Skip to main content Accessibility help
×
Home
Hostname: page-component-78dcdb465f-hcvhd Total loading time: 0.242 Render date: 2021-04-16T01:38:25.336Z Has data issue: true Feature Flags: { "shouldUseShareProductTool": true, "shouldUseHypothesis": true, "isUnsiloEnabled": true, "metricsAbstractViews": false, "figures": false, "newCiteModal": false, "newCitedByModal": true }

FLASHLIGHT: Fluorescent Lyman-Alpha Survey of cosmic Hydrogen iLlumInated by hIGH-redshifT quasars.

Published online by Cambridge University Press:  25 July 2014

Fabrizio Arrigoni Battaia
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany email: arrigoni@mpia.de
J. F. Hennawi
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany email: arrigoni@mpia.de
S. Cantalupo
Affiliation:
Department of Astronomy and Astrophysics, University of California, 1156 High Street, Santa Cruz, CA, 95064, USA University of California Observatories, Lick Observatory, 1156 High Street, Santa Cruz, CA, 95064, USA
J. X. Prochaska
Affiliation:
Department of Astronomy and Astrophysics, University of California, 1156 High Street, Santa Cruz, CA, 95064, USA University of California Observatories, Lick Observatory, 1156 High Street, Santa Cruz, CA, 95064, USA
Corresponding
E-mail address:
Rights & Permissions[Opens in a new window]

Abstract

The current galaxy formation paradigm postulates that a significant amount of gas accretes onto galaxies from the IGM in a cold T ~ 104K phase, and many have argued that this gas should be detectable in diffuse Lyα emission. However, so far, there are no convincing direct detections.

We are conducting a deep (down to 1σ ~ 5 − 10 × 10−19 erg s−1 cm−2 arcsec−2) and the first statistical survey matching the Lyα line around radio-quiet quasars at z ~ 2. By taking advantage of the boost in fluorescent Lyα emission due to the ionizing radiation emitted by a luminous QSO that, like a flashlight, can illuminate the hydrogen in its vicinity, we will be able to constrain some of the properties of the gas sorrounding z ~ 2 QSOs. In particular, with this unique dataset, we can conduct the first deep statistical census of the size, morphology, luminosity, frequency, and covering factor of Lyα emission around QSOs.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

Adelberger, K. L., Steidel, C. C., Kollmeier, J. A., & Reddy, N. A. 2006, ApJ, 637, 74CrossRefGoogle Scholar
Bergeron, J., Petitjean, P., Cristiani, S., et al. 1999, A&A, 343, L40Google Scholar
Binette, L., Wang, J. C. L., Zuo, L., & Magris, C. G. 1993, AJ, 105, 797CrossRefGoogle Scholar
Cantalupo, S., Porciani, C., Lilly, S. J., & Miniati, F. 2005, ApJ, 628, 61CrossRefGoogle Scholar
Cantalupo, S., Lilly, S. J., & Haehnelt, M. G. 2012, MNRAS, 425, 1992CrossRefGoogle Scholar
Cattaneo, A., Blaizot, J., Weinberg, D. H., et al. 2007, MNRAS, 377, 63CrossRefGoogle Scholar
Charlot, S. & Fall, S. M. 1993, ApJ, 415, 580CrossRefGoogle Scholar
Christensen, L., Jahnke, K., Wisotzki, L., & Sanchez, S. F. 2006, A&A, 459, 717Google Scholar
Erb, D. K. 2008, ApJ, 674, 151CrossRefGoogle Scholar
Fardal, M. A., Katz, N., Gardner, J. P., et al. 2001, ApJ, 562, 605CrossRefGoogle Scholar
Frank, S., Rasera, Y., Vibert, D., et al. 2012, MNRAS, 420, 1731CrossRefGoogle Scholar
Fynbo, J. U., Møller, P., & Warren, S. J. 1999, MNRAS, 305, 849CrossRefGoogle Scholar
Gould, A. & Weinberg, D. H. 1996, ApJ, 468, 462CrossRefGoogle Scholar
Haiman, Z., Spaans, M., & Quataert, E. 2000, ApJ (Letters), 537, L5CrossRefGoogle Scholar
Hennawi, J. F. & Prochaska, J. X. 2013, ApJ, 766, 58CrossRefGoogle Scholar
Hogan, C. J. & Weymann, R. J. 1987, MNRAS, 225, 1PCrossRefGoogle Scholar
Kereš, D., Katz, N., Weinberg, D. H., & Davé, R. 2005, MNRAS, 363, 2CrossRefGoogle Scholar
Lowenthal, J. D., Hogan, C. J., Leach, R. W., Schmidt, G. D., & Foltz, C. B. 1990, ApJ, 357, 3CrossRefGoogle Scholar
Ocvirk, P., Pichon, C., & Teyssier, R. 2008, MNRAS, 390, 1326Google Scholar
Prochaska, J. X., Hennawi, J. F., & Simcoe, R. A. 2013a, ApJ (Letters), 762, L19CrossRefGoogle Scholar
Prochaska, J. X., Hennawi, J. F., Lee, K.-G., et al. 2013b, ApJ, 776, 136CrossRefGoogle Scholar
Rauch, M., Haehnelt, M., Bunker, A., et al. 2008, ApJ, 681, 856CrossRefGoogle Scholar
Solomon, P. M. & Vanden Bout, P. A. 2005, ARAA, 43, 677CrossRefGoogle Scholar
White, S. D. M. & Rees, M. J. 1978, MNRAS, 183, 341CrossRefGoogle Scholar

Full text views

Full text views reflects PDF downloads, PDFs sent to Google Drive, Dropbox and Kindle and HTML full text views.

Total number of HTML views: 0
Total number of PDF views: 99 *
View data table for this chart

* Views captured on Cambridge Core between September 2016 - 16th April 2021. This data will be updated every 24 hours.

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.

FLASHLIGHT: Fluorescent Lyman-Alpha Survey of cosmic Hydrogen iLlumInated by hIGH-redshifT quasars.
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.

FLASHLIGHT: Fluorescent Lyman-Alpha Survey of cosmic Hydrogen iLlumInated by hIGH-redshifT quasars.
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.

FLASHLIGHT: Fluorescent Lyman-Alpha Survey of cosmic Hydrogen iLlumInated by hIGH-redshifT quasars.
Available formats
×
×

Reply to: Submit a response


Your details


Conflicting interests

Do you have any conflicting interests? *