Search

Your search keyword '"Dombeck, T."' showing total 109 results
Start Over Author "Dombeck, T."
109 results on '"Dombeck, T."'

1. Ultra-bright optical transients are linked with type Ic supernovae

Author

Pastorello, A., Smartt, S. J., Botticella, M. T., Maguire, K., Fraser, M., Smith, K., Kotak, R., Magill, L., Valenti, S., Young, D. R., Gezari, S., Bresolin, F., Kudritzki, R., Howell, D. A., Rest, A., Metcalfe, N., Mattila, S., Kankare, E., Huang, K. Y., Urata, Y., Burgett, W. S., Chambers, K. C., Dombeck, T., Flewelling, T., Grav, T., Heasley, J. N., Hodapp, K. W., Kaiser, N., Luppino, G. A., Lupton, R. H., Magnier, E. A., Monet, D. G., Morgan, J. S., Onaka, P. M., Price, P. A., Rhoads, P. H., Siegmund, W. A., Stubbs, C. W., Sweeney, W. E., Tonry, J. L., Wainscoat, R. J., Waterson, M. F., Waters, C., and Wynn-Williams, C. G.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

Recent searches by unbiased, wide-field surveys have uncovered a group of extremely luminous optical transients. The initial discoveries of SN 2005ap by the Texas Supernova Search and SCP-06F6 in a deep Hubble pencil beam survey were followed by the Palomar Transient Factory confirmation of host redshifts for other similar transients. The transients share the common properties of high optical luminosities (peak magnitudes ~ -21 to -23), blue colors, and a lack of H or He spectral features. The physical mechanism that produces the luminosity is uncertain, with suggestions ranging from jet-driven explosion to pulsational pair-instability. Here we report the most detailed photometric and spectral coverage of an ultra-bright transient (SN 2010gx) detected in the Pan-STARRS 1 sky survey. In common with other transients in this family, early-time spectra show a blue continuum, and prominent broad absorption lines of O II. However, about 25d after discovery, the spectra developed type Ic supernova features, showing the characteristic broad Fe II and Si II absorption lines. Detailed, post-maximum follow-up may show that all SN 2005ap and SCP-06F6 type transients are linked to supernovae Ic. This poses problems in understanding the physics of the explosions: there is no indication from late-time photometry that the luminosity is powered by 56Ni, the broad lightcurves suggest very large ejected masses, and the slow spectral evolution is quite different from typical Ic timescales. The nature of the progenitor stars and the origin of the luminosity are intriguing and open questions., Comment: 16 pages, 4 figures, 1 table. Accepted for publication in the Astrophysical Journal Letters on September 9

Published
2010
Full Text
View/download PDF

2. GALEX and Pan-STARRS1 Discovery of SN IIP 2010aq: The First Few Days After Shock Breakout in a Red Supergiant Star

Author

Gezari, S., Rest, A., Huber, M. E., Narayan, G., Forster, K., Neill, J. D., Martin, D. C., Valenti, S., Smartt, S. J., Chornock, R., Berger, E., Soderberg, A. M., Mattila, S., Kankare, E., Burgett, W. S., Chambers, K. C., Dombeck, T., Grav, T., Heasley, J. N., Hodapp, K. W., Jedicke, R., Kaiser, N., Kudritzki, R., Luppino, G., Lupton, R. H., Magnier, E. A., Monet, D. G., Morgan, J. S., Onaka, P. M., Price, P. A., Rhoads, P. H., Siegmund, W. A., Stubbs, C. W., Tonry, J. L., Wainscoat, R. J., Waterson, M. F., and Wynn-Williams, C. G.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present the early UV and optical light curve of Type IIP supernova (SN) 2010aq at z=0.0862, and compare it to analytical models for thermal emission following SN shock breakout in a red supergiant star. SN 2010aq was discovered in joint monitoring between the Galaxy Evolution Explorer (GALEX) Time Domain Survey (TDS) in the NUV and the Pan-STARRS1 Medium Deep Survey (PS1 MDS) in the g, r, i, and z bands. The GALEX and Pan-STARRS1 observations detect the SN less than 1 day after shock breakout, measure a diluted blackbody temperature of 31,000 +/- 6,000 K 1 day later, and follow the rise in the UV/optical light curve over the next 2 days caused by the expansion and cooling of the SN ejecta. The high signal-to-noise ratio of the simultaneous UV and optical photometry allows us to fit for a progenitor star radius of 700 +/- 200 R_sun, the size of a red supergiant star. An excess in UV emission two weeks after shock breakout compared to SNe well fitted by model atmosphere-code synthetic spectra with solar metallicity, is best explained by suppressed line blanketing due to a lower metallicity progenitor star in SN 2010aq. Continued monitoring of PS1 MDS fields by the GALEX TDS will increase the sample of early UV detections of Type II SNe by an order of magnitude, and probe the diversity of SN progenitor star properties., Comment: 4 pages, 3 color figures. Accepted for publication in ApJ Letters, corrections from proofs added

