S
Smriti Mahajan
Researcher at Indian Institute of Science Education and Research, Mohali
Publications - 43
Citations - 2179
Smriti Mahajan is an academic researcher from Indian Institute of Science Education and Research, Mohali. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 21, co-authored 40 publications receiving 1886 citations. Previous affiliations of Smriti Mahajan include University of Birmingham & University of Queensland.
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Journal ArticleDOI
The SAMI Galaxy Survey: Instrument specification and target selection
Julia J. Bryant,Julia J. Bryant,Matt S. Owers,Aaron S. G. Robotham,Scott M. Croom,Simon P. Driver,Simon P. Driver,Michael J. Drinkwater,Nuria P. F. Lorente,Luca Cortese,Nicholas Scott,Matthew Colless,Adam L. Schaefer,Adam L. Schaefer,Edward N. Taylor,I. S. Konstantopoulos,I. S. Konstantopoulos,J. T. Allen,Ivan K. Baldry,Luke A. Barnes,Amanda E. Bauer,Joss Bland-Hawthorn,J. V. Bloom,Alyson Brooks,Sarah Brough,Gerald Cecil,Gerald Cecil,Warrick J. Couch,Darren J. Croton,R. I. Davies,Simon Ellis,L. M. R. Fogarty,Caroline Foster,Karl Glazebrook,Michael Goodwin,Andrew W. Green,Madusha Gunawardhana,Elise Hampton,I-Ting Ho,Andrew M. Hopkins,Lisa J. Kewley,Jon Lawrence,Sergio G. Leon-Saval,Sarah K. Leslie,Rebecca McElroy,Geraint F. Lewis,Jochen Liske,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Smriti Mahajan,Smriti Mahajan,Anne M. Medling,Nigel Metcalfe,Martin Meyer,Jeremy Mould,Danail Obreschkow,Simon J. O'Toole,Michael Pracy,Samuel N. Richards,Samuel N. Richards,Tom Shanks,Rob Sharp,Rob Sharp,Sarah M. Sweet,Sarah M. Sweet,A. D. Thomas,C. Tonini,C. J. Walcher +67 more
TL;DR: The SAMI Galaxy Survey as discussed by the authors is a 3-year survey of 3400 galaxies with the Sydney-AAO Multi-Object Integral Field Spectrograph (SAMI) on the Anglo-Australian Telescope (AAT).
Journal ArticleDOI
The SAMI Galaxy Survey: the link between angular momentum and optical morphology
Luca Cortese,L. M. R. Fogarty,Kenji Bekki,J. van de Sande,Warrick J. Couch,Barbara Catinella,Matthew Colless,Danail Obreschkow,Dan S. Taranu,Edoardo Tescari,Dilyar Barat,Joss Bland-Hawthorn,J. V. Bloom,Julia J. Bryant,Julia J. Bryant,Michelle E. Cluver,Scott M. Croom,Michael J. Drinkwater,Francesco D'Eugenio,Iraklis S. Konstantopoulos,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Smriti Mahajan,Nicholas Scott,C. Tonini,O. I. Wong,J. T. Allen,Sarah Brough,Michael Goodwin,Andrew W. Green,I-Ting Ho,I-Ting Ho,Lee S. Kelvin,Jon Lawrence,Nuria P. F. Lorente,Anne M. Medling,Matt S. Owers,Matt S. Owers,Samuel N. Richards,Samuel N. Richards,Rob Sharp,Sarah M. Sweet +41 more
TL;DR: In this article, the authors investigated the relationship between stellar and gas specific angular momentum j, stellar mass M-* and optical morphology for a sample of 488 galaxies extracted from the Sydney-AAO Multi-Object Integral field Galaxy Survey.
