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1. Physical modelling of near-Earth asteroid (23187) 2000 PN9 with ground-based optical and radar observations

Author

Dover, L., Lowry, S. C., Rożek, A., Rozitis, B., Jackson, S. L., Zegmott, T., Krugly, Yu. N., Belskaya, I. N., Fitzsimmons, A., Green, S. F., Snodgrass, C., Weissman, P. R., Brozović, M., Benner, L. A. M., Busch, M. W., Ayvazian, V. R., Chiorny, V., Inasaridze, R. Ya., Krugov, M., Mykhailova, S., Reva, I., and Hibbert, J.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

We present a physical model and spin-state analysis of the potentially hazardous asteroid (23187) 2000 PN9. As part of a long-term campaign to make direct detections of the YORP effect, we collected optical lightcurves of the asteroid between 2006 and 2020. These observations were combined with planetary radar data to develop a detailed shape model which was used to search for YORP acceleration. We report that 2000 PN9 is a relatively large top-shaped body with a sidereal rotation period of 2.53216$\pm$0.00015 h. Although we find no evidence for rotational acceleration, YORP torques smaller than $\sim$10$^{-8}$$\,\rm rad/day^{2}$ cannot be ruled out. It is likely that 2000 PN9 is a YORP-evolved object, and may be an example of YORP equilibrium or self limitation., Comment: Accepted for publication in Monthly Notices of the Royal Astronomical Society. Main paper: 15 pages, 12 figures. Appendix: 9 pages, 8 figures

Published
2023

2. Spin State Evolution of (99942) Apophis during its 2029 Earth Encounter

Author

Benson, C. J., Scheeres, D. J., Brozovic, M., Chesley, S., Pravec, P., and Scheirich, P.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

We explore the effects of the 2029 Earth encounter on asteroid (99942) Apophis' non-principal axis spin state, leveraging refined orbit, spin state, and inertia information provided by more recent optical and radar observations. Propagating the asteroids' coupled orbit and rigid body attitude dynamics through the flyby, we present the range of possible post-flyby spin states. These spin state distributions will be valuable for planning Apophis observation campaigns and spacecraft missions, most notably OSIRIS-APEX. The simulations indicate that gravitationally induced changes to the asteroid's tumbling periods and rotational angular momentum direction (pole) will likely be significant and measurable. For the current spin state and inertia estimates and their uncertainties, Apophis is likely to remain in a short axis mode (SAM) tumbling state but its effective spin rate could halve or double. Its pole is likely to shift by 10 degrees or more and increase in longitude while moving closer to the ecliptic plane. These spin state changes are very sensitive to the asteroid's close approach attitude and mass distribution. With ground-based tracking of the asteroid's spin state through the encounter, this sensitivity will help refine mass distribution knowledge. We also discuss the implications of this abrupt spin state alteration for Apophis' Yarkovsky acceleration and geophysical properties, identifying possible pathways for surface and internal changes, most notably if Apophis is a contact binary. Comparison of the pre and post-flyby inertia estimates obtained from the ground-based observations will help assess the extent of possible geophysical changes.

Published
2022
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3. Combined Emerging Capabilities for Near-Earth Objects (NEOs)

Author

Milam, S. N., Hammel, H. B., Bauer, J., Brozovic, M., Grav, T., Holler, B. J., Lisse, C., Mainzer, A., Reddy, V., Schwamb, M. E., Spahr, T., Thomas, C. A., and Woods, D.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics
Abstract

Assess the joint capabilities of emerging telescopes for near-Earth objects (NEOs) survey and characterization, and what they will add to the current capabilities or replace. NASA telescopes in prime mission, in development, or under study, and requested for this assessment, include: - The Transiting Exoplanet Survey Satellite (TESS) - The James Webb Space Telescope (JWST) - The Wide Field Infrared Survey Telescope (WFIRST) - The Near-Earth Object Camera (NEOCam). Also requested for this assessment is the Large Synoptic Survey Telescope (LSST), an 8.4-meter ground-based telescope in development by the National Science Foundation and Department of Energy (DOE), with the capability to discover and catalogue NEOs., Comment: White Paper for NASA on astrophysics assets

Published
2019

4. Planetary Bistatic Radar

Author

Brozovic, M., Butler, B. J., Margot, Jean-Luc, Naidu, Shantanu P., and Lazio, T. Joseph W.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

Planetary radar observations offer the potential for probing the properties of characteristics of solid bodies throughout the inner solar system and at least as far as the orbit of Saturn. In addition to the direct scientific value, precise orbital determinations can be obtained from planetary radar observations, which are in turn valuable for mission planning or spacecraft navigation and planetary defense. The next-generation Very Large Array would not have to be equipped with a transmitter to be an important asset in the world's planetary radar infrastructure. Bistatic radar, in which one antenna transmits (e.g., Arecibo or Goldstone) and another receives, are used commonly today, with the Green Bank Telescope (GBT) serving as a receiver. The improved sensitivity of the ngVLA relative to the GBT would improve the signal-to-noise ratios on many targets and increase the accessible volume specifically for asteroids. Goldstone-ngVLA bistatic observations would have the potential of rivaling the sensitivity of Arecibo, but with much wider sky access., Comment: 11 pages, 2 figures, To be published in the ASP Monograph Series, "Science with a Next-Generation VLA", ed. E. J. Murphy (ASP, San Francisco, CA)

Published
2018

5. Planetary Bistatic Radar

Author

Brozovic, M, Butler, BJ, Margot, Jean-Luc, Naidu, Shantanu P, and Lazio, T Joseph W

Subjects
astro-ph.EP
Abstract

Planetary radar observations offer the potential for probing the propertiesof characteristics of solid bodies throughout the inner solar system and atleast as far as the orbit of Saturn. In addition to the direct scientificvalue, precise orbital determinations can be obtained from planetary radarobservations, which are in turn valuable for mission planning or spacecraftnavigation and planetary defense. The next-generation Very Large Array wouldnot have to be equipped with a transmitter to be an important asset in theworld's planetary radar infrastructure. Bistatic radar, in which one antennatransmits (e.g., Arecibo or Goldstone) and another receives, are used commonlytoday, with the Green Bank Telescope (GBT) serving as a receiver. The improvedsensitivity of the ngVLA relative to the GBT would improve the signal-to-noiseratios on many targets and increase the accessible volume specifically forasteroids. Goldstone-ngVLA bistatic observations would have the potential ofrivaling the sensitivity of Arecibo, but with much wider sky access.

