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researcher

A. Moro

13 papers hereh-index 292.6k citations75 works total

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

author position
  • first author1
  • middle author7

Across the 8 of 13 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA5
  • astro-ph.HE4
  • astro-ph.CO3
  • astro-ph.IM1
same name
  • A. Moro — 45 papers, h 23
  • A. Moro — 34 papers, h 12
  • A. Moro — 19 papers, h 20
  • A. Moro — 4 papers, h 7
  • A. Moro — 4 papers, h 2
  • A. Moro — 3 papers

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
20122022
most citedThe Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library

356 citations · 1.2k across the 13 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.IM2018★ 356 cited

The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library

D. S. Aguado, Romina Ahumada, Andres Almeida +230

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years o…

astro-ph.GA2018★ 17 cited

Investigating the Covering Fraction Distribution of Swift/BAT AGN with X-ray and IR Observations

Lauranne Lanz, Ryan C. Hickox, Mislav Baloković +12

We present an analysis of a sample of 69 local obscured Swift/Burst Alert Telescope active galactic nuclei (AGNs) with X-ray spectra from NuSTAR and infrared (IR) spectral energy d…

astro-ph.GA2018★ 40 cited

Storm in a Teacup: X-ray view of an obscured quasar and superbubble

G. B. Lansbury, M. E. Jarvis, C. M. Harrison +5

We present the X-ray properties of the 'Teacup AGN' (SDSS J1430+1339), a z=0.085 type 2 quasar which is interacting dramatically with its host galaxy. Spectral modelling of the c…

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