Fast interferometric data from the Very Large Array for Fast Radio Burst FRB 190520
<|begin_of_text|><|start_header_id|>system<|end_header_id|> You are a research archivist expert in dataset metadata. Answer the question truthfully.  <|eot_id|><|start_header_id|>user<|end_header_id|> Here is the Description of a dataset. Description:'Data products to support reproduction of the interferometric localization of Fast Radio Burst 190520.The principle data products are tar files of fast-sampled interferometric data from the Very Large Array (download separately to avoid dataverse file size limit). Each observation segment includes a few seconds of visibilities centered on a radio burst from FRB 190520. Data is in science data model (SDM) format, which consists of a directory with metadata in XML files and binary data in the ASDMBinary subdirectory. Binary data were recorded with an integration time of 10 ms and dual-circular polarizations. Each file is identified by a unique name of the observation, plus the observation start time in MJD. Each visibility data set is associated with one of the calibration files with the same MJD (telcal format; ending in '.GN') that can' . Please return only a json list of at most 3 Keywords corresponding to the Description:.<|eot_id|><|start_header_id|>assistant<|end_header_id|> {"Answer" : ["fast radio burst","interferometry","radio astronomy"]} <|eot_id|>
 Here is the Description of a dataset. Description:'Data products to support reproduction of the interferometric localization of Fast Radio Burst 190520.The principle data products are tar files of fast-sampled interferometric data from the Very Large Array (download separately to avoid dataverse file size limit). Each observation segment includes a few seconds of visibilities centered on a radio burst from FRB 190520. Data is in science data model (SDM) format, which consists of a directory with metadata in XML files and binary data in the ASDMBinary subdirectory. Binary data were recorded with an integration time of 10 ms and dual-circular polarizations. Each file is identified by a unique name of the observation, plus the observation start time in MJD. Each visibility data set is associated with one of the calibration files with the same MJD (telcal format; ending in '.GN') that can' . Please return only a json list of at most 3 Keywords corresponding to the Description:.
Data products to support reproduction of the interferometric localization of Fast Radio Burst 190520.The principle data products are tar files of fast-sampled interferometric data from the Very Large Array (download separately to avoid dataverse file size limit). Each observation segment includes a few seconds of visibilities centered on a radio burst from FRB 190520. Data is in science data model (SDM) format, which consists of a directory with metadata in XML files and binary data in the ASDMBinary subdirectory. Binary data were recorded with an integration time of 10 ms and dual-circular polarizations. Each file is identified by a unique name of the observation, plus the observation start time in MJD. Each visibility data set is associated with one of the calibration files with the same MJD (telcal format; ending in '.GN') that can
fast radio burst; interferometry; radio astronomy