Published
2018

7. The Pluto system: Initial results from its exploration by New Horizons

Author

Stern, S. A., Bagenal, F., Ennico, K., Gladstone, G. R., Grundy, W. M., McKinnon, W. B., Moore, J. M., Olkin, C. B., Spencer, J. R., Weaver, H. A., Young, L. A., Andert, T., Andrews, J., Banks, M., Bauer, B., Bauman, J., Barnouin, O. S., Bedini, P., Beisser, K., Beyer, R. A., Bhaskaran, S., Binzel, R. P., Birath, E., Bird, M., Bogan, D. J., Bowman, A., Bray, V. J., Brozovic, M., Bryan, C., Buckley, M. R., Buie, M. W., Buratti, B. J., Bushman, S. S., Calloway, A., Carcich, B., Cheng, A. F., Conard, S., Conrad, C. A., Cook, J. C., Cruikshank, D. P., Custodio, O. S., Ore, C. M. Dalle, Deboy, C., Dischner, Z. J. B., Dumont, P., Earle, A. M., Elliott, H. A., Ercol, J., Ernst, C. M., Finley, T., Flanigan, S. H., Fountain, G., Freeze, M. J., Greathouse, T., Green, J. L., Guo, Y., Hahn, M., Hamilton, D. P., Hamilton, S. A., Hanley, J., Harch, A., Hart, H. M., Hersman, C. B., Hill, A., Hill, M. E., Hinson, D. P., Holdridge, M. E., Horanyi, M., Howard, A. D., Howett, C. J. A., Jackman, C., Jacobson, R. A., Jennings, D. E., Kammer, J. A., Kang, H. K., Kaufmann, D. E., Kollmann, P., Krimigis, S. M., Kusnierkiewicz, D., Lauer, T. R., Lee, J. E., Lindstrom, K. L., Linscott, I. R., Lisse, C. M., Lunsford, A. W., Mallder, V. A., Martin, N., McComas, D. J., McNutt Jr., R. L., Mehoke, D., Mehoke, T., Melin, E. D., Mutchler, M., Nelson, D., Nimmo, F., Nunez, J. I., Ocampo, A., Owen, W. M., Paetzold, M., Page, B., Parker, A. H., Parker, J. W., Pelletier, F., Peterson, J., Pinkine, N., Piquette, M., Porter, S. B., Protopapa, S., Redfern, J., Reitsema, H. J., Reuter, D. C., Roberts, J. H., Robbins, S. J., Rogers, G., Rose, D., Runyon, K., Retherford, K. D., Ryschkewitsch, M. G., Schenk, P., Schindhelm, R., Sepan, B., Showalter, M. R., Singer, K. N., Soluri, M., Stanbridge, D., Steffl, A. J., Strobel, D. F., Stryk, T., Summers, M. E., Szalay, J. R., Tapley, M., Taylor, A., Taylor, H., Throop, H. B., Tsang, C. C. C., Tyler, G. L., Umurhan, O. M., Verbiscer, A. J., Versteeg, M. H., Vincent, M., Webbert, R., Weidner, S., Weigle II, G. E., White, O. L., Whittenburg, K., Williams, B. G., Williams, K., Williams, S., Woods, W. W., Zangari, A. M., and Zirnstein, E.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

The Pluto system was recently explored by NASA's New Horizons spacecraft, making closest approach on 14 July 2015. Pluto's surface displays diverse landforms, terrain ages, albedos, colors, and composition gradients. Evidence is found for a water-ice crust, geologically young surface units, surface ice convection, wind streaks, volatile transport, and glacial flow. Pluto's atmosphere is highly extended, with trace hydrocarbons, a global haze layer, and a surface pressure near 10 microbars. Pluto's diverse surface geology and long-term activity raise fundamental questions about how small planets remain active many billions of years after formation. Pluto's large moon Charon displays tectonics and evidence for a heterogeneous crustal composition, its north pole displays puzzling dark terrain. Small satellites Hydra and Nix have higher albedos than expected., Comment: 8 pages - Initial Science paper from NASA's New Horizons Pluto Encounter

Published
2015
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8. Asteroid 1566 Icarus's size, shape, orbit, and Yarkovsky drift from radar observations

Author

Greenberg, AH, Margot, J-L, Verma, AK, Taylor, PA, Naidu, SP, Brozovic, M, and Benner, LAM

Subjects
astro-ph.EP, Space Sciences, Physical Sciences, methods: data analysis, minor planets, asteroids: individual, planets and satellites: dynamical evolution and stability, planets and satellites: surfaces, techniques: radar astronomy, Astronomical and Space Sciences, Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics
Abstract

Near-Earth asteroid (NEA) 1566 Icarus ($a=1.08\,\mathrm{au}$, e = 0.83, $i=22\buildrel{\circ}\over{.} 8$) made a close approach to Earth in 2015 June at 22 lunar distances (LD). Its detection during the 1968 approach (16 LD) was the first in the history of asteroid radar astronomy. A subsequent approach in 1996 (40 LD) did not yield radar images. We describe analyses of our 2015 radar observations of Icarus obtained at the Arecibo Observatory and the DSS-14 antenna at Goldstone. These data show that the asteroid is a moderately flattened spheroid with an equivalent diameter of 1.44 km with 18% uncertainties, resolving long-standing questions about the asteroid size. We also solve for Icarus's spin-axis orientation ($\lambda =270^\circ \pm 10^\circ ,\beta =-81^\circ \pm 10^\circ $), which is not consistent with the estimates based on the 1968 light-curve observations. Icarus has a strongly specular scattering behavior, among the highest ever measured in asteroid radar observations, and a radar albedo of ~2%, among the lowest ever measured in asteroid radar observations. The low cross section suggests a high-porosity surface, presumably related to Icarus's cratering, spin, and thermal histories. Finally, we present the first use of our orbit-determination software for the generation of observational ephemerides, and we demonstrate its ability to determine subtle perturbations on NEA orbits by measuring Icarus's orbit-averaged drift in semimajor axis ($(-4.62\pm 0.48)\times {10}^{-4}$ au My−1, or ~60 m per revolution). Our Yarkovsky rate measurement resolves a discrepancy between two published rates that did not include the 2015 radar astrometry.

Published
2017

10. RADAR IMAGING AND CHARACTERIZATION OF THE BINARY NEAR-EARTH ASTEROID (185851) 2000 DP107

Author

Naidu, SP, Margot, JL, Taylor, PA, Nolan, MC, Busch, MW, Benner, LAM, Brozovic, M, Giorgini, JD, Jao, JS, and Magri, C

Subjects
minor planets, asteroids: individual, techniques: radar astronomy, astro-ph.EP, Astronomical and Space Sciences, Astronomy & Astrophysics
Abstract

The potentially hazardous asteroid (185851) 2000 DP107 was the first binary near-Earth asteroid to be imaged. Radar observations in 2000 provided images at 75m resolution that revealed the shape, orbit, and spin-up formation mechanism of the binary. The asteroid made a more favorable flyby of the Earth in 2008, yielding images at 30m resolution. We used these data to obtain shape models for the two components and to improve the estimates of the mutual orbit, component masses, and spin periods. The primary has a sidereal spin period of 2.7745 ± 0.0007 hr and is roughly spheroidal with an equivalent diameter of 863m ± 5%. It has a mass of 4.656 ± 0.43 × 1011 kg and a density of 1381 ± 244 kgm.3. It exhibits an equatorial ridge similar to the (66391) 1999 KW4 primary; however, the equatorial ridge in this case is not as regular and has a .300 m diameter concavity on one side. The secondary has a sidereal spin period of 1.77 ± 0.02 days commensurate with the orbital period. The secondary is slightly elongated and has overall dimensions of 377 × 314 × 268 m (6% uncertainties). Its mass is 0.178 ± 0.021 × 1011 kg and its density is 1047 ± 230 kgm.3. The mutual orbit has a semimajor axis of 2.659 ± 0.08 km, an eccentricity of 0.019 ± 0.01, and a period of 1.7556 ± 0.0015 days. The normalized total angular momentum of this system exceeds the amount required for the expected spin-up formation mechanism. An increase of angular momentum from nongravitational forces after binary formation is a possible explanation. The two components have similar radar reflectivity, suggesting a similar composition consistent with formation by spin-up. The secondary appears to exhibit a larger circular polarization ratio than the primary, suggesting a rougher surface or subsurface at radar wavelength scales.

Published
2015

12. Next-Generation Ground-Based Planetary Radar

Author

Judd, M, Vilnorotter, V, Taylor, M, 'D'Addario, L.', 'Murphy, E, Campbell, B, Butler, B, Brozovic, M, Andrews, K, Sanchez-Net, M, and Lazio, Joseph

Published
2021

13. Orbits of near-earth asteroid triples 2001 SN263 and 1994 CC: Properties, origin, and evolution

Author

Fang, J, Margot, JL, Brozovic, M, Nolan, MC, Benner, LAM, and Taylor, PA

Subjects
minor planets, asteroids: general, minor planets, asteroids: individual, astro-ph.EP, minor planets, asteroids: general, asteroids: individual, Astronomy & Astrophysics, Astronomical and Space Sciences
Abstract

Three-body model fits to Arecibo and Goldstone radar data reveal the nature of two near-Earth asteroid triples. The triple-asteroid system 2001 SN263 is characterized by a primary of ∼1013 kg, an inner satellite 1% as massive orbiting at c∼3 primary radii in 0.7 days, and an outer satellite ∼2.5% as massive orbiting at ∼13 primary radii in 6.2 days. 1994 CC is a smaller system with a primary of mass ∼2.6 ×1011 kg and two satellites 2% and ≲1% as massive orbiting at distances of ∼5.5 and ∼19.5 primary radii. Their orbital periods are 1.2 and 8.4days. Examination of resonant arguments shows that the satellites are not currently in a mean-motion resonance. Precession of the apses and nodes are detected in both systems (2001 SN263 inner body: d/dt 1.1 deg day-1; 1994 CC inner body: d/dt ∼ -0.2 deg day-1), which is in agreement with analytical predictions of the secular evolution due to mutually interacting orbits and primary oblateness. Nonzero mutual inclinations between the orbital planes of the satellites provide the best fits to the data in both systems (2001 SN263: 14deg; 1994 CC: 16 ∼ deg). Our best-fit orbits are consistent with nearly circular motion, except for 1994 CC's outer satellite which has an eccentric orbit of e ∼ 0.19. We examine several processes that can generate the observed eccentricity and inclinations, including the Kozai and evection resonances, past mean-motion resonance crossings, and close encounters with terrestrial planets. In particular, we find that close planetary encounters can easily excite the eccentricities and mutual inclinations of the satellites' orbits to the currently observed values. © 2011. The American Astronomical Society. All rights reserved.

Published
2011

14. Radar observations and the shape of near-Earth ASTEROID 2008 EV5

Author

Busch, MW, Ostro, SJ, Benner, LAM, Brozovic, M, Giorgini, JD, Jao, JS, Scheeres, DJ, Magri, C, Nolan, MC, Howell, ES, Taylor, PA, Margot, JL, and Brisken, W

Subjects
Asteroids, Asteroids, Surfaces, Asteroids, Dynamics, Radar observations, astro-ph.EP, Surfaces, Dynamics, Astronomy & Astrophysics, Astronomical and Space Sciences, Geochemistry, Geophysics
Abstract

We observed the near-Earth ASTEROID 2008 EV5 with the Arecibo and Goldstone planetary radars and the Very Long Baseline Array during December 2008. EV5 rotates retrograde and its overall shape is a 400 ± 50 m oblate spheroid. The most prominent surface feature is a ridge parallel to the asteroid's equator that is broken by a concavity about 150. m in diameter. Otherwise the asteroid's surface is notably smooth on decameter scales. EV5's radar and optical albedos are consistent with either rocky or stony-iron composition. The equatorial ridge is similar to structure seen on the rubble-pile near-Earth asteroid (66391) 1999 KW4 and is consistent with YORP spin-up reconfiguring the asteroid in the past. We interpret the concavity as an impact crater. Shaking during the impact and later regolith redistribution may have erased smaller features, explaining the general lack of decameter-scale surface structure. © 2011 Elsevier Inc.

Published
2011

19. OSIRIS-REx Gravity Field Estimates for Bennu Using Spacecraft and Natural Particle Tracking Data

Author

Scheeres, D. J, French, A. S, McMahon, J. W, Davis, A. B, Brack, D. N, Leonard, J. M, Antreasian, P, Brozovic, M, Chesley, S. R, Farnocchia, D, Jacobson, R. A, Takahashi, Y, Mazarico, E. M, Liounis, A, Rowlands, D, Highsmith, D. E, Getzandanner, K, Moreau, M, Tricarico, P, Goossens, S, Johnson, C. L, Al Asad, M. M, Daly, M. G, Seabrook, J. A, Roberts, J, Perry, M, Barnouin, O. S, Hergenrother, C. W, Nolan, M. C, and Lauretta, D. S

Subjects
Lunar And Planetary Science And Exploration
Abstract

The current best estimates of Bennu’s gravity field will be presented, based on the independent solutions from four different teams involved on the OSIRIS-REx mission. The discovery of ejected particles about Bennu that may remain in orbit for several days or more provide a unique opportunity to probe the gravity field to higher degree and order than possible by using conventional spacecraft tracking. However, the non-gravitational forces acting on these particles must also be characterized, and their impact on solution accuracy must be assessed. This talk will present the latest results from the mission, incorporating spacecraft tracking from the lowest orbit in which the satellite will be during the mission.

Published
2019

20. Radar Astronomy

Author

Lazio, Joseph, Benner, L, Brozovic, M, Giorgini, J, Naidu, S, and Preston, R

Published
2019

21. Radar Astronomy

Author

Preston, R, Naidu, S, Giorgini, J, Brozovic, M, Benner, L, and Lazio, Joseph

Abstract

UNKNOWN

Published
2019

26. Ground-based radar observations of Didymos

Author

Scheeres, D.J, Virkki, A, Scheirich, P, Pravec, P, Margot, J.L, Nolan, M.C, Ostro, S.J, Giorgini, J.D, Brozovic, M, Benner, L.A.M, and Naidu, S.P

Abstract

UNKNOWN

Published
2018

27. Ground-based radar observations of Didymos

Author

Naidu, S.P, Benner, L.A.M, Brozovic, M, Giorgini, J.D, Ostro, S.J, Nolan, M.C, Margot, J.L, Pravec, P, Scheirich, P, Virkki, A, and Scheeres, D.J

Published
2018

30. Spin state evolution of (99942) Apophis during its 2029 Earth encounter

Author

Benson, C. J., Scheeres, D. J., Brozovic, M., Chesley, S., Pravec, P., and Scheirich, P.

