[{"id": 611380, "created": "2025-07-27T19:05:55.523295", "project_id": 302, "task_id": 651093, "user_id": 315, "user_ip": null, "finish_time": "2025-07-27T19:06:54.302755", "timeout": null, "calibration": null, "external_uid": null, "media_url": null, "info": {"id": 37, "url": "https://en.wikinews.org/wiki/Sun%27s_mood_swings_not_so_strange_after_all,_say_scientists", "topic": "sciece", "domain": "wikinews", "clarity": "clear", "has_image": "yes", "iso_639_3": "hin", "glottocode": "hind1269", "faithfulness": "faithful", "last_updated": "1.0", "plausibility": "plausible", "has_hyperlink": "yes", "src_iso_15924": "Latn", "src_iso_639_3": "eng", "tar_iso_15924": "Deva", "tar_iso_639_3": "hin", "text_eng_Latn": "The luminosity and rotation are used together to determine a star's Rossby number, which is related to plasma flow.", "text_hin_Deva": "\u090f\u0915 \u0924\u093e\u0930\u0947 \u0915\u0940 \u0930\u0949\u0938\u094d\u092c\u0940 \u0938\u0902\u0916\u094d\u092f\u093e, \u091c\u094b \u092a\u094d\u0932\u093e\u091c\u093c\u094d\u092e\u093e \u092b\u093c\u094d\u0932\u094b \u0938\u0947 \u0938\u0902\u092c\u0902\u0927\u093f\u0924 \u0939\u0948, \u0915\u093e \u092a\u0924\u093e \u0932\u0917\u093e\u0928\u0947 \u0915\u0947 \u0932\u093f\u090f \u0909\u0938\u0915\u0940 \u091a\u092e\u0915 \u0914\u0930 \u0930\u094b\u091f\u0947\u0936\u0928 \u0915\u093e \u090f\u0915 \u0938\u093e\u0925 \u0907\u0938\u094d\u0924\u0947\u092e\u093e\u0932 \u0915\u093f\u092f\u093e \u091c\u093e\u0924\u093e \u0939\u0948,", "informativeness": "very_informative"}}, {"id": 618017, "created": "2025-08-10T12:23:46.639668", "project_id": 302, "task_id": 651093, "user_id": 325, "user_ip": null, "finish_time": "2025-08-10T12:24:32.984235", "timeout": null, "calibration": null, "external_uid": null, "media_url": null, "info": {"id": 37, "url": "https://en.wikinews.org/wiki/Sun%27s_mood_swings_not_so_strange_after_all,_say_scientists", "topic": "sciece", "domain": "wikinews", "clarity": "very_clear", "has_image": "yes", "iso_639_3": "hin", "glottocode": "hind1269", "faithfulness": "very_faithful", "last_updated": "1.0", "plausibility": "highly_plausible", "has_hyperlink": "yes", "src_iso_15924": "Latn", "src_iso_639_3": "eng", "tar_iso_15924": "Deva", "tar_iso_639_3": "hin", "text_eng_Latn": "The luminosity and rotation are used together to determine a star's Rossby number, which is related to plasma flow.", "text_hin_Deva": "\u090f\u0915 \u0924\u093e\u0930\u0947 \u0915\u0940 \u0930\u0949\u0938\u094d\u092c\u0940 \u0938\u0902\u0916\u094d\u092f\u093e, \u091c\u094b \u092a\u094d\u0932\u093e\u091c\u093c\u094d\u092e\u093e \u092b\u093c\u094d\u0932\u094b \u0938\u0947 \u0938\u0902\u092c\u0902\u0927\u093f\u0924 \u0939\u0948, \u0915\u093e \u092a\u0924\u093e \u0932\u0917\u093e\u0928\u0947 \u0915\u0947 \u0932\u093f\u090f \u0909\u0938\u0915\u0940 \u091a\u092e\u0915 \u0914\u0930 \u0930\u094b\u091f\u0947\u0936\u0928 \u0915\u093e \u090f\u0915 \u0938\u093e\u0925 \u0907\u0938\u094d\u0924\u0947\u092e\u093e\u0932 \u0915\u093f\u092f\u093e \u091c\u093e\u0924\u093e \u0939\u0948,", "informativeness": "informative"}}]