… UV-selected galaxies at z $ 3, the z $ 2 galaxies are on … a feature of star-forming galaxies
at z $ 3 are also common at later … Far from being hostile to observations, the universe at z $ 2 …

… ") around the value of L* at z∼ 2, implying that dust obscuration … z∼ 2. Accounting for
systematic differences in local and high-redshift metallicity calibrations, we find that L* galaxies at z…

A 3.6 ha experimental fire was conducted in a black spruce peatland forest that had undergone
thinning the year prior. After 50 m of spread in a natural stand at 35–60 m min −1 , the …

We present new results on the kinematics and spatial distribution of metal-enriched gas
within∼ 125 kpc of star-forming (" Lyman break") galaxies at redshifts 2≲ z≲ 3. In particular, we …

… We focus on a sample of 251 galaxies with redshifts 2.0 < z < … We show unambiguously
that the locus of z ∼ 2.3 galaxies … the offset of the z ∼ 2.3 BPT locus relative to that at z ∼ 0 is …

We use a sample of 87 rest-frame UV-selected star-forming galaxies with mean spectroscopic
redshift⟨ z⟩= 2.26±0.17 to study the correlation between metallicity and stellar mass at …

… -resolved, UV/optically selected z $ 2 star-forming galaxies … and bulges of massive galaxies
at z $ 2 can be driven by the … an order of magnitude faster than in z $ 0 disk galaxies. Early …

… The results from our own SINFONI survey of kinematics of z ∼ 2 galaxies (the subject of
the present paper), as well as similar studies carried out by other teams (eg, Erb et al. 2003, …

… early z $ 3 LBG studies. The UV LF appears to undergo little evolution … z $ 4 and z $ 2.
Corrected for extinction, the UV luminosity density (LD) at z $ 2 is at least as large as the value at z …

… of four z $ 2 submillimeter galaxies (SMGs), and sensitive CO(3Y2) flux limits toward three z
$ … gas mass conversion factors at z $ 2Y3 are probably similar to those assumed at z $ 0. The …