Published
2010
Full Text
View/download PDF

3. SN 2009kf : a UV bright type IIP supernova discovered with Pan-STARRS 1 and GALEX

Author

Botticella, M. T., Trundle, C., Pastorello, A., Rodney, S., Rest, A., Gezari, S., Smartt, S. J., Narayan, G., Huber, M. E., Tonry, J. L., Young, D., Smith, K., Bresolin, F., Valenti, S., Kotak, R., Mattila, S., Kankare, E., Wood-Vasey, W. M., Riess, A., Neill, J. D., Forster, K., Martin, D. C., Stubbs, C. W., Burgett, W. S., Chambers, K. C., Dombeck, T., Flewelling, H., Grav, T., Heasley, J. N., Hodapp, K. W., Kaiser, N., Kudritzki, R., Luppino, G., Lupton, R. H., Magnier, E. A., Monet, D. G., Morgan, J. S., Onaka, P. M., Price, P. A., Rhoads, P. H., Siegmund, W. A., Sweeney, W. E., Wainscoat, R. J., Waters, C., Waterson, M. F., and Wynn-Williams, C. G.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present photometric and spectroscopic observations of a luminous type IIP Supernova 2009kf discovered by the Pan-STARRS 1 (PS1) survey and detected also by GALEX. The SN shows a plateau in its optical and bolometric light curves, lasting approximately 70 days in the rest frame, with absolute magnitude of M_V = -18.4 mag. The P-Cygni profiles of hydrogen indicate expansion velocities of 9000km/s at 61 days after discovery which is extremely high for a type IIP SN. SN 2009kf is also remarkably bright in the near-ultraviolet (NUV) and shows a slow evolution 10-20 days after optical discovery. The NUV and optical luminosity at these epochs can be modelled with a black-body with a hot effective temperature (T ~16,000 K) and a large radius (R ~1x10^{15} cm). The bright bolometric and NUV luminosity, the lightcurve peak and plateau duration, the high velocities and temperatures suggest that 2009kf is a type IIP SN powered by a larger than normal explosion energy. Recently discovered high-z SNe (0.7 < z < 2.3) have been assumed to be IIn SNe, with the bright UV luminosities due to the interaction of SN ejecta with a dense circumstellar medium (CSM). UV bright SNe similar to SN 2009kf could also account for these high-z events, and its absolute magnitude M_NUV = -21.5 +/- 0.5 mag suggests such SNe could be discovered out to z ~2.5 in the PS1 survey., Comment: Accepted for publication in APJL

Published
2010
Full Text
View/download PDF

4. Searching for sub-kilometer TNOs using Pan-STARRS video mode lightcurves: Preliminary study and evaluation using engineering data

Author

Wang, J. -H., Protopapas, P., Chen, W. -P., Alcock, C. R., Burgett, W. S., Dombeck, T., Morgan, J. S., Price, P. A., and Tonry, J. L.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

