_id,doi,title
11619,10.1051/0004-6361/201834289,"TESS’s first planet: A super-Earth transiting the naked-eye star π Mensae"
11631,10.48550/arXiv.1811.12140,FliPer: Classifying TESS pulsating stars
11518,10.3847/1538-4357/aa9931,ALMA reveals metals yet no dust within multiple components in CR7
11564,10.1093/mnras/stw2973,"The production and escape of Lyman-Continuum radiation from star-forming galaxies at z ∼ 2 and their redshift evolution"
11572,10.1093/mnras/stx2061,"Spectroscopic properties of luminous Ly α emitters at z ≈ 6–7 and comparison to the Lyman-break population"
11633,10.48550/arXiv.1711.02890,FliPer: Checking the reliability of global seismic parameters from automatic pipelines
11574,10.1093/mnras/stw2076,"The Lyα luminosity function at z= 5.7–6.6 and the steep drop of the faint end: Implications for reionization"
11575,10.1093/mnras/stw717,The Fundamental Plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
11519,10.1088/0004-637X/808/2/139,Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation
11579,10.1093/mnras/stv1795,The brightest Lyα emitter: Pop III or black hole?
11583,10.1093/mnras/stu392,A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys