Search

Your search keyword '"Carter, AL"' showing total 297 results
Start Over Author "Carter, AL"
297 results on '"Carter, AL"'

1. The JWST Early-release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 μm Spectrum of the Planetary-mass Companion VHS 1256-1257 b

Author

Miles, BE, Biller, BA, Patapis, P, Worthen, K, Rickman, E, Hoch, KKW, Skemer, A, Perrin, MD, Whiteford, N, Chen, CH, Sargent, B, Mukherjee, S, Morley, CV, Moran, SE, Bonnefoy, M, Petrus, S, Carter, AL, Choquet, E, Hinkley, S, Ward-Duong, K, Leisenring, JM, Millar-Blanchaer, MA, Pueyo, L, Ray, S, Sallum, S, Stapelfeldt, KR, Stone, JM, Wang, JJ, Absil, O, Balmer, WO, Boccaletti, A, Bonavita, M, Booth, M, Bowler, BP, Chauvin, G, Christiaens, V, Currie, T, Danielski, C, Fortney, JJ, Girard, JH, Grady, CA, Greenbaum, AZ, Henning, T, Hines, DC, Janson, M, Kalas, P, Kammerer, J, Kennedy, GM, Kenworthy, MA, Kervella, P, Lagage, PO, Lew, BWP, Liu, MC, Macintosh, B, Marino, S, Marley, MS, Marois, C, Matthews, EC, Matthews, BC, Mawet, D, McElwain, MW, Metchev, S, Meyer, MR, Molliere, P, Pantin, E, Quirrenbach, A, Rebollido, I, Ren, BB, Schneider, G, Vasist, M, Wyatt, MC, Zhou, Y, Briesemeister, ZW, Bryan, ML, Calissendorff, P, Cantalloube, F, Cugno, G, De Furio, M, Dupuy, TJ, Factor, SM, Faherty, JK, Fitzgerald, MP, Franson, K, Gonzales, EC, Hood, CE, Howe, AR, Kraus, AL, Kuzuhara, M, Lagrange, AM, Lawson, K, Lazzoni, C, Liu, P, Llop-Sayson, J, Lloyd, JP, Martinez, RA, Mazoyer, J, Quanz, SP, Redai, JA, Samland, M, Schlieder, JE, Miles, BE [0000-0002-5500-4602], Biller, BA [0000-0003-4614-7035], Patapis, P [0000-0001-8718-3732], Worthen, K [0000-0002-5885-5779], Rickman, E [0000-0003-4203-9715], Hoch, KKW [0000-0002-9803-8255], Skemer, A [0000-0001-6098-3924], Perrin, MD [0000-0002-3191-8151], Whiteford, N [0000-0001-8818-1544], Chen, CH [0000-0002-8382-0447], Sargent, B [0000-0001-9855-8261], Mukherjee, S [0000-0003-1622-1302], Morley, CV [0000-0002-4404-0456], Moran, SE [0000-0002-6721-3284], Bonnefoy, M [0000-0001-5579-5339], Petrus, S [0000-0003-0331-3654], Carter, AL [0000-0001-5365-4815], Choquet, E [0000-0002-9173-0740], Hinkley, S [0000-0001-8074-2562], Ward-Duong, K [0000-0002-4479-8291], Leisenring, JM [0000-0002-0834-6140], Millar-Blanchaer, MA [0000-0001-6205-9233], Ray, S [0000-0003-2259-3911], Sallum, S [0000-0001-6871-6775], Stapelfeldt, KR [0000-0002-2805-7338], Stone, JM [0000-0003-0454-3718], Wang, JJ [0000-0003-0774-6502], Absil, O [0000-0002-4006-6237], Balmer, WO [0000-0001-6396-8439], Boccaletti, A [0000-0001-9353-2724], Bonavita, M [0000-0002-7520-8389], Booth, M [0000-0001-8568-6336], Bowler, BP [0000-0003-2649-2288], Chauvin, G [0000-0003-4022-8598], Christiaens, V [0000-0002-0101-8814], Currie, T [0000-0002-7405-3119], Danielski, C [0000-0002-3729-2663], Fortney, JJ [0000-0002-9843-4354], Girard, JH [0000-0001-8627-0404], Greenbaum, AZ [0000-0002-7162-8036], Henning, T [0000-0002-1493-300X], Hines, DC [0000-0003-4653-6161], Janson, M [0000-0001-8345-593X], Kalas, P [0000-0002-6221-5360], Kammerer, J [0000-0003-2769-0438], Kennedy, GM [0000-0001-6831-7547], Kenworthy, MA [0000-0002-7064-8270], Kervella, P [0000-0003-0626-1749], Lew, BWP [0000-0003-1487-6452], Liu, MC [0000-0003-2232-7664], Macintosh, B [0000-0003-1212-7538], Marino, S [0000-0002-5352-2924], Marley, MS [0000-0002-5251-2943], Marois, C [0000-0002-4164-4182], Matthews, EC [0000-0003-0593-1560], Matthews, BC [0000-0003-3017-9577], Mawet, D [0000-0002-8895-4735], McElwain, MW [0000-0003-0241-8956], Metchev, S [0000-0003-3050-8203], Meyer, MR [0000-0003-1227-3084], Molliere, P [0000-0003-4096-7067], Pantin, E [0000-0001-6472-2844], Rebollido, I [0000-0002-4388-6417], Ren, BB [0000-0003-1698-9696], Schneider, G [0000-0002-4511-5966], Vasist, M [0000-0002-4511-3602], Wyatt, MC [0000-0001-9064-5598], Zhou, Y [0000-0003-2969-6040], Briesemeister, ZW [0000-0002-1764-2494], Bryan, ML [0000-0002-6076-5967], Calissendorff, P [0000-0002-5335-0616], Cantalloube, F [0000-0002-3968-3780], Cugno, G [0000-0001-7255-3251], De Furio, M [0000-0003-1863-4960], Dupuy, TJ [0000-0001-9823-1445], Factor, SM [0000-0002-8332-8516], Faherty, JK [0000-0001-6251-0573], Fitzgerald, MP [0000-0002-0176-8973], Franson, K [0000-0003-4557-414X], Gonzales, EC [0000-0003-4636-6676], Hood, CE [0000-0003-1150-7889], Howe, AR [0000-0002-4884-7150], Kraus, AL [0000-0001-9811-568X], Kuzuhara, M [0000-0002-4677-9182], Lawson, K [0000-0002-6964-8732], Lazzoni, C [0000-0001-7819-9003], Liu, P [0000-0001-7047-0874], Llop-Sayson, J [0000-0002-3414-784X], Martinez, RA [0000-0001-6301-896X], Mazoyer, J [0000-0002-9133-3091], Quanz, SP [0000-0003-3829-7412], Redai, JA [0000-0002-4489-3168], Samland, M [0000-0001-9992-4067], Schlieder, JE [0000-0001-5347-7062], and Apollo - University of Cambridge Repository