We present a pre-survey study of using Pan-STARRS high sampling rate video mode guide star images to search for TNOs. With suitable selection of the guide stars within the Pan-STARRS 7 deg^{2} field of view, the lightcurves of these guide stars can also be used to search for occultations by TNOs. The best target stars for this purpose are stars with high signal-to-noise ratio (SNR) and small angular size.In order to do this, we compiled a catalog using the SNR calculated from stars with m_V <13 mag in the Tycho2 catalog then cross matched these stars with the 2MASS catalog and estimated their angular sizes from (V-K) color. We also outlined a new detection method based on matched filter that is optimized to search for diffraction patterns in the lightcurves due to occultation by sub-kilometer TNOs. A detection threshold is set to compromise between real detections and false positives. Depending on the theoretical size distribution model used, we expect to find up to a hundred events during the three-year life time of the Pan-STARRS-1 project. We have tested the detection algorithm and the pipeline on a set of engineering data (taken at 10Hz in stead of 30Hz). No events were found within the engineering data, which is consistent with the small size of the data set and the theoretical models. Meanwhile, with a total of ~ 22 star-hours video mode data (|\beta| < 10^{\circ}), we are able to set an upper limit of N(>0.5 km) ~ 2.47x10^10 deg^-2 at 95% confidence limit., Comment: 27 pages, 17 figures, add co-author, citation

Published
2009
Full Text
View/download PDF

5. Physics Potential at FNAL with Stronger Proton Sources

Author

Barenboim, G., de Gouvea, A., Dombeck, T., Grossman, N., Harris, D., Michael, D., Szleper, M., Velasco, M., and Werkema, S.

Subjects
High Energy Physics - Experiment
Abstract

This document is the second in a series of reports on the exciting physics that would be accessible at Fermilab in the event of an upgraded proton source. Where the first report covered a broad range of topics, this report focuses specifically on three areas of study: there are brief discussions on the new measurements one could make in both the neutron and anti-proton sectors, and then a detailed discussion of what could be achieved in the neutrino oscillation sector using an upgraded proton source to supply the NuMI beamline with more protons. If one places a new detector optimized for $\nu_e$ appearance at a new location slightly off the axis defined by the MINOS experiment, that new experiment would be ideal for making the next important steps in lepton flavor studies, namely, the search for $\nu_\mu \to \nu_e$ at the atmospheric mass splitting, and CP violations. The report concludes with a summary of proton economics and demands for increased proton intensity for the Booster and Main Injector: what the proton source at Fermilab can currently supply, and what adiabatic changes could be implemented to boost the proton supply on the way from here to a proton driver upgrade., Comment: 44 pages, 18 figures, Latex

Published
2002

6. A Proposed Method for Measuring the Electric Dipole Moment of the Neutron Using Acceleration in an Electric-Field Gradient and Ultracold Neutron Interferometry

Author

Freedman, M. S., Ringo, G. R., and Dombeck, T. W.

Subjects
Nuclear Experiment, High Energy Physics - Experiment
Abstract

The use of an ultracold neutron interferometer incorporating an electrostatic accelerator having a strong electric field gradient to accelerate neutrons by their possible electric moments is proposed as a method of measuring the neutron electric dipole moment. Such electrical acceleration, followed by an amplifier and a generator of phase difference, could develop relatively large phase differences and these could be measured by a Mach-Zehnder interferometer. This method might extend the sensitivity of the measurement by several orders of magnitude beyond the current limit of 10^{-25} e.cm. Furthermore the systematic errors in such a measurement could be significantly different from those of the current EDM experiments., Comment: 33 pages, now including figures. REVTEX

Published
1998
Full Text
View/download PDF

7. Test results and operational characteristics of prototype SSCL half cell

Author

McInturff, A.D., Burgett, W., Carter, H., Dombeck, T., Gannon, J., Kraushaar, P., Mulholland, G., Savord, T., Tool, G., Robinson, W., Weisend, J.G., II, Voy, D., and Zbasnik, J.

Subjects
Business, Electronics, Electronics and electrical industries, Superconducting Super Collider -- Research
Abstract

The SSCL Accelerator System's String Test (ASST) has had several cool down, subsequent operational test series, and warm up cycles. The first cycle of these was rather limited in scope as mandated by Congress. The subsequent tests have been performed to obtain more complete information about parameters of, or operating experience with, the ensemble of magnets and spools when operating serially as in accelerator operations. The tests and procedures performed to date have emphasized cryogenic, mechanical, and electrical operations. These have included running, as well as upset conditions, i.e., superconducting to normal transition of the string (quench). This paper represents a summary of the operational test results and characteristics seen to date. A limited discussion will be included as to their implications with respect to a successful accelerator operation.

