Science with the WEAVE-LOFAR Survey

Shravya正在努力利用低频射电选择(使用LOFAR两米天文测量)和使用新的WEAVE频谱设施获得的100多万个频谱的变革性组合，作为WEAVE-LOFAR测量的一部分。她已经开始利用多波长数据集确定影响恒星形成率射电光度关系的因素，一旦编织-LOFAR数据在2022年底开始到达，一系列不同的方向是可能的。

Shravya is working on exploiting the transformational combination of low-frequency radio selection (using the LOFAR two-metre sky survey) and more than a million spectra obtained using the new WEAVE spectroscopic facility as part of the WEAVE-LOFAR survey. She has started to work on determining the forces shaping the star formation rate radio luminosity relation using multiwavelength data sets, and a range of different directions are possible once the WEAVE-LOFAR data begin to arrive at the end of 2022.