Ghent University Academic Bibliography

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VALES V : a kinematic analysis of the molecular gas content in H-ATLAS galaxies at z ∼ 0.03-0.35 using ALMA

J Molina, Edo Ibar, V Villanueva, A Escala, C Cheng, Maarten Baes (UGent) , H Messias, C Yang, FE Bauer, . van der Werf, et al.

(2019) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 482(2). p.1499-1524
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VALES, II : the physical conditions of interstellar gas in normal star-forming galaxies up to z = 0.2 revealed by ALMA

TM Hughes, E Ibar, V Villanueva, M Aravena, Maarten Baes (UGent) , N Bourne, A Cooray, L Dunne, S Dye, S Eales, et al.

(2017) ASTRONOMY & ASTROPHYSICS. 602.
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The Herschel Virgo Cluster Survey, XX : dust and gas in the foreground Galactic cirrus

S Bianchi, C Giovanardi, MWL Smith, J Fritz, JI Davies, MP Haynes, R Giovanelli, Maarten Baes (UGent) , M Bocchio, S Boissier, et al.

(2017) ASTRONOMY & ASTROPHYSICS. 597.
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VALES, III : the calibration between the dust continuum and interstellar gas content of star-forming galaxies

TM Hughes, E Ibar, V Villanueva, M Aravena, Maarten Baes (UGent) , N Bourne, A Cooray, LJM Davies, S Driver, L Dunne, et al.

(2017) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 468(1). p.L103-L107
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VALES, I : the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35

V Villanueva, E Ibar, TM Hughes, MA Lara-López, L Dunne, S Eales, RJ Ivison, M Aravena, Maarten Baes (UGent) , N Bourne, et al.

(2017) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 470(4). p.3775-3805

Academic Bibliography

VALES V : a kinematic analysis of the molecular gas content in H-ATLAS galaxies at z ∼ 0.03-0.35 using ALMA

VALES, II : the physical conditions of interstellar gas in normal star-forming galaxies up to z = 0.2 revealed by ALMA

The Herschel Virgo Cluster Survey, XX : dust and gas in the foreground Galactic cirrus

VALES, III : the calibration between the dust continuum and interstellar gas content of star-forming galaxies

VALES, I : the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35

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