Published
1994

8. Half cell operations tests of the Superconducting Super Collider Laboratory

Author

McInturff, A.D., Augustynowicz, S., Burgett, W., Coombes, R., Dickey, C., Dombeck, T., Feitz, W., Flora, R., Gannon, J., Haenni, D., Kraushaar, P., Levin, M., McAshan, M., Mulholland, G., Murray, D., Robinson, W., Savord, T., Spinos, F., Tool, G., Weisend, J., II, Wallis, D., Voy, D., and Zbasnik, J.

Subjects
Magnetic fusion -- Research, Business, Electronics, Electronics and electrical industries, Superconducting Super Collider -- Research
Abstract

The experimental operation of a 100-m half cell for a superconducting super collider are reported. The tests on the 50-mm apeture magnet string, which are known as the Accelerator System String Test, involves data acquisition on operating procedures and parameters to supplement information obtained from test runs of a 17-m half cell with a 40-mm aperture. The 100-m long half cell is at the N-15 facility in Waxahachie, TX.

Published
1993

15. Informationsgrundlage für das Umweltpräsentationssystem des BMU 'Umwelt 2000 im Rahmen des Teilvorhabens 2 des Globalansatzes Expo 2000'. Anhang I: Katalog zur konsistenten Vorgehensweise bei der Erfassung von Rahmeninformationen in der Datenbank Grunddaten. Anhang II: Datengrundlage für Umwelt Deutschland

Author

Schön, M., Hillenbrand, T., Kuntze, U., Nathani, C., Toussaint, D., Behnke, L., Michi, S., Rauscher, J., Ziesing, H.-J., Knörr, W., Tochtermann, K., Dombeck, T., Kadric, L., and Publica

Subjects
Projektion, Umweltzustand, DB-Grunddaten, projection, Zeitreihe, time series, basic data, environmental situation, Szenarium, scenario
Abstract

Für eine flächendeckende Gesamtdarstellung des Umweltzustandes in Deutschland sollten die auf Bundesebene verfügbaren Informationsbausteine in einem Dokumentationssystem bereitgestellt werden. Der im Lauf der Bearbeitung erweiterte und modifizierte Themenkatalog umfasste ca. 150 Positionen. Die Ordnung dieses Themenkataloges ist an den Pressure-State-Response-Ansatz angelehnt. Zur Ermöglichung von Trendaussagen sollte dort, wo möglich und sinnvoll, ein Darstellungszeitraum von mindestens zehn Jahren von 1990 bis 2000 gewählt werden. Da die verfügbaren empirischen Zeitreihen meist nicht weiter als bis zum Jahr 1998 reichten, waren darauf aufbauende Projektionen der mittelfristigen Entwicklung über einen Zeitraum von zwei Jahren oder mehr erforderlich. In zwei ausgewählten Themenbereichen waren auch über das Jahr 2000 hinausgehende Szenarien zu erstellen, nämlich Szenarien der Emissionen von Treibhausgasen und Vorläufersubstanzen sowie Szenarien für den Bereich Verkehr und verkehrsbedingte Umweltbelastungen bis zum Jahr 2020. Basis für die Dokumentenverwaltung ist die im Umweltbundesamt entwickelte Datenbank, Grundbestand an Berichtsdaten (kurz: \'84DB Grunddaten"), die für die Zwecke von Umwelt Deutschland and auszubauen And zu befüllen war.

