about
Suppressing star formation in quiescent galaxies with supermassive black hole winds.Overview of the SDSS-IV MaNGA survey: Mapping Nearby Galaxies at Apache Point ObservatoryThe DEEP2 Galaxy Redshift Survey: AEGIS Observations of a Dual AGN at z = 0.7The evolution of dusty star formation in galaxy clusters to z = 1: Spitzer infrared observations of the first Red-Sequence Cluster SurveyThe Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the Extended Baryon Oscillation Spectroscopic Survey and from the Second Phase of the Apache Point Observatory Galactic Evolution ExperimentSloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant UniverseThe 13th Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey Mapping Nearby Galaxies at Apache Point ObservatoryThe DEEP2 Galaxy Redshift Survey: The Evolution of Void Statistics from z ∼ 1 to z ∼ 0Mock Catalogs for the DEEP2 redshift surveyConstraining Evolution in the Halo Model Using Galaxy Redshift SurveysSDSS IV MaNGA – sSFR profiles and the slow quenching of discs in green valley galaxiesLow Metallicities and Old Ages for Three Ultra-diffuse Galaxies in the Coma ClusterSDSS-IV MaNGA: constraints on the conditions for star formation in galaxy discsThe SDSS-IV MaNGA Sample: Design, Optimization, and Usage ConsiderationsSDSS-IV MaNGA – the spatially resolved transition from star formation to quiescenceSDSS-IV MaNGA IFS GALAXY SURVEY—SURVEY DESIGN, EXECUTION, AND INITIAL DATA QUALITYSDSS-IV MaNGA: A SERENDIPITOUS OBSERVATION OF A POTENTIAL GAS ACCRETION EVENTSDSS-IV MaNGA: properties of galaxies with kinematically decoupled stellar and gaseous componentsThe data reduction pipeline for the SDSS-IV MaNGA IFU galaxy surveySDSS IV MaNGA – spatially resolved diagnostic diagrams: a proof that many galaxies are LIERsX-ray Surface Brightness Profiles of Active Galactic Nuclei in the Extended Groth Strip: Implications for AGN FeedbackThe DEEP2 Galaxy Redshift Survey: the red sequence AGN fraction and its environment and redshift dependenceNitrogen-to-Oxygen abundance ratio variation in quiescent galaxiesShocks or photoionization: direct temperature measurements of the low-ionization gas in quiescent galaxiesSDSS-IV MaNGA: Spatially Resolved Star Formation Main Sequence and LI(N)ER SequenceBiases in Metallicity Measurements from Global Galaxy Spectra: The Effects of Flux Weighting and Diffuse Ionized Gas ContaminationEvolution of Galactic Outflows at $z\sim 0\mbox{--}2$ Revealed with SDSS, DEEP2, and Keck SpectraThe quenching timescale and quenching rate of galaxiesStellar metallicity gradients in SDSS galaxiesObserving strategy for the SDSS-IV/MaNGA IFU galaxy surveyMetal-poor, strongly star-forming galaxies in the DEEP2 survey: the relationship between stellar mass, temperature-based metallicity, and star formation rateP-MaNGA: GRADIENTS IN RECENT STAR FORMATION HISTORIES AS DIAGNOSTICS FOR