SAS-LBG SSA22a-M38 , the SIMBAD biblio

SAS-LBG SSA22a-M38 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST20:12:59


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Title First 3 Authors
2003ApJ...592..728S viz 2596 653 Lyman break galaxies at redshift z ∼ 3: survey description and full data set. STEIDEL C.C., ADELBERGER K.L., SHAPLEY A.E., et al.
2008A&A...488..463M 132       D       C       4 10 854 AMAZE. I. The evolution of the mass-metallicity relation at z>3. MAIOLINO R., NAGAO T., GRAZIAN A., et al.
2010MNRAS.401.1521M viz 15       D               1 245 104 On the stellar masses of IRAC detected Lyman break galaxies at z ∼ 3. MAGDIS G.E., RIGOPOULOU D., HUANG J.-S., et al.
2010Natur.467..811C 35 3 212 Gas accretion as the origin of chemical abundance gradients in distant galaxies. CRESCI G., MANNUCCI F., MAIOLINO R., et al.
2010Msngr.142...36M 11 4 AMAZE and LSD: Metallicity and dynamical evolution of galaxies in the early universe. MAIOLINO R., MANNUCCI F., CRESCI G., et al.
2011A&A...528A..88G 400       D     X C       10 36 137 Dynamical properties of AMAZE and LSD galaxies from gas kinematics and the Tully-Fisher relation at z∼3. GNERUCCI A., MARCONI A., CRESCI G., et al.
2011A&A...533A.124G 15       D               1 11 14 A dynamical mass estimator for high z galaxies based on spectroastrometry. GNERUCCI A., MARCONI A., CRESCI G., et al.
2013MNRAS.435.2918M 20       D               2 4 37 Abundance gradients in spiral discs: is the gradient inversion at high redshift real ? MOTT A., SPITONI E. and MATTEUCCI F.
2014A&A...563A..58T 18       D   O           1 43 205 Metallicity evolution, metallicity gradients, and gas fractions at z ∼ 3.4. TRONCOSO P., MAIOLINO R., SOMMARIVA V., et al.
2014ApJ...787..120S 1 17 62 Stars were born in significantly denser regions in the early universe. SHIRAZI M., BRINCHMANN J. and RAHMATI A.
2021ApJ...919...51M viz 44           X         1 24 7 On the nature of AGN and star formation enhancement in the z = 3.1 SSA22 protocluster: the HST WFC3 IR view. MONSON E.B., LEHMER B.D., DOORE K., et al.

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