about
Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10¹¹ solar massesHerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurementsThe dust morphology of the elliptical Galaxy M 86 with SPIREThe Multiband Imaging Photometer forSpitzer(MIPS)On-orbit performance of the MIPS instrumentTheHerschel-SPIRE instrument and its in-flight performanceCold dust and young starbursts: spectral energy distributions of Herschel SPIRE sources from the HerMES survey★Evolution of dust temperature of galaxies through cosmic time as seen by HerschelFirst results from HerMES on the evolution of the submillimetre luminosity functionHerMES: deep galaxy number counts from a P(D) fluctuation analysis of SPIRE Science Demonstration Phase observationsHerMES: Far infrared properties of known AGN in the HerMES fieldsHerMES: The SPIRE confusion limitHerMES: The submillimeter spectral energy distributions of Herschel/SPIRE-detected galaxiesHerschel unveils a puzzling uniformity of distant dusty galaxiesMeasures of star formation rates from infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fieldsThe Deep SPIRE HerMES Survey: spectral energy distributions and their astrophysical indications at high redshiftThe HerMES SPIRE submillimeter local luminosity functionThe Herschel Multi-Tiered Extragalactic Survey: source extraction and cross-identifications in confusion-dominated SPIRE imagesThe far-infrared/radio correlation as probed by HerschelLocal benchmarks for the evolution of major-merger galaxies--Spitzer observations of a K-band selected sampleA Herschel/PACS Far-infrared Line Emission Survey of Local Luminous Infrared GalaxiesALMA [N ii] 205 μm Imaging Spectroscopy of the Interacting Galaxy System BRI 1202-0725 at Redshift 4.7AHerschel Space ObservatorySpectral Line Survey of Local Luminous Infrared Galaxies from 194 to 671 MicronsMeasuring star formation rate and far-infrared color in high-redshift galaxies using the CO(7-6) and [N II] 205 {mu}m linesALMA observations of warm dense gas in NGC 1614--Breaking of the star formation law in the central kiloparsecThe identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratiosFIR colours and SEDs of nearby galaxies observed with HerschelALMA Maps of Dust and Warm Dense Gas Emission in the Starburst Galaxy IC 5179ALMA imaging of the CO (6-5) line emission in NGC 7130THE [N ii] 205μm EMISSION IN LOCAL LUMINOUS INFRARED GALAXIESExtended [C II] emission in local luminous infrared galaxiesWarm molecular gas in luminous infrared galaxiesALMA observations of warm molecular gas and cold dust in NGC 34Explaining the [C II]157.7 {mu}m deficit in luminous infrared Galaxies--First results from a Herschel/PACS study of the GOALS sampleA Herschel survey of the [N II] 205 {mu}m line in local luminous infrared galaxies: the [N II] 205 {mu}m emission as a star formation rate indicatorErratum: The Herschel PEP/HerMES Luminosity Function – I. Probing the Evolution of PACS selected Galaxies to z ≃ 4The Herschel PEP/HerMES luminosity function – I. Probing the evolution of PACS selected Galaxies to z ≃ 4Herschel reveals a Tdust-unbiased selection of z∼ 2 ultraluminous infrared galaxiesHerMES: SPIRE galaxy number counts at 250, 350, and 500 μmHigh-J CO versus far-infrared relations in normal and starburst galaxies
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description
Chinees onderzoeker
@nl
Chinese astrophysicist
@en
astrofísico chino
@es
astrophysicisien chinois
@fr
chiński badacz
@pl
réaltfhisiceoir Síneach
@ga
name
Nanyao Lu
@ast
Nanyao Lu
@cy
Nanyao Lu
@en
Nanyao Lu
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Nanyao Lu
@fr
Nanyao Lu
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Nanyao Lu
@nl
type
label
Nanyao Lu
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altLabel
N. Lu
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Nanyao Lu
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Nanyao Lu
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Nanyao Lu
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Nanyao Lu
@es
Nanyao Lu
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Nanyao Lu
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Nanyao Lu
@nl
P106
P21
P31
P496
0000-0002-8948-1044