Published
2001

16. ULTRA-BRIGHT OPTICAL TRANSIENTS ARE LINKED WITH TYPE Ic SUPERNOVAE

Author

Pastorello, A., primary, Smartt, S. J., additional, Botticella, M. T., additional, Maguire, K., additional, Fraser, M., additional, Smith, K., additional, Kotak, R., additional, Magill, L., additional, Valenti, S., additional, Young, D. R., additional, Gezari, S., additional, Bresolin, F., additional, Kudritzki, R., additional, Howell, D. A., additional, Rest, A., additional, Metcalfe, N., additional, Mattila, S., additional, Kankare, E., additional, Huang, K. Y., additional, Urata, Y., additional, Burgett, W. S., additional, Chambers, K. C., additional, Dombeck, T., additional, Flewelling, H., additional, Grav, T., additional, Heasley, J. N., additional, Hodapp, K. W., additional, Kaiser, N., additional, Luppino, G. A., additional, Lupton, R. H., additional, Magnier, E. A., additional, Monet, D. G., additional, Morgan, J. S., additional, Onaka, P. M., additional, Price, P. A., additional, Rhoads, P. H., additional, Siegmund, W. A., additional, Stubbs, C. W., additional, Sweeney, W. E., additional, Tonry, J. L., additional, Wainscoat, R. J., additional, Waterson, M. F., additional, Waters, C., additional, and Wynn-Williams, C. G., additional

Published
2010
Full Text
View/download PDF

17. GALEX AND PAN-STARRS1 DISCOVERY OF SN IIP 2010aq: THE FIRST FEW DAYS AFTER SHOCK BREAKOUT IN A RED SUPERGIANT STAR

Author

Gezari, S., primary, Rest, A., additional, Huber, M. E., additional, Narayan, G., additional, Forster, K., additional, Neill, J. D., additional, Martin, D. C., additional, Valenti, S., additional, Smartt, S. J., additional, Chornock, R., additional, Berger, E., additional, Soderberg, A. M., additional, Mattila, S., additional, Kankare, E., additional, Burgett, W. S., additional, Chambers, K. C., additional, Dombeck, T., additional, Grav, T., additional, Heasley, J. N., additional, Hodapp, K. W., additional, Jedicke, R., additional, Kaiser, N., additional, Kudritzki, R., additional, Luppino, G., additional, Lupton, R. H., additional, Magnier, E. A., additional, Monet, D. G., additional, Morgan, J. S., additional, Onaka, P. M., additional, Price, P. A., additional, Rhoads, P. H., additional, Siegmund, W. A., additional, Stubbs, C. W., additional, Tonry, J. L., additional, Wainscoat, R. J., additional, Waterson, M. F., additional, and Wynn-Williams, C. G., additional

Published
2010
Full Text
View/download PDF

18. SUPERNOVA 2009kf: AN ULTRAVIOLET BRIGHT TYPE IIP SUPERNOVA DISCOVERED WITH PAN-STARRS 1 AND GALEX

Author

Botticella, M. T., primary, Trundle, C., additional, Pastorello, A., additional, Rodney, S., additional, Rest, A., additional, Gezari, S., additional, Smartt, S. J., additional, Narayan, G., additional, Huber, M. E., additional, Tonry, J. L., additional, Young, D., additional, Smith, K., additional, Bresolin, F., additional, Valenti, S., additional, Kotak, R., additional, Mattila, S., additional, Kankare, E., additional, Wood-Vasey, W. M., additional, Riess, A., additional, Neill, J. D., additional, Forster, K., additional, Martin, D. C., additional, Stubbs, C. W., additional, Burgett, W. S., additional, Chambers, K. C., additional, Dombeck, T., additional, Flewelling, H., additional, Grav, T., additional, Heasley, J. N., additional, Hodapp, K. W., additional, Kaiser, N., additional, Kudritzki, R., additional, Luppino, G., additional, Lupton, R. H., additional, Magnier, E. A., additional, Monet, D. G., additional, Morgan, J. S., additional, Onaka, P. M., additional, Price, P. A., additional, Rhoads, P. H., additional, Siegmund, W. A., additional, Sweeney, W. E., additional, Wainscoat, R. J., additional, Waters, C., additional, Waterson, M. F., additional, and Wynn-Williams, C. G., additional

