Testing the 10 spectrograph units for DESI: approach and results

Autor: Perruchot, S., Blanc, P. -E., Guy, J., Guillou, L. Le, Ronayette, S., Régal, X., Castagnoli, G., Van Suu, A. Le, Sepulveda, E., Jullo, E., Cuby, J. -G., Karkar, S., Ghislain, P., Repain, P., Carton, P. -H., Magneville, C., Ealet, A., Escoffier, S., Secroun, A., Honscheid, K., Elliot, A., Jelinsky, P., Brooks, D., Doel, P., Duan, Y., Edelstein, J., Estrada, J. C., Gastañaga, E., Karcher, A., Landriau, M., Levi, M., Martini, P., Palanque-Delabrouille, N., Prada, F., Tarle, G., Zhang, K.

Publikováno v: Proc. SPIE 11447, Ground-based and Airborne Instrumentation for Astronomy VIII, 1144786 (13 December 2020)

The recently commissioned Dark Energy Spectroscopic Instrument (DESI) will measure the expansion history of the Universe using the Baryon Acoustic Oscillation technique. The spectra of 35 million galaxies and quasars over 14000 sqdeg will be measured

Externí odkaz: http://arxiv.org/abs/2101.12181

The Mid-Infrared Instrument for the James Webb Space Telescope, III: MIRIM, The MIRI Imager

Autor: Bouchet, P., Garcia-Marin, M., Lagage, P. -O., Amiaux, J., Augueres, J. -L., Bauwens, E., Blommaert, J. A. D. L., Chen, C. H., Detre, O. H., Dicken, D., Dubreuil, D., Galdemard, Ph., Gastaud, R., Glasse, A., Gordon, K. D., Gougnaud, F., Guillard, P., Justtanont, K., Krause, O., Leboeuf, D., Longval, Y., Martin, L., Mazy, E., Moreau, V., Olofsson, G., Ray, T. P., Reess, J. -M., Renotte, E., Ressler, M. E., Ronayette, S., Salasca, S., Scheithauer, S., Sykes, J., Thelen, M. P., Wells, M., Wright, D., Wright, G. S.

Publikováno v: 2015 Publications of the Astronomical Society of the Pacific, Volume 127, issue 953, pp.612-622

In this article, we describe the MIRI Imager module (MIRIM), which provides broad-band imaging in the 5 - 27 microns wavelength range for the James Webb Space Telescope. The imager has a 0"11 pixel scale and a total unobstructed view of 74"x113". The

