

Vedant Chandra
725 posts

@vedantchandra
proto-astronomer @Harvard @CenterForAstro @mpi_astro | previously @JohnsHopkins @STScI |



while biasing mass estimates too high. Left: Wolf+ 2010 mass estimates compared to NFW profiles. Right: mass estimates for the *same galaxies* if outer stars below a certain effective surface brightness are removed. The galaxies are incorrectly placed in more massive halos. (3/6)







Detecting the first stars (PopIII) is a long-held dream for astronomers. We developed a novel technique, applied it to JWST legacy data, and discovered a promising PopIII galaxy candidate at z=6.5 in GLIMPSE!



















Putting everything together, we can use the full kinematics of our sample to infer the motion of the inner MW relative to the outer halo: the Milky Way is lurching towards a recent location along the LMC's orbit at over 40 kilometers per second!