The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope

Autor: Birkmann, SM, Ferruit, P, Giardino, G, Nielsen, LD, García Munoz, A, Kendrew, S, Rauscher, BJ, Beck, TL, Keyes, C, Valenti, JA, Jakobsen, P, Dorner, B, Alves De Oliveira, C, Arribas, S, Boker, T, Bunker, AJ, Charlot, S, De Marchi, G, Kumari, N, López-Caniego, M, Lutzgendorf, N, Maiolino, R, Manjavacas, E, Marston, A, Moseley, SH, Prizkal, N, Proffitt, C, Rawle, T, Rix, HW, Te Plate, M, Sabbi, E, Sirianni, M, Willott, CJ, Zeidler, P

Publikováno v: Birkmann, S M, Ferruit, P, Giardino, G, Nielsen, L D, García Muñoz, A, Kendrew, S, Rauscher, B J, Beck, T L, Keyes, C, Valenti, J A, Jakobsen, P, Dorner, B, Alves De Oliveira, C, Arribas, S, Böker, T, Bunker, A J, Charlot, S, De Marchi, G, Kumari, N, López-caniego, M, Lützgendorf, N, Maiolino, R, Manjavacas, E, Marston, A, Moseley, S H, Prizkal, N, Proffitt, C, Rawle, T, Rix, H, Te Plate, M, Sabbi, E, Sirianni, M, Willott, C J & Zeidler, P 2022, ' The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope IV. Capabilities and predicted performance for exoplanet characterization ', Astronomy & Astrophysics, vol. 661, A83 . https://doi.org/10.1051/0004-6361/202142592
Astronomy & Astrophysics

The Near-Inrared Spectrograph (NIRSpec) on the James Webb Space Telescope (JWST) is a very versatile instrument, offering multiobject and integral field spectroscopy with varying spectral resolution ($\sim$30 to $\sim$3000) over a wide wavelength ran

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f47a29d7d23c5924af44eec13dba4db2
https://doi.org/10.1051/0004-6361/202142592

Obscured AGN from the ELAIS Deep X-ray Survey

Autor: Willott, CJ, Simpson, C, Almaini, O, Manners, JC, Johnson, O, Lawrence, A, Dunlop, JS, Ivison, RJ, Rawlings, S, Gonzalez-Solares, E, Perez-Fournon, I, Serjeant, S, Oliver, SJ, Roche, ND, Mann, RG, Rowan-Robinson, M

The sources discovered in deep hard X-ray surveys with 2-8 keV fluxes of 10^-14 erg cm^-2 s^-1 make up the bulk of the X-ray background at these energies. We present here detailed multi-wavelength observations of three such sources from the ELAIS Dee

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9bb55f0162bbfe1e1db5ecd7fc372702
https://doi.org/10.1046/j.1365-8711.2003.06192.x

STAR FORMATION AND DUST OBSCURATION AT z approximate to 2: GALAXIES AT THE DAWN OF DOWNSIZING

Autor: Pannella, M, Carilli, Cl, Daddi, E, Mccracken, Hj, Owen, Fn, Renzini, A, Strazzullo, V, Civano, F, Koekemoer, Am, Schinnerer, E, Scoville, N, Smolcic, V, Taniguchi, Y, Aussel, H, Kneib, Jp, Ilbert, O, Mellier, Y, Salvato, M, Thompson, D, Willott, Cj

We present first results of a study aimed to constrain the star formation rate (SFR) and dust content of galaxies at z approximate to 2. We use a sample of BzK-selected star-forming galaxies, drawn from the Cosmic Evolution Survey, to perform a stack

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::0f9ecbdc82e6407541f5722286ba29f5
https://hdl.handle.net/11368/2956942

The European Large Area ISO Survey - I. Goals, definition and observations RID A-1248-2009

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

We describe the European Large Area ISO Survey (ELAIS). ELAIS was the largest single Open Time project conducted by ISO, mapping an area of 12 deg(2) at 15 mu m with ISOCAM and at 90 mu m with ISOPHOT. Secondary surveys in other ISO bands were undert

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______3668::c1add994162b0035acac76e0aad8710e
https://hdl.handle.net/11590/114417

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