Subjects
Earth and Planetary Astrophysics (astro-ph.EP), Space and Planetary Science, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics - Earth and Planetary Astrophysics
Abstract

We explore the effects of the 2029 Earth encounter on asteroid (99942) Apophis' non-principal axis spin state, leveraging refined orbit, spin state, and inertia information provided by more recent optical and radar observations. Propagating the asteroids' coupled orbit and rigid body attitude dynamics through the flyby, we present the range of possible post-flyby spin states. These spin state distributions will be valuable for planning Apophis observation campaigns and spacecraft missions, most notably OSIRIS-APEX. The simulations indicate that gravitationally induced changes to the asteroid's tumbling periods and rotational angular momentum direction (pole) will likely be significant and measurable. For the current spin state and inertia estimates and their uncertainties, Apophis is likely to remain in a short axis mode (SAM) tumbling state but its effective spin rate could halve or double. Its pole is likely to shift by 10 degrees or more and increase in longitude while moving closer to the ecliptic plane. These spin state changes are very sensitive to the asteroid's close approach attitude and mass distribution. With ground-based tracking of the asteroid's spin state through the encounter, this sensitivity will help refine mass distribution knowledge. We also discuss the implications of this abrupt spin state alteration for Apophis' Yarkovsky acceleration and geophysical properties, identifying possible pathways for surface and internal changes, most notably if Apophis is a contact binary. Comparison of the pre and post-flyby inertia estimates obtained from the ground-based observations will help assess the extent of possible geophysical changes.

Published
2023

31. PLANETARY SCIENCE: The Pluto system: Initial results from its exploration by New Horizons

Author

Stern, S. A., Bagenal, F., Ennico, K., Gladstone, G. R., Grundy, W. M., McKinnon, W. B., Moore, J. M., Olkin, C. B., Spencer, J. R., Weaver, H. A., Young, L. A., Andert, T., Andrews, J., Banks, M., Bauer, B., Bauman, J., Barnouin, O. S., Bedini, P., Beisser, K., Beyer, R. A., Bhaskaran, S., Binzel, R. P., Birath, E., Bird, M., Bogan, D. J., Bowman, A., Bray, V. J., Brozovic, M., Bryan, C., Buckley, M. R., Buie, M. W., Buratti, B. J., Bushman, S. S., Calloway, A., Carcich, B., Cheng, A. F., Conard, S., Conrad, C. A., Cook, J. C., Cruikshank, D. P., Custodio, O. S., Ore, Dalle C. M., Deboy, C., Dischner, Z. J. B., Dumont, P., Earle, A M., Elliott, H. A, Ercol, J., Ernst, C. M., Finley, T., Flanigan, S. H., Fountain, G., Freeze, M. J., Greathouse, T., Green, J. L., Guo, Y., Hahn, M., Hamilton, D. P., Hamilton, S. A., Hanley, J., Harch, A., Hart, H. M., Hersman, C. B., Hill, A., Hill, M. E., Hinson, D. P., Holdridge, M. E., Horanyi, M., Howard, A. D., Howett, C. J. A., Jackman, C., Jacobson, R. A., Jennings, D. E., Kammer, J. A., Kang, H. K., Kaufmann, D. E., Kollmann, P., Krimigis, S. M., Kusnierkiewicz, D., Lauer, T. R., Lee, J. E., Lindstrom, K. L., Linscott, I. R., Lisse, C. M., Lunsford, A. W., Mallder, V. A., Martin, N., McComas, D. J., McNutt, R. L., Jr., Mehoke, D., Mehoke, T., Melin, E. D., Mutchler, M., Nelson, D., Nimmo, F., Nunez, J. I., Ocampo, A., Owen, W. M., Paetzold, M., Page, B., Parker, A. H., Parker, J. W., Pelletier, F., Peterson, J., Pinkine, N., Piquette, M., Porter, S. B., Protopapa, S., Redfern, J., Reitsema, H. J., Reuter, D. C., Roberts, J. H., Bobbins, S. J., Rogers, G., Rose, D., Runyon, K., Retherford, K. D., Ryschkewitsch, M. G., Schenk, P., Schindhelm, E., Sepan, B., Showalter, M. R., Singer, K. N., Soluri, M., Stanbridge, D., Steffl, A. J., Strobel, D. F., Stryk, T., Summers, M. E., Szalay, J. R., Tapley, M., Taylor, A., Taylor, H., Throop, H. B., Tsang, C. C. C., Tyler, G. L., Umurhan, O. M., Verbiscer, A. J., Versteeg, M. H., Vincent, M., Webbert, R., Weidner, S., Weigle, G. E., II, White, O. L., Whittenburg, K., Williams, B. G., Williams, K., Williams, S., Woods, W. W., Zangari, A. M., and Zirnstein, E.

Published
2015
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32. The Next-Generation Ground-Based Planetary Radar

Author

Lazio, Joseph, primary, Virkki, Anne K., additional, Pinilla-Alonso, Noemi, additional, Benner, L. A. M., additional, Brozovic, M., additional, Butler, B. J., additional, Campbell, B. A., additional, Cordova, F., additional, Kleer, K. de, additional, Edwards, P. G., additional, Eubanks, T. M., additional, Fernandez, Y. R., additional, Giorgini, J. D., additional, Kruzins, E., additional, Margot, J. L., additional, Mainzer, A., additional, Marshall, S. E., additional, Paganelli, F., additional, Raymond, C. A., additional, Taylor, P. A., additional, Rivera-Valentín, E., additional, Slade, M. A., additional, and Venditti, F. C. F., additional

Published
2021
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33. Combined Emerging Capabilities for Near-Earth Objects (NEOs)

Author

Milam, Stefanie, primary, Hammel, H.B., additional, Bauer, J., additional, Brozovic, M., additional, Grav, T., additional, Holler, B. J., additional, Lisse, C., additional, Mainzer, A., additional, Reddy, V., additional, Schwamb, M. E., additional, Spahr, T., additional, Thomas, C. A., additional, and Woods, D., additional

Published
2021
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37. Improved Impact Hazard Assessment with Existing Radar Sites and a New 70-m Southern Hemisphere Radar Installation

Author

Giorgini, J. D, Slade, M. A, Silva, A, Preston, R. A, Brozovic, M, Taylor, P. A, and Magri, C

Subjects
Communications And Radar
Abstract

Add radar capability to the existing southern hemisphere 70-m Deep Space Network (DSN) site at Canberra, Australia, thereby increasing by 1.5-2x the observing time available for high-precision NEO trajectory refinement and characterization. Estimated cost: approx.$16 million over 3 years, $2.5 million/year for operations (FY09).

