559 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- California Institute of TechnologyUS20 papers
- The University of SydneyAU15 papers
- ARC Centre of Excellence for All-sky AstrophysicsAU13 papers
- Australian Astronomical ObservatoryAU13 papers
- International Centre for Radio Astronomy ResearchAU13 papers
- Macquarie UniversityAU13 papers
- The University of Western AustraliaAU13 papers
- Ames Research CenterUS12 papers
- Australian National UniversityAU12 papers
- Jet Propulsion LaboratoryUS12 papers
- UNSW SydneyAU11 papers
- Johns Hopkins UniversityUS10 papers
13 papers · 1 filter
The SAMI Galaxy Survey: Exploring the gas-phase Mass-Metallicity Relation
S. F. Sanchez, J. K. Barrera-Ballesteros, C. Lopez-Coba +13
We present a detailed exploration of the stellar mass vs. gas-phase metallicity relation (MZR) using integral field spectroscopy data obtained from ~1000 galaxies observed by the S…
SOFIA Far Infrared Imaging Polarimetry of M82 and NGC 253: Exploring the Super-Galactic Wind
Terry Jay Jones, C. Darren Dowell, Enrique Lopez Rodriguez +22
We present Far-Infrared polarimetry observations of M82 at 53 and and NGC 253 at , which were taken with HAWC+ in polarimetry mode on the Stratospheric Ob…
The SAMI Galaxy Survey: Stellar and gas misalignments and the origin of gas in nearby galaxies
J. J. Bryant, S. M. Croom, J. van de Sande +16
Misalignment of gas and stellar rotation in galaxies can give clues to the origin and processing of accreted gas. Integral field spectroscopic observations of 1213 galaxies from th…
KROSS-SAMI: A Direct IFS Comparison of the Tully-Fisher Relation Across 8 Gyr Since
A. L. Tiley, M. Bureau, L. Cortese +27
We construct Tully-Fisher relations (TFRs), from large samples of galaxies with spatially-resolved H emission maps from the K-band Multi-Object Spectrograph (KMOS) Redshift One…
HAWC+/SOFIA Multiwavelength Polarimetric Observations of OMC-1
David T. Chuss, B-G Andersson, John Bally +35
We report new polarimetric and photometric maps of the massive star-forming region OMC-1 using the HAWC+ instrument on the Stratospheric Observatory for Infrared Astronomy (SOFIA).…
The SAMI Galaxy Survey: Data Release Two with absorption-line physics value-added products
Nicholas Scott, Jesse van de Sande, Scott M. Croom +34
We present the second major release of data from the SAMI Galaxy Survey. Data Release Two includes data for 1559 galaxies, about 50% of the full survey. Galaxies included have a re…
The SAMI Galaxy Survey: embedded discs and radial trends in outer dynamical support across the Hubble sequence
Caroline Foster, J. van de Sande, L. Cortese +11
We study the balance in dynamical support of 384 galaxies with stellar kinematics out to >1.5R_e in the Sydney AAO Multi-object Integral Field (SAMI) Galaxy Survey. We present radi…
The SAMI Galaxy Survey: Spatially Resolved Metallicity and Ionization Mapping
Henry Poetrodjojo, Brent Groves, Lisa J. Kewley +16
We present gas-phase metallicity and ionization parameter maps of 25 star-forming face-on spiral galaxies from the SAMI Galaxy Survey Data Release 1. Self-consistent metallicity an…
Dust Production Rates in the Fomalhaut Debris Disk from SOFIA/FORCAST Mid-infrared Imaging
J. D. Adams, T. L. Herter, R. M. Lau +2
We present the first spatially resolved mid-infrared (37.1 m) image of the Fomalhaut debris disk. We use PSF fitting and subtraction to distinctly measure the flux from the unre…
Anatomy of the massive star-forming region S106: The OI 63 micron line observed with GREAT/SOFIA as a versatile diagnostic tool for the evolution of massive stars
N. Schneider, M. Roellig, R. Simon +9
The central area (40"x40") of the bipolar nebula S106 was mapped in the OI line at 63.2 micron with high angular (6") and spectral resolution, using GREAT on board SOFIA. The OI em…
A relation between characteristic stellar age of galaxies and their intrinsic shape
Jesse van de Sande, Nicholas Scott, Joss Bland-Hawthorn +15
Stellar population and stellar kinematic studies provide unique but complementary insights into how galaxies build-up their stellar mass and angular momentum. A galaxy's mean stell…
The SAMI Galaxy Survey: gravitational potential and surface density drive stellar populations -- I. early-type galaxies
Tania M. Barone, Francesco D'Eugenio, Matthew Colless +15
The well-established correlations between the mass of a galaxy and the properties of its stars are considered evidence for mass driving the evolution of the stellar population. How…
The SAMI Galaxy Survey: Spatially Resolving the Main Sequence of Star Formation
Anne M. Medling, Luca Cortese, Scott M. Croom +42
We present the ~800 star formation rate maps for the SAMI Galaxy Survey based on Hα emission maps, corrected for dust attenuation via the Balmer decrement, that are included in the…