Journal ArticleDOI
Galaxy And Mass Assembly (GAMA): galaxy close pairs, mergers and the future fate of stellar mass
Aaron S. G. Robotham,Simon P. Driver,Simon P. Driver,Luke J. M. Davies,Andrew M. Hopkins,Ivan K. Baldry,N. K. Agius,Amanda E. Bauer,Jonathan Bland-Hawthorn,Sarah Brough,Michael J. I. Brown,Michelle E. Cluver,R. De Propris,Michael J. Drinkwater,Benne W. Holwerda,Lee S. Kelvin,Maritza A. Lara-López,Jochen Liske,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Jonathan Loveday,Smriti Mahajan,Smriti Mahajan,T. Mcnaught-Roberts,Amanda J. Moffett,Peder Norberg,Danail Obreschkow,Matt S. Owers,Samantha J. Penny,Kevin A. Pimbblet,Kevin A. Pimbblet,Matthew Prescott,Edward N. Taylor,E. van Kampen,Stephen M. Wilkins +34 more
TL;DR: In this paper, the authors used a highly complete subset of the Galaxy And Mass Assembly II (GAMA-II) redshift sample to fully describe the stellar mass dependence of close pairs and mergers between 10 8 and 10 12 M�.
Journal ArticleDOI
Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV --- far-IR) and the low-z energy budget
Simon P. Driver,Simon P. Driver,A. H. Wright,Stephen K. Andrews,Luke J. M. Davies,Prajwal R. Kafle,Rebecca A. Lange,Amanda J. Moffett,Elizabeth Mannering,Aaron S. G. Robotham,Kevin Vinsen,Mehmet Alpaslan,E. Andrae,Ivan K. Baldry,Amanda E. Bauer,Steven P. Bamford,Joss Bland-Hawthorn,Nathan Bourne,Sarah Brough,Michael J. I. Brown,Michelle E. Cluver,Scott M. Croom,Matthew Colless,Christopher J. Conselice,Elisabete da Cunha,Roberto De Propris,Michael J. Drinkwater,Loretta Dunne,Loretta Dunne,Stephen Anthony Eales,Alastair C. Edge,Carlos S. Frenk,Alister W. Graham,Meiert W. Grootes,Benne W. Holwerda,Andrew M. Hopkins,Edo Ibar,Eelco van Kampen,Lee S. Kelvin,Thomas H. Jarrett,D. Heath Jones,Maritza A. Lara-López,Jochen Liske,Angel R. Lopez-Sanchez,Jon Loveday,Steve Maddox,Steve Maddox,Barry F. Madore,Smriti Mahajan,Martin Meyer,Peder Norberg,Samantha J. Penny,Steven Phillipps,Cristina Popescu,Richard J. Tuffs,John A. Peacock,Kevin A. Pimbblet,Kevin A. Pimbblet,Matthew Prescott,Kate Rowlands,Anne E. Sansom,Mark Seibert,Matthew Smith,William J. Sutherland,Edward N. Taylor,Elisabetta Valiante,J. Antonio Vazquez-Mata,Lingyu Wang,Lingyu Wang,Stephen M. Wilkins,Richard P. Williams +70 more
TL;DR: The Galaxy And Mass Assembly (GAMA) Panchromatic data release (PDR) as mentioned in this paper consists of over 230 deg2 of imaging with photometry in 21 bands extending from far-UV to the far-IR, with the GAMA regions currently surveyed by VLT Survey Telescope (VST) and scheduled for observations by Australian Square Kilometer Array Pathfinder (ASKAP).
Journal ArticleDOI
The velocity modulation of galaxy properties in and near clusters: quantifying the decrease in star formation in backsplash galaxies
TL;DR: In this article, the authors investigate how, at a given projected radius from the cluster center, the stellar mass and star formation properties of a galaxy depend on its absolute line-of-sight velocity in the cluster rest frame, and they find that for projected radii R l 05 Rv, the fraction of high-mass non-brightest cluster galaxies increases towards the center for low |vLOS|, which may be the consequence of the faster orbital decay of massive galaxies by dynamical friction.