activity
20012023
most citedAMAZE. I. The evolution of the mass-metallicity relation at z>3

990 citations · 2.3k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.IM2023★ 490 cited

The James Webb Space Telescope Mission

Jonathan P. Gardner, John C. Mather, Randy Abbott +1004

Twenty-six years ago a small committee report, building on earlier studies, expounded a compelling and poetic vision for the future of astronomy, calling for an infrared-optimized…

astro-ph.GA2022★ 87 cited

First Sample of H+[O III] 5007 Line Emitters at Through JWST/NIRCam Slitless Spectroscopy: Physical Properties and Line Luminosity Functions

Fengwu Sun, Eiichi Egami, Nor Pirzkal +26

We present a sample of four emission-line galaxies at that were serendipitously discovered using the commissioning data for the JWST/NIRCam wide-field slitless spectr…

astro-ph.CO2013★ 5 cited

Chronos: A NIR spectroscopic galaxy survey. From the formation of galaxies to the peak of activity

I. Ferreras, R. Sharples, J. S. Dunlop +30

Chronos is our response to ESA's call for white papers to define the science for the future L2, L3 missions. Chronos targets the formation and evolution of galaxies, by collecting…

astro-ph.CO2010★ 80 cited

PEP: first Herschel probe of dusty galaxy evolution up to z~3

C. Gruppioni, F. Pozzi, P. Andreani +32

We exploit the deepest existing far-infrared (FIR) data obtained so far by Herschel at 100 and 160 um in the GOODS-N, as part of the PACS Evolutionary Probe (PEP) survey, to derive…

astro-ph.CO2010★ 254 cited

The first Herschel view of the mass-SFR link in high-z galaxies

G. Rodighiero, A. Cimatti, C. Gruppioni +37

We exploit deep observations of the GOODS-N field taken with PACS, on board of Herschel, as part of the PEP guaranteed time, to study the link between star formation and stellar ma…

astro-ph.CO2010★ 120 cited

Dissecting the cosmic infra-red background with Herschel/PEP

S. Berta, B. Magnelli, D. Lutz +34

The constituents of the cosmic IR background (CIB) are studied at its peak wavelengths (100 and 160 um) by exploiting Herschel/PACS observations of the GOODS-N, Lockman Hole, and C…