Published
2009

38. CDF Central Outer Tracker

Author

Affolder, T, Allspach, D, Ambrose, D, Bialek, J, Bokhari, W, Brozovic, M, Binkley, M, Burkett, K, Byon-Wagner, A, Cogswell, F, Dressnandt, N, Feng, Z, Franklin, M, Galtieri, L, Gerdes, D.W, Greenwood, J, Guarino, V, Guimaraes da Costa, J, Haggerty, R, Hall, C, Heinrich, J, Holloway, A, Jacobi, T, Kephart, K, Khazins, D, Kim, Y.K, Kirby, M, Kononenko, W, Kotwal, A.V, Kraus, J, Liss, T.M, Lockyer, N, Madrak, R, Miao, T, Mukherjee, A, Neu, C, Newcomer, M, Niczyporuk, J.M, Nodulman, L, Orejudous, W, Phillips, T.J, Pitts, K.T, Reigler, W, Richards, R, Rivetta, C, Robertson, W.J, Roser, R, Sadler, L, Sandberg, R, Sansone, S, Schmitt, R, Schultz, K, Shuman, D, Silva, R, Singh, P, Snihur, R, Tamburello, P, Taylor, J, Thurman-Keup, R, Tousignant, D, Ukegawa, F, Van Berg, R, Veramendi, G, Vickey, T, Wacker, J, Wagner, R.L, Weidenbach, R, Wester, W.C, III, Williams, H.H, Wilson, P, Wittich, P, Yagil, A, Yu, I, Yu, S, and Yun, J.C

Published
2004
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39. Patterns of mortality in sickle cell disease in the United Kingdom

Author

Gray, A., Anionwu, E.N., Davies, S.C., and Brozovic, M.

Subjects
Erythrocytes -- Deformability, Genetic disorders -- Reports, Sickle cell anemia -- Patient outcomes, Epidemiological research -- Reports, Health
Abstract

Sickle cell disease is a disease that causes red blood cells to become deformed. The red blood cells of patients with sickle cell disease are crescent or sickle-shaped instead of their normal circular shape and do not function properly. In a previous survey conducted in the UK, 37 deaths out of 1,367 cases of sickle cell disease were reported; 25 of the deaths occurred in children under the age of 16, and 14 of these deaths were sudden. In a study conducted in North America, 49 out of 422 patients with sickle cell disease died before they reached the age of 10. Lung infections were one of the most common causes of death in these patients. The National Cooperative Study of Sickle Cell Disease in the US predicted that 89 percent of the patients with sickle cell disease will survive to the age of 20. The majority of the deaths reported in this study were caused by infections and occurred within the first three years of life. To determine the incidence of and factors associated with mortality from sickle cell disease in the UK, the medical records of 384 patients with sickle cell disease, who were listed in the Brent sickle cell disease register, were reviewed. Between 1974 and 1989, 18 (5 percent) of the patients died. Five of the patients were less 16 years of age at the time of death. Twelve of the 18 deaths were caused by lung problems, and 10 of the deaths occurred suddenly. It is concluded that early diagnosis of the disease and identifying the causes of death that can be prevented, such as lung infection, are the most likely methods of reducing mortality from sickle cell disease. (Consumer Summary produced by Reliance Medical Information, Inc.)

Published
1991

41. e-Learning in Higher Institutions and Secondary Schools during Covid-19: Crisis Solving and Future Perspectives

Author

Brozović Mateja, Ercegović Marina, and Meeh-Bunse Gunther

Subjects
e-learning, digital tools, covid-19 pandemic, e-exams, university, high school, a20, i21, i23, 033, Business, HF5001-6182
Abstract

Background: The pandemic of Covid-19 brought significant changes to the education system and forcibly accelerated the process of digitizing teaching. Students and educators had to adapt to the new way of education, facing challenges such as technical problems and a lack of technical skills and social contact.

Published
2022
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42. HYPERTENSION AND CARDIOVASCULAR RISK FACTORS IN CROATIA. DATA FROM THE 2017. WORLD HYPERTENSION DAY

Author

Milicic, B., primary, Dapic, K., additional, Domislovic, V., additional, Brozovic, M., additional, Drenjancevic, I., additional, Dobrincic, Z., additional, Gulin, M., additional, Cavrak, V. Herceg, additional, Josipovic, J., additional, Jelakovic, A., additional, Kolar, L., additional, Leko, N., additional, Pavlovic, D., additional, Prkacin, I., additional, Radic, J., additional, Stevanovic, R., additional, Stupin, A., additional, Brinar, I. Vukovic, additional, Vrkic, T. Zeljkovic, additional, and Jelakovic, B., additional

Published
2018
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43. HIGH PREVALENCE OF SUBJECTS WITH HIGH CARDIOVASCULAR RISK IN COMMUNITY PHARMACIES – HIC RHODUS. HIC SALTO. PHYSICIAN-PHARMACIST COLLABORATIVE PROJECT OF THE CROATIAN SOCIETY OF HYP

Author

Jelakovic, A., primary, Brozovic, M., additional, Dobrincic, Z., additional, Domislovic, V., additional, Djapic, K., additional, Lugovic, N., additional, Mrsic, M., additional, Radovcic, M., additional, Skopic, O. Velkovski, additional, and Jelakovic, B., additional

Published
2018
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48. Double diffraction dissociation at the Fermilab Tevatron collider