Subjects
The Solar System, Exoplanets, and Astrobiology, 5109 Space Sciences, 51 Physical Sciences
Abstract

We present the highest fidelity spectrum to date of a planetary-mass object. VHS 1256 b is a M Jup widely separated (∼8″, a = 150 au), young, planetary-mass companion that shares photometric colors and spectroscopic features with the directly imaged exoplanets HR 8799c, d, and e. As an L-to-T transition object, VHS 1256 b exists along the region of the color–magnitude diagram where substellar atmospheres transition from cloudy to clear. We observed VHS 1256 b with JWST's NIRSpec IFU and MIRI MRS modes for coverage from 1 to 20 μm at resolutions of ∼1000–3700. Water, methane, carbon monoxide, carbon dioxide, sodium, and potassium are observed in several portions of the JWST spectrum based on comparisons from template brown dwarf spectra, molecular opacities, and atmospheric models. The spectral shape of VHS 1256 b is influenced by disequilibrium chemistry and clouds. We directly detect silicate clouds, the first such detection reported for a planetary-mass companion.

Published
2023

3. Ground-based transmission spectroscopy with FORS2: A featureless optical transmission spectrum and detection of H2O for the ultra-hot Jupiter WASP-103b

Author

Wilson, J, Gibson, NP, Nikolov, N, Constantinou, S, Madhusudhan, N, Goyal, J, Barstow, JK, Carter, AL, De Mooij, EJW, Drummond, B, Mikal-Evans, T, Helling, C, Mayne, NJ, Sing, DK, Constantinou, Savvas [0000-0001-6839-4569], Nikku, Madhusudhan [0000-0002-4869-000X], and Apollo - University of Cambridge Repository

Subjects
stars: individual (WASP-103), Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Earth and Planetary Astrophysics, methods: data analysis, planetary systems, Astrophysics::Galaxy Astrophysics, techniques: spectroscopic
Abstract

We report ground-based transmission spectroscopy of the highly irradiated and ultra-short period hot-Jupiter WASP-103b covering the wavelength range $\approx$ 400-600 nm using the FORS2 instrument on the Very Large Telescope. The light curves show significant time-correlated noise which is mainly invariant in wavelength and which we model using a Gaussian process. The precision of our transmission spectrum is improved by applying a common-mode correction derived from the white light curve, reaching typical uncertainties in transit depth of $\approx$ 2x10$^{-4}$ in wavelength bins of 15 nm. After correction for flux contamination from a blended companion star, our observations reveal a featureless spectrum across the full range of the FORS2 observations and we are unable to confirm the Na absorption previously inferred using Gemini/GMOS or the strong Rayleigh scattering observed using broad-band light curves. We performed a Bayesian atmospheric retrieval on the full optical-infrared transmission spectrum using the additional data from Gemini/GMOS, HST/WFC3 and Spitzer observations and recover evidence for H$_2$O absorption at the 4.0$\sigma$ level. However, our observations are not able to completely rule out the presence of Na, which is found at 2.0$\sigma$ in our retrievals. This may in part be explained by patchy/inhomogeneous clouds or hazes damping any absorption features in our FORS2 spectrum, but an inherently small scale height also makes this feature challenging to probe from the ground. Our results nonetheless demonstrate the continuing potential of ground-based observations for investigating exoplanet atmospheres and emphasise the need for the application of consistent and robust statistical techniques to low-resolution spectra in the presence of instrumental systematics.

Published
2020

5. The transiting exoplanet community early release science program for JWST

Author

Bean, JL, Stevenson, KB, Batalha, NM, Berta-Thompson, Z, Kreidberg, L, Crouzet, N, Benneke, B, Line, MR, Sing, DK, Wakeford, HR, Knutson, HA, Kempton, EMR, Désert, JM, Crossfield, I, Batalha, NE, De Wit, J, Parmentier, V, Harrington, J, Moses, JI, Lopez-Morales, M, Alam, MK, Blecic, J, Bruno, G, Carter, AL, Chapman, JW, Decin, L, Dragomir, D, Evans, TM, Fortney, JJ, Fraine, JD, Gao, P, Muñoz, AG, Gibson, NP, Goyal, JM, Heng, K, Hu, R, Kendrew, S, Kilpatrick, BM, Krick, J, Lagage, PO, Lendl, M, Louden, T, Madhusudhan, N, Mandell, AM, Mansfield, M, May, EM, Morello, G, Morley, CV, Nikolov, N, Redfield, S, Roberts, JE, Schlawin, E, Spake, JJ, Todorov, KO, Tsiaras, A, Venot, O, Waalkes, WC, Wheatley, PJ, Zellem, RT, Angerhausen, D, Barrado, D, Carone, L, Casewell, SL, Cubillos, PE, Damiano, M, Borro, MDV, Drummond, B, Edwards, B, Endl, M, Espinoza, N, France, K, Gizis, JE, Greene, TP, Henning, TK, Hong, Y, Ingalls, JG, Iro, N, Irwin, PGJ, Kataria, T, Lahuis, F, Leconte, J, Lillo-Box, J, Lines, S, Lothringer, JD, Mancini, L, Marchis, F, Mayne, N, Palle, E, Rauscher, E, Roudier, G, Shkolnik, EL, Southworth, J, Swain, MR, Taylor, J, Teske, J, Tinetti, G, Tremblin, P, Tucker, GS, Boekel, RV, Waldmann, IP, Bean, JL [0000-0003-4733-6532], and Apollo - University of Cambridge Repository

Subjects
planets and satellites: atmospheres, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Earth and Planetary Astrophysics, methods: observational, planets and satellites: individual (WASP-79b, WASP-43b, WASP-18b)
Abstract

