We propose to observe the HI in 56 very low surface brightness galaxies (vLSBs) that were detected in the Hyper Suprime-Cam Subaru Strategic Program. vLSBs are a cosmologically significant population of galaxies, yet are not well understood: such galaxies appear to have effective radii similar to the Milky Way, yet very small stellar masses. To date, only 8 of the 781 vLSBs in the Hyper Suprime-Cam sample have measured distances. Our goal is to determine redshift distances to a carefully selected subset of vLSB galaxies likely to have HI and to be in the field. Based on HI scaling relations, we expect to detect roughly 70% of our targets. This represents nearly a five-fold increase in the number of known redshifts for such galaxies with a modest investment of observing time compared with optical spectroscopy. In addition, HI gas fractions and masses will be used to probe their star formation histories and line widths will be used to probe rotation and dark matter content. These measurements will constrain the cosmic number density and formation models for this enigmatic population of vLSB galaxies in low density environments.
Name | Institution |
---|---|
Lukas Leisman * | Cornell University; Valparaiso University |
D.J. Pisano | Cape Town, University of |
Katherine Rabidoux | West Virginia University; Wisconsin-Platteville, University of |
Evan (old) Smith | Green Bank Observatory; West Virginia University |
Rebecca Koopmann | Union College |
Joseph Ribaudo | Providence College |
Jenny Greene | Princeton University |
Johnny Greco | Ohio State University; Princeton University |
MIchael Strauss | Princeton University |
Martha Haynes | Cornell University |
Jessica Rosenberg | George Mason University |
David Craig | West Texas A&M University |
Gregory Hallenbeck | Cornell University; Union College |
Aileen O'Donoghue | St. Lawrence University |
Grant Denn | Denver, Metropolitan State University of |
Andy Goulding | Princeton University |
Adriana Durbala | Wisconsin-Stevens Point, University of |
Song Huang | California at Santa Cruz, University of |
* indicates the PI