Published
2010
Full Text
View/download PDF

21. Design of the Pan-STARRS telescopes

Author

Hodapp, K. W., primary, Kaiser, N., additional, Aussel, H., additional, Burgett, W., additional, Chambers, K. C., additional, Chun, M., additional, Dombeck, T., additional, Douglas, A., additional, Hafner, D., additional, Heasley, J., additional, Hoblitt, J., additional, Hude, C., additional, Isani, S., additional, Jedicke, R., additional, Jewitt, D., additional, Laux, U., additional, Luppino, G. A., additional, Lupton, R., additional, Maberry, M., additional, Magnier, E., additional, Mannery, E., additional, Monet, D., additional, Morgan, J., additional, Onaka, P., additional, Price, P., additional, Ryan, A., additional, Siegmund, W., additional, Szapudi, I., additional, Tonry, J., additional, Wainscoat, R., additional, and Waterson, M., additional

Published
2004
Full Text
View/download PDF

28. Muon-neutrino carbon charged-current interaction near the muon threshold

Author

Koetke, D. D., primary, Fisk, R., additional, Koetke, D. S., additional, Manweiler, R., additional, Bowles, T. J., additional, Brown, A., additional, Brown, R. E., additional, Burman, R. L., additional, Clark, D. A., additional, Clearwater, S., additional, Dombeck, T., additional, Kruse, H., additional, Lee, D., additional, Aas, B., additional, Igo, G., additional, Newsom, C., additional, Beavis, D., additional, Fung, S. Y., additional, Gorn, W., additional, Poe, R. T., additional, VanDalen, G. J., additional, Bassalleck, B., additional, Dieterle, B., additional, Gregory, C., additional, Hill, R. E., additional, Kang, J. H., additional, Leavitt, C., additional, Auerbach, L., additional, Datta, S., additional, and Huang, Y., additional

Published
1992
Full Text
View/download PDF

29. Performance of an expanding telescope used to obtain a low divergence H− beam

Author

Blind, B., primary, Christian, R., additional, Clout, P., additional, Dombeck, T., additional, Flicker, D., additional, Fuka, M., additional, Gilpatrick, D., additional, Hardekopf, R., additional, Heighway, E., additional, Jason, A., additional, McKee, R., additional, Mottershead, C.T., additional, Sawyer, G., additional, Shafer, R., additional, Simmons, J.E., additional, Stratton, T., additional, Walton, R.B., additional, Zander, M., additional, Bellinger, F., additional, Brumwell, F., additional, Fink, C., additional, Hummer, C., additional, Meades, P., additional, Novick, A., additional, Roche, C., additional, Rosing, M., additional, Yule, T., additional, Bos, R., additional, and McGehee, S., additional

Published
1992
Full Text
View/download PDF

33. Physics Study Group report on physics potential at FNAL with stronger proton sources

Author

Ankenbrandt, C., Barenboim, G., Carena, M., Carpenter, J., Chou, W., Corcoran, M., Dejongh, F., Dombeck, T., Fleming, B., Geer, S., Hartouni, Edward P., Jackson, G., Kasper, P., Kaplan, D., Alberto Marchionni, Morfin, J., Narain, M., Parke, S., Popovic, M., Pordes, Stephen H., Ray, R., Romanino, A., Rumerio, P., Schmitt, M., Spentzouris, P., Stefanski, R., Velasco, M. M., Wah, Y., Wai, L. L., Werkema, S., and Zimmermann, E.

36. Study of the Isospin Properties of Single-Pion Production by Neutrinos

Author

Barish, S. J., primary, Cho, Y., additional, Derrick, M., additional, Dombeck, T., additional, Hyman, L. G., additional, Musgrave, B., additional, Schreiner, P., additional, Singer, R., additional, Smith, R. P., additional, Swanson, D., additional, Yuta, H., additional, Barnes, V. E., additional, Carmony, D. D., additional, and Garfinkel, A. F., additional

Published
1976
Full Text
View/download PDF

37. Current and target jets produced in high energy neutrino-deuterium interactions

Author

Kitagaki, T., primary, Tanaka, S., additional, Yuta, H., additional, Abe, K., additional, Hasegawa, K., additional, Yamaguchi, A., additional, Tamai, K., additional, Hayashino, T., additional, Kunori, S., additional, Ohtani, Y., additional, Hayano, H., additional, Burnstein, R.A., additional, Hanlon, J., additional, Rubin, H.A., additional, Chang, C.Y., additional, Dombeck, T., additional, Snow, G.A., additional, Son, D., additional, Steinberg, P.H., additional, Engelmann, R., additional, Kafka, T., additional, Sommars, S., additional, Chang, C.C., additional, Mann, W.A., additional, and Schneps, J., additional

