About: Sherry H. Suyu

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researcher

Attributes	Values
rdf:type	Item
description	researcher (en) 연구원 (ko) 研究者 (ja) Astrophysikerin (de) wetenschapper (nl) дослідниця (uk) 研究者 (zh) հետազոտող (hy)
rdfs:label	Sherry H Suyu (nl) Sherry H. Suyu (en) Sherry Suyu (de)
skos:prefLabel	Sherry H Suyu (nl) Sherry H. Suyu (en) Sherry Suyu (de)
name	Sherry H Suyu (nl) Sherry H. Suyu (en) Sherry Suyu (de)
given name	wds:Q90083610-1B8B0663-4D96-4DCB-97F9-E698BCECD359
given name	Sherry
instance of	wds:Q90083610-699C528F-4D18-4B21-BB47-1A98C407E006
instance of	Homo sapiens
Google Knowledge Graph ID	wds:Q90083610-4FDA0A85-E1FF-4D9F-BC61-EA6DCFD2039F
Google Knowledge Graph ID	http://g.co/kg/g/11gbj5l1h7
Google Knowledge Graph ID	/g/11gbj5l1h7
skos:altLabel	S H Suyu (en) S. H. Suyu (en) S.H. Suyu (en) Sherry H Suyu (en) Sherry Suyu (en) Sherry Suyu (nl)
occupation	wds:Q90083610-313C2B00-38A0-4580-B731-B389472E58C5 wds:Q90083610-55619E27-0A87-40F2-AF96-8458EDDCEDB8
sex or gender	wds:Q90083610-FD6A3692-6A4E-4FEF-8BC9-136F000C56CB
VIAF ID	wds:Q90083610-5883BD15-7BC1-4203-B720-557016114592
GND ID	wds:Q90083610-8590267C-EEA7-464A-A62E-88D7757B8224
date of birth	wds:Q90083610-C081FB08-7C6D-4F55-97F7-9FDAF097692B
VIAF ID	http://viaf.org/viaf/6778164357932613250009
GND ID	https://d-nb.info/gnd/1250328454
occupation	astrophysicist researcher
sex or gender	female organism
VIAF ID	6778164357932613250009
GND ID	1250328454
date of birth	2000-01-01 00:00:00Z (xsd:dateTime)
ORCID iD	wds:Q90083610-1A25ED04-7474-4D7E-8A94-5B9852F11814
ORCID iD	https://orcid.org/0000-0001-5568-6052
ORCID iD	0000-0001-5568-6052
is owl:sameAs of	Sherry H. Suyu
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q90083610 https://de.wikipedia.org/wiki/Sherry_Suyu
is author of	Strong lensing as a probe of the mass distributionbeyondthe Einstein radius A new window of exploration in the mass spectrum: strong lensing by galaxy groups in the SL2S CLASH-VLT: insights on the mass substructures in the frontier fields cluster MACS J0416.1-2403 through accurate strong lens modeling J0454-0309: evidence of a strong lensing fossil group falling into a poor galaxy cluster Discovery of a strong lensing galaxy embedded in a cluster at z = 1.62 "Refsdal" meets popper: comparing predictions of the re-appearance of the multiply imaged supernova behind MACSJ1149.5+2223 H0LiCOW VII: cosmic evolution of the correlation between black hole mass and host galaxy luminosity H0LiCOW – II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE 0435−1223 The STRong lensing Insights into the Dark Energy Survey (STRIDES) 2016 follow-up campaign – I. Overview and classification of candidates selected by two techniques Is every strong lens model unhappy in its own way? Uniform modelling of a sample of 13 quadruply+ imaged quasars Separating galaxies from the cluster dark matter halo in Abell 611 Precise strong lensing mass profile of the CLASH galaxy cluster MACS 2129 Constraining the galaxy mass content in the core of A383 using velocity dispersion measurements for individual cluster members DES meets Gaia: discovery of strongly lensed quasars from a multiplet search TDCOSMO. IV. Hierarchical time-delay cosmography - joint inference of the Hubble constant and galaxy density profiles HOLISMOKES. III. Achromatic Phase of Strongly Lensed Type Ia Supernovae Cosmology from gravitational lens time delays and Planck data H0LiCOW – V. New COSMOGRAIL time delays of HE 0435−1223:H0to 3.8 per cent precision from strong lensing in a flat ΛCDM model Models of the strongly lensed quasar DES J0408−5354 CLASH-VLT: A highly precise strong lensing model of the galaxy cluster RXC J2248.7−4431 (Abell S1063) and prospects for cosmography CLASH: z ∼ 6 young galaxy candidate quintuply lensed by the frontier field cluster RXC J2248.7−4431 H0LiCOW – I. H0 Lenses in COSMOGRAIL's Wellspring: program overview H0LiCOW – III. Quantifying the effect of mass along the line of sight to the gravitational lens HE 0435−1223 through weighted galaxy counts Reconstructing the lensing mass in the Universe from photometric catalogue data Discovery of the Lensed Quasar System DES J0408-5354 COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses. XVI. Time delays for the quadruply imaged quasar DES J0408-5354 with high-cadence photometric monitoring Discovery of two gravitationally lensed quasars in the Dark Energy Survey HOLISMOKES. II. Identifying galaxy-scale strong gravitational lenses in Pan-STARRS using convolutional neural networks Galaxy halo truncation and giant arc surface brightness reconstruction in the cluster MACSJ1206.2-0847 H0LiCOW – IV. Lens mass model of HE 0435−1223 and blind measurement of its time-delay distance for cosmology The Hyper Suprime-Cam SSP Survey: Overview and survey design Strongly lensed SNe Ia in the era of LSST: observing cadence for lens discoveries and time-delay measurements Toward an Internally Consistent Astronomical Distance Scale H0LiCOW - IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant The story of supernova "Refsdal" told by MUSE Cosmic dissonance: are new physics or systematics behind a short sound horizon? Improving the precision of time-delay cosmography with observations of galaxies along the line of sight Galaxy-scale gravitational lens candidates from the Hyper Suprime-Cam imaging survey and the Galaxy And Mass Assembly spectroscopic survey HOLISMOKES. VII. Time-delay measurement of strongly lensed Type Ia supernovae using machine learning Two peculiar fast transients in a strongly lensed host galaxy Measuring the Value of the Hubble Constant “à la Refsdal” Editorial: Topical Collection on Astronomical Distance Determination in the Space Age Gravitational Lensing and Dynamics (GLaD): combined analysis to unveil properties of high-redshift galaxies HOLISMOKES. VI. New galaxy-scale strong lens candidates from the HSC-SSP imaging survey HOLISMOKES. I. Highly Optimised Lensing Investigations of Supernovae, Microlensing Objects, and Kinematics of Ellipticals and Spirals A measurement of the Hubble constant from angular diameter distances to two gravitational lenses HOLISMOKES. IV. Efficient mass modeling of strong lenses through deep learning HOLISMOKES. IV. Efficient mass modeling of strong lenses through deep learning (Corrigendum) HOLISMOKES. V. Microlensing of type II supernovae and time-delay inference through spectroscopic phase retrieval

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