about
On the classification of UGC 1382 as a giant low surface brightness galaxyThe HETDEX pilot survey. V. The physical origin of Ly{alpha} emitters probed by near-infrared spectroscopyThe 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 ObservatoryCorrigendum to “Spectroscopic needs for imaging dark energy experiments” [Astropart. Phys. 63 (2015) 81–100]Spectroscopic needs for imaging dark energy experimentsLearning from FITS: Limitations in use in modern astronomical researchBayesian Redshift Classification of Emission-line Galaxies with Photometric Equivalent Widths3D-HST emission line galaxies at z ~ 2: discrepancies in the Optical/UV star formation ratesTo stack or not to stack: spectral energy distribution properties of ly{alpha}-emitting galaxies at z = 2.1Searching for neutral hydrogen halos around z ~ 2.1 and z ~ 3.1 Ly{alpha} emitting galaxiesSDSS IV MaNGA: Discovery of an Hα Blob Associated with a Dry Galaxy Pair—Ejected Gas or a “Dark” Galaxy Candidate?The biases of optical line-ratio selection for active galactic nuclei and the intrinsic relationship between black hole accretion and galaxy star formationSDSS-IV MaNGA: Spatially Resolved Star Formation Main Sequence and LI(N)ER SequenceThe Astropy Project: Building an Open-science Project and Status of the v2.0 Core PackageMid-infrared photometric analysis of main belt asteroids: a technique for color-color differentiation from background astrophysical sourcesHST emission line galaxies at z ~ 2: comparing physical properties of Lyman alpha and optical emission line selected galaxiesThe dust attenuation curve versus stellar mass for emission line galaxies at z ~ 2Spectral energy distribution fitting of HETDEX pilot survey Ly{alpha} emitters in COSMOS and GOODS-NIs the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies?Young, star-forming galaxies and their local counterparts: the evolving relationship of mass-SFR-metallicity since z ~ 2.1The evolution of the Far-UV luminosity function and star formation rate density of the Chandra Deep Field-South from z = 0.2 to 1.2 with Swift/UVOTSurveying galaxy proto-clusters in emission: a large-scale structure at z = 2.44 and the outlook for HETDEXPhysical and morphological properties of [O II] emitting galaxies in the HETDEX pilot surveyHubble Space Telescope emission-line galaxies at z ~ 2: the mystery of neonHubble Space Telescope emission line galaxies at z ~ 2: the Ly{alpha} escape fractionGalaxy redshift surveys with sparse samplingThe Lyα Reference Sample. VIII. Characterizing Lyα Scattering in Nearby GalaxiesSwift Ultraviolet Survey of the Magellanic Clouds (SUMaC). I. Shape of the Ultraviolet Dust Extinction Law and Recent Star Formation History of the Small Magellanic CloudThe spectrally resolved Ly{alpha} emission of three ly{alpha}-selected field galaxies at z ~ 2.4 from the HETDEX pilot survey
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description
onderzoeker
@nl
researcher
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հետազոտող
@hy
name
Alex Hagen
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Alex Hagen
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Alex Hagen
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Alex Hagen
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Alex Hagen
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Alex Hagen
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Alex Hagen
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Alex Hagen
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Alex Hagen
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Alex Hagen
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Alex Hagen
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Alex Hagen
@nl
P106
P21
P31
P496
0000-0003-2031-7737