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1. Strong-Field Gravity Tests with the Double Pulsar

Author: Kramer, M, Stairs, IH, Manchester, RN, Wex, N, Deller, AT, Coles, WA, Ali, M, Burgay, M, Camilo, F, Cognard, I, Damour, T, Desvignes, G, Ferdman, RD, Freire, PCC, Grondin, S, Guillemot, L, Hobbs, GB, Janssen, G, Karuppusamy, R, Lorimer, DR, Lyne, AG, McKee, JW, McLaughlin, M, Münch, LE, Perera, BBP, Pol, N, Possenti, A, Sarkissian, J, Stappers, BW, and Theureau, G
Subjects: Astronomical and Space Sciences, Condensed Matter Physics, Quantum Physics
Abstract: Continued timing observations of the double pulsar PSR J0737-3039A/B, which consists of two active radio pulsars (A and B) that orbit each other with a period of 2.45 h in a mildly eccentric (e=0.088) binary system, have led to large improvements in the measurement of relativistic effects in this system. With a 16-yr data span, the results enable precision tests of theories of gravity for strongly self-gravitating bodies and also reveal new relativistic effects that have been expected but are now observed for the first time. These include effects of light propagation in strong gravitational fields which are currently not testable by any other method. In particular, we observe the effects of retardation and aberrational light bending that allow determination of the spin direction of the pulsar. In total, we detect seven post-Keplerian parameters in this system, more than for any other known binary pulsar. For some of these effects, the measurement precision is now so high that for the first time we have to take higher-order contributions into account. These include the contribution of the A pulsar's effective mass loss (due to spin-down) to the observed orbital period decay, a relativistic deformation of the orbit, and the effects of the equation of state of superdense matter on the observed post-Keplerian parameters via relativistic spin-orbit coupling. We discuss the implications of our findings, including those for the moment of inertia of neutron stars, and present the currently most precise test of general relativity's quadrupolar description of gravitational waves, validating the prediction of general relativity at a level of 1.3×10-4 with 95% confidence. We demonstrate the utility of the double pulsar for tests of alternative theories of gravity by focusing on two specific examples and also discuss some implications of the observations for studies of the interstellar medium and models for the formation of the double pulsar system. Finally, we provide context to other types of related experiments and prospects for the future.
Published: 2021

2. INTERSTELLAR SCINTILLATION OF THE DOUBLE PULSAR J0737−3039

Author: Rickett, BJ, Coles, WA, Nava, CF, McLaughlin, MA, Ransom, SM, Camilo, F, Ferdman, RD, Freire, PCC, Kramer, M, Lyne, AG, and Stairs, IH
Subjects: binaries: general, ISM: general, pulsars: general, pulsars: individual, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract: We report a series of observations of the interstellar scintillation (ISS) of the double pulsar J0737-3039 over the course of 18 months. As in earlier work, the basic phenomenon is the variation in the ISS caused by the changing transverse velocities of each pulsar, the ionized interstellar medium (IISM), and the Earth. The transverse velocity of the binary system can be determined both by very long baseline interferometry and timing observations. The orbital velocity and inclination is almost completely determined from timing observations, but the direction of the orbital angular momentum is not known. Since the Earth's velocity is known, and can be compared with the orbital velocity by its effect on the timescale of the ISS, we can determine the orientation Ω of the pulsar orbit with respect to equatorial coordinates (Ω = 65 ± 2°). We also resolve the ambiguity (i = 88.°7 or 91.°3) in the inclination of the orbit deduced from the measured Shapiro delay by our estimate i = 88.°1 ± 0.°5. This relies on the analysis of the ISS over both frequency and time, and provides a model for the location, anisotropy, turbulence level, and transverse phase gradient of the IISM. We find that the IISM can be well-modeled during each observation, typically of a few orbital periods, but its turbulence level and mean velocity vary significantly over the 18 months. © 2014. The American Astronomical Society. All rights reserved.
Published: 2014

