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L. Stella

22 papers hereh-index 6017.1k citations501 works total

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

author position
  • first author2
  • middle author10
  • last author7

Across the 19 of 22 papers where every author was matched, so the position is known.

fields
  • astro-ph22
same name
  • L. Stella — 12 papers
  • L. Stella — 2 papers, h 36
  • L. Stella — 2 papers
  • L. Stella — 1 paper, h 17
  • L. Stella — 1 paper

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
19942008
most citedMulticolor observations of the afterglow of the short/hard GRB 050724

61 citations · 118 across the 6 of their papers we have counts for

collaborators
Showing 1999Show all

4 papers · 1 filter

astro-ph1999

XTE and SAX observations of the Be/neutron star system RX J0146.9+6121

S. Mereghetti, A. Tiengo, G. L. Israel +1

We report XTE and SAX observations of the X-ray pulsar RX J0146.9+612, the neutron star/Be binary system with the longest known spin period. Data obtained one month after the most…

astro-ph1999

A BeppoSAX study of the pulsating transient X0115+63: the first X-ray spectrum with four cyclotron harmonic features

A. Santangeo, A. Segreto, S. Giarrusso +9

The recurrent hard pulsating X-ray transient §was observed with \B on March 19, when the source was at a 2--10 keV flux level of ∼310~mCrab. We report on the high energy spect…

astro-ph1999

GRB 990510: linearly polarized radiation from a fireball

S. Covino, D. Lazzati, G. Ghisellini +12

Models for gamma-ray burst afterglows envisage an hyper-relativistic fireball that is decelerated in the ambient medium around the explosion site. This interaction produces a shock…

astro-ph1999

BeppoSAX monitoring of the ``anomalous'' X-ray pulsar 4U 0142+61

G. L. Israel, T. Oosterbroek, L. Angelini +7

The 8.7s X-ray pulsar 4U 0142+61 was monitored by BeppoSAX between January 1997 and February 1998. This source belongs to the rapidly growing class of "anomalous" X-ray pulsars (AX…

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