activity
20092026
most citedThe DESI Experiment Part I: Science,Targeting, and Survey Design

1.3k citations · 8.2k across the 112 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.GA2020★ 6 cited

New Determination of Fundamental Properties of Palomar 5 Using Deep DESI Imaging Data

Xin Xu, Hu Zou, Xu Zhou +6

The legacy imaging surveys for the Dark Energy Spectroscopic Instrument project provides multiplecolor photometric data, which are about 2 mag deeper than the SDSS. In this study,…

astro-ph.GA2020★ 96 cited

An Extended Halo-based Group/Cluster finder: application to the DESI legacy imaging surveys DR8

Xiaohu Yang, Haojie Xu, Min He +20

We extend the halo-based group finder developed by \citet[][]{Yang2005a} to use data {\it simultaneously} with either photometric or spectroscopic redshifts. A mock galaxy redshift…

astro-ph.GA2020★ 2 cited

A Mysterious Ring in Dark Space?

Wei Zhang, Fan Yang, Hong Wu +10

We report the discovery of a low-surface-brightness (27.42 mag arcsec^(-2) in g band) nebula, which has a ring-like shape in the Beijing-Arizona Sky Survey (BASS). Positive detecti…

astro-ph.GA2020★ 13 cited

Spatially-resolved Stellar Population Properties of the M 51-NGC 5195 System from Multi-wavelength Photometric Data

Peng Wei, Hu Zou, Lin Lin +5

Using multi-band photometric images of M 51 and its companion NGC 5195 from ultraviolet to optical and infrared, we investigate spatially resolved stellar population properties of…

astro-ph.GA2020★ 7 cited

The Sloan Digital Sky Survey Reverberation Mapping Project: Photometric g and i Light Curves

K. Kinemuchi, Patrick B. Hall, Ian McGreer +28

The Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) program monitors 849 active galactic nuclei (AGN) both spectroscopically and photometrically. The photometric observati…

astro-ph.GA2020★ 7 cited

Physical Properties of H II Regions in M51 from Spectroscopic Observations

Peng Wei, Hu Zou, Xu Kong +13

M51 and NGC 5195 is an interacting system that can be explored in great details with ground-based telescopes. The H II regions in M51 were observed using the 2.16 m telescope of th…