The James Webb Space Telescope (JWST) presents the opportunity to transform our understanding of planets and the origins of life by revealing the atmospheric compositions, structures, and dynamics of transiting exoplanets in unprecedented detail. However, the high-precision, time-series observations required for such investigations have unique technical challenges, and prior experience with other facilities indicates that there will be a steep learning curve when JWST becomes operational. In this paper we describe the science objectives and detailed plans of the Transiting Exoplanet Community Early Release Science (ERS) Program, which is a recently approved program for JWST observations early in Cycle 1. The goal of this project, for which the obtained data will have no exclusive access period, is to accelerate the acquisition and diffusion of technical expertise for transiting exoplanet observations with JWST, while also providing a compelling set of representative datasets that will enable immediate scientific breakthroughs. The Transiting Exoplanet Community ERS Program will exercise the time-series modes of all four JWST instruments that have been identified as the consensus highest priorities, observe the full suite of transiting planet characterization geometries (transits, eclipses, and phase curves), and target planets with host stars that span an illustrative range of brightnesses. The observations in this program were defined through an inclusive and transparent process that had participation from JWST instrument experts and international leaders in transiting exoplanet studies. Community engagement in the project will be centered on a two-phase Data Challenge that culminates with the delivery of planetary spectra, time-series instrument performance reports, and open-source data analysis toolkits in time to inform the agenda for Cycle 2 of the JWST mission.

Published
2018

7. Endnotes

Author

Carter, Albert Howard

Published
2016

8. Index

Author

Carter, Albert Howard

Published
2016

11. Bibliography

Author

Carter, Albert Howard

Published
2016

21. Figures

Author

Carter, Albert Howard

Published
2016

25. Geostatistical interpolation can reliably extend coverage of a very high-resolution model of temperature-dependent sex determination

Author

Carter, AL, Kearney, MR, Hartley, S, Porter, WP, Nelson, NJ, Carter, AL, Kearney, MR, Hartley, S, Porter, WP, and Nelson, NJ

Abstract

AIM: Recognition that statistical models do not always reliably predict habitat suitability under future climate scenarios is leading increasingly to explicit incorporation of the physiological constraints that underlie species’ distributions into spatially explicit predictions. However, computational intensity constrains the use of high‐resolution, process‐explicit models. We examined whether geostatistical analysis can effectively interpolate a biophysical model, reducing the computational investment typically required for using mechanistic methods to inform physiological predictions. LOCATION: New Zealand [40°40′00″ S 174°00′00″ E]. METHODS: We used a spatially explicit, mechanistic microclimate model to predict hourly temperatures at five soil depths under two scenarios of climate warming. Using the predicted soil temperatures as input to a biophysical model of temperature‐dependent embryonic development, we estimated incubation temperatures and corresponding hatchling sex ratios for tuatara, a reptile with temperature‐dependent sex determination, at a submetre horizontal spatial resolution. We then applied ordinary kriging, a robust method of geostatistical interpolation, to estimate predictions throughout the full extent of our study location, an additional 480,000+ microsites, and validated the interpolation against an independent set of predictions. RESULTS: Ordinary kriging accurately predicted spatial variability in incubation temperatures. Mean predictions were similar between methods, and error in the geospatial model generally decreased with increasing soil depth. Error was higher for the geospatial model of the ‘maximum warming’, compared with the ‘minimum warming’, scenario of climate change. MAIN CONCLUSIONS: Our results show that ordinary kriging can be a reliable method for interpolating variability in high‐resolution predictions. However, the effects of error on the accuracy of interpolated predictions will become more severe as values approach a

