Showing 1–20 of 47 results
/ Date/ Name
Aug 14, 2024Star-formation Properties of z ~ 1 Galaxy Clusters and Groups from Horizon Run 5Jul 9, 2024Multi-Object Spectroscopy of Galaxy Clusters at $z \sim 0.95$ in Ultra Deep Survey Field with Different Star-formation Properties and Large-scale EnvironmentsOct 24, 2019More connected, more active: galaxy clusters and groups at z~1 and the connection between their quiescent galaxy fractions and large-scale environmentsDec 30, 2008Biases and Uncertainties in Physical Parameter Estimates of Lyman Break Galaxies from Broad-band PhotometryOct 10, 2010Improving the Estimation of Star formation Rates and Stellar Population Ages of High-redshift Galaxies from Broadband PhotometryMar 25, 2014Steadily Increasing Star Formation Rates in Galaxies Observed at 3 <~ z <~ 5 in the CANDELS/GOODS-S FieldAug 6, 2015Evolution of Star-formation Properties of High-redshift Cluster Galaxies since $z = 2$Dec 16, 2014Stellar masses from the CANDELS survey: the GOODS-South and UDS fieldsMay 4, 2017CANDELS Sheds Light on the Environmental Quenching of Low-mass GalaxiesMar 17, 2015The AKARI 2.5-5.0 Micron Spectral Atlas of Type-1 Active Galactic Nuclei: Black Hole Mass Estimator, Line Ratio, and Hot Dust TemperatureJun 12, 2024ODIN: Identifying Protoclusters and Cosmic Filaments Traced by Ly$α$-emitting GalaxiesJul 31, 2015Host Galaxy Properties and Black Hole Mass of Swift J164449.3+573451 from Multi-Wavelength Long-Term Monitoring and HST DataDec 19, 2025ODIN: A New Lyman Alpha Blob Selection Method, Sample, and Statistical Analysis at $z\sim3.1$Mar 30, 2026KMTNet Synoptic Survey of Southern Sky III: The First Data ReleaseMar 16, 2017CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth StripDec 18, 2017Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0Feb 11, 2016Evolution of Intrinsic Scatter in the SFR-Stellar Mass Correlation at 0.5<z<3Oct 15, 2014The Infrared Medium-Deep Survey II: How to Trigger Radio-AGN? Hints from Their EnvironmentsJul 20, 2015The Evolution of the Galaxy Stellar Mass Function at z= 4-8: A Steepening Low-mass-end Slope with Increasing RedshiftOct 10, 2024Galaxy populations in protoclusters at cosmic noon