FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3126144573> ?p ?o ?g. }

• W3126144573 endingPage "23" @default.
• W3126144573 startingPage "11" @default.
• W3126144573 abstract "We report the discovery of the optical and near-infrared counterparts to GRB 001011. The GRB 001011 error box determined by Beppo-SAX was simultaneously imaged in the near-infrared by the 3.58-m New Technology Telescope and in the optical by the 1.54-m Danish Telescope ~8 hr after the gamma-ray event. Here we implement the colour-colour discrimination technique proposed by Rhoads ([CITE]) and extend it using near-IR data as well. We present the results provided by an automatic colour-colour discrimination pipe-line developed to discern the different populations of objects present in the GRB 001011 error box. Our software revealed three candidates based on single-epoch images. Second-epoch observations carried out ~3.2 days after the burst revealed that the most likely candidate had faded, thus identifying it with the counterpart to the GRB. In deep R-band images obtained 7 months after the burst a faint () elongated object, presumably the host galaxy of GRB 001011, was detected at the position of the afterglow. The GRB 001011 afterglow is the first discovered with the assistance of colour-colour diagram techniques. We discuss the advantages of using this method and its application to error boxes determined by future missions." @default.
• W3126144573 created "2021-02-01" @default.
• W3126144573 creator A5000383073 @default.
• W3126144573 creator A5001557702 @default.
• W3126144573 creator A5006347940 @default.
• W3126144573 creator A5009212329 @default.
• W3126144573 creator A5013979618 @default.
• W3126144573 creator A5015282171 @default.
• W3126144573 creator A5015837326 @default.
• W3126144573 creator A5020170655 @default.
• W3126144573 creator A5024232124 @default.
• W3126144573 creator A5029524464 @default.
• W3126144573 creator A5037496050 @default.
• W3126144573 creator A5040689025 @default.
• W3126144573 creator A5042154966 @default.
• W3126144573 creator A5044841126 @default.
• W3126144573 creator A5047037347 @default.
• W3126144573 creator A5048353300 @default.
• W3126144573 creator A5049622471 @default.
• W3126144573 creator A5055371146 @default.
• W3126144573 creator A5055517739 @default.
• W3126144573 creator A5058199394 @default.
• W3126144573 creator A5060377458 @default.
• W3126144573 creator A5068204153 @default.
• W3126144573 creator A5073071738 @default.
• W3126144573 creator A5079431206 @default.
• W3126144573 creator A5083123082 @default.
• W3126144573 creator A5085670376 @default.
• W3126144573 creator A5087925506 @default.
• W3126144573 creator A5091011269 @default.
• W3126144573 date "2002-03-01" @default.
• W3126144573 modified "2023-10-15" @default.
• W3126144573 title "Strategies for prompt searches for GRB afterglows: The discovery of the GRB 001011 optical/near-infrared counterpart using colour-colour selection" @default.
• W3126144573 cites W1604778255 @default.
• W3126144573 cites W1645847612 @default.
• W3126144573 cites W1658820183 @default.
• W3126144573 cites W1896972225 @default.
• W3126144573 cites W1913860194 @default.
• W3126144573 cites W1966885955 @default.
• W3126144573 cites W1968746069 @default.
• W3126144573 cites W1981205161 @default.
• W3126144573 cites W1981847637 @default.
• W3126144573 cites W1983607761 @default.
• W3126144573 cites W1991465935 @default.
• W3126144573 cites W1994454575 @default.
• W3126144573 cites W1997255077 @default.
• W3126144573 cites W2000477601 @default.
• W3126144573 cites W2012056991 @default.
• W3126144573 cites W2013110124 @default.
• W3126144573 cites W2024223537 @default.
• W3126144573 cites W2030154533 @default.
• W3126144573 cites W2031042483 @default.
• W3126144573 cites W2035661619 @default.
• W3126144573 cites W2035879704 @default.
• W3126144573 cites W2039817747 @default.
• W3126144573 cites W2043235990 @default.
• W3126144573 cites W2055820250 @default.
• W3126144573 cites W2067089387 @default.
• W3126144573 cites W2070584376 @default.
• W3126144573 cites W2070722652 @default.
• W3126144573 cites W2074747635 @default.
• W3126144573 cites W2075883630 @default.
• W3126144573 cites W2080697714 @default.
• W3126144573 cites W2082616294 @default.
• W3126144573 cites W2110974585 @default.
• W3126144573 cites W2111817932 @default.
• W3126144573 cites W2114951275 @default.
• W3126144573 cites W2121015243 @default.
• W3126144573 cites W2129966461 @default.
• W3126144573 cites W2132174891 @default.
• W3126144573 cites W2143803573 @default.
• W3126144573 cites W2143905502 @default.
• W3126144573 cites W2163765120 @default.
• W3126144573 cites W2165084703 @default.
• W3126144573 cites W2168204758 @default.
• W3126144573 cites W2170344725 @default.
• W3126144573 cites W2331282111 @default.
• W3126144573 cites W2599165762 @default.
• W3126144573 cites W2952250576 @default.
• W3126144573 cites W2963075213 @default.
• W3126144573 cites W2983493793 @default.
• W3126144573 cites W3101021073 @default.
• W3126144573 cites W3104298768 @default.
• W3126144573 cites W3105340307 @default.
• W3126144573 cites W3105502586 @default.
• W3126144573 cites W4289253751 @default.
• W3126144573 doi "https://doi.org/10.1051/0004-6361:20011598" @default.
• W3126144573 hasPublicationYear "2002" @default.
• W3126144573 type Work @default.
• W3126144573 sameAs 3126144573 @default.
• W3126144573 citedByCount "17" @default.
• W3126144573 countsByYear W31261445732015 @default.
• W3126144573 countsByYear W31261445732019 @default.
• W3126144573 crossrefType "journal-article" @default.
• W3126144573 hasAuthorship W3126144573A5000383073 @default.
• W3126144573 hasAuthorship W3126144573A5001557702 @default.
• W3126144573 hasAuthorship W3126144573A5006347940 @default.
• W3126144573 hasAuthorship W3126144573A5009212329 @default.

• next