1. The swift gamma-ray burst mission
- Author
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Gehrels, N, Chincarini, G, Giommi, P, Mason, K, Nousek, J, Wells, A, White, N, Barthelmy, S, Burrows, D, Cominsky, L, Hurley, K, Marshall, F, Meszaros, P, Roming, P, Angelini, L, Barbier, L, Belloni, T, Boyd, P, Campana, S, Caraveo, P, Chester, M, Citterio, O, Cline, T, Cropper, M, Cummings, J, Dean, A, Feigelson, E, Fenimore, E, Frail, D, Fruchter, A, Garmire, G, Gendreau, K, Ghisellini, G, Greiner, J, Hill, J, Hunsberger, S, Krimm, H, Kulkarni, S, Kumar, P, Lebrun, F, Lloyd Ronning, N, Markwardt, C, Mattson, B, Mushotzky, R, Norris, J, Paczynski, B, Palmer, D, Park, H, Parsons, A, Paul, J, Rees, M, Reynolds, C, Rhoads, J, Sasseen, T, Schaefer, B, Short, A, Smale, A, Smith, I, Stella, L, Still, M, Tagliaferri, G, Takahashi, T, Tashiro, M, Townsley, L, Tueller, J, Turner, M, Vietri, M, Voges, W, Ward, M, Willingale, R, Zerbi, F, Zhang, W, Mason, KO, Nousek, JA, Wells, AA, White, NE, Barthelmy, SD, Burrows, DN, Cominsky, LR, Hurley, KC, Marshall, FE, Roming, PWA, Barbier, LM, Boyd, PT, Caraveo, PA, Chester, MM, Cline, TL, Cropper, MS, Cummings, JR, Dean, AJ, Feigelson, ED, Fenimore, EE, Frail, DA, Fruchter, AS, Garmire, GP, Hill, JE, Hunsberger, SD, Krimm, HA, Kulkarni, SR, Lloyd Ronning, NM, Markwardt, CB, Mattson, BJ, Mushotzky, RF, Norris, JP, Palmer, DM, Park, HS, Parsons, AM, Rees, MJ, Reynolds, CS, Rhoads, JE, Sasseen, TP, Schaefer, BE, Short, AT, Smale, AP, Smith, IA, Townsley, LK, Turner, MJL, Ward, MJ, Zerbi, FM, Zhang, WW, CHINCARINI, GUIDO, Gehrels, N, Chincarini, G, Giommi, P, Mason, K, Nousek, J, Wells, A, White, N, Barthelmy, S, Burrows, D, Cominsky, L, Hurley, K, Marshall, F, Meszaros, P, Roming, P, Angelini, L, Barbier, L, Belloni, T, Boyd, P, Campana, S, Caraveo, P, Chester, M, Citterio, O, Cline, T, Cropper, M, Cummings, J, Dean, A, Feigelson, E, Fenimore, E, Frail, D, Fruchter, A, Garmire, G, Gendreau, K, Ghisellini, G, Greiner, J, Hill, J, Hunsberger, S, Krimm, H, Kulkarni, S, Kumar, P, Lebrun, F, Lloyd Ronning, N, Markwardt, C, Mattson, B, Mushotzky, R, Norris, J, Paczynski, B, Palmer, D, Park, H, Parsons, A, Paul, J, Rees, M, Reynolds, C, Rhoads, J, Sasseen, T, Schaefer, B, Short, A, Smale, A, Smith, I, Stella, L, Still, M, Tagliaferri, G, Takahashi, T, Tashiro, M, Townsley, L, Tueller, J, Turner, M, Vietri, M, Voges, W, Ward, M, Willingale, R, Zerbi, F, Zhang, W, Mason, KO, Nousek, JA, Wells, AA, White, NE, Barthelmy, SD, Burrows, DN, Cominsky, LR, Hurley, KC, Marshall, FE, Roming, PWA, Barbier, LM, Boyd, PT, Caraveo, PA, Chester, MM, Cline, TL, Cropper, MS, Cummings, JR, Dean, AJ, Feigelson, ED, Fenimore, EE, Frail, DA, Fruchter, AS, Garmire, GP, Hill, JE, Hunsberger, SD, Krimm, HA, Kulkarni, SR, Lloyd Ronning, NM, Markwardt, CB, Mattson, BJ, Mushotzky, RF, Norris, JP, Palmer, DM, Park, HS, Parsons, AM, Rees, MJ, Reynolds, CS, Rhoads, JE, Sasseen, TP, Schaefer, BE, Short, AT, Smale, AP, Smith, IA, Townsley, LK, Turner, MJL, Ward, MJ, Zerbi, FM, Zhang, WW, and CHINCARINI, GUIDO
- Abstract
The Swift mission, scheduled for launch in 2004, is a multiwavelength observatory for gamma-ray burst (GRB) astronomy. It is a first-of-its-kind autonomous rapid-slewing satellite for transient astronomy and pioneers the way for future rapid-reaction and multiwavelength missions. It will be far more powerful than any previous GRB mission, observing more than 100 bursts yr 1 and performing detailed X-ray and UV/optical afterglow observations spanning timescales from 1 minute to several days after the burst. The objectives are to (1) determine the origin of GRBs, (2) classify GRBs and search for new types, (3) study the interaction of the ultrarelativistic outflows of GRBs with their surrounding medium, and (4) use GRBs to study the early universe out to z>10. The mission is being developed by a NASA-led international collaboration. It will carry three instruments: a newgeneration wide-field gamma-ray (15–150 keV) detector that will detect bursts, calculate 10–40 positions, and trigger autonomous spacecraft slews; a narrow-field X-ray telescope that will give 500 positions and perform spectroscopy in the 0.2–10 keV band; and a narrow-field UV/optical telescope that will operate in the 170– 600 nm band and provide 0B3 positions and optical finding charts. Redshift determinations will be made for most bursts. In addition to the primary GRB science, the mission will perform a hard X-ray survey to a sensitivity of 1 mcrab ( 2 ; 10 11 ergs cm 2 s 1 in the 15–150 keV band), more than an order of magnitude better than HEAO 1 A-4. A flexible data and operations system will allow rapid follow-up observations of all types of high-energy transients, with rapid data downlink and uplink available through the NASA TDRSS system. Swift transient data will be rapidly distributed to the astronomical community, and all interested observers are encouraged to participate in follow-up measurements. A Guest Investigator program for the mission will provide funding for community involvement.
- Published
- 2004