alphaFeedback
astro-ph.GAastro-ph.COastro-ph.EPastro-ph.HEastro-ph.IM

On Valency

published · living versions
W_kgqm4te3·v1 · currentpublished
Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionised gas
with Zhi-Yu Zhang, R. J. Ivison, R. D. George, Yinghe Zhao +13
1 version

Preprints & journals

48 papers in the corpus · 2010–2020
The unusual ISM in Blue and Dusty Gas Rich Galaxies (BADGRS)1910.04596v1 · L. Dunne, Z. Zhang, P. de Vis et al.2019 · 4 citationsMonthly Notices of the Royal Astronomical Society, 2018, 479, p.1221-1239
A SCUBA-2 Selected Herschel-SPIRE Dropout and the Nature of this Population1910.03512v1 · J. Greenslade, E. Aguilar, D. L. Clements et al.2019 · 6 citationsarXiv
Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS1910.03596v1 · FangXia An, J. M. Simpson, Ian Smail et al.2019 · 31 citationsThe Astrophysical Journal, Volume 886, Issue 1, article id. 48, 18 pp. (2019)
Spitzer catalog of Herschel-selected ultrared dusty, star-forming galaxies1908.08043v1 · Jingzhe Ma, Asantha Cooray, Hooshang Nayyeri et al.2019 · 17 citationsarXiv
The molecular-gas properties in the gravitationally lensed merger HATLAS J142935.3-0028361904.00307v1 · Hugo Messias, Neil Nagar, Zhi-Yu Zhang et al.2019 · 2 citationsarXiv
ALMACAL V: Absorption-selected galaxies with evidence for excited ISMs1810.01418v1 · A. Klitsch, M. A. Zwaan, C. Peroux et al.2018 · 26 citationsarXiv
A magnified view of circumnuclear star formation and feedback around an AGN at z=2.61807.03313v2 · J. E. Geach (Hertfordshire), R. J. Ivison (ESO/IfA, Edinburgh) et al.2018 · 28 citationsarXiv
ALMACAL IV: A catalogue of ALMA calibrator continuum observations1805.00024v1 · M. Bonato, E. Liuzzo, A. Giannetti et al.2018 · 81 citationsarXiv
The nature of luminous Lyman-alpha emitters at z~2-3: maximal dust-poor starbursts and highly ionising AGN1802.10102v2 · David Sobral, Jorryt Matthee, Behnam Darvish et al.2018 · 89 citationsarXiv
Candidate high-z proto-clusters among the Planck compact sources, as revealed by Herschel-SPIRE1712.07141v1 · J. Greenslade, D. L. Clements, T. Cheng et al.2017 · 40 citationsarXiv
Ultra-Red Galaxies Signpost Candidate Proto-Clusters at High Redshift1711.08803v1 · A. J. R. Lewis, R. J. Ivison, P. N. Best et al.2017 · 33 citationsarXiv
280 one-opposition near-Earth asteroids recovered by the EURONEAR with the Isaac Newton Telescope1711.00709v2 · O. Vaduvescu, L. Hudin, T. Mocnik et al.2017 · 14 citationsA&A 609, A105 (2018)
The Herschel Bright Sources (HerBS): Sample definition and SCUBA-2 observations1709.01514v1 · Tom J. L. C. Bakx, S. A. Eales, M. Negrello et al.2017 · 60 citationsarXiv
Large turbulent reservoirs of cold molecular gas around high-redshift starburst galaxies.28813416 · Falgarone, E, Zwaan, M A, Godard, B et al.2018 · 90 citationsNature. 2017;548(7668):430-433
A dusty star-forming galaxy at z=6 revealed by strong gravitational lensing1707.09022v3 · Jorge A. Zavala, Alfredo Montana, David H. Hughes et al.2017 · 104 citationsNature Astronomy, 2, 56-62, 2018
Low-redshift analogs of submm galaxies: a diverse population1707.05329v1 · I. Oteo, I. Smail, T. Hughes et al.2017 · 3 citationsarXiv
SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Faint-End Counts at 450 um1707.00990v3 · Wei-Hao Wang, Wei-Ching Lin, Chen-Fatt Lim et al.2017 · 60 citationsarXiv
Rise of the Titans: A Dusty, Hyper-Luminous "870 micron Riser" Galaxy at z~61705.09660v2 · Dominik A. Riechers, T. K. Daisy Leung, Rob J. Ivison et al.2017 · 93 citationsarXiv
Planck's dusty GEMS. IV. Star formation and feedback in a maximum starburst at z=3 seen at 60-pc resolution1704.05853v2 · R. Canameras, N. Nesvadba, R. Kneissl et al.2017 · 43 citationsA&A 604, A117 (2017)
Planck's Dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.51703.02984v1 · R. Canameras, N. P. H. Nesvadba, R. Kneissl et al.2017 · 24 citationsA&A 600, L3 (2017)
New ALMA and Fermi/LAT Observations of the large-scale jet of PKS 0637-752 Strengthen the Case Against the IC/CMB Model1702.00015v2 · Eileen T. Meyer, Peter Breiding, Markos Georganopoulos et al.2017 · 27 citationsarXiv
The CALYMHA survey: Lya luminosity function and global escape fraction of Lya photons at z=2.231609.05897v2 · David Sobral, Jorryt Matthee, Philip Best et al.2016 · 105 citationsarXiv
GAMA/H-ATLAS: Common star-formation rate indicators and their dependence on galaxy physical parameters1607.02971v2 · L. Wang, P. Norberg, M. L. P. Gunawardhana et al.2016 · 20 citationsarXiv
Detecting microvariability in type 2 quasars using enhanced F-test1605.09424v1 · J. Polednikova, A. Ederoclite, J.A. de Diego et al.2016 · 14 citationsarXiv
H-ATLAS: A Candidate High Redshift Cluster/Protocluster of Star-Forming Galaxies1605.06433v1 · D.L. Clements, F. Braglia, G. Petitpas et al.2016 · 35 citationsarXiv
An Accurate Cluster Selection Function for the J-PAS Narrow-Band wide-field survey1601.00656v1 · Begona Ascaso, Narciso Ben'itez, Renato Dupke et al.2016 · 21 citationsarXiv
Extinction and nebular line properties of a Herschel-selected lensed dusty starburst AT z=1.0271501.01638v2 · Nicholas Timmons, Asantha Cooray, Hooshang Nayyeri et al.2015 · 9 citationsarXiv
The UV to FIR spectral energy distribution of star-forming galaxies in the redshift desert1307.0971v2 · I. Oteo, 'A. Bongiovanni, G. Magdis et al.2013 · 18 citationsarXiv
Lyman break and UV-selected galaxies at z ~ 1: II. PACS-100um/160um FIR detections1306.1121v2 · I. Oteo, G. Magdis, 'A. Bongiovanni et al.2013 · 15 citationsarXiv
PACS-Herschel FIR detections of Lyman-alpha emitters at 2.0<z<3.51202.0997v1 · I. Oteo, A. Bongiovanni, A. M. P'erez Garc'ia et al.2012 · 26 citationsarXiv
FIR measurements of Ly-α\alpha emitters at z$\lesssim$1.0: dust attenuation from PACS-\emph{Herschel}1108.3122v1 · I. Oteo, A. Bongiovanni, A. M. P'erez Garc'ia et al.2011 · 13 citationsarXiv
Career total: 80 works. 48 are in this corpus.

Profile built from the corpus for this byline.

Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.