FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4283389473> ?p ?o ?g. }

• W4283389473 abstract "We investigate the possibility of fast radio burst (FRB) observation on new special geodetic 13[Formula: see text]m wideband radio telescopes in Very Large Base Interferometry (VLBI) and single-dish modes. The Crab Pulsar Giant Pulses (GPs) were used as a reference source of FRB. In order to verify our results we use joint simultaneous observations with 32[Formula: see text]m legacy and 13[Formula: see text]m new VLBI Global Observing System (VGOS) radio telescopes of the Quasar VLBI network in the L and S/X frequency bands. The special observation session contains two 10-min scans of Crab Pulsar. We successfully detect a total of 712 pulses with flux density [Formula: see text][Formula: see text]Jy at 1653.5[Formula: see text]MHz on 32-m antenna and 262 pulses with flux density [Formula: see text][Formula: see text]Jy at 2406.3[Formula: see text]MHz on 13-m antenna in Badary observatory. The VLBI fringes were obtained for approximately every third pulse. The energy distribution of detected pulses has a break in the power law fit at [Formula: see text] and [Formula: see text]-values are [Formula: see text]0.2 and [Formula: see text]1.8 for lower and higher energies. A GP with a fluence of the order of 190[Formula: see text][Formula: see text] in L-band was detected and 48[Formula: see text][Formula: see text] in S-band. We found that the peak coincidence of right and left circular polarizations of dedispersed data on a single antenna can provide a maximum detection rate with fixed false probability. It was shown that the best GP detection rate on 13[Formula: see text]m VGOS radio telescope was achieved at Badary observatory with 13 pulses per minute in the S-band." @default.
• W4283389473 created "2022-06-25" @default.
• W4283389473 creator A5021349163 @default.
• W4283389473 creator A5072707749 @default.
• W4283389473 date "2022-07-27" @default.
• W4283389473 modified "2023-09-26" @default.
• W4283389473 title "Probing the New Generation Geodetic Radio Telescopes for FRB Observations" @default.
• W4283389473 cites W1601277342 @default.
• W4283389473 cites W1669489440 @default.
• W4283389473 cites W177930392 @default.
• W4283389473 cites W1967953542 @default.
• W4283389473 cites W1972013583 @default.
• W4283389473 cites W1973820399 @default.
• W4283389473 cites W1979306856 @default.
• W4283389473 cites W1981952207 @default.
• W4283389473 cites W1990311414 @default.
• W4283389473 cites W2050306203 @default.
• W4283389473 cites W2055704529 @default.
• W4283389473 cites W2091339103 @default.
• W4283389473 cites W2135625048 @default.
• W4283389473 cites W2279504778 @default.
• W4283389473 cites W2323329379 @default.
• W4283389473 cites W2509710860 @default.
• W4283389473 cites W2563744641 @default.
• W4283389473 cites W2592916001 @default.
• W4283389473 cites W2794558609 @default.
• W4283389473 cites W2885390567 @default.
• W4283389473 cites W2887307977 @default.
• W4283389473 cites W2902341323 @default.
• W4283389473 cites W2902412678 @default.
• W4283389473 cites W2975306330 @default.
• W4283389473 cites W3098071475 @default.
• W4283389473 cites W3099051975 @default.
• W4283389473 cites W3099186512 @default.
• W4283389473 cites W3099614782 @default.
• W4283389473 cites W3104971983 @default.
• W4283389473 cites W3105690826 @default.
• W4283389473 cites W3106210156 @default.
• W4283389473 cites W3141689353 @default.
• W4283389473 cites W3157331758 @default.
• W4283389473 cites W3177890725 @default.
• W4283389473 cites W3182008403 @default.
• W4283389473 cites W3201398336 @default.
• W4283389473 cites W4214933114 @default.
• W4283389473 cites W4220913758 @default.
• W4283389473 doi "https://doi.org/10.1142/s2251171722500155" @default.
• W4283389473 hasPublicationYear "2022" @default.
• W4283389473 type Work @default.
• W4283389473 citedByCount "0" @default.
• W4283389473 crossrefType "journal-article" @default.
• W4283389473 hasAuthorship W4283389473A5021349163 @default.
• W4283389473 hasAuthorship W4283389473A5072707749 @default.
• W4283389473 hasConcept C110363677 @default.
• W4283389473 hasConcept C121332964 @default.
• W4283389473 hasConcept C135041427 @default.
• W4283389473 hasConcept C192887742 @default.
• W4283389473 hasConcept C2776409865 @default.
• W4283389473 hasConcept C2778538162 @default.
• W4283389473 hasConcept C2781282464 @default.
• W4283389473 hasConcept C44870925 @default.
• W4283389473 hasConcept C79896159 @default.
• W4283389473 hasConcept C98444146 @default.
• W4283389473 hasConceptScore W4283389473C110363677 @default.
• W4283389473 hasConceptScore W4283389473C121332964 @default.
• W4283389473 hasConceptScore W4283389473C135041427 @default.
• W4283389473 hasConceptScore W4283389473C192887742 @default.
• W4283389473 hasConceptScore W4283389473C2776409865 @default.
• W4283389473 hasConceptScore W4283389473C2778538162 @default.
• W4283389473 hasConceptScore W4283389473C2781282464 @default.
• W4283389473 hasConceptScore W4283389473C44870925 @default.
• W4283389473 hasConceptScore W4283389473C79896159 @default.
• W4283389473 hasConceptScore W4283389473C98444146 @default.
• W4283389473 hasIssue "03" @default.
• W4283389473 hasLocation W42833894731 @default.
• W4283389473 hasOpenAccess W4283389473 @default.
• W4283389473 hasPrimaryLocation W42833894731 @default.
• W4283389473 hasRelatedWork W1968312381 @default.
• W4283389473 hasRelatedWork W2014334174 @default.
• W4283389473 hasRelatedWork W2035984952 @default.
• W4283389473 hasRelatedWork W2068754364 @default.
• W4283389473 hasRelatedWork W2139702176 @default.
• W4283389473 hasRelatedWork W2151560968 @default.
• W4283389473 hasRelatedWork W3102739446 @default.
• W4283389473 hasRelatedWork W3103046839 @default.
• W4283389473 hasRelatedWork W3104025681 @default.
• W4283389473 hasRelatedWork W4220769593 @default.
• W4283389473 hasVolume "11" @default.
• W4283389473 isParatext "false" @default.
• W4283389473 isRetracted "false" @default.
• W4283389473 workType "article" @default.