The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH

By Q. Parker, A. Acker, D. Frew, M. Hartley, A. Peyaud, F. Ochsenbein, Steve Phillipps, D. Russeil, S. Beaulieu, Marvin L. Cohen and 6 more. 2006

225 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/0bffddf1734806e7bfdbfb6a4efe3533ee3e269a

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Robert G. Izzard
2. O. De Marco
3. I. Bojičić
4. Q. Parker
5. D. Frew
6. B. Gänsicke
7. T. Naylor
8. C. Knigge

In Instrumentation

1. I. Bojičić
2. Q. Parker
3. O. De Marco
4. D. Frew
5. Robert G. Izzard
6. B. Gänsicke
7. T. Naylor
8. C. Knigge

Citations in the corpus

• Dawes Review 6: The Impact of Companions on Stellar Evolution (2016, background): “Yet, 80% of all PN are non-spherical (Parker et al., 2006), only some of which could be explained at the moment by single stars.”
• The optical emission nebulae in the vicinity of WR 48 (Θ Mus): true Wolf–Rayet ejecta or unconnected supernova remnant? (2009, background): “…brightness and more extreme, evolved examples of these different objects are increasingly uncovered from the next generation on narrow-band imaging surveys, e.g. Parker et al. (2006), Miszalski et al. (2008) these optical diagnostics are not always clear cut (Frew 2008; Frew & Parker 2009).”
• Binary planetary nebulae nuclei towards the Galactic bulge - I. Sample discovery, period distribution, and binary fraction (2009, methodology): “…2007) are required to survey regions outside microlensing surveys or where the sampling is not always ideal and such surveys would prove very fruitful indeed in monitoring the now very large population of Galactic bulge and Southern Galactic Plane PNe (Parker et al. 2006; Miszalski et al. 2008a).”
• The Hα surface brightness–radius relation: a robust statistical distance indicator for planetary nebulae (2015, methodology): “This high-excitation, optically-thin nebula was discovered by Fesen, Gull & Heckathorn (1983), and later confirmed by Parker et al. (2006).”
• The VST Photometric Hα Survey of the Southern Galactic Plane and Bulge (VPHAS (2014, background): “This was the last survey using photographic emulsions that the UK Schmidt Telescope undertook.”