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researcher

P. van der Werf

54 papers here

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

author position
  • sole author1
  • first author1
  • middle author28
  • last author13

Across the 43 of 54 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA43
  • astro-ph.CO6
  • astro-ph2
  • astro-ph.SR2
  • astro-ph.IM1
ORCID 0000-0001-5434-5942
same name
  • P. van der Werf — 2 papers, h 4
  • P. van der Werf — 2 papers
  • P. van der Werf — 1 paper
  • P. van der Werf — 1 paper
  • P. van der Werf — 1 paper
  • P. van der Werf — 1 paper, h 10

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
20002025
most citedMolecular line emission in NGC1068 imaged with ALMA. I An AGN-driven outflow in the dense molecular gas

476 citations · 3.6k across the 54 of their papers we have counts for

collaborators
Showing 2024 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2024★ 33 cited

Insight into the Starburst Nature of Galaxy GN-z11 with JWST MIRI Spectroscopy

J. Álvarez-Márquez, A. Crespo Gómez, L. Colina +21

This paper presents a deep MIRI/JWST medium resolution spectroscopy (MRS) covering the rest-frame optical spectrum of the GN-z11 galaxy. The [OIII]5008 and Hα emission lines are…

astro-ph.GA2024

Components of star formation in NGC 253 : Non-negative Matrix Factorization Analysis with the ALCHEMI integrated intensity images

Ryo Kishikawa, Nanase Harada, Toshiki Saito +12

It is essential to examine the physical or chemical properties of molecular gas in starburst galaxies to reveal the underlying mechanisms characterizing starbursts. We used non-neg…

astro-ph.GA2024★ 39 cited

The Structure of Massive Star-Forming Galaxies from JWST and ALMA: Dusty, High Redshift Disk Galaxies

Steven Gillman, Ian Smail, Bitten Gullberg +15

We present an analysis of the JWST NIRCam and MIRI morphological properties of 80 massive (log10​(M∗​[M⊙​])=11.2±0.1) dusty star-forming galaxies at z=2.7$^{+…

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