Ghent University Academic Bibliography

Your filters: cql: author="Michałowski, MJ" or (type any "bookEditor issueEditor" and editor="Michałowski, MJ")

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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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Modelling high-resolution ALMA observations of strongly lensed highly star-forming galaxies detected by Herschel

S Dye, C Furlanetto, L Dunne, SA Eales, M Negrello, H Nayyeri, PP van der Werf, S Serjeant, D Farrah, MJ Michałowski, et al.

(2018) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 476(4). p.4383-4394
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Candidate high-z protoclusters among the Planck compact sources, as revealed by Herschel-SPIRE

J Greenslade, DL Clements, T Cheng, G De Zotti, D Scott, E Valiante, S Eales, MN Bremer, H Dannerbauer, M Birkinshaw, et al.

(2018) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 476(3). p.3336-3359
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The Herschel Bright Sources (HerBS) : sample definition and SCUBA-2 observations

Tom JLC Bakx, SA Eales, M Negrello, MWL Smith, E Valiante, WS Holland, Maarten Baes (UGent) , N Bourne, DL Clements, H Dannerbauer, et al.

(2018) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 473(2). p.1751-1773
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ALMA observations of lensed Herschel sources : testing the dark matter halo paradigm

A Amvrosiadis, SA Eales, M Negrello, L Marchetti, MWL Smith, N Bourne, DL Clements, G De Zotti, L Dunne, S Dye, et al.

(2018) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 475(4). p.4939-4952
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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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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
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The Herschel-ATLAS : a sample of 500 μm-selected lensed galaxies over 600 deg2

M Negrello, S Amber, A Amvrosiadis, Z-Y Cai, A Lapi, J Gonzalez-Nuevo, G De Zotti, C Furlanetto, SJ Maddox, M Allen, et al.

(2017) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 465(3). p.3558-3580
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GRB 980425 host: [C II], [O I], and CO lines reveal recent enhancement of star formation due to atomic gas inflow

MJ Michałowski, JM Castro Cerón, JL Wardlow, A Karska, H Messias, P van der Werf, LK Hunt, Maarten Baes (UGent) , AJ Castro-Tirado, Gianfranco Gentile (UGent) , et al.

(2016) ASTRONOMY & ASTROPHYSICS. 595.

Academic Bibliography

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

Modelling high-resolution ALMA observations of strongly lensed highly star-forming galaxies detected by Herschel

Candidate high-z protoclusters among the Planck compact sources, as revealed by Herschel-SPIRE

The Herschel Bright Sources (HerBS) : sample definition and SCUBA-2 observations

ALMA observations of lensed Herschel sources : testing the dark matter halo paradigm

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

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

The Herschel-ATLAS : a sample of 500 μm-selected lensed galaxies over 600 deg2

GRB 980425 host: [C II], [O I], and CO lines reveal recent enhancement of star formation due to atomic gas inflow

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