260 @default.
• W2146255680 creator A5034701856 @default.
• W2146255680 creator A5036040105 @default.
• W2146255680 creator A5036632849 @default.
• W2146255680 creator A5041770370 @default.
• W2146255680 creator A5043157830 @default.
• W2146255680 creator A5043902535 @default.
• W2146255680 creator A5045015912 @default.
• W2146255680 creator A5058111055 @default.
• W2146255680 creator A5060123759 @default.
• W2146255680 creator A5060830225 @default.
• W2146255680 creator A5061705666 @default.
• W2146255680 creator A5061759484 @default.
• W2146255680 creator A5061947430 @default.
• W2146255680 creator A5065652129 @default.
• W2146255680 creator A5066862766 @default.
• W2146255680 creator A5067537085 @default.
• W2146255680 creator A5069079247 @default.
• W2146255680 creator A5070753051 @default.
• W2146255680 creator A5071423484 @default.
• W2146255680 creator A5071812644 @default.
• W2146255680 creator A5073396149 @default.
• W2146255680 creator A5077516181 @default.
• W2146255680 creator A5078703670 @default.
• W2146255680 creator A5079619306 @default.
• W2146255680 creator A5083476174 @default.
• W2146255680 creator A5086150954 @default.
• W2146255680 creator A5087786912 @default.
• W2146255680 creator A5088464138 @default.
• W2146255680 creator A5089846654 @default.
• W2146255680 creator A5090229583 @default.
• W2146255680 date "2008-07-14" @default.
• W2146255680 modified "2023-10-18" @default.
• W2146255680 title "Science case for 1 mas spectro-imagining in the near-infrared" @default.
• W2146255680 cites W1606086464 @default.
• W2146255680 cites W2005467021 @default.
• W2146255680 cites W2026926262 @default.
• W2146255680 cites W2043059855 @default.
• W2146255680 cites W2065864905 @default.
• W2146255680 cites W2135894620 @default.
• W2146255680 cites W2145214706 @default.
• W2146255680 doi "https://doi.org/10.1117/12.789216" @default.
• W2146255680 hasPublicationYear "2008" @default.
• W2146255680 type Work @default.
• W2146255680 sameAs 2146255680 @default.
• W2146255680 citedByCount "0" @default.
• W2146255680 crossrefType "proceedings-article" @default.
• W2146255680 hasAuthorship W2146255680A5000384663 @default.
• W2146255680 hasAuthorship W2146255680A5001982498 @default.
• W2146255680 hasAuthorship W2146255680A5003972178 @default.
• W2146255680 hasAuthorship W2146255680A5008100631 @default.
• W2146255680 hasAuthorship W2146255680A5010821359 @default.
• W2146255680 hasAuthorship W2146255680A5011405198 @default.
• W2146255680 hasAuthorship W2146255680A5015544930 @default.
• W2146255680 hasAuthorship W2146255680A5020754900 @default.
• W2146255680 hasAuthorship W2146255680A5020853714 @default.
• W2146255680 hasAuthorship W2146255680A5022012017 @default.
• W2146255680 hasAuthorship W2146255680A5027255654 @default.
• W2146255680 hasAuthorship W2146255680A5029367093 @default.
• W2146255680 hasAuthorship W2146255680A5029595425 @default.
• W2146255680 hasAuthorship W2146255680A5030634186 @default.
• W2146255680 hasAuthorship W2146255680A5033009567 @default.
• W2146255680 hasAuthorship W2146255680A5034337260 @default.
• W2146255680 hasAuthorship W2146255680A5034701856 @default.
• W2146255680 hasAuthorship W2146255680A5036040105 @default.
• W2146255680 hasAuthorship W2146255680A5036632849 @default.
• W2146255680 hasAuthorship W2146255680A5041770370 @default.
• W2146255680 hasAuthorship W2146255680A5043157830 @default.
• W2146255680 hasAuthorship W2146255680A5043902535 @default.
• W2146255680 hasAuthorship W2146255680A5045015912 @default.
• W2146255680 hasAuthorship W2146255680A5058111055 @default.
• W2146255680 hasAuthorship W2146255680A5060123759 @default.
• W2146255680 hasAuthorship W2146255680A5060830225 @default.
• W2146255680 hasAuthorship W2146255680A5061705666 @default.
• W2146255680 hasAuthorship W2146255680A5061759484 @default.
• W2146255680 hasAuthorship W2146255680A5061947430 @default.
• W2146255680 hasAuthorship W2146255680A5065652129 @default.
• W2146255680 hasAuthorship W2146255680A5066862766 @default.
• W2146255680 hasAuthorship W2146255680A5067537085 @default.
• W2146255680 hasAuthorship W2146255680A5069079247 @default.
• W2146255680 hasAuthorship W2146255680A5070753051 @default.
• W2146255680 hasAuthorship W2146255680A5071423484 @default.
• W2146255680 hasAuthorship W2146255680A5071812644 @default.

• next