Published
2018

27. The Sudbury Neutrino Observatory

Author

Boger, J, Hahn, RL, Rowley, JK, Carter, AL, Hollebone, B, Kessler, D, Blevis, I, Dalnoki-Veress, F, DeKok, A, Farine, J, Grant, DR, Hargrove, CK, Laberge, G, Levine, I, McFarlane, K, Mes, H, Noble, AT, Novikov, VM, O'Neill, M, Shatkay, M, Shewchuk, C, Sinclair, D, Clifford, ETH, Deal, R, Earle, ED, Gaudette, E, Milton, G, Sur, B, Bigu, J, Cowan, JHM, Cluff, DL, Hallman, ED, Haq, RU, Hewett, J, Hykawy, JG, Jonkmans, G, Michaud, R, Roberge, A, Roberts, J, Saettler, E, Schwendener, MH, Seifert, H, Sweezey, D, Tafirout, R, Virtue, CJ, Beck, DN, Chan, YD, Chen, X, Dragowsky, MR, Dycus, FW, Gonzalez, J, Isaac, MCP, Kajiyama, Y, Koehler, GW, Lesko, KT, Moebus, MC, Norman, EB, Okada, CE, Poon, AWP, Purgalis, P, Schuelke, A, Smith, AR, Stokstad, RG, Turner, S, Zlimen, I, Anaya, JM, Bowles, TJ, Brice, SJ, Esch, EI, Fowler, MM, Goldschmidt, A, Hime, A, McGirt, AF, Miller, GG, Teasdale, WA, Wilhelmy, JB, Wouters, JM, Anglin, JD, Bercovitch, M, Davidson, WF, Storey, RS, Biller, S, Black, RA, Boardman, RJ, Bowler, MG, Cameron, J, Cleveland, B, Ferraris, AP, Doucas, G, Heron, H, Howard, C, Jelley, NA, Knox, AB, Lay, M, Locke, W, Lyon, J, Majerus, S, Moorhead, M, Omori, M, Tanner, NW, Taplin, RK, Thorman, M, Wark, DL, West, N, Barton, JC, Trent, PT, Kouzes, R, Lowry, MM, Bell, AL, Bonvin, E, Boulay, M, Dayon, M, Duncan, F, Erhardt, LS, Evans, HC, Ewan, GT, Ford, R, Hallin, A, Hamer, A, Hart, PM, Harvey, PJ, Haslip, D, Hearns, CAW, Heaton, R, Hepburn, JD, Jillings, CJ, Korpach, EP, Lee, HW, Leslie, JR, Liu, MQ, Mak, HB, McDonald, AB, MacArthur, JD, McLatchie, W, Moffat, BA, Noel, S, Radcliffe, TJ, Robertson, BC, Skensved, P, Stevenson, RL, Zhu, X, Gil, S, Heise, J, Helmer, RL, Komar, RJ, Nally, CW, Ng, HS, Waltham, CE, Allen, RC, Buhler, G, Chen, HH, Aardsma, G, Andersen, T, Cameron, K, Chon, MC, Hanson, RH, Jagam, P, Karn, J, Law, J, Ollerhead, RW, Simpson, JJ, Tagg, N, Wang, JX, Alexander, C, Beier, EW, Cook, JC, Cowen, DF, Frank, ED, Frati, W, Keener, PT, Klein, JR, Mayers, G, McDonald, DS, Neubauer, MS, Newcomer, FM, Pearce, RJ, Van de Water, RG, Van Berg, R, Wittich, P, Ahmad, QR, Beck, JM, Browne, MC, Burritt, TH, Doe, PJ, Duba, CA, Elliott, SR, Franklin, JE, Germani, JV, Green, P, Hamian, AA, Heeger, KM, Howe, M, Drees, RM, Myers, A, Robertson, RGH, Smith, MWE, Steiger, TD, Van Wechel, T, Wilkerson, JF, and Collaboration, SNO

Subjects
Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), 0103 physical sciences, Nuclear Experiment (nucl-ex), Nuclear Experiment, 010306 general physics, Neutrino oscillation, Instrumentation, Physics, Standard solar model, Sudbury Neutrino Observatory, 010308 nuclear & particles physics, Astrophysics (astro-ph), High Energy Physics::Phenomenology, Instrumentation and Detectors (physics.ins-det), High Energy Physics - Phenomenology, Neutrino detector, High Energy Physics::Experiment, Neutrino, Electron neutrino, Lepton
Abstract

The Sudbury Neutrino Observatory is a second generation water Cherenkov detector designed to determine whether the currently observed solar neutrino deficit is a result of neutrino oscillations. The detector is unique in its use of D2O as a detection medium, permitting it to make a solar model-independent test of the neutrino oscillation hypothesis by comparison of the charged- and neutral-current interaction rates. In this paper the physical properties, construction, and preliminary operation of the Sudbury Neutrino Observatory are described. Data and predicted operating parameters are provided whenever possible., 58 pages, 12 figures, submitted to Nucl. Inst. Meth. Uses elsart and epsf style files. For additional information about SNO see http://www.sno.phy.queensu.ca . This version has some new references

Published
2000

30. READERS RESPOND

Author

Carter, Al, Mcnew, William, Shores, David V., Hillegass, Chuck, Sowers, Charles, Schwartz, Jerry, and Ellicott, Tom

Subjects
General interest, News, opinion and commentary
Abstract

Portrayal was misleading The majority community is often puzzled by the seemingly unwarranted outcry among African-Americans regarding the manner in which we are presented in the media. Generally, our view [...]

