Limits on quark-lepton compositeness scales from dileptons produced in 1.8 TeV pp-collisions

Physical Review Letters 79:12 (1997) 2198-2203

Authors:

F Abe, H Akimoto, A Akopian, MG Albrow, SR Amendolia, D Amidei, J Antos, S Aota, G Apollinari, T Asakawa, W Ashmanskas, M Atac, F Azfar, P Azzi-Bacchetta, N Bacchetta, W Badgett, S Bagdasarov, MW Bailey, J Bao, P de Barbaro, A Barbaro-Galtieri, VE Barnes, BA Barnett, M Barone, E Barzi, G Bauer, T Baumann, F Bedeschi, S Behrends, S Belforte, G Bellettini, J Bellinger, D Benjamin, J Benlloch, J Bensinger, D Benton, A Beretvas, JP Berge, J Berryhill, S Bertolucci, B Bevensee, A Bhatti, K Biery, M Binkley, D Bisello, RE Blair, C Blocker, A Bodek, W Bokhari, V Bolognesi, G Bolla, D Bortoletto, J Boudreau, L Breccia, C Bromberg, N Bruner, E Buckley-Geer, HS Budd, K Burkett, G Busetto, A Byon-Wagner, KL Byrum, J Cammerata, C Campagnari, M Campbell, A Caner, W Carithers, D Carlsmith, A Castro, D Cauz, Y Cen, F Cervelli, PS Chang, PT Chang, HY Chao, J Chapman, MT Cheng, G Chiarelli, T Chikamatsu, CN Chiou, L Christofek, S Cihangir, AG Clark, M Cobal, E Cocca, M Contreras, J Conway, J Cooper, M Cordelli, C Couyoumtzelis, D Crane, D Cronin-Hennessy, R Culbertson, T Daniels, F DeJongh, S Delchamps, S Dell’agnello, M Dell’orso, R Demina, L Demortier

Abstract:

The dilepton mass spectrum in pp-→|+|-+X interactions is studied using dielectrons (ee) and dimuons (μμ) in 100 pb- of data collected with the Collider Detector at Fermilab. The data are consistent with standard model predictions. The mass spectrum, being a probe for new physics, is examined for new interactions of quarks and leptons from a common composite structure. Assuming a contact interaction with the conventional coupling g20/4π = 1, limits on chiral quark-electron and quark-muon compositeness scales in the range of 2.5 to 4.2 TeV are obtained. © 1997 The American Physical Society.

Multiwavelength observations of GX 339−4

AIP Publishing (1997) 932-936

Authors:

IA Smith, EP Liang, M Moss, J Dobrinskaya, RP Fender, Ph Durouchoux, S Corbel, R Sood, AV Filippenko, DC Leonard

New radio observations of Circinus X-1

AIP Conference Proceedings AIP Publishing 410:1 (1997) 798-802

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.

Radio observations of the black hole candidate GX 339−4

AIP Conference Proceedings AIP Publishing 410:1 (1997) 937-941

Authors:

S Corbel, RP Fender, P Durouchoux, RK Sood, AK Tzioumis, RE Spencer, D Campbell-Wilson