Conference
A large area search for radio-loud quasars within the epoch of reionization
- Abstract:
- The Universe became fully reionized, and observable optically, at a time corresponding to redshift z ~ 6.5, so it is only by studying the HI and molecular absorption lines against higher-redshift, radio-loud sources that one can hope to make detailed studies of the earliest stages of galaxy formation. At present no targets for such studies are known. In these proceedings we describe a survey which is underway to find radio-loud quasars at z > 6.5, and present broad-band SEDs of our most promising candidates.
- Publication status:
- Published
- Version:
- Accepted Manuscript
Actions
Access Document
- Files:
-
-
(pdf, 132.7KB)
-
- Publisher copy:
- 10.1142/9789812702432_0034
Why is the content I wish to access not available via ORA?
Bibliographic data (the information relating to research outputs) and full-text items (e.g. articles, theses, reports, etc.) arrive in ORA from several different sources. Unfortunately we are not able to make available the full-text for every research output.
Please contact the ORA team (
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
Content may be unavailable for the following four reasons
-
Version unsuitable
-
We have not obtained a suitable full-text for a given research output. See this page for more information.
-
Recently completed
-
Sometimes content is held in ORA but is unavailable for a fixed period of time to comply with the policies and wishes of rights holders.
-
Permissions
-
All content made available in ORA should comply with relevant rights, such as copyright. See this page for more information.
-
Clearance
-
Some thesis volumes scanned as part of the digitisation scheme funded by Dr Leonard Polonsky are currently unavailable due to sensitive material or uncleared third-party copyright content. We are attempting to contact authors whose theses are affected.
Alternative access to the full-text
You may be able to access the full-text directly from the publisher's website using the 'Publisher Copy' link in the 'Links & Downloads' box from a research output's ORA record page. This method may require an institutional or individual subscription to the journal/resource.
Bibliographic Details
- Publisher:
- World Scientific Publishing Co. Pte. Ltd. Publisher's website
- Pages:
- 133–136
- Publication date:
- 2004-10-05
- DOI:
- URN:
-
uuid:a744b7e4-0e82-44f1-964d-7959094595f8
- Source identifiers:
-
10666
- Local pid:
- pubs:10666
- ISBN:
- 981-256-049-1
Item Description
- Keywords:
Terms of use
- Copyright holder:
- World Scientific Publishing Co. Pte. Ltd.
- Copyright date:
- 2004
- Notes:
-
adsurl: http://adsabs.harvard.edu/abs/2004mas..conf..133J
adsnote: Provided by the SAO/NASA Astrophysics Data System
Electronic version of an article published as Multiwavelength AGN Surveys, 2004, 133–136, http://dx.doi.org/10.1142/9789812702432_0034. Copyright © 2004 by World Scientific Publishing Co. Pte. Ltd. http://www.worldscientific.com/doi/abs/10.1142/9789812702432_0034
If you are the owner of this record, you can report an update to it here: Report update to this record