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researcher

J. Emerson

35 papers hereh-index 356.6k citations154 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author29
  • last author3

Across the 32 of 35 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA16
  • astro-ph.SR8
  • astro-ph4
  • astro-ph.CO4
  • astro-ph.IM3
same name
  • J. Emerson — 58 papers, h 35
  • J. Emerson — 10 papers, h 5
  • J. Emerson — 8 papers, h 7
  • J. Emerson — 2 papers, h 3
  • J. Emerson — 1 paper, h 22
  • J. Emerson — 1 paper, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19982020
most citedUltraVISTA: a new ultra-deep near-infrared survey in COSMOS

829 citations · 4.2k across the 35 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2007★ 483 cited

The WFCAM Science Archive

N. C. Hambly, R. S. Collins, N. J. G. Cross +13

We describe the WFCAM Science Archive (WSA), which is the primary point of access for users of data from the wide-field infrared camera WFCAM on the United Kingdom Infrared Telesco…

astro-ph2007★ 1 cited

The UKIRT Infrared Deep Sky Survey Second Data Release

S. J. Warren, N. J. G. Cross, S. Dye +26

The UKIRT Infrared Deep Sky Survey (UKIDSS) is a set of five large near-infrared surveys, covering a complementary range of areas, depths, and Galactic latitudes. The UKIDSS Second…

astro-ph2006★ 215 cited

The UKIRT Infrared Deep Sky Survey First Data Release

S. J. Warren, N. C. Hambly, S. Dye +37

The First Data Release (DR1) of the UKIRT Infrared Deep Sky Survey (UKIDSS) took place on 2006 July 21. UKIDSS is a set of five large near-infrared surveys, covering a complementar…

astro-ph1998★ 12 cited

Magnetospheric Accretion and PMS Stellar Masses

Ian A. Bonnell, Kester W. Smith, Michael R. Meyer +3

We present a method of determining lower limits on the masses of pre-main-sequence (PMS) stars and so constraining the PMS evolutionary tracks. This method uses the red-shifted abs…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.