Dr Aprajita Verma: Publications

Far-infrared line deficits in galaxies with extreme LFIR/M H2 ratios

Astrophysical Journal 728:1 PART II (2011)

Authors:

J Graciá-Carpio, E Sturm, S Hailey-Dunsheath, J Fischer, A Contursi, A Poglitsch, R Genzel, E González-Alfonso, A Sternberg, A Verma, N Christopher, R Davies, H Feuchtgruber, JA De Jong, D Lutz, LJ Tacconi

Green Bank Telescope Zpectrometer CO(1-0) observations of the strongly lensed submillimeter galaxies From the Herschel ATLAS

Astrophysical Journal 726:2 PART II (2011)

Authors:

DT Frayer, AI Harris, AJ Baker, RJ Ivison, I Smail, M Negrello, R Maddalena, I Aretxaga, M Baes, M Birkinshaw, DG Bonfield, D Burgarella, S Buttiglione, A Cava, DL Clements, A Cooray, H Dannerbauer, A Dariush, G De Zotti, JS Dunlop, L Dunne, S Dye, S Eales, J Fritz, J Gonzalez-Nuevo, D Herranz, R Hopwood, DH Hughes, E Ibar, MJ Jarvis, G Lagache, LL Leeuw, M Lopez-Caniego, S Maddox, MJ Michałlowski, A Omont, M Pohlen, E Rigby, G Rodighiero, D Scott, S Serjeant, DJB Smith, AM Swinbank, P Temi, MA Thompson, I Valtchanov, PP Van Der Werf, A Verma

STAR FORMATION AND THE ISM IN INFRARED BRIGHT GALAXIES - SHINING

CONDITIONS AND IMPACT OF STAR FORMATION: NEW RESULTS WITH HERSCHEL AND BEYOND 52 (2011) 55-+

Authors:

E Sturm, A Poglitsch, A Contursi, J Gracia-Carpio, J Fischer, E Gonzalez-Alfonso, R Genzel, S Hailey-Dunsheath, D Lutz, L Tacconi, J deJong, A Sternberg, A Verma, S Madden, L Vigroux, D Cormier, U Klaas, M Nielbock, O Krause, J Schreiber, M Haas

Spitzer imaging of Herschel-atlas gravitationally lensed submillimeter sources

Astrophysical Journal 728:1 PART II (2011)

Authors:

R Hopwood, J Wardlow, A Cooray, AA Khostovan, S Kim, M Negrello, E Da Cunha, D Burgarella, I Aretxaga, R Auld, M Baes, E Barton, F Bertoldi, DG Bonfield, R Blundell, S Buttiglione, A Cava, DL Clements, J Cooke, H Dannerbauer, A Dariush, G De Zotti, J Dunlop, L Dunne, S Dye, S Eales, J Fritz, D Frayer, MA Gurwell, DH Hughes, E Ibar, RJ Ivison, MJ Jarvis, G Lagache, L Leeuw, S Maddox, MJ Michałlowski, A Omont, E Pascale, M Pohlen, E Rigby, G Rodighiero, D Scott, S Serjeant, I Smail, DJB Smith, P Temi, MA Thompson, I Valtchanov, P Van Der Werf, A Verma, JD Vieira

Expected performance and simulated observations of the instrument HARMONI at the European Extremely Large Telescope (E-ELT)

Proceedings of SPIE - The International Society for Optical Engineering 7735:PART 1 (2010)

Authors:

S Arribas, NA Thatte, M Tecza, T Goodsall, F Clarke, RL Davies, R Bacon, L Colina, D Lunney, E Mediavilla, A Remillieux, D Rigopoulou, M Swinbank, A Verma

Abstract:

HARMONI has been conceived as a workhorse visible and near-infrared (0.47-2.45 microns) integral field spectrograph for the European Extremely Large Telescope (E-ELT). It provides both seeing and diffraction limited observations at several spectral resolutions (R= 4000, 10000, 20000). HARMONI can operate with almost any flavor of AO (e.g. GLAO, LTAO, SCAO), and it is equipped with four spaxel scales (4, 10, 20 and 40 mas) thanks to which it can be optimally configured for a wide variety of science programs, from ultra-sensitive observations of point sources to highangular resolution spatially resolved studies of extended objects. In this paper we describe the expected performance of the instrument as well as its scientific potential. We show some simulated observations for a selected science program, and compare HARMONI with other ground and space based facilities, like VLT, ALMA, and JWST, commenting on their synergies and complementarities. © 2010 Copyright SPIE - The International Society for Optical Engineering.

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