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researcher

N. Pirzkal

213 papers hereh-index 459.2k citations310 works total

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

author position
  • first author11
  • middle author144
  • last author11

Across the 166 of 213 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA151
  • astro-ph.CO26
  • astro-ph23
  • astro-ph.IM10
  • astro-ph.HE2
  • astro-ph.SR1
same name
  • N. Pirzkal — 13 papers, h 9
  • N. Pirzkal — 4 papers, h 4
  • N. Pirzkal — 2 papers, h 2
  • N. Pirzkal — 2 papers
  • N. Pirzkal — 1 paper
  • N. Pirzkal — 1 paper, h 4

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
19972026
most citedPassively Evolving Early-type Galaxies at 1.4<z<2.5 in the Hubble Ultra Deep Field

873 citations · 10.5k across the 211 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.GA2012★ 58 cited

Emission-Line Galaxies from the Hubble Space Telescope Probing Evolution and Reionization Spectroscopically (PEARS) Grism Survey. II: The Complete Sample

Nor Pirzkal, Barry Rothberg, Chun Ly +13

We present a full analysis of the Probing Evolution And Reionization Spectroscopically (PEARS) slitess grism spectroscopic data obtained with the Advanced Camera for Surveys on HST…

astro-ph.CO2012★ 32 cited

Quantified H i Morphology VII: The Morphology of Extended Disks in UV and H i

B. W. Holwerda, N. Pirzkal, J. S. Heiner

Extended UltraViolet (xuv) disks have been found in a substantial fraction of late-type --S0, spiral and irregular-- galaxies. Similarly, most late-type spirals have an extended ga…

astro-ph.CO2012★ 29 cited

Metallicities of Emission-Line Galaxies from HST ACS PEARS and HST WFC3 ERS Grism Spectroscopy at 0.6 < z < 2.4

Lifang Xia, Sangeeta Malhotra, James Rhoads +9

Galaxies selected on the basis of their emission line strength show low metallicities, regardless of their redshifts. We conclude this from a sample of faint galaxies at redshifts…

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