Published
2003

33. No. 3 Oklahoma stays within a game of Kansas

Author

Carter, Al

Subjects
General interest, News, opinion and commentary
Abstract

Byline: Al Carter COLLEGE STATION, Texas _ Hanging by their fingertips in the Big 12 race, the Oklahoma Sooners turned to the best fingertips around on Saturday. Hollis Price, silky [...]

Published
2003

35. Texas A&M, Slocum miss bowl cut

Author

Carter, Al

Subjects
General interest, News, opinion and commentary
Abstract

Byline: Al Carter COLLEGE STATION, Texas _ The R.C. Slocum era at Texas A&M came to a quiet end Sunday when the Aggies were not included in a group of [...]

Published
2002

36. Examiner: Blood clot killed Texas A&M player

Author

Carter, Al

Subjects
General interest, News, opinion and commentary
Abstract

COLLEGE STATION, Texas _ Texas A&M freshman football player Brandon Fails died from a blood clot that formed as the result of an injury to his right leg, a spokesman [...]

Published
2002

37. Texans follow precise outline for building team from scratch

Author

Carter, Al

Subjects
General interest, News, opinion and commentary
Abstract

HOUSTON _ Three years ago, Charley Casserly presented Bob McNair, the founder and principal owner of Houston's NFL expansion franchise, with his resume, gleaned from nearly a quarter-century of deep [...]

Published
2002

38. `Next year' has never come for some tournament teams

Author

Carter, Al

Subjects
General interest, News, opinion and commentary, Williams College, NCAA
Abstract

No doubt the student reporter from the campus radio station at tiny Williams College sensed a big story. Maybe a once-in-a-lifetime story. Anyone's lifetime. It was 1955 and the faculty [...]

Published
2002

41. Rice's comeback shocks Baylor in regional final

Author

Carter, Al

Subjects
General interest, News, opinion and commentary
Abstract

HOUSTON _ Rice's comeback Monday wasn't as unbelievable as Baylor's resurrection rally two days earlier. But it was far more permanent. The top-seeded Owls squeezed three runs out of a [...]

Published
2001

42. Huskers, then all the rest in Big 12

Author

Carter, Al

Subjects
General interest, News, opinion and commentary, NCAA
Abstract

OKLAHOMA CITY _ Wednesday's opening rounds of the Big 12 baseball tournament weren't lacking for flavor to begin with. Now, thanks to the NCAA, the entire tournament is ripe with [...]

Published
2001

45. Aggies focus on UT, not bowl picture

Author

Carter, Al

Subjects
College sports, Football (College), General interest, News, opinion and commentary, Texas A&M University, University of Texas
Abstract

COLLEGE STATION, Texas _ R.C. Slocum has just one thing to say about Texas A&M's prospects of playing for the national championship. Enough said. The 10-1 Aggies could be just [...]

Published
1998

48. Football now in focus for A&M's freshman blur

Author

Carter, Al

Subjects
College sports, General interest, News, opinion and commentary, Texas A&M University -- Competitions
Abstract

SAN ANTONIO _ Toya Jones, the track prodigy from Refugio, never lost sight of his football dream. All he really lost sight of, when he arrived at Texas A&M last [...]

Published
1995

49. Arkansas wrecks Texas' Top 10 credentials

Author

Carter, Al

Abstract

Byline: Al Carter AUSTIN, Texas _ To what extent it was part of the ploy, the Arkansas Razorbacks wouldn't confess. Certainly there was a degree of self-deception at play when, […]

Published
2003

50. BCS schools, outsiders plan to meet again

Author

Carter, Al

Abstract

Byline: Al Carter The much-anticipated collision between Bowl Championship Series schools and reform-minded outsiders on Monday generated little more than pleasantries and a plan to meet again in two months. […]

Published
2003

Catalog

Books, media, physical & digital resources
See catalog results