Resolving H i in damped Lyman α systems that drive star formation

Weinberg, DH, Miralda-Escude, J., Hernquist, L. & Katz, N. A lower bound on cosmic baryon density. Astrophysic. J 490564-570 (1997).
Cen, R. & Ostriker, JP Where are the baryons? Astrophysic. J 5141–6 (1999).
Shull, JM, Smith, BD & Danforth, CW Census of baryons in a multiphase intergalactic medium: 30% of baryons could still be missing. Astrophysic. J 75923 (2012).
Péroux, C. & Howk, JC The cosmic cycles of baryon and metal. Ann. Reverend Astron. Astrophysic. 58363–406 (2020).
Wolfe, AM, Gawiser, E. & Prochaska, JX Damped Lyα systems. Ann. Reverend Astron. Astrophysic. 43861–918 (2005).
Neeleman, M. et al. [C ii] Emission at 158 µm from host galaxies of damped Lyman-alpha systems. Science 3551285-1288 (2017).
Neeleman, M., Prochaska, JX, Kanekar, N. & Rafelski, M. A cold, massive, rotating disk galaxy 1.5 billion years after the Big Bang. Nature 581269-272 (2020).
Prochaska, JX et al. The UCSD/Keck Damped Lyα Abundance Database: A Decade of High-Resolution Spectroscopy. Astrophysic. J. Suppl. Ser. 17129–60 (2007).
Rafelski, M., Wolfe, AM, Prochaska, JX, Neeleman, M. & Mendez, AJ Metallicity evolution of damped Lyα systems towards z ~5. Astrophysic. J 75589 (2012).
Fox, AJ, Petitjean, P., Ledoux, C. & Srianand, R. Multiphase plasma in underdamped Ly α systems: a hidden metal reservoir. Astrophysic. J. Lett. 668L15–L18 (2007).
Morrissey, P. et al. The Keck Cosmic Web Imager integral field spectrograph. Astrophysic. J 86493 (2018).
Koester, BP et al. Two lenses z ~ 3 Lyman Rupture galaxies discovered during the SDSS Giant Arc Study. Astrophysic. J. Lett. 723L73–L77 (2010).
Rigby, JR et al. Spectroscopic and Ultraviolet Reference Atlas of the Magellanic Evolution of Galaxies (MegaSaura). I. The sample and the spectra. Star. J 155104 (2018).
Lopez, S. et al. A clumped, anisotropic galaxy halo at redshift 1 of gravitational arc tomography. Nature 554493–496 (2018).
Péroux, C., Rahmani, H., Battaia, F. & Augustin, R. Spatial resolution metallic gas clouds. Mon. No. R.Astron. Soc. 479L50–L54 (2018).
Rauch, M., Sargent, W., Barlow, T. & Simcoe, R. High redshift small-scale structure. IV. Low ionization gas crossing three lines of sight to Q2237+0305. Astrophysic. J 57645–60 (2002).
Ellison, SL et al. The sizes and the kinematic structure of the absorption systems towards the quasar lens APM08279+5255. Star. Astrophysic. 41479–93 (2004).
Bordoloi, R. et al. Spatially resolved galactic wind in lens galaxy RCSGA 032727-132609. Mon. No. R.Astron. Soc. 4581891-1908 (2016).
Peeples, MS et al. Understanding gases and galaxies in Enzo (FOGGIE). I. Resolution of the simulated circumgalactic absorption at 2 z Astrophysic. J 873129 (2019).
Nelson, D. et al. First results of the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback. Mon. No. R.Astron. Soc. 4903234–3261 (2019).
Mawatari, K. et al. Discovery of a damped Lyα absorber at z = 3.3 along a galaxy line of sight in the SSA22 field. Astrophysic. J 817161 (2016).
Cooke, J. & O’Meara, JM A new constraint on the physical nature of damped Lyman alpha systems. Astrophysic. J. Lett. 812L27 (2015).
Walter, F. et al. THINGS: The HI survey nearby galaxies. Star. J 1362563–2647 (2008).
Broeils, AH & van Woerden, H. A search for spiral galaxies with extended HI discs. Star. Astrophysic. Supplement Ser. 107129-176 (1994).
Zwaan, M. et al. Is the kinematics of DLAs consistent with their appearance in the gas disks of galaxies? Star. J 1362886–2896 (2008).
Krogager, JK et al. Dissection of cold gas in a high redshift galaxy using a lensed background quasar. Star. Astrophysic. 619A142 (2018).
Fumagalli, M., O’Meara, JM, Prochaska, JX, Rafelski, M. & Kanekar, N. Direct imaging of damped Ly α galaxies at z> 2 — III. The star formation rates of neutral gas reservoirs at z~2.7. Mon. No. R.Astron. Soc. 4463178–3198 (2015).
Law, DR et al. The physical nature of UV-rest galaxy morphology during the peak epoch of galaxy formation. Astrophysic. J 6561–26 (2007).
Law, D. et al. An HST/WFC3-IR morphological survey of the galaxies at z=1.5–3.6. I. Description of the study and morphological properties of star-forming galaxies. Astrophysic. J 74585 (2012).
Jacob, JC et al. Montage: a toolbox for mosaicking astronomical images. Astrophysics Source Code Library https://www.ascl.net/1010.036 (2010).
Avila, RJ et al. in Astronomical Data Analysis Software and Systems XXIV (ADASS XXIV)(eds Taylor, AR & Rosolowsky, E.) 281–284 (Astronomical Society of the Pacific, 2015).
Sharon, K. et al. Strong lensing models for 37 galaxy clusters from the SDSS study of giant arcs. Astrophysic. J. Suppl. Ser. 24712 (2020).
Sharon, K. & Johnson, TL Revised lens model for the multi-image lens supernova, ‘SN Refsdal’ in MACS J1149+2223. Astrophysic. J. Lett. 800L26 (2015).
Jullo, E. et al. A Bayesian approach to modeling strong lensing of galaxy clusters. New J. Phys. 9447 (2007).
Bayliss, MB et al. Gemini/GMOS spectroscopy of 26 selected strong-lens galaxy cluster nuclei. Astrophysic. J. Suppl. Ser. 1938 (2011).
Fathivavsari, H. et al. A ghostly damped Ly α system revealed by metallic absorption lines. Mon. No. R.Astron. Soc. 466L58–L62 (2017).