Author

Affolder, T., Akimoto, H., Akopian, A., Albrow, M. G., Amaral, P., Amidei, D., Anikeev, K., Antos, J., Apollinari, G., Arisawa, T., Asakawa, T., Ashmanskas, W., Azfar, F., Azzi-Bacchetta, P., Bacchetta, N., Bailey, M. W., Bailey, S., De Barbaro, P., Barbaro-Galtieri, A., Barnes, V. E., Barnett, B. A., Baroiant, S., Barone, M., Bauer, G., Bedeschi, F., Belforte, S., Bell, W. H., Bellettini, G., Bellinger, J., Benjamin, D., Bensinger, J., Beretvas, Andrew, Berge, J. P., Berryhill, J., Bhatti, A., Binkley, M., Bisello, D., Bishai, M., Blair, R. E., Blocker, C., Bloom, K., Blumenfeld, B., Blusk, S. R., Bocci, A., Bodek, A., Bokhari, W., Bolla, G., Bonushkin, Yu Ye, Borras, K., Bortoletto, D., Boudreau, J., Brandl, A., Van Den Brink, S., Bromberg, C., Brozovic, M., Bruner, N., Buckley-Geer, E., Budagov, J., Budd, H. S., Burkett, K., Busetto, G., Byon-Wagner, A., Byrum, K. L., Cabrera, S., Calafiura, P., Campbell, M., Carithers, W., Carlson, J., Carlsmith, D., Caskey, W., Castro, A., Cauz, D., Cerri, A., Chan, A. W., Chang, P. S., Chang, P. T., Chapman, J., Chen, C., Chen, Y. C., Cheng, M. -T, Chertok, M., Chiarelli, G., Chirikov-Zorin, I., Chlachidze, G., Chlebana, F., Christofek, L., Chu, M. L., Chung, Y. S., Ciobanu, C. I., Clark, A. G., Connolly, A., Convery, M., Conway, J., Cordelli, M., Cranshaw, J., Cropp, R., Culbertson, R., Dagenhart, D., D'Auria, S., DeJongh, F., Dell'Agnello, Simone, Dell'Orso, M., Demortier, L., Deninno, M., Derwent, P. F., Devlin, T., Dittmann, J. R., Dominguez, A., Donati, S., Done, J., D'Onofrio, M., Dorigo, T., Eddy, N., Einsweiler, K., Elias, John E., Engels Jr., E., Erbacher, R., Errede, D., Errede, S., Fan, Q., Feild, R. G., Fernandez, J. P., Ferretti, C., Field, R. D., Fiori, I., Flaugher, B., Foster, G. W., Franklin, M., Freeman, J., Friedman, J., Fukui, Y., Furic, I., Galeotti, S., Gallas, A., Gallinaro, M., Gao, T., Garcia-Sciveres, M., Garfinkel, A. F., Gatti, P., Gay, C., Gerdes, D. W., Giannetti, P., Glagolev, V., Glenzinski, D., Gold, M., Goldstein, J., Gorelov, I., Goshaw, A. T., Gotra, Y., Goulianos, Konstantin, Green, C., Grim, G., Gris, P., Groer, L., Grosso-Pilcher, C., Guenther, M., Guillian, G., Guimaraes Da Costa, J., Haas, R. M., Haber, C., Hahn, S. R., Hall, C., Handa, T., Handler, R., Hao, W., Happacher, F., Hara, K., Hardman, A. D., Harris, R. M., Hartmann, F., Hatakeyama, K., Hauser, J., Heinrich, J., Heiss, A., Herndon, M., Hill, C., Hoffman, K. D., Holck, C., Hollebeek, R., Holloway, L., Hughes, R., Huston, J., Huth, J., Ikeda, H., Incandela, J., Introzzi, G., Iwai, J., Iwata, Y., James, E., Jones, M., Joshi, U., Kambara, H., Kamon, T., Kaneko, T., Karr, K., Kasha, H., Kato, Y., Keaffaber, T. A., Kelley, K., Kelly, M., Kennedy, R. D., Kephart, R., Khazins, D., Kikuchi, T., Kilminster, B., Kim, B. J., Kim, D. H., Kim, H. S., Kim, M. J., Kim, S. B., Kim, S. H., Kim, Y. K., Kirby, M., Kirk, M., Kirsch, L., Klimenko, S., Koehn, P., Kondo, K., Konigsberg, J., Korn, A., Korytov, A., Kovács, Eve V., Kroll, J., Kruse, M., Kuhlmann, S. E., Kurino, K., Kuwabara, T., Laasanen, A. T., Lai, N., Lami, S., Lammel, S., Lancaster, J., Lancaster, M., Lander, R., Latino, G., LeCompte, T., Lee IV, A. M., Lee, K., Leone, S., Lewis, J. D., Lindgren, M., Liss, T. M., Liu, J. B., Liu, Y. C., Litvintsev, D. O., Lobban, O., Lockyer, N., Loken, J., Loreti, M., Lucchesi, D., Lukens, P., Lusin, S., Lyons, L., Lys, J., Madrak, R., Maeshima, K., Maksimovic, P., Malferrari, L., Mangano, M., Mariotti, M., Martignon, G., Martin, A., Matthews, J. A. J., Mayer, J., Mazzanti, P., McFarland, K. S., McIntyre, P., McKigney, E., Menguzzato, M., Menzione, A., Mesropian, C., Meyer, A., Miao, T., Miller, R., Miller, J. S., Minato, H., Miscetti, S., Mishina, M., Mitselmakher, G., Moggi, N., Moore, E., Moore, R., Morita, Y., Moulik, T., Mulhearn, M., Mukherjee, A., Muller, T., Munar, A., Murat, P., Murgia, S., Nachtman, J., Nagaslaev, V., Nahn, S., Nakada, H., Nakano, I., Nelson, C., Nelson, T., Neu, C., Neuberger, D., Newman-Holmes, C., Ngan, C. -Y P., Niu, H., Nodulman, L., Nomerotski, A., Oh, S. H., Oh, Y. D., Ohmoto, T., Ohsugi, T., Oishi, R., Okusawa, T., Olsen, J., Orejudos, W., Pagliarone, C., Palmonari, F., Paoletti, R., Papadimitriou, Vaia, Partos, D., Patrick, J., Pauletta, G., Paulini, M., Paus, C., Pescara, L., Phillips, T. J., Piacentino, G., Pitts, K. T., Pompos, A., Pondrom, L., Pope, G., Popovic, M., Prokoshin, F., Proudfoot, J., Ptohos, Fotios, Pukhov, O., Punzi, G., Rakitine, A., Reher, D., Reichold, A., Ribon, A., Riegler, W., Rimondi, F., Ristori, L., Riveline, M., Robertson, W. J., Robinson, A., Rodrigo, T., Rolli, S., Rosenson, L., Roser, R., Rossin, R., Roy, A., Ruiz, A., Safonov, A., St. Denis, R., Sakumoto, W. K., Saltzberg, D., Sanchez, C., Sansoni, A., Santi, L., Sato, H., Savard, P., Schlabach, P., Schmidt, E. E., Schmidt, M. P., Schmitt, M., Scodellaro, L., Scott, A., Scribano, A., Segler, S., Seidel, S., Seiya, Y., Semenov, A., Semeria, F., Shah, T., Shapiro, M. D., Shepard, P. F., Shibayama, T., Shimojima, M., Shochet, M., Sidoti, A., Siegrist, J., Sill, A., Sinervo, P., Singh, P., Slaughter, A. J., Sliwa, K., Smith, C., Snider, F. D., Solodsky, A., Spalding, J., Speer, T., Sphicas, Paris A., Spinella, F., Spiropulu, Maria, Spiegel, L., Steele, J., Stefanini, A., Strologas, John, Strumia, F., Stuart, D., Sumorok, K., Suzuki, T., Takano, T., Takashima, R., Takikawa, K., Tamburello, P., Tanaka, M., Tannenbaum, B., Tecchio, M., Tesarek, R., Teng, P. K., Terashi, K., Tether, S., Thompson, A. S., Thurman-Keup, R., Tipton, P., Tkaczyk, S., Toback, D., Tollefson, K., Tollestrup, A., Tonelli, D., Toyoda, H., Trischuk, W., de Trocóniz, J. F., Tseng, J., Turini, N., Ukegawa, F., Vaiciulis, T., Valls, J., Vejcik III, S., Velev, G., Vidal, R., Vila, I., Vilar, R., Volobouev, I., Vucinic, D., Wagner, R. G., Wagner, R. L., Wallace, N. B., Wang, C., Wang, M. J., Ward, B., Waschke, S., Watanabe, T., Waters, D., Watts, T., Webb, R., Wenzel, H., Wester III, W. C., Wicklund, A. B., Wicklund, E., Wilkes, T., Williams, H. H., Wilson, P., Winer, B. L., Winn, D., Wolbers, S., Wolinski, D., Wolinski, J., Wolinski, S., Worm, S., Wu, X., Wyss, J., Yagil, A., Yao, W., Yeh, G. P., Yeh, P., Yoh, J., Yosef, C., Yoshida, T., Yu, I., Yu, S., Yu, Z., Zanetti, A., Zetti, F., Zucchelli, S., Clark, Allan Geoffrey, Kambara, Hisanori, Speer, Thomas, Strumia Michelini, Federica, Wu, Xin, and Ptohos, Fotios [0000-0002-3432-3452]