3. Collected papers on the biology of the skin and hair growth and other contributions

Author: Lyne, AG
Abstract: This collection of papers is the results, obtained since 1951, of research concerned mainly with the biology of the skin and hair growth. The other contributions deal mainly with the body growth and development of marsupials. None of the work has been submitted elsewhere for the degree of Doctor of Science. A large proportion of the research has been on sheep and marsupials. Particular attention is drawn to the usefulness of marsupials as experimental material in studies on the integument and body growth. The early birth in marsupials is a most desirable feature for many developmental studies, as development in a pouch, unlike development in the uterus, lends itself to both observation and experiment. Papers 1-10, 12, 14 and 46 were incorporated in a thesis for the degree of Ph.D. in the University of Tasmania (1958). I am responsible for one third of the work reported in three papers (21, 24, 49), half of the work reported in ten papers (4, 6, 8, 15, 18, 19, 31, 36, 38, 44), and at least half of the work reported in the other publications with two or more authors. Publications 11, 29, 47, 51, 53, 54 and 56 are essentially popular or review contributions. All other works report original research.
Published: 2023
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4. A thesis on the vibrissae and pelage hairs on the marsupialia and supporting papers

Author: Lyne, AG
Abstract: The thesis is divided into two parts; one on the systematic and adaptive significance of the vibrissae in the marsupials and the other on the development and replacement of pelage hairs in the bandicoot, Perameles nasuta. The supporting papers are on: (a) the external characters of five species of bandicoot, Iscodon obesulus, Perameles gunnii, Perameles eremiana, Macrotis lagotis and Chaeropus ecaudatus, (b) syndactyly in the manus of a marsupial, (c) bundles of primary wool follicles in sheep, and (d) the development of the epidermis and hair canals in the Merino sheep foetus.
Published: 2023
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5. Noise analysis in the European Pulsar Timing Array data release 2 and its implications on the gravitational-wave background search

Author: Chalumeau, A, Babak, S, Petiteau, A, Chen, S, Samajdar, A, Caballero, R, Theureau, G, Guillemot, L, Desvignes, G, Parthasarathy, A, Liu, K, Shaifullah, G, Hu, H, van der Wateren, E, Antoniadis, J, Bak Nielsen, A, Bassa, C, Berthereau, A, Burgay, M, Champion, D, Cognard, I, Falxa, M, Ferdman, R, Freire, P, Gair, J, Graikou, E, Guo, Y, Jang, J, Janssen, G, Karuppusamy, R, Keith, M, Kramer, M, Lee, K, Liu, X, Lyne, A, Main, R, Mckee, J, Mickaliger, M, Perera, B, Perrodin, D, Porayko, N, Possenti, A, Sanidas, S, Sesana, A, Speri, L, Stappers, B, Tiburzi, C, Vecchio, A, Verbiest, J, Wang, J, Wang, L, Xu, H, Caballero, RN, Bak Nielsen, A-S, Bassa, CG, Champion, DJ, Ferdman, RD, Freire, PCC, Gair, JR, Guo, YJ, Janssen, GH, Keith, MJ, Lee, KJ, Liu, XJ, Lyne, AG, Main, RA, McKee, JW, Mickaliger, MB, Perera, BBP, Porayko, NK, Sanidas, SA, Stappers, BW, Verbiest, JPW, Chalumeau, A, Babak, S, Petiteau, A, Chen, S, Samajdar, A, Caballero, R, Theureau, G, Guillemot, L, Desvignes, G, Parthasarathy, A, Liu, K, Shaifullah, G, Hu, H, van der Wateren, E, Antoniadis, J, Bak Nielsen, A, Bassa, C, Berthereau, A, Burgay, M, Champion, D, Cognard, I, Falxa, M, Ferdman, R, Freire, P, Gair, J, Graikou, E, Guo, Y, Jang, J, Janssen, G, Karuppusamy, R, Keith, M, Kramer, M, Lee, K, Liu, X, Lyne, A, Main, R, Mckee, J, Mickaliger, M, Perera, B, Perrodin, D, Porayko, N, Possenti, A, Sanidas, S, Sesana, A, Speri, L, Stappers, B, Tiburzi, C, Vecchio, A, Verbiest, J, Wang, J, Wang, L, Xu, H, Caballero, RN, Bak Nielsen, A-S, Bassa, CG, Champion, DJ, Ferdman, RD, Freire, PCC, Gair, JR, Guo, YJ, Janssen, GH, Keith, MJ, Lee, KJ, Liu, XJ, Lyne, AG, Main, RA, McKee, JW, Mickaliger, MB, Perera, BBP, Porayko, NK, Sanidas, SA, Stappers, BW, and Verbiest, JPW
Abstract: The European Pulsar Timing Array (EPTA) collaboration has recently released an extended data set for six pulsars (DR2) and reported evidence for a common red noise signal. Here we present a noise analysis for each of the six pulsars. We consider several types of noise: (i) radio frequency independent, 'achromatic', and time-correlated red noise; (ii) variations of dispersion measure and scattering; (iii) system and band noise; and (iv) deterministic signals (other than gravitational waves) that could be present in the PTA data. We perform Bayesian model selection to find the optimal combination of noise components for each pulsar. Using these custom models we revisit the presence of the common uncorrelated red noise signal previously reported in the EPTA DR2 and show that the data still supports it with a high statistical significance. Next, we confirm that there is no preference for or against the Hellings-Downs spatial correlations expected for the stochastic gravitational-wave background. The main conclusion of the EPTA DR2 paper remains unchanged despite a very significant change in the noise model of each pulsar. However, modelling the noise is essential for the robust detection of gravitational waves and its impact could be significant when analysing the next EPTA data release, which will include a larger number of pulsars and more precise measurements.
Published: 2022

6. A comparative analysis of pulse time-of-arrival creation methods

Author: Wang, J, Shaifullah, G, Verbiest, J, Tiburzi, C, Champion, D, Cognard, I, Gaikwad, M, Graikou, E, Guillemot, L, Hu, H, Karuppusamy, R, Keith, M, Kramer, M, Liu, Y, Lyne, A, Mickaliger, M, Stappers, B, Theureau, G, Shaifullah, GM, Verbiest, JPW, Champion, DJ, Keith, MJ, Lyne, AG, Mickaliger, MB, Stappers, BW, Wang, J, Shaifullah, G, Verbiest, J, Tiburzi, C, Champion, D, Cognard, I, Gaikwad, M, Graikou, E, Guillemot, L, Hu, H, Karuppusamy, R, Keith, M, Kramer, M, Liu, Y, Lyne, A, Mickaliger, M, Stappers, B, Theureau, G, Shaifullah, GM, Verbiest, JPW, Champion, DJ, Keith, MJ, Lyne, AG, Mickaliger, MB, and Stappers, BW
Abstract: Context. Extracting precise pulse times of arrival (TOAs) and their uncertainties is the first and most fundamental step in high-precision pulsar timing. In the classical method, TOAs are derived from total intensity pulse profiles of pulsars via cross-correlation with an idealised 1D template of that profile. While a number of results have been presented in the literature that rely on the ever increasing sensitivity of these pulsar timing experiments, there is no consensus on the most reliable methods for creating TOAs, and, more importantly, on the associated TOA uncertainties for each scheme. Aims. We present a comprehensive comparison of TOA determination practices. We focus on creating timing templates, TOA determination methods, and the most useful TOA bandwidth. The aim is to present a possible approach towards TOA optimisation, the (partial) identification of an optimal TOA-creation scheme, and the demonstration of optimisation differences between pulsars and data sets. Methods. We compared the values of data-derived template profiles with analytic profiles and evaluated the three most commonly used template-matching methods. Finally, we studied the relation between timing precision and TOA bandwidth to identify any potential breaks in this relation. As a practical demonstration, we applied our selected methods to European Pulsar Timing Array data on three test pulsars, PSRs J0218+4232, J1713+0747, and J2145-0750. Results. Our demonstration shows that data-derived and smoothed templates are typically preferred to some more commonly applied alternatives. The template-matching method called Fourier domain with Markov chain Monte Carlo is generally superior to or competitive with other methods. While the optimal TOA bandwidth is strongly dependent on pulsar brightness, telescope sensitivity, and scintillation properties, some significant frequency averaging seems required for the data we investigated.
Published: 2022

7. The first fermi large area telescope catalog of gamma-ray pulsars (vol 187, pg 460, 2010)

Author: Abdo, Aa, Ackermann, M, Ajello, M, Atwood, Wb, Axelsson, M, Baldini, L, Ballet, J, Barbiellini, G, Baring, Mg, Bastieri, D, Baughman, Bm, Bechtol, K, Bellazzini, R, Berenji, B, Blandford, Rd, Bloom, Ed, Bonamente, E, Borgland, Aw, Bregeon, J, Brez, A, Brigida, M, Bruel, P, Burnett, Th, Buson, S, Caliandro, Ga, Cameron, Ra, Camilo, F, Caraveo, Pa, Casandjian, Jm, Cecchi, C, Celik, O, Charles, E, Chekhtman, A, Cheung, Cc, Chiang, J, Ciprini, S, Claus, R, Cognard, I, Cohen Tanugi, J, Cominsky, Lr, Conrad, J, Corbet, R, Cutini, S, den Hartog PR, Dermer, Cd, DE ANGELIS, Alessandro, de Luca, A, de Palma, F, Digel, Sw, Dormody, M, Silva, Ede, Drell, Ps, Dubois, R, Dumora, D, Espinoza, C, Farnier, C, Favuzzi, C, Fegan, Sj, Ferrara, Ec, Focke, Wb, Fortin, P, Frailis, M, Freire, Pcc, Fukazawa, Y, Funk, S, Fusco, P, Gargano, F, Gasparrini, D, Gehrels, N, Germani, S, Giavitto, G, Giebels, B, Giglietto, N, Giommi, P, Giordano, F, Glanzman, T, Godfrey, G, Gotthelf, Ev, Grenier, Ia, Grondin, Mh, Grove, Je, Guillemot, L, Guiriec, S, Gwon, C, Hanabata, Y, Harding, Ak, Hayashida, M, Hays, E, Hughes, Re, Jackson, Ms, Johannesson, G, Johnson, As, Johnson, Rp, Johnson, Tj, Johnson, Wn, Johnston, S, Kamae, T, Kanbach, G, Kaspi, Vm, Katagiri, H, Kataoka, J, Kawai, N, Kerr, M, Knoedlseder, J, Kocian, Ml, Kramer, M, Kuss, M, Lande, J, Latronico, L, Lemoine Goumard, M, Livingstone, M, Longo, F, Loparco, F, Lott, B, Lovellette, Mn, Lubrano, P, Lyne, Ag, Madejski, Gm, Makeev, A, Manchester, Rn, Marelli, M, Mazziotta, Mn, Mcconville, W, Mcenery, Je, Mcglynn, S, Meurer, C, Michelson, Pf, Mineo, T, Mitthumsiri, W, Mizuno, T, Moiseev, Aa, Monte, C, Monzani, Me, Morselli, A, Moskalenko, Iv, Murgia, S, Nakamori, T, Nolan, Pl, Norris, Jp, Noutsos, A, Nuss, E, Ohsugi, T, Omodei, N, Orlando, E, Ormes, Jf, Ozaki, M, Paneque, D, Panetta, Jh, Parent, D, Pelassa, V, Pepe, M, Pesce Rollins, M, Piron, F, Porter, Ta, Raino, S, Rando, R, Ransom, Sm, Ray, Ps, Razzano, M, Rea, N, Reimer, A, Reimer, O, Reposeur, T, Ritz, S, Rodriguez, Ay, Romani, Rw, Roth, M, Ryde, F, Sadrozinski, Hfw, Sanchez, D, Sander, A, Parkinson, Pms, Scargle, Jd, Schalk, Tl, Sellerholm, A, Sgro, C, Siskind, Ej, Smith, Da, Smith, Pd, Spandre, G, Spinelli, P, Stappers, Bw, Starck, Jl