Calendar

Nov
6
Mon
ASTR 535 – Observational Techniques I
Nov 6 @ 9:30 am – 10:20 am
ASTR 670 – Heliophysics
Nov 6 @ 11:00 am – 12:15 pm
Pizza Lunch: Ethan Dederick
Nov 6 @ 12:30 pm – 1:30 pm
Pizza Lunch: Ethan Dederick @ AY 119

Cool Science Results

Nov
7
Tue
ASTR 565 – Stellar Interiors
Nov 7 @ 11:45 am – 1:00 pm
Astro-ph Discussion
Nov 7 @ 2:30 pm – 3:00 pm
Astro-ph Discussion @ AY119
Nov
8
Wed
ASTR 535 – Observational Techniques I
Nov 8 @ 9:30 am – 10:20 am
ASTR 670 – Heliophysics
Nov 8 @ 11:00 am – 12:15 pm
Astro-ph Discussion
Nov 8 @ 2:30 pm – 3:00 pm
Astro-ph Discussion @ AY119
Nov
9
Thu
ASTR 565 – Stellar Interiors
Nov 9 @ 11:45 am – 1:00 pm
Special Pizza Lunch: Jane Rigby
Nov 9 @ 1:00 pm – 2:00 pm
Special Pizza Lunch: Jane Rigby @ AY 119

Galaxy Evolution in High Definition Via Gravitational Lensing

Dr. Jane Rigby

Deputy Project Scientist for JWST, NASA Goddard Space Flight Center

Abstract: In hundreds of known cases, “gravitational lenses” have deflected, distorted, and amplified images of galaxies or quasars behind them.  As such, gravitational lensing is a way to “cheat” at studying how galaxies evolve:  lensing can magnify galaxies by factors of 10–100 times, transforming them from objects we can barely detect to bright objects we can study in detail.   For such rare objects, we are studying how galaxies formed stars at redshifts of 1–4, the epoch when most of the Universe’s stars were formed. For lensed galaxies, we can obtained spectral diagnostics that are currently unavailable for the distant universe, but will become routine with next-generation telescopes.

In particular, I’ll discuss MEGaSaURA, The Magellan Evolution of Galaxies Spectroscopic and Ultraviolet Reference Atlas, which comprises high signal-to-noise, medium spectral resolution (R~3300) spectra of 15 extremely bright gravitationally lensed galaxies at redshifts of 1.6<z<3.6.   The sample, drawn from the SDSS Giant Arcs Survey, are many of the brightest lensed galaxies known.  The MEGaSaURA spectra reveal a wealth of spectral diagnostics: absorption from the outflowing wind; nebular emission lines that will be key diagnostics for JWST, GMT, and TMT; and photospheric absorption lines and P Cygni profiles from the massive stars that power the outflow.