Subjects
Diffraction, Particle physics, Tevatron, HADRONIC DIFFRACTION, POMERON, General Physics and Astronomy, FOS: Physical sciences, ddc:500.2, Central region, Dissociation (chemistry), High Energy Physics - Experiment, Nuclear physics, Pomeron, Physics and Astronomy (all), High Energy Physics - Experiment (hep-ex), Factorization, Colliding beam accelerators, Quantum number, Double diffraction dissociation, Electron energy levels, Fermilab, High energy physics, Nuclear Experiment, QC, Physics, Pseudorapidity gap, Elementary particles, Monte Carlo methods, Computer simulation, Pseudorapidity, Quantum theory, Hadron, High Energy Physics::Experiment, Protons, Fermilab tevatron collider, Regge theory
Abstract

We present results from a measurement of double diffraction dissociation in $\bar pp$ collisions at the Fermilab Tevatron collider. The production cross section for events with a central pseudorapidity gap of width $\Delta\eta^0>3$ (overlapping $\eta=0$) is found to be $4.43\pm 0.02{(stat)}{\pm 1.18}{(syst) mb}$ [$3.42\pm 0.01{(stat)}{\pm 1.09}{(syst) mb}$] at $\sqrt{s}=1800$ [630] GeV. Our results are compared with previous measurements and with predictions based on Regge theory and factorization., Comment: 10 pages, 4 figures, using RevTeX. Submitted to Physical Review Letters

Published
2016

49. The Pluto system: Initial results from its exploration by New Horizons

Author

Stern, S. A., primary, Bagenal, F., additional, Ennico, K., additional, Gladstone, G. R., additional, Grundy, W. M., additional, McKinnon, W. B., additional, Moore, J. M., additional, Olkin, C. B., additional, Spencer, J. R., additional, Weaver, H. A., additional, Young, L. A., additional, Andert, T., additional, Andrews, J., additional, Banks, M., additional, Bauer, B., additional, Bauman, J., additional, Barnouin, O. S., additional, Bedini, P., additional, Beisser, K., additional, Beyer, R. A., additional, Bhaskaran, S., additional, Binzel, R. P., additional, Birath, E., additional, Bird, M., additional, Bogan, D. J., additional, Bowman, A., additional, Bray, V. J., additional, Brozovic, M., additional, Bryan, C., additional, Buckley, M. R., additional, Buie, M. W., additional, Buratti, B. J., additional, Bushman, S. S., additional, Calloway, A., additional, Carcich, B., additional, Cheng, A. F., additional, Conard, S., additional, Conrad, C. A., additional, Cook, J. C., additional, Cruikshank, D. P., additional, Custodio, O. S., additional, Dalle Ore, C. M., additional, Deboy, C., additional, Dischner, Z. J. B., additional, Dumont, P., additional, Earle, A. M., additional, Elliott, H. A., additional, Ercol, J., additional, Ernst, C. M., additional, Finley, T., additional, Flanigan, S. H., additional, Fountain, G., additional, Freeze, M. J., additional, Greathouse, T., additional, Green, J. L., additional, Guo, Y., additional, Hahn, M., additional, Hamilton, D. P., additional, Hamilton, S. A., additional, Hanley, J., additional, Harch, A., additional, Hart, H. M., additional, Hersman, C. B., additional, Hill, A., additional, Hill, M. E., additional, Hinson, D. P., additional, Holdridge, M. E., additional, Horanyi, M., additional, Howard, A. D., additional, Howett, C. J. A., additional, Jackman, C., additional, Jacobson, R. A., additional, Jennings, D. E., additional, Kammer, J. A., additional, Kang, H. K., additional, Kaufmann, D. E., additional, Kollmann, P., additional, Krimigis, S. M., additional, Kusnierkiewicz, D., additional, Lauer, T. R., additional, Lee, J. E., additional, Lindstrom, K. L., additional, Linscott, I. R., additional, Lisse, C. M., additional, Lunsford, A. W., additional, Mallder, V. A., additional, Martin, N., additional, McComas, D. J., additional, McNutt, R. L., additional, Mehoke, D., additional, Mehoke, T., additional, Melin, E. D., additional, Mutchler, M., additional, Nelson, D., additional, Nimmo, F., additional, Nunez, J. I., additional, Ocampo, A., additional, Owen, W. M., additional, Paetzold, M., additional, Page, B., additional, Parker, A. H., additional, Parker, J. W., additional, Pelletier, F., additional, Peterson, J., additional, Pinkine, N., additional, Piquette, M., additional, Porter, S. B., additional, Protopapa, S., additional, Redfern, J., additional, Reitsema, H. J., additional, Reuter, D. C., additional, Roberts, J. H., additional, Robbins, S. J., additional, Rogers, G., additional, Rose, D., additional, Runyon, K., additional, Retherford, K. D., additional, Ryschkewitsch, M. G., additional, Schenk, P., additional, Schindhelm, E., additional, Sepan, B., additional, Showalter, M. R., additional, Singer, K. N., additional, Soluri, M., additional, Stanbridge, D., additional, Steffl, A. J., additional, Strobel, D. F., additional, Stryk, T., additional, Summers, M. E., additional, Szalay, J. R., additional, Tapley, M., additional, Taylor, A., additional, Taylor, H., additional, Throop, H. B., additional, Tsang, C. C. C., additional, Tyler, G. L., additional, Umurhan, O. M., additional, Verbiscer, A. J., additional, Versteeg, M. H., additional, Vincent, M., additional, Webbert, R., additional, Weidner, S., additional, Weigle, G. E., additional, White, O. L., additional, Whittenburg, K., additional, Williams, B. G., additional, Williams, K., additional, Williams, S., additional, Woods, W. W., additional, Zangari, A. M., additional, and Zirnstein, E., additional

Published
2015
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50. Measurement of prompt charm meson production cross sections in p(p)over-bar collisions at root s=1.96 TeV RID C-1693-2008 RID G-1087-2011 RID E-4473-2011

Author

Acosta D, Affolder T, Ahn MH, Akimoto T, Albrow MG, Ambrose D, Amidei D, Anastassov A, Anikeev K, Annovi A, Antos J, Aoki M, Apollinari G, Arguin JF, Arisawa T, Artikov A, Asakawa T, Ashmanskas W, Attal A, Azfar F, Azzi Bacchetta P, Bacchetta N, Bachacou H, Badgett W, Bailey S, Barbaro Galtieri A, Barker G, Barnes VE, Barnett BA, Baroiant S, Barone M, Bauer G, Bedeschi F, Behari S, Belforte S, Bell WH, Bellettini G, Bellinger J, Benjamin D, Beretvas A, Bhatti A, Binkley M, Bisello D, Bishai M, Blair RE, Blocker C, Bloom K, Blumenfeld B, Bocci A, Bodek A, Bolla G, Bolshov A, Booth PSL, Bortoletto D, Boudreau J, Bourov S, Bromberg C, Brozovic M, Brubaker E, Budagov J, Budd HS, Burkett K, Busetto G, Bussey P, Byrum KL, Cabrera S, Calafiura P, Campanelli M, Campbell M, Canepa A, Carlsmith D, Carron S, Carosi R, Casarsa M, Caskey W, Castro A, Catastini P, Cauz D, Cerri A, Cerri C, Cerrito L, Chapman J, Chen C, Chen YC, Chertok M, Chiarelli G, Chlachidze G, Chlebana F, Cho K, Chokheli D, Chu ML, Chung JY, Chung WH, Chung YS, Ciobanu CI, Ciocci MA, Clark AG, Coca MN, Connolly A, Convery ME, Conway J, Cordelli M, Cortiana G, Cranshaw J, Culbertson R, Currat C, Cyr D, Dagenhart D, DaRonco S, D'Auria S, de Barbaro P, De Cecco S, Dell'Agnello S, Dell'Orso M, Demers S, Demortier L, Deninno M, De Pedis D, Derwent PF, Dionisi C, Dittmann JR, Doksus P, Dominguez A, Donati S, D'Onofrio M, Dorigo T, Drollinger V, Ebina K, Eddy N, Ely R, Erbacher R, Erdmann M, Errede D, Errede S, Eusebi R, Fang HC, Farrington S, Fedorko I, Feild RG, Feindt M, Fernandez JP, Ferretti C, Field RD, Fiori I, Flanagan G, Flaugher B, Flores Castillo LR, Foland A, Forrester S, Foster GW, Franklin M, Frisch H, Fujii Y, Furic I, Gallas A, Gallinaro M, Galyardt J, Garcia Sciveres M, Garfinkel AF, Gay C, Gerberich H, Gerchtein E, Gerdes DW, Giagu S, Giannetti P, Gibson A, Gibson K, Ginsburg C, Giolo K, Giordani M, Giurgiu G, Glagolev V, Glenzinski D, Gold M, Goldschmidt N, Goldstein D, Goldstein J, Gomez G, Gomez Ceballos G, Goncharov M, Gorelov I, Goshaw AT, Gotra Y, Goulianos K, Gresele A, Grim G, Grosso Pilcher C, Guenther M, da Costa JG, Haber C, Hahn K, Hahn SR, Halkiadakis E, Hall C, Handler R, Happacher F, Hara K, Hare M, Harr RF, Harris RM, Hartmann F, Hatakeyama K, Hauser J, Hays C, Heider E, Heinemann B, Heinrich J, Hennecke M, Herndon M, Hill C, Hirschbuehl D, Hocker A, Hoffman KD, Holloway A, Hou S, Houlden MA, Huffman BT, Hughes RE, Huston J, Ikado K, Incandela J, Introzzi G, Iori M, Ishizawa Y, Issever C, Ivanov A, Iwata Y, Iyutin B, James E, Jang D, Jarrell J, Jeans D, Jensen H, Jones M, Jun SY, Junk T, Kamon T, Kang J, Unel MK, Karchin PE, Kartal S, Kato Y, Kemp Y, Kephart R, Kerzel U, Khazins D, Khotilovich V, Kilminster B, Kim BJ, Kim DH, Kim HS, Kim JE, Kim MJ, Kim MS, Kim SB, Kim SH, Kim TH, Kim YK, King BT, Kirby M, Kirk M, Kirsch L, Klimenko S, Knuteson B, Kobayashi H, Koehn P, Kondo K, Konigsberg J, Kordas K, Korn A, Korytov A, Kotelnikov K, Kotwal AV, Kovalev A, Kraus J, Kravchenko I, Kreymer A, Kroll J, Kruse M, Krutelyov V, Kuhlmann SE, Kuznetsova N, Laasanen AT, Lai S, Lami S, Lammel S, Lancaster J, Lancaster M, Lander R, Lannon K, Lath A, Latino G, Lauhakangas R, Lazzizzera I, Le Y, Lecci C, LeCompte T, Lee J, Lee SW, Leonardo N, Leone S, Lewis JD, Li K, Lin CS, Lindgren M, Liss TM, Litvintsev DO, Liu T, Liu Y, Lockyer NS, Loginov A, Loken J, Loreti M, Loverre P, Lucchesi D, Lukens P, Lyons L, Lys J, MacQueen D, Madrak R, Maeshima K, Maksimovic P, Malferrari L, Manca G, Marginean R, Martin A, Martin M, Martin V, Martinez M, Maruyama T, Matsunaga H, Mattson M, Mazzanti P, McFarland KS, McGivern D, McIntyre PM, McNamara P, McNulty R, Menzemer S, Menzione A, Merkel P, Mesropian C, Messina A, Meyer A, Miao T, Miller L, Miller R, Miller JS, Miquel R, Miscetti S, Mishina M, Mitselmakher G, Miyamoto A, Miyazaki Y, Moggi N, Moore R, Moulik T, Mukherjee A, Mulhearn M, Muller T, Mumford R, Munar A, Murat P, Murgia S, Nachtman J, Nahn S, Nakamura I, Nakano I, Napier A, Napora R, Necula V, Niell F, Nielsen J, Nelson C, Nelson T, Neu C, Neubauer MS, Newman Holmes C, Nicollerat AS, Nigmanov T, Niu H, Nodulman L, Oesterberg K, Ogawa T, Oh S, Oh YD, Ohsugi T, Oishi R, Okusawa T, Oldeman R, Orava R, Orejudos W, Pagliarone C, Palmonari F, Paoletti R, Papadimitriou V, Partos D, Pashapour S, Patrick J, Pauletta G, Paulini M, Pauly T, Paus C, Pellett D, Penzo A, Phillips TJ, Piacentino G, Piedra J, Pitts KT, Pompos A, Pondrom L, Pope G, Poukhov O, Prakoshyn F, Pratt T, Pronko A, Proudfoot J, Ptohos F, Punzi G, Rademacker J, Rakitine A, Rappoccio S, Ratnikov F, Ray H, Reichold A, Rekovic V, Renton P, Rescigno M, Rimondi F, Rinnert K, Ristori L, Riveline M, Robertson WJ, Robson A, Rodrigo T, Rolli S, Rosenson L, Roser R, Rossin R, Rott C, Russ J, Ruiz A, Ryan D, Saarikko H, Safonov A, St Denis R, Sakumoto WK, Saltzberg D, Sanchez C, Sansoni A, Santi L, Sarkar S, Sato K, Savard P, Savoy Navarro A, Schemitz P, Schlabach P, Schmidt EE, Schmidt MP, Schmitt 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Subjects
High Energy Physics::Phenomenology, High Energy Physics::Experiment, Nuclear Experiment
Abstract

We report on measurements of differential cross sections dsigma/dp(T) for prompt charm meson production in p (p) over bar collisions at roots=1.96 TeV using 5.8+/-0.3 pb(-1) of data from the CDF II detector at the Fermilab Tevatron. The data are collected with a new trigger that is sensitive to the long lifetime of hadrons containing heavy flavor. The charm meson cross sections are measured in the central rapidity region \y\less than or equal to1 in four fully reconstructed decay modes: D(0)-->K(-)pi(+), D(*+)-->D(0)pi(+), D(+)-->K(-)pi(+)pi(+), D(s)(+)-->phipi(+), and their charge conjugates. The measured cross sections are compared to theoretical calculations.

Published
2003

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