![UR #21: Confirmation of Broadband Selection of Extreme [OIII] Emitters at z~0.5](https://astrobites.org/wp-content/uploads/2020/06/EELG-320x260.jpg)
UR #21: Confirmation of Broadband Selection of Extreme [OIII] Emitters at z~0.5
This month’s undergraduate research post features a student who looked at statistically improving extreme emission line galaxy identification in wide field surveys.
Dwarf Galaxies at the cutting EDGE of galaxy formation
What can we use dwarf galaxies for?
How Do You Weigh a Galaxy?
How much does our galaxy weigh? The authors of today’s paper use globular clusters in the halo of the galaxy to try to answer this question!
Twinkle, Twinkle, Little Quasar
Can the ‘twinkle’ of an infrared source be used to find AGN?
A Stellar M-SFR-Z Relation MOSt DEFinitely Exists at z~2.3
Is there a M∗-SFR-Z relation at high redshift? Yep! Read me to find how it was discovered!
Shaken, Not Stirred: Subgrid Metal Diffusion in Galaxy Simulations
A lot of physics happens below the resolution limit of galaxy simulations that must be represented with “subgrid” models. Today’s paper shows the importance of including a subgrid model for the mixing of metals in galaxy simulations.