Australian Road Research Board

output

20142024

most citedThe Spitzer Survey of Stellar Structure in Galaxies (S

^{4}

G): Precise Stellar Mass Distributions from Automated Dust Correction at 3.6 microns

262 citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

Ada Böhm1 · h 1
Benjamin Davis1 · h 1
Christopher Wilson1 · h 2
D. Sharafi1 · h 6
Farhad Billimoria1 · h 9
Jan Kulveit1 · h 8
L. Kwek1 · h 2
M. Garbutt1 · h 4
N. Lal1 · h 13
Peli Grietzer1 · h 3
T. Gavenčiak1 · h 13
Toby Price1 · h 2

collaborating institutions

Align Technology (United States)US1 paper
Andover Eye AssociatesUS1 paper
Aroma Praha (Czechia)CZ1 paper
California Institute of TechnologyUS1 paper
Carnegie Institution for ScienceUS1 paper
Carnegie ObservatoriesUS1 paper
Center for Theoretical PhysicsPL1 paper
Charles UniversityCZ1 paper
European Southern ObservatoryCL1 paper
Florida Institute of TechnologyUS1 paper
FZI Research Center for Information TechnologyDE1 paper
Institute of Process EngineeringCN1 paper

Showing 2014Show all

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astro-ph.GA2014★ 262 cited

The Spitzer Survey of Stellar Structure in Galaxies (S $^{4}$ G): Precise Stellar Mass Distributions from Automated Dust Correction at 3.6 microns

M. Querejeta, S. E. Meidt, E. Schinnerer +26

The mid-infrared is an optimal window to trace stellar mass in nearby galaxies and the 3.6 $μ m$ IRAC band has been exploited to this effect, but such mass estimates can be biased by…

The Spitzer Survey of Stellar Structure in Galaxies (S4G): Precise Stellar Mass Distributions from Automated Dust Correction at 3.6 microns

The Spitzer Survey of Stellar Structure in Galaxies (S $^{4}$ G): Precise Stellar Mass Distributions from Automated Dust Correction at 3.6 microns