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researcher

M. Tang

47 papers hereh-index 201.7k citations59 works total

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

author position
  • first author13
  • middle author25
  • last author7

Across the 45 of 47 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA46
  • astro-ph.CO1
same name
  • M. Tang — 62 papers, h 5
  • M. Tang — 50 papers, h 25
  • M. Tang — 33 papers, h 4
  • M. Tang — 31 papers, h 10
  • M. Tang — 24 papers, h 17
  • M. Tang — 21 papers, h 8

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
20152026
most citedJADES NIRSpec Spectroscopy of GN-z11: Lyman-α emission and possible enhanced nitrogen abundance in a z=10.60 luminous galaxy

396 citations · 2.4k across the 46 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.GA2020★ 50 cited

Lyman-alpha spectroscopy of extreme [OIII] emitting galaxies at z≃2−3: Implications for Lyα visibility and LyC leakage at z>6

Mengtao Tang, Daniel Stark, Jacopo Chevallard +3

Spectroscopic observations of massive z>7 galaxies selected to have extremely large [OIII]+Hβ equivalent width (EW ∼1500 Å) have recently revealed large Lyα detection ra…

astro-ph.GA2020★ 56 cited

The Lyman Continuum Escape Survey: Connecting Time-Dependent [OIII] and [OII] Line Emission with Lyman Continuum Escape Fraction in Simulations of Galaxy Formation

Kirk S. S. Barrow, Brant E. Robertson, Richard S. Ellis +4

Escaping Lyman continuum photons from galaxies likely reionized the intergalactic medium at redshifts z≳6. However, the Lyman continuum is not directly observable at these…

astro-ph.GA2020★ 49 cited

Rest-frame UV spectroscopy of extreme [OIII] emitters at 1.3<z<3.7: Toward a high-redshift UV reference sample for JWST

Mengtao Tang, Daniel Stark, Jacopo Chevallard +3

Deep spectroscopy of galaxies in the reionization-era has revealed intense CIII] and CIV line emission (EW >15−20 Å). In order to interpret the nebular emission emerging at z>6…

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