GALAXY GROWTH AND DEATHImproved mock galaxy catalogs for the DEEP2 galaxy redshift survey from subhalo abundance and environment matchingTesting diagnostics of nuclear activity and star formation in galaxies at z > 1Origin and Ionization of the Warm Ionized Gas in Massive Early-type GalaxiesThe DEEP2 Galaxy Redshift Survey: First Results on Galaxy GroupsGalaxy assembly bias on the red sequenceSDSS-IV MaNGA: bulge–disc decomposition of IFU data cubes (BUDDI)Stellar mass-gas-phase metallicity relation at 0.5 <= z <= 0.7: a power law with increasing scatter toward the low-mass regimeA CANDELS WFC3 grism study of emission-line galaxies at z ~ 2: a mix of nuclear activity and low-metallicity star formation
P50
Q50638697-335E2F37-9792-4303-9B71-7053AAAB02BCQ56432485-3094F143-0ED7-4F39-B99B-E202A638D633Q56882015-9322EC43-D7CE-4046-A200-344F6708F817Q57088396-31E088FE-D02A-4D05-9FBF-6ACFE130CF33Q57442000-B0B0ECC1-E8F7-43BC-AFC6-1BEE95402308Q57446723-F61491D6-CDB1-471D-93D7-9F3EB2A36FC2Q57450290-5CDC6981-BE8D-4466-9E0E-8E8A069A7B40Q57630881-AE3B23C7-3E7C-4D11-A2F8-FAE260A8F39CQ57630901-43A4FB91-648A-41D7-9D51-5FCB6F2A7B07Q57630933-F733B15D-091F-4C50-B6F5-5546B3070905Q58229795-A0453F68-8926-4D8F-8C05-9D56209A9AE1Q58229800-7AFFC029-5BAB-4684-AB7A-33C4B809F473Q58229815-4E8B70A7-BEBE-4CBC-8AEC-AFDF554D2A98Q58229860-EB52AE3F-E881-4114-AA7B-BD0FE59DC854Q58229876-E5195B35-0C2C-435F-A55D-50D8A780D654Q58229894-090DC108-9CE6-44AF-9026-1C50C7799620Q58229901-1BD1B603-C69A-42F3-9B7C-6F2A12845D0EQ58229913-12116A4D-E68B-495C-8474-0B8D1BEE64C3Q58229919-22056558-8438-4471-BEBB-EE0713CF7E89Q58229922-E1A146F7-B0BF-4898-A3F3-6831944A95DBQ58258236-8204490E-707E-45D2-9B20-E59708B8D7E5Q58258262-DAD343AB-DBDB-4F79-8B4C-4C3B14F5E6F0Q58265579-5380386E-F481-477B-8561-1F560B5DC6C4Q58265583-C1A90AD0-5F58-4269-A9DB-1DA7FCB4DAA7Q58265588-16A3691B-3551-41DA-B136-08503CE97750Q58265591-C06692BA-B98E-4824-A9D8-6858C83458A6Q58265595-293061A4-0BB9-42D2-B37E-A2ADBD61D315Q58265599-181B7AEA-9D12-4DBE-834E-638673728E1CQ58265605-E8EF0C7F-74B5-44E9-A137-8716923E1E67Q58265612-58FA4A13-FD4D-4893-83B9-DA6C24205AC9Q58265620-C4E16BE7-FE85-4955-8AAD-3A38F4095DE3Q58265626-C2E48B92-52EB-40D6-A457-F81AE60A548BQ58265633-F8AC4585-E082-400B-8352-88547706E8CAQ58265639-BB88B6E2-21B1-448D-B9ED-32254BD6C66BQ58265645-1C532F98-310F-4CA7-B761-E97640E167DCQ58265648-25C48D6A-EE7A-4273-8296-EFFDBA99B52CQ58265652-4C6D72D3-C103-4FDB-BF4D-2B273E4D9A8EQ58302632-AE70AB26-D4D3-4F4F-B4B2-115E725ECB39Q58908156-53E84D2E-81C5-466A-A7AF-B3BAAF1EB980Q58908673-7331B208-A3DD-4AC8-B63C-C5E246888479
P50
description
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
Renbin Yan
@ast
Renbin Yan
@en
Renbin Yan
@es
Renbin Yan
@nl
type
label
Renbin Yan
@ast
Renbin Yan
@en
Renbin Yan
@es
Renbin Yan
@nl
altLabel
严人斌
@en
prefLabel
Renbin Yan
@ast
Renbin Yan
@en
Renbin Yan
@es
Renbin Yan
@nl
P108
P106
P21
P31
P496
0000-0003-1025-1711