Published
1980
Full Text
View/download PDF

38. Inclusive ηp and ηn charged-current neutrino reactions below 6 GeV

Author

Barish, S.J., primary, Derrick, M., additional, Dombeck, T., additional, Hyman, L.G., additional, Musgrave, B., additional, Schreiner, P., additional, Singer, R., additional, Szczekowski, M., additional, Barnes, V.E., additional, Carmony, D.D., additional, Fernandez, E., additional, and Garfinkel, A.F., additional

Published
1977
Full Text
View/download PDF

39. Multiplicity distributions and rescattering effects inpdinteractions at 200 GeV/c

Author

Dombeck, T., primary, Hyman, L. G., additional, Koetke, D. D., additional, Phelan, J. J., additional, Singer, R., additional, Barish, S. J., additional, Hartner, G. F., additional, Patel, P. M., additional, Levman, G. M., additional, Sreedhar, V. A., additional, Yoon, T. -S., additional, Grechko, V. E., additional, Grishin, V. G., additional, Kuznetsov, A. A., additional, Leikin, E. M., additional, Melnikova, N. N., additional, Murzin, V. S., additional, Pozhidaeva, N. A., additional, Sarycheva, L. I., additional, Scheglova, L. M., additional, Shevchenko, V. G., additional, Smirnova, L. N., additional, Solomin, A. N., additional, and Jancso, G., additional

Published
1978
Full Text
View/download PDF

41. Charged particle multiplicity distributions for 32 GeV/c K±p and interactions and for 50 GeV/c π±p interactions

Author

Akopdjanov, G.A., primary, Babincev, V.V., additional, Baccari, B., additional, Beilliere, P., additional, Chliapnikov, P.V., additional, Csejthey-Barth, M., additional, Daudin, A., additional, Deler, B., additional, Dombeck, T., additional, Dumont, J.J., additional, Ermolov, P.F., additional, Fenjuk, A.B., additional, Gensch, U., additional, Gerdyukov, L.N., additional, Ghesquiere, C., additional, Graessler, H., additional, Gumenyuk, S.A., additional, Johnstad, H., additional, Kellner, G., additional, Kuhn, D., additional, Laurent, J., additional, Lambacher, H., additional, Manyukov, B.A., additional, Moiseev, A.M., additional, Mosca, L., additional, Novak, H., additional, Schlesinger, J., additional, Smadja, G., additional, Sulyaev, R.M., additional, Triantis, F.A., additional, Vlasov, E.V., additional, Vogt, H., additional, and Windmolders, R., additional

Published
1974
Full Text
View/download PDF

43. Study of High-Energy Antineutrino-Proton Interactions

Author

Derrick, M., primary, Dombeck, T., additional, Hyman, L., additional, Jaeger, K., additional, Lissauer, D., additional, Miller, R. J., additional, Musgrave, B., additional, Phelan, J. J., additional, Schreiner, P., additional, Singer, R., additional, Barish, S. J., additional, Engler, A., additional, Keyes, G., additional, Kraemer, R. W., additional, and Schlereth, J., additional

Published
1976
Full Text
View/download PDF

44. Charmed-Baryon Production in High-Energy Neutrino-Deuterium Interactions

Author

Kitagaki, T., primary, Tanaka, S., additional, Yuta, H., additional, Abe, K., additional, Hasegawa, K., additional, Yamaguchi, A., additional, Tamai, K., additional, Hayashino, T., additional, Kunori, S., additional, Ohtani, Y., additional, Hayano, H., additional, Burnstein, R. A., additional, Hanlon, J., additional, Rubin, H. A., additional, Chang, C. Y., additional, Dombeck, T., additional, Snow, G. A., additional, Son, D., additional, Steinberg, P. H., additional, Engelmann, R., additional, Kafka, T., additional, Sommars, S., additional, Callas, J., additional, Chang, C. C., additional, Mann, W. A., additional, and Schneps, J., additional

