24 results on '"Chatterjee, Suchetana"'
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2. Cosmological Simulation of Galaxy Groups and Clusters. II. Studying Different Modes of Feedback through X-Ray Observations
3. Radio dichotomy in quasars with H β FWHM greater than 15 000 km s−1
4. The Signatures of Self-interacting Dark Matter and Subhalo Disruption on Cluster Substructure
5. Properties of Very Broad Line MgII Radio-Loud and Radio-Quiet Quasars
6. Simulated X‐ray emission in galaxy clusters with feedback from active galactic nuclei
7. The Chandra Deep Wide-field Survey: A New Chandra Legacy Survey in the Boötes Field. I. X-Ray Point Source Catalog, Number Counts, and Multiwavelength Counterparts
8. Cosmological Simulation of Galaxy Groups and Clusters. I. Global Effect of Feedback from Active Galactic Nuclei
9. X-Ray Surface Brightness Profiles of Optically Selected Active Galactic Nuclei: Comparison with X-Ray AGNs
10. Gender status in the Indian physics profession and the way forward
11. Cosmological evolution of supermassive black holes
12. Direct detection of quasar feedback via the Sunyaev–Zeldovich effect
13. Mean Occupation Function of High-redshift Quasars from the Planck Cluster Catalog
14. The Halo Occupation Distribution of obscured quasars: revisiting the unification model
15. Sunyaev–Zel’Dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
16. X-ray Surface Brightness Profiles of Active Galactic Nuclei in the Extended Groth Strip: Implications for AGN Feedback
17. X-RAY EMISSION IN NON-AGN GALAXIES ATz≃ 1
18. A DIRECT MEASUREMENT OF THE MEAN OCCUPATION FUNCTION OF QUASARS: BREAKING DEGENERACIES BETWEEN HALO OCCUPATION DISTRIBUTION MODELS
19. THE HALO OCCUPATION DISTRIBUTION OF X-RAY-BRIGHT ACTIVE GALACTIC NUCLEI: A COMPARISON WITH LUMINOUS QUASARS
20. THE HALO OCCUPATION DISTRIBUTION OF SDSS QUASARS
21. The halo occupation distribution of active galactic nuclei
22. The halo occupation distribution of black holes
23. TENTATIVE DETECTION OF QUASAR FEEDBACK FROM WMAP AND SDSS CROSS-CORRELATION
24. The Sunyaev-Zel'dovich Effect from Quasar Feedback
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