activity
20142023
most citedThe SAMI Galaxy Survey: instrument specification and target selection

506 citations · 1.1k across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA20231 cited

Dashing through the cluster: An X-ray to radio view of UGC 10420 undergoing ram-pressure stripping

Smriti Mahajan, Kulinder Pal Singh, Juhi Tiwari +1

We present multi-wavelength data and analysis, including new FUV AstroSat/UVIT observations of the spiral galaxy UGC 10420 (z=0.032), a member of the cluster Abell 2199. UGC 10420…

astro-ph.GA201731 cited

Galaxy And Mass Assembly (GAMA): Blue spheroids within 87 Mpc

Smriti Mahajan, Michael J. Drinkwater, S. Driver +7

In this paper we test if nearby blue spheroid (BSphs) galaxies may become the progenitors of star-forming spiral galaxies or passively-evolving elliptical galaxies. Our sample comp…

astro-ph.GA201623 cited

The SAMI galaxy survey: Galaxy Interactions and Kinematic Anomalies in Abell 119

Sree Oh, Sukyoung K. Yi, Luca Cortese +25

Galaxy mergers are important events that can determine the fate of a galaxy by changing its morphology, star-formation activity and mass growth. Merger systems have commonly been i…

astro-ph.GA2016173 cited

The SAMI Galaxy Survey: the link between angular momentum and optical morphology

L. Cortese, L. M. R. Fogarty, K. Bekki +34

We investigate the relationship between stellar and gas specific angular momentum , stellar mass and optical morphology for a sample of 488 galaxies extracted from the S…

astro-ph.GA201498 cited

The SAMI Galaxy Survey: Towards a unified dynamical scaling relation for galaxies of all types

L. Cortese, L. M. R. Fogarty, I. -T. Ho +27

We take advantage of the first data from the Sydney-AAO Multi-object Integral field (SAMI) Galaxy Survey to investigate the relation between the kinematics of gas and stars, and st…

astro-ph.GA201418 cited

Galaxy And Mass Assembly (GAMA): The unimodal nature of the dwarf galaxy population

Smriti Mahajan, Michael J. Drinkwater, S. Driver +9

In this paper we aim to (i) test the number of statistically distinct classes required to classify the local galaxy population, and, (ii) identify the differences in the physical a…