Start Presentation: The column density distribution of galaxies at z=0.5-3 from GRBs and implications for obscured AGN

(back to all presentations)

Table of contents

Author: Johannes Buchner

Homepage: http://astrost.at/istics/

Further information:

The column density distribution of galaxies at z=0.5-3 from GRBs and implications for obscured AGN

Download presentation

Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: Conclusions GRBs have obscuration 1020-1023 cm-2 GRBs live in Compton-thin environments, consistent with GMC-like clouds GRBs in high-M hosts have more obscuration No evolution around cosmic SF peak AGN obscuration: