1,723,034 research outputs found
SAMPLING Data Release 1
No full textDR1 of the SAMPLING survey.
12CO/13CO(2-1) cubes of 124 fields, nominal map size 5arcmin x 5 arcmin.
Resolution 36 arcsec, channel width 0.3 km/s, rms 0.2 K. Calibrated to main beam temperature Tmb.
Data quality assurance
QA1: remote observations
by Ke Wang, Jinjin Xie, Tie Liu, Viktor Toth, Xing Lu, Yuan Wang, Shen Wang, Giuliana Cosentino, Ren-Shiang Sung, Maria Cunningham, Vlas Sokolov, Sarolta Zahorecz, and Yuwei Wang.
QA2: data reduction
by Ke Wang.
QA3: manual inspection
by Sarolta Zahorecz.
Acknowledgments
We encourage the community to contact us for collaboration and to make use of the data. Please credit the survey by including the following sentence in your publication:
The data presented in this paper are based on the ESO-ARO programme ID 196.C-0999(A).
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Temperature maps of P1, C1S regions in Infrared Dark Cloud G28.34+0.06, the Dragon Nebula
No full textNH3 fitted temperature map
Temperature maps of P1, C1S regions in Infrared Dark Cloud G28.34+0.06, the Dragon Nebula
No full textNH3 fitted temperature map
G339 (Nessie)
No full textColumn density, Temperature, Mass, Luminosity maps - after background subtractio
H2 column density maps for large-scale Herschel filaments
No full textH2 column density maps of the 9 most prominent filaments identified by Herschel Space Observatory. The maps are derived by pixel-by-pixel SED fitting of Herschel Hi-GAL images, with a resolution 28 arcsec.
See Figure 2 in Wang et al. 2015MNRAS.450.4043W
<a href=
"http://adsabs.harvard.edu/abs/2015MNRAS.450.4043W"
>
"Large-scale filaments associated with Milky Way spiral arms"
G11 (Snake)
No full textColumn density, Temperature, Mass, Luminosity maps - after background subtractio
H2 column density maps for large-scale Herschel filaments
No full textH2 column density maps of the 9 most prominent filaments identified by Herschel Space Observatory. The maps are derived by pixel-by-pixel SED fitting of Herschel Hi-GAL images, with a resolution 28 arcsec.
See Figure 2 in Wang et al. 2015MNRAS.450.4043W
<a href=
"http://adsabs.harvard.edu/abs/2015MNRAS.450.4043W"
>
"Large-scale filaments associated with Milky Way spiral arms"
- …
