Skip to main content Accessibility help
×
Home
Hostname: page-component-544b6db54f-8tjh8 Total loading time: 0.264 Render date: 2021-10-23T02:56:21.503Z Has data issue: true Feature Flags: { "shouldUseShareProductTool": true, "shouldUseHypothesis": true, "isUnsiloEnabled": true, "metricsAbstractViews": false, "figures": true, "newCiteModal": false, "newCitedByModal": true, "newEcommerce": true, "newUsageEvents": true }

The Large-scale Structure in the Chandra Deep Field South

Published online by Cambridge University Press:  05 December 2011

Dario Trevese
Affiliation:
Sapienza Università di Roma, P.le Aldo Moro 5, 001865 Roma, Italy email: dario.trevese@roma1.infn.it
Fabrizio Fiore
Affiliation:
INAF-Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monteporzio (RM), Italy
Enrico Piconcelli
Affiliation:
INAF-Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monteporzio (RM), Italy
Marco Castellano
Affiliation:
INAF-Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monteporzio (RM), Italy
Laura Pentericci
Affiliation:
INAF-Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monteporzio (RM), Italy
Piero Ranalli
Affiliation:
Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, 40127 Bologna, Italy INAF-Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy
Andrea Comastri
Affiliation:
INAF-Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy
Rights & Permissions[Opens in a new window]

Abstract

HTML view is not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have studied the large scale distribution of matter in the Chandra Deep Field South on the basis of photometric redshifts and we have identified several over-densities between redshift 0.6 and 2.3. We analyse two of these structures using the deepest X-ray observations ever obtained: 4 Ms with the Chandra satellite and 2.5 Ms with XMM-Newton. We set a very faint upper limit on the X-ray luminosity of a structure at redshift 1.6, and we find an extended X-ray emission from a structure at redshift 0.96 of which we can estimate the gas temperature and make a comparison with the scaling relations between the X-ray luminosity and mass or temperature of high redshift galaxy clusters.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Catellano, M., Salimbeni, S., Trevese, D., Grazian, A., et al. 2007, ApJ, 671, 1497CrossRefGoogle Scholar
Comastri, A., Ranalli, P., Iwasawa, K. et al. 2011, A&A, 526, L9, in press [arXiv:1012.4011]Google Scholar
Ettori, S., Tozzi, P., Borgani, S., & Rosati, P. 2004, A&A, 417, 13Google Scholar
Gladders, M. D. & Yee, H. K. C. 2005, ApJS, 157, 1CrossRefGoogle Scholar
Grazian, A., Fontana, A., deAAAASantis, C., Nonino, M., et al. 2006, A&A, 449, 951Google Scholar
Hicks, A. K., Ellingson, E., Bautz, M., Cain, B., et al. 2008, AJ, 680, 1022CrossRefGoogle Scholar
Kurk, J., Cimatti, A., Zamorani, G., Halliday, C., et al. 2009, A&A, 504, 331Google Scholar
Salimbeni, S., Castellano, M., Pentericci, L., Trevese, D. et al. 2009, A&A, 501, 865Google Scholar
Popesso, P, Biviano, A., Bhringer, H., Romaniello, M., & Voges, W. 2005, A&A, 433, 431Google Scholar
Trevese, D., Castellano, M., Fontana, A., & Giallongo, E. 2007, A&A, 463, 853Google Scholar
Szokoly, G. P., Bergeron, J., Hasinger, G., Lehmann, I., et al. 2004, ApJS, 155, 271CrossRefGoogle Scholar
You have Access

Send article to Kindle

To send this article to your Kindle, first ensure no-reply@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about sending to your Kindle. Find out more about sending to your Kindle.

Note you can select to send to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be sent to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

The Large-scale Structure in the Chandra Deep Field South
Available formats
×

Send article to Dropbox

To send this article to your Dropbox account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Dropbox.

The Large-scale Structure in the Chandra Deep Field South
Available formats
×

Send article to Google Drive

To send this article to your Google Drive account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Google Drive.

The Large-scale Structure in the Chandra Deep Field South
Available formats
×
×

Reply to: Submit a response

Please enter your response.

Your details

Please enter a valid email address.

Conflicting interests

Do you have any conflicting interests? *