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RESOLVE DR4 and ECO DR3 G3 groups HI catalogs
We present a four-step group-finding algorithm for the Gas in Galaxy Groups (G3) initiative, a spin-off of the z~0 REsolved Spectroscopy Of a Local VolumE (RESOLVE) and... -
ASKAP & FAST HI data for the NGC4636 group members
Combining new HI data from a synergetic survey of Australian Square Kilometre Array Pathfinder (ASKAP) Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) and... -
PANDISC. I. HI model applied to ALFAFA & SPARC gal.
Modeling the integrated HI spectra of galaxies has been a difficult task, due to their diverse shapes, but more dynamical information is waiting to be explored in HI line... -
WALLABY pilot survey: HI gas in Hydra cluster
This study uses HI image data from the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) pilot survey with the Australian Square Kilometre Array Pathfinder (ASKAP)... -
GBT HI obs. of ultradiffuse galaxies
We present neutral hydrogen (HI) observations using the Robert C. Byrd Green Bank Telescope (GBT) of 70 optically detected UDG candidates in the Coma region from the... -
Cosmicflows-4: Tully-Fisher distances
We present the distances of 9792 spiral galaxies lying within 15000km/s using the relation between luminosity and rotation rate of spiral galaxies. The sample is dominantly, but... -
Parameters for the 58 {tau}HI(v) sightlines
Resolving the phase structure of neutral hydrogen (HI) is crucial for understanding the life cycle of the interstellar medium (ISM). However, accurate measurements of HI... -
Cosmicflows-4: Tully-Fisher relation calibrations
This study is a part of the Cosmicflows-4 project with the aim of measuring the distances of more than ~10000 spiral galaxies in the local universe up to ~15000km/s. New HI line... -
COS CGM compendium (CCC). III. z<=1 Ly{alpha} syst.
We characterize the metallicities and physical properties of cool, photoionized gas in a sample of 152 z<=1 strong Ly{alpha} forest systems (SLFSs, absorbers with 15 -
OB stars embedded in the HI gas of SMC
We investigate the kinematics of neutral gas in the Small Magellanic Cloud (SMC) and test the hypothesis that it is rotating in a disk. To trace the 3D motions of the neutral... -
SDSS, WISE and HI data of local spiral galaxies
The emerging light from a galaxy is under the influence of its own interstellar medium, as well as its spatial orientation. Considering a sample of 2239 local spiral galaxies in... -
The COS CGM Compendium (CCC). II. Lyman limit syst.
We present the results from our COS circumgalactic medium (CGM) compendium (CCC), a survey of the CGM at z<~1 using HI-selected absorbers with 15<logN_HI_<19. We focus... -
The COS CGM compendium. I. Initial results
We present a neutral hydrogen-selected absorption-line survey of gas with HI column densities 15<logN_HI_<19 at z<~1 using the Cosmic Origins Spectrograph on the Hubble... -
The HIPASS Catalog (HICAT) + WISE galaxies
We have measured the relationships between HI mass, stellar mass, and star formation rate using the HI Parkes All-Sky Survey Catalog (HICAT) and the Wide-field Infrared Survey... -
Galaxy groups from SDSS DR7 and ALFALFA
Using the group crossing time t_c_ as an age indicator for galaxy groups, we have investigated the correlation between t_c_ and the group spiral fraction, as well as between... -
ALFALFA extragalactic HI source catalog
We present the catalog of ~31500 extragalactic HI line sources detected by the completed Arecibo Legacy Fast ALFA (ALFALFA) survey out to z<0.06, including both high... -
Compact clouds in a sensitive GBT HI survey
We present the results of a new sensitive survey of neutral hydrogen above and below the Galactic Center with the Green Bank Telescope. The observations extend up to Galactic... -
HI-bearing ultra-diffuse ALFALFA galaxies
We present a sample of 115 very low optical surface brightness, highly extended, HI-rich galaxies carefully selected from the ALFALFA survey that have similar optical absolute... -
HI-selected Lyman limit systems metallicities
We present the first results from our KODIAQ Z survey aimed at determining the metallicity distribution and physical properties of the z>~2 partial and full Lyman limit... -
Milky Way kinematics. II.
Using atomic hydrogen (HI) data from the VLA Galactic Plane Survey, we measure the HI terminal velocity as a function of longitude for the first quadrant of the Milky Way. We...
