Zhen-Yi Cai

Dr. Zhen-Yi Cai

orcid

Research Focus & Metrics

Academic Career Length

17Years (2010-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 February 2014 in Journal of Cosmology and Astroparticle Physics
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Journal Article
Closed access
PAPhilippe André
Philippe André
CBCarlo Baccigalupi
Carlo Baccigalupi
ABAnthony Banday
Anthony Banday
DBDomingos Barbosa
Domingos Barbosa
BBBelen Barreiro
Belen Barreiro
SWStafford Withington
Stafford Withington

1 April 2018 in Journal of Cosmology and Astroparticle Physics
Verified
Journal Article
Closed access
PDF file
FFF. Finelli
F. Finelli
MBM. Bucher
M. Bucher
AAA. Achúcarro
A. Achúcarro
MBMario Ballardini
Mario Ballardini
NBN. Bartolo
N. Bartolo
MZM. Zannoni
M. Zannoni

1 April 2018 in Journal of Cosmology and Astroparticle Physics
Verified
Journal Article
Open access
PDF file
JDJ. Delabrouille
J. Delabrouille
PBP. de Bernardis
P. de Bernardis
FBF.R. Bouchet
F.R. Bouchet
AAA. Achúcarro
A. Achúcarro
PAP. A. R. Ade
P. A. R. Ade
MZM. Zannoni
M. Zannoni

1 April 2018 in Journal of Cosmology and Astroparticle Physics
Verified
Journal Article
Closed access
PDF file
EVE. Di Valentino
E. Di Valentino
TBT. Brinckmann
T. Brinckmann
MGM. Gerbino
M. Gerbino
VPV. Poulin
V. Poulin
FBF.R. Bouchet
F.R. Bouchet
MZM. Zannoni
M. Zannoni

10 November 2016 in Monthly Notices of the Royal Astronomical Society
Verified
Journal Article
Open access
PDF file
MNM. Negrello
M. Negrello
SAS. Amber
S. Amber
AAA. Amvrosiadis
A. Amvrosiadis
ZCZhen-Yi Cai
Zhen-Yi Cai
ALA. Lapi
A. Lapi
PWP. van der Werf
P. van der Werf
We present a sample of 80 candidate strongly lensed galaxies with flux density above 100 mJy at 500 μm extracted from the Herschel Astrophysical Terahertz Large Area Survey, over an area of 600 deg2. Available imaging and spectroscopic data allow us to confirm the strong lensing in 20 cases and to reject it in one case. For other eight objects, the lensing scenario is strongly supported by the presence of two sources along the same line of sight with distinct photometric redshifts. The remaining objects await more follow-up observations to confirm their nature. The lenses and the background sources have median redshifts zL = 0.6 and zS = 2.5, respectively, and are observed out to zL = 1.2 and zS = 4.2. We measure the number counts of candidate lensed galaxies at 500 μm and compare them with theoretical predictions, finding a good agreement for a maximum magnification of the background sources in the range 10–20. These values are consistent with the magnification factors derived from the lens modelling of individual systems. The catalogue presented here provides sub-mm bright targets for follow-up observations aimed at exploiting gravitational lensing, to study with unprecedented details the morphological and dynamical properties of dusty star-forming regions in z ≳ 1.5 galaxies.

10 April 2013 in The Astrophysical Journal
Verified
Journal Article
Closed access
ZCZhen-Yi Cai
Zhen-Yi Cai
ALAndrea Lapi
Andrea Lapi
JXJunqing Xia
Junqing Xia
GZGianfranco De Zotti
Gianfranco De Zotti
MNMattia Negrello
Mattia Negrello
LDLuigi Danese
Luigi Danese