activity
20092026
most citedEuclid. I. Overview of the Euclid mission

550 citations · 3.9k across the 60 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.IM2020★ 6 cited

Joint Survey Processing of Euclid, Rubin and Roman: Final Report

R. Chary, G. Helou, G. Brammer +22

The Euclid, Rubin/LSST and Roman (WFIRST) projects will undertake flagship optical/near-infrared surveys in the next decade. By mapping thousands of square degrees of sky and cover…

astro-ph.GA2020★ 31 cited

Selection of massive evolved galaxies at in the CANDELS fields

Abtin Shahidi, Bahram Mobasher, Hooshang Nayyeri +14

Using the CANDELS photometric catalogs for the HST/ACS and WFC3, we identified massive evolved galaxies at , employing three different selection methods. We find the c…

astro-ph.CO2020★ 117 cited

Cosmology with the Wide-Field Infrared Survey Telescope -- Multi-Probe Strategies

Tim Eifler, Hironao Miyatake, Elisabeth Krause +25

We simulate the scientific performance of the Wide-Field Infrared Survey Telescope (WFIRST) High Latitude Survey (HLS) on dark energy and modified gravity. The 1.6 year HLS Referen…

astro-ph.CO2020★ 51 cited

Cosmology with the Wide-Field Infrared Survey Telescope -- Synergies with the Rubin Observatory Legacy Survey of Space and Time

Tim Eifler, Melanie Simet, Elisabeth Krause +27

We explore synergies between the space-based Wide-Field Infrared Survey Telescope (WFIRST) and the ground-based Rubin Observatory Legacy Survey of Space and Time (LSST). In particu…

astro-ph.GA2020★ 2 cited

Bridging between the integrated and resolved main sequence of star formation

Shoubaneh Hemmati, Bahram Mobasher, Hooshang Nayyeri +6

The position of galaxies on the stellar mass, star formation rate plane with respect to the star-forming main sequence at each redshift is a convenient way to infer where the galax…

astro-ph.GA2020★ 40 cited

Spectroscopic Confirmation of a Coma Cluster Progenitor at z ~ 2.2

Behnam Darvish, Nick Z. Scoville, Christopher Martin +17

We report the spectroscopic confirmation of a new protocluster in the COSMOS field at 2.2, COSMOS Cluster 2.2 (CC2.2), originally identified as an overdensity of narrowb…