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20172019
most citedAttenuation modified by DIG and dust as seen in M31

20 citations · 59 across the 4 of their papers we have counts for

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5 papers · 1 filter

astro-ph.GA2019★ 17 cited

Calibrating star-formation rate prescriptions at different scales (10 pc to 1 kpc) in M31

Neven Tomicic, I-Ting Ho, Kathryn Kreckel +9

We calibrate commonly used star formation rate (SFR) prescriptions using observations in five kpc-sized fields in the nearby galaxy Andromeda (M31) at 10\,pc spatial resolution. Ou…

astro-ph.GA2018

A SOFIA Survey of [CII] in the galaxy M51 I. [CII] as a tracer of Star Formation

Jorge L. Pineda, Christian Fischer, Maria Kapala +12

We present a [CII] 158um map of the entire M51 (including M51b) grand--design spiral galaxy observed with the FIFI-LS instrument on SOFIA. We compare the [CII] emission with the to…

astro-ph.GA2017★ 9 cited

An Overview of the MHONGOOSE Survey: Observing Nearby Galaxies with MeerKAT

W. J. G. de Blok, E. A. K. Adams, P. Amram +65

MHONGOOSE is a deep survey of the neutral hydrogen distribution in a representative sample of 30 nearby disk and dwarf galaxies with HI masses from 10^6 to ~10^{11} M_sun, and lumi…

astro-ph.GA2017★ 20 cited

Attenuation modified by DIG and dust as seen in M31

Neven Tomicic, Kathryn Kreckel, Brent Groves +5

The spatial distribution of dust in galaxies affects the global attenuation, and hence inferred properties, of galaxies. We trace the spatial distribution of dust in five fields (a…

astro-ph.GA2017★ 13 cited

The Survey of Lines in M31 (SLIM): The Drivers of the [CII]/TIR Variation

Maria Julia Kapala, Brent Groves, Karin Sandstrom +7

The ratio of the [CII] 158m emission line over the total infrared emission (TIR) is often used as a proxy for the photoelectric (PE) heating efficiency () of the f…