Published
1980
Full Text
View/download PDF

46. Study ofνdcharged-current two-pion production in the threshold region

Author

Day, D., primary, Ammar, R., additional, Coppage, D., additional, Davis, R., additional, Kwak, N., additional, Stump, R., additional, Barish, S. J., additional, Engler, A., additional, Kraemer, R. W., additional, Miller, K., additional, Stacey, B. J., additional, Derrick, M., additional, Dombeck, T., additional, Fernandez, E., additional, Hyman, L., additional, Levman, G., additional, Koetke, D., additional, Musgrave, B., additional, Schreiner, P., additional, Singer, R., additional, Snyder, A., additional, Toaff, S., additional, Barnes, V. E., additional, Carmony, D. D., additional, Garfinkel, A. F., additional, and Radecky, G. M., additional

Published
1983
Full Text
View/download PDF

47. Properties of a neutrino-induced dilepton event

Author

Barish, S. J., primary, Derrick, M., additional, Dombeck, T., additional, Musgrave, B., additional, Schreiner, P., additional, Singer, R., additional, Szczekowski, M., additional, Barnes, V. E., additional, Carmony, D. D., additional, Fernandez, E., additional, and Garfinkel, A. F., additional

Published
1977
Full Text
View/download PDF

48. Analysis of the exclusive interaction νμ−12C→μ−12 N near threshold

Author

Bowles, T., primary, Brown, A., additional, Brown, R. E., additional, Burman, R., additional, Clark, D., additional, Clearwater, S., additional, Dombeck, T., additional, Kruse, H., additional, Lee, D., additional, Auerbach, L., additional, Datta, S., additional, Huang, Y., additional, Bas, A., additional, Igo, G., additional, Beavis, D., additional, Fung, S. Y., additional, Gorn, B., additional, Poe, R., additional, Van Dalen, G., additional, Newsom, C., additional, Bassalleck, B., additional, Dieterle, B., additional, Hill, R., additional, Kang, J., additional, Leavitt, C., additional, Fisk, R., additional, Koetke, D. D., additional, Koetke, D. S., additional, and Manweiler, R. W., additional

Published
1988
Full Text
View/download PDF

49. The search for neutrino oscillations in the appearance mode νν→νe for neutrino energies near the muon threshold

Author

Dombeck, T., primary, Bowles, T.J., additional, Brown, A., additional, Brown, R.E., additional, Burman, R.L., additional, Clark, D., additional, Clearwater, S., additional, Kruse, H., additional, Lee, D., additional, Aas, B., additional, Igo, G., additional, Newsom, C., additional, Beavis, D., additional, Fung, S.Y., additional, Gorn, W., additional, Poe, R.T., additional, Vandalen, G.J., additional, Bassalleck, B., additional, Dieterle, B., additional, Hill, R.E., additional, Kang, J.H., additional, Leavitt, C., additional, Auerbach, L., additional, Datta, S., additional, Huang, Y., additional, Fisk, R., additional, Koetke, D., additional, and Manweiler, R., additional

Published
1987
Full Text
View/download PDF

50. Comparison ofνnandνpCharged-Current Cross Sections from High-Energy Neutrino Interactions in Deuterium

Author

Hanlon, J., primary, Burnstein, R. A., additional, Rubin, H. A., additional, Chang, C. Y., additional, Dombeck, T., additional, Snow, G. A., additional, Son, D., additional, Steinberg, P. H., additional, Engelmann, R., additional, Kafka, T., additional, Sommars, S., additional, Kitagaki, T., additional, Tanaka, S., additional, Yuta, H., additional, Abe, K., additional, Hasegawa, K., additional, Yamaguchi, A., additional, Tamai, K., additional, Hayashino, T., additional, Kunori, S., additional, Ohtani, Y., additional, Hayano, H., additional, Chang, C. C., additional, Mann, W. A., additional, and Schneps, J., additional

Published
1980
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results