Erratum: Atlas and Catalog of Dark Clouds Based on Digitized Sky Survey I

By K. Dobashi, Hayato Uehara, R. Kandori, T. Sakurai, M. Kaiden, T. Umemoto, F. Sato. 2005

221 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Computational Mechanics, Global and Planetary Change

View Paper: https://www.semanticscholar.org/paper/11d4dbf614e1ff6959a6e80f50e2ef39b4c3c381

How researchers see this paper

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

In Aerospace Engineering

1. R. Romani
2. Pascal Bruel

In Computational Mechanics

1. J. Ridder
2. K. Belkacem
3. M. Goupil
4. C. Barban
5. R. Samadi
6. F. Baudin
7. A. Baglin
8. M. Auvergne

In Global and Planetary Change

1. Adam Van Etten

Citations in the corpus

• Constraining the thick disc formation scenario of the Milky Way (2014, unknown): “We did consider the maps of Schlegel et al. (1998) because they only give the 2D extinction value integrated over lines of sight and might suffer from systematics, as shown by Dobashi et al. (2005), and more recently by Schlafly & Finkbeiner (2011), and by Berry et al. (2012) using SDSS data.”
• OBSERVATION OF SUPERNOVA REMNANT IC 443 WITH THE FERMI LARGE AREA TELESCOPE (2010, methodology): “…GALPROP for Fermi LAT (GALDEF 54_59Xvarh8S; Strong & Moskalenko 1998; Strong et al. 2001, 2009) made of the CO line survey by Dame et al. (2001) and H i survey by Kalberla et al. (2005) as well as with a gas model made of the AV map by Dobashi et al. (2005) and H i survey by Kalberla et al. (2005).”
• FILAMENTARY STRUCTURE OF STAR-FORMING COMPLEXES (2009, background): “The two northernmost lanes are seen more clearly here than in the star-count images of Dobashi et al (2005) or the 13CO map of Loren (1989), probably because of finer resolution.”
• THE RELATION BETWEEN GAS AND DUST IN THE TAURUS MOLECULAR CLOUD (2010, background): “The H2 column density can be independently inferred by measuring the optical or near–infrared light from background stars that has been extincted by the dust present in the molecular cloud (Lada et al. 1994; Cambrésy 1999; Dobashi et al. 2005).”
• Empirical extinction coefficients for the GALEX, SDSS, 2MASS and WISE passbands (2013, unknown): “Various studies, however, have shown that SFD may have overestimated extinction in both the high- and the low-extinction regime (Arce & Goodman 1999; Chen et al. 1999; Dobashi et al. 2005; Yasuda, Fukugita & Schneider 2007; Rowles & Froebrich 2009).”
• Red-giant seismic properties analyzed with CoRoT (2010, methodology): “We have adopted AV = 0.6 mag for LRa01 based on the extinction maps of Dobashi et al. (2005) and Rowles & Froebrich (2009).”
• Cold Dark Clouds: The Initial Conditions for Star Formation (2007, methodology): “A similar star-counting technique, but with a fixed cell spacing, has been used by Dobashi et al. (2005) to make an atlas of dark clouds using DSS-I data.”