Aprajita Verma: Publications

The European Large Area ISO Survey - VI. Discovery of a new hyperluminous infrared galaxy

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 327:4 (2001) 1187-1192

Authors:

T Morel, A Efstathiou, S Serjeant, I Márquez, J Masegosa, P Héraudeau, C Surace, A Verma, S Oliver, M Rowan-Robinson, I Georgantopoulos, D Farrah, DM Alexander, I Pérez-Fournon, CJ Willott, F Cabrera-Guerra, EA Gonzalez-Solares, A Cabrera-Lavers, JI Gonzalez-Serrano, P Ciliegi, F Pozzi, I Matute, H Flores

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The European Large Area ISO Survey — I. Goals, definition and observations

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 316:4 (2000) 749-767

Authors:

Seb Oliver, Michael Rowan-Robinson, DM Alexander, O Almaini, M Balcells, AC Baker, X Barcons, M Barden, I Bellas-Velidis, F Cabrera-Guerra, R Carballo, CJ Cesarsky, P Ciliegi, DL Clements, H Crockett, L Danese, A Dapergolas, B Drolias, N Eaton, A Efstathiou, E Egami, D Elbaz, D Fadda, M Fox, A Franceschini, R Genzel, P Goldschmidt, M Graham, JI Gonzalez-Serrano, EA Gonzalez-Solares, GL Granato, C Gruppioni, U Herbstmeier, P Héraudeau, M Joshi, E Kontizas, M Kontizas, JK Kotilainen, D Kunze, F La Franca, C Lari, A Lawrence, D Lemke, MJD Linden-Vørnle, RG Mann, I Márquez, J Masegosa, K Mattila, RG McMahon, G Miley, V Missoulis, B Mobasher, T Morel, H Nørgaard-Nielsen, A Omont, P Papadopoulos, I Perez-Fournon, J-L Puget, D Rigopoulou, B Rocca-Volmerange, S Serjeant, L Silva, T Sumner, C Surace, P Vaisanen, PP van der Werf, A Verma, L Vigroux, M Villar-Martin, CJ Willott

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Deep Surveys and Cosmology

Highlights of Astronomy Cambridge University Press (CUP) 11:2 (1998) 1122-1124

Authors:

SJ Oliver, S Sergeant, P Goldschmidt, RG Mann, M Rowan-Robinson, N Eaton, A Efsathiou, C Gruppioni, TJ Sumner, B Mobasher, A Verma, L Danese, E Egami, D Elbaz, A Franceschini, I Gonzalez-Serrano, M Kontizas, A Lawrence, R Mcmahon, HU Nørgaard-Nielsen, I Pérez-Fournon

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Deep Surveys and Cosmology

Chapter in Highlights of Astronomy, Springer Nature (1998) 1122-1124

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Observations of the Hubble Deep Field with the Infrared Space Observatory - III. Source counts and P(D) analysis

Monthly Notices of the Royal Astronomical Society 289:2 (1997) 471-481

Authors:

SJ Oliver, P Goldschmidt, A Franceschini, SBG Serjeant, A Efstathiou, A Verma, C Gruppioni, N Eaton, RG Mann, B Mobasher, CP Pearson, M Rowan-Robinson, TJ Sumner, L Danese, D Elbaz, E Egami, M Kontizas, A Lawrence, R McMahon, HU Norgaard-Nielsen, I Perez-Fournon, JI Gonzalez-Serrano

Abstract:

We present source counts at 6.7 and 15 μm from our maps of the Hubble Deep Field (HDF) region, reaching 38.6 μJy at 6.7 μm and 255 μJy at 15 μm. These are the first ever extragalactic number counts to be presented at 6.7 μm, and are three decades fainter than IRAS at 12 μm. Both source counts and a P(D) analysis suggest that we have reached the Infrared Space Obsen'atory (ISO) confusion limit at 15 μm: this will have important implications for future space missions. These data provide an excellent reference point for other ongoing ISO surveys. A no-evolution model at 15 μm is ruled out at > 3σ, while two models which fit the steep IRAS 60-μm counts are acceptable. This provides important confirmation of the strong evolution seen in IRAS surveys. One of these models can then be ruled out from the 6.7-μm data. © 1997 RAS.

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Aprajita Verma

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The European Large Area ISO Survey - VI. Discovery of a new hyperluminous infrared galaxy

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The European Large Area ISO Survey — I. Goals, definition and observations

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Deep Surveys and Cosmology

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Deep Surveys and Cosmology

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Observations of the Hubble Deep Field with the Infrared Space Observatory - III. Source counts and P(D) analysis

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The European Large Area ISO Survey - VI. Discovery of a new hyperluminous infrared galaxy

Authors:

The European Large Area ISO Survey — I. Goals, definition and observations

Authors:

Deep Surveys and Cosmology

Authors:

Deep Surveys and Cosmology

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Observations of the Hubble Deep Field with the Infrared Space Observatory - III. Source counts and P(D) analysis

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Abstract: