<transcript><audio_15> llamamos una curva de luz. Ok, la imagen que les mostré anterior, esta es una estrella que se llama Beta Cepheus, es la segunda estrella</transcript><transcript><audio_16> es como, se le podría llamar como un mapa, un mapa para ubicar las estrellas. En el centro, no sé si ven una crucita, ¿sí? En el centro se encuentra la estrella que nosotros queremos observar, ¿sí? Ah,</transcript><transcript><audio_17> las llegan, pero alrededor hay numeritos, hay puntitos con numeritos. Todos esos puntitos con numeritos son estrellas de referencia. ¿Por qué? Porque como nosotros queremos saber cómo varía el</transcript><transcript><audio_18> pues obviamente necesitamos una estrella de referencia. Y bueno, ahí al menos en este mapa, por así decirlo, pues nos dan todas esas estrellas.</transcript><caption><image_19>The image shows a room with a projector screen in the center. The screen displays a map with various geographical features such as mountains, rivers, and cities. The text on the screen is in Portuguese and appears to be explaining the map. On the right side of the screen, there are two flags, one of the United States and the other of the Philippines. The room has a tiled floor and a white wall with a coat of arms hanging on it. There is a person standing in front of the projector screen, looking at the screen.</caption><transcript><audio_20> poder hacer la fotometría. Y en esta imagen es la curva de luz de Beta Cfeo. En la parte de abajo tenemos días julianos.</transcript><transcript><audio_21> la magnitud en el visual. Otra forma de observar estrellas es a través del espectro. Básicamente lo que hacemos es observar cómo cambia</transcript> is what we call a light curve ok the image that I will show you above this is a star that is  called veins efe it is the second brightest star thing that you see there is what you could call it like a map a map to locate the stars in the center it is not served in a cross and it is in the  In the center is the star that we want to observe, yes, and surely they won't reach them, but around there are little numbers, there are little dots with little numbers, all those little dots with little numbers are reference stars because, since we want to know how the brightness of a star varies, we obviously need a star.  reference yes and well there is at least in this one on this map so to speak because they give us all those reference stars to be able to do the and in this image it is the light curve of efe veins or at the bottom we have Díaz Julián  os and this on the axis and we have the magnitude another way to observe stars is through the spectrum basically what we do is observe how the
{"source": "grass-yt-cc-by.-mVz_7eGh_g|shard_10033_41|create_multimodal_data.extract_yt_and_generate_transcripts.63|shard_10033|create_multimodal_data.generate_captions.53|shard_10033|create_multimodal_data.generate_captions.65", "params": {"id": "-mVz_7eGh_g", "channel_id": "UCIuRHuJbfeXtHvXFDcrNc4g", "duration": 2455, "view_count": 92, "age_limit": 0, "like_count": 4, "channel_follower_count": 917, "license": "Creative Commons Attribution license (reuse allowed)", "uploader_id": "@fisicauaz", "yt_tar_file": "/leonardo_work/EUHPC_E03_068/audio/fixed_download/grass-yt-cc-by//shard_10033/-mVz_7eGh_g.tar.gz"}}