• No results found

University of Groningen Gravitational lensing at milliarcsecond angular resolution Spingola, Cristiana

N/A
N/A
Protected

Academic year: 2021

Share "University of Groningen Gravitational lensing at milliarcsecond angular resolution Spingola, Cristiana"

Copied!
2
0
0

Bezig met laden.... (Bekijk nu de volledige tekst)

Hele tekst

(1)

University of Groningen

Gravitational lensing at milliarcsecond angular resolution Spingola, Cristiana

IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below.

Document Version

Publisher's PDF, also known as Version of record

Publication date: 2019

Link to publication in University of Groningen/UMCG research database

Citation for published version (APA):

Spingola, C. (2019). Gravitational lensing at milliarcsecond angular resolution. Rijksuniversiteit Groningen.

Copyright

Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons).

Take-down policy

If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim.

Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. For technical reasons the number of authors shown on this cover page is limited to 10 maximum.

(2)

Propositions

accompanying the dissertation

Gravitational lensing

at milliarcsecond angular resolution

by

Cristiana Spingola

1. Astrometric anomalies in strong gravitational lenses measured with VLBI observations indicate the failure of a smooth lens mass model at milliarcsec-ond scales (Chapter 2).

2. A mass density slope steeper than isothermal in low-mass elliptical lensing galaxies supports the two-phase galaxy formation model (Chapter 2). 3. The combination of strong gravitational lensing with high-resolution

spa-tially resolved kinematics reveals rotation and interaction in molecular gas of high-redshift galaxies, providing new clues to their formation (Chapter 3).

4. Multi-epoch VLBI observations of gravitationally lensed radio sources at high redshift can reveal astrometric positional changes of the order of tens of microarcseconds, testing formation models for supermassive black holes (Chapter 4).

5. Major advances in wide-field VLBI surveys enable efficient one-step high-resolution searches for gravitationally lensed radio sources (Chapter 5). 6. The gravitational imaging technique applied to sensitive VLBI observations

of strong lensing systems is a promising method to probe low-mass sub-structures, which are the key population for testing dark matter models. 7. The mindful sharing of data and software in Astronomy should be adopted

by the entire scientific community, as it ensures the progress of science rather than that of individual research groups.

8. The culinary art requiring the highest accuracy is patisserie. 9. Kindness is a relief in a society afflicted by hatred.

Referenties

GERELATEERDE DOCUMENTEN

Then, we forward ray-trace the source components to the image plane and determine if the predicted positions of the lensed images match the observations at Epoch 2.. We find that

However, once a gravitationally lensed radio source has been identified from the survey data, an indication for ex- tended emission that wasn’t fully detected from the

VLBI observations at milliarcsecond angular resolution of gravitationally lensed radio jets give a large number of constraints on the mass density distribution of a lensing

Om hier een verklaring voor te vinden is het noodzakelijk om alle satellieten, die mogelijk door duistere materie worden gedomineerd, binnen en buiten de Lokale Groep te detecteren

Le osservazioni global VLBI ad alta risoluzione di questi archi gravitazionali hanno fornito un numero elevato di vincoli al modello di massa delle galassie lenti, perciò abbiamo

If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim.. Downloaded

Ringrazio di cuore la commissione esterna, Peter Barthel, Stephen Ser- jeant e Rachel Webster, per aver trova- to il tempo di leggere questa tesi e per le loro correzioni, che

We consider new scalar quantities in the context of High Angular Resolution Diffusion Imaging (HARDI), namely, the principal invariants of fourth-order tensors modeling the