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20002023
most citedStar Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies

2k citations · 4.9k across the 51 of their papers we have counts for

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Showing 2005Show all

15 papers · 1 filter

astro-ph2005

An investigation of the submillimeter background radiation using SCUBA and Spitzer

S. Dye, S. A. Eales, M. L. N. Ashby +8

We investigate the redshift dependence of the contribution to the extragalactic far-infrared/sub-millimeter background from galaxies detected by the Spitzer Space Telescope at 8um…

astro-ph2005

The Chandra XBootes Survey - III: Optical and Near-IR Counterparts

Kate Brand, Michael J. I. Brown, Arjun Dey +14

The XBootes Survey is a 5-ks Chandra survey of the Bootes Field of the NOAO Deep Wide-Field Survey (NDWFS). This survey is unique in that it is the largest (9.3 deg^2), contiguous…

astro-ph2005

Discovery of a Planetary-Mass Brown Dwarf with a Circumstellar Disk

K. L. Luhman, Lucia Adame, Paola D'Alessio +4

Using the Hubble Space Telescope, the 4 m Blanco telescope at the Cerro Tololo Inter-American Observatory, and the Spitzer Space Telescope, we have performed deep imaging from 0.8…

astro-ph2005

Identifying Primordial Substructure in NGC 2264

Paula S. Teixeira, Charles J. Lada, Erick T. Young +8

We present new Spitzer Space Telescope observations of the young cluster NGC2264. Observations at 24 micron with the Multiband Imaging Photometer has enabled us to identify the mos…

astro-ph2005

Star Formation in Distant Red Galaxies: Spitzer observations in the Hubble Deep Field South

Tracy Webb, Pieter van Dokkum, Eiichi Egami +12

We present Spitzer 24micron imaging of 1.5 < z < 2.5 Distant Red Galaxies (DRGs) in the 10arcmin by 10arcmin Extended Hubble Deep Field South of the Multiwavelength Survey by Yale-…

astro-ph2005

Spitzer/IRAC Photometry of the Eta Chameleontis Association

S. T. Megeath, L. Hartmann, K. L. Luhman +1

We present IRAC 3.6, 4.5, 5.8 and 8 micron photometry for the 17 A, K and M type members of the Eta Chameleontis association. These data show infrared excesses toward six of the 15…