|
Narayanan, D. |
Volume |
Paper Title |
Page Number |
Authors |
290 |
Quasar Intrinsic Absorption Lines: Probing High Redshift Galaxy Evolution |
593 |
Hamann, F.; Sabra, B.; Narayanan, D.; Barlow, T.; Chaffee, F.; Junkkarinen, V. |
381 |
Simulated Molecular Gas Emission in Galaxy Mergers with Embedded AGN |
491 |
Narayanan, D.; Cox, T.J.; Robertson, B.; Davé, R.; Di Matteo, T.; Hernquist, L.; Hopkins, P.; Kulesa, C.; Walker, C.K. |
440 |
Do Sub-Millimeter Galaxy Number Counts Provide Evidence for a Top-Heavy IMF? |
369 |
Hayward, C. C.; Narayanan, D.; Jonsson, P.; Cox, T. J.; Kereš, D.; Hopkins, P. F.; Hernquist, L. |
476 |
Reformation of Cold Molecular Disks in Merger Remnants |
61 |
Ueda, J.; Iono, D.; Yun, M.; Wilner, D.; Narayanan, D.; Hatsukade, B.; Tamura, Y.; Kaneko, H.; Crocker, A.; Espada, D.; Kawabe, R. |
477 |
Charting the Evolution of Merger Remnants Through Molecular Gas Observations |
297 |
Iono, D.; Ueda, J.; Yun, M. S.; Crocker, A.; Espada, D.; Hatsukade, B.; Kaneko, H.; Kawabe, R.; Narayanan, D.; Tamura, Y. |
517 |
Cold Gas in High-z Galaxies: The Molecular Gas Budget |
565 |
Decarli, R.; Carilli, C.; Casey, C.; Emonts, B.; Hodge, J.; Kohno, K.; Narayanan, D.; Riechers, D.; Sargent, M.; Walter, F. |
517 |
Cold Gas in High-z Galaxies: The Dense ISM |
575 |
Decarli, R.; Carilli, C.; Casey, C.; Emonts, B.; Hodge, J.; Kohno, K.; Narayanan, D.; Riechers, D.; Sargent, M.; Walter, F. |
517 |
Imaging Cold Gas to 1 kpc Scales in High-Redshift Galaxies with the ngVLA |
629 |
Casey, C. M.; Narayanan, D.; Carilli, C.; Champagne, J.; Hung, C.; Davé, R.; Decarli, R.; Murphy, E. J.; Popping, G.; Riechers, D.; Somerville, R. S.; Walter, F. |
517 |
The Molecular High-z Universe on Large Scales: Low-Surface-Brightness CO and the Strength of the ngVLA Core |
587 |
Emonts, B.; Carilli, C.; Narayanan, D.; Lehnert, M.; Nyland, K. |
517 |
Cold Gas in High-z Galaxies: CO as Redshift Beacon |
581 |
Decarli, R.; Carilli, C.; Casey, C.; Emonts, B.; Hodge, J.; Kohno, K.; Narayanan, D.; Riechers, D.; Sargent, M.; Walter, F. |
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