Externí odkaz: http://arxiv.org/abs/1508.02488

Euclid Definition Study Report

Autor: Laureijs, R., Amiaux, J., Arduini, S., Auguères, J. -L., Brinchmann, J., Cole, R., Cropper, M., Dabin, C., Duvet, L., Ealet, A., Garilli, B., Gondoin, P., Guzzo, L., Hoar, J., Hoekstra, H., Holmes, R., Kitching, T., Maciaszek, T., Mellier, Y., Pasian, F., Percival, W., Rhodes, J., Criado, G. Saavedra, Sauvage, M., Scaramella, R., Valenziano, L., Warren, S., Bender, R., Castander, F., Cimatti, A., Fèvre, O. Le, Kurki-Suonio, H., Levi, M., Lilje, P., Meylan, G., Nichol, R., Pedersen, K., Popa, V., Lopez, R. Rebolo, Rix, H. -W., Rottgering, H., Zeilinger, W., Grupp, F., Hudelot, P., Massey, R., Meneghetti, M., Miller, L., Paltani, S., Paulin-Henriksson, S., Pires, S., Saxton, C., Schrabback, T., Seidel, G., Walsh, J., Aghanim, N., Amendola, L., Bartlett, J., Baccigalupi, C., Beaulieu, J. -P., Benabed, K., Cuby, J. -G., Elbaz, D., Fosalba, P., Gavazzi, G., Helmi, A., Hook, I., Irwin, M., Kneib, J. -P., Kunz, M., Mannucci, F., Moscardini, L., Tao, C., Teyssier, R., Weller, J., Zamorani, G., Osorio, M. R. Zapatero, Boulade, O., Foumond, J. J., Di Giorgio, A., Guttridge, P., James, A., Kemp, M., Martignac, J., Spencer, A., Walton, D., Blümchen, T., Bonoli, C., Bortoletto, F., Cerna, C., Corcione, L., Fabron, C., Jahnke, K., Ligori, S., Madrid, F., Martin, L., Morgante, G., Pamplona, T., Prieto, E., Riva, M., Toledo, R., Trifoglio, M., Zerbi, F., Abdalla, F., Douspis, M., Grenet, C., Borgani, S., Bouwens, R., Courbin, F., Delouis, J. -M., Dubath, P., Fontana, A., Frailis, M., Grazian, A., Koppenhöfer, J., Mansutti, O., Melchior, M., Mignoli, M., Mohr, J., Neissner, C., Noddle, K., Poncet, M., Scodeggio, M., Serrano, S., Shane, N., Starck, J. -L., Surace, C., Taylor, A., Verdoes-Kleijn, G., Vuerli, C., Williams, O. R., Zacchei, A., Altieri, B., Sanz, I. Escudero, Kohley, R., Oosterbroek, T., Astier, P., Bacon, D., Bardelli, S., Baugh, C., Bellagamba, F., Benoist, C., Bianchi, D., Biviano, A., Branchini, E., Carbone, C., Cardone, V., Clements, D., Colombi, S., Conselice, C., Cresci, G., Deacon, N., Dunlop, J., Fedeli, C., Fontanot, F., Franzetti, P., Giocoli, C., Garcia-Bellido, J., Gow, J., Heavens, A., Hewett, P., Heymans, C., Holland, A., Huang, Z., Ilbert, O., Joachimi, B., Jennins, E., Kerins, E., Kiessling, A., Kirk, D., Kotak, R., Krause, O., Lahav, O., van Leeuwen, F., Lesgourgues, J., Lombardi, M., Magliocchetti, M., Maguire, K., Majerotto, E., Maoli, R., Marulli, F., Maurogordato, S., McCracken, H., McLure, R., Melchiorri, A., Merson, A., Moresco, M., Nonino, M., Norberg, P., Peacock, J., Pello, R., Penny, M., Pettorino, V., Di Porto, C., Pozzetti, L., Quercellini, C., Radovich, M., Rassat, A., Roche, N., Ronayette, S., Rossetti, E., Sartoris, B., Schneider, P., Semboloni, E., Serjeant, S., Simpson, F., Skordis, C., Smadja, G., Smartt, S., Spano, P., Spiro, S., Sullivan, M., Tilquin, A., Trotta, R., Verde, L., Wang, Y., Williger, G., Zhao, G., Zoubian, J., Zucca, E.

Euclid is a space-based survey mission from the European Space Agency designed to understand the origin of the Universe's accelerating expansion. It will use cosmological probes to investigate the nature of dark energy, dark matter and gravity by tra

Externí odkaz: http://arxiv.org/abs/1110.3193

In-flight calibration of the Herschel-SPIRE instrument

Autor: Swinyard, B. M., Ade, P., Baluteau, J-P., Aussel, H., Barlow, M. J., Bendo, G. J., Benielli, D., Bock, J., Brisbin, D., Conley, A., Conversi, L., Dowell, A., Dowell, D., Ferlet, M., Fulton, T., Glenn, J., Glauser, A., Griffin, D., Griffin, M., Guest, S., Imhof, P., Isaak, K., Jones, S., King, K., Leeks, S., Levenson, L., Lim, T. L., Lu, N., Makiwa, G., Naylor, D., Nguyen, H., Oliver, S., Panuzzo, P., Papageorgiou, A., Pearson, C., Pohlen, M., Polehampton, E., Pouliquen, D., Rigopoulou, D., Ronayette, S., Roussel, H., Rykala, A., Savini, G., Schulz, B., Schwartz, A., Shupe, D., Sibthorpe, B., Sidher, S., Smith, A. J., Spencer, L., Trichas, M., Triou, H., Valtchanov, I., Wesson, R., Woodcraft, A., Xu, C. K., Zemcov, M., Zhang, L.

SPIRE, the Spectral and Photometric Imaging Receiver, is the Herschel Space Observatory's submillimetre camera and spectrometer. It contains a three-band imaging photometer operating at 250, 350 and 500 {\mu}m, and an imaging Fourier transform spectr

Externí odkaz: http://arxiv.org/abs/1005.5073

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