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Spectroscopically Identified Emission Line Galaxy Pairs in the WISP survey
Y. Sophia Dai, Matthew M. Malkan, Harry I. Teplitz +20
We identify a sample of spectroscopically measured emission line galaxy (ELG) pairs up to z=1.6 from the WFC3 Infrared Spectroscopic Parallels (WISP) survey. WISP obtained slitless…
How identifying circumgalactic gas by line-of-sight velocity instead of the location in 3D space affects O VI measurements
Stephanie H. Ho, Crystal L. Martin, Joop Schaye
The high incidence rate of the O VI 1032,1038 absorption around low-redshift, star-forming galaxies has generated interest in studies of the circumgalactic medium.…
The mass-metallicity relation at z~1-2 and its dependence on star formation rate
Alaina Henry, Marc Rafelski, Ben Sunnquist +24
We present a new measurement of the gas-phase mass-metallicity relation (MZR), and its dependence on star formation rates (SFRs) at 1.3 < z < 2.3. Our sample comprises 1056 galaxie…
Disentangling the physical origin of emission line ratio offsets at high redshift with spatially resolved spectroscopy
Jessie Hirtenstein, Tucker Jones, Ryan L. Sanders +6
We present spatially resolved Hubble Space Telescope grism spectroscopy of 15 galaxies at drawn from the DEEP2 survey. We analyze H+[N II], [S II] and [S III] emissio…
Connecting Galactic Outflows and Star Formation: Inferences from H-alpha Maps and Absorption Line Spectroscopy at 1 < z < 1.5
Nikolaus Z. Prusinski, Dawn K. Erb, Crystal L. Martin
We investigate the connection between galactic outflows and star formation using two independent data sets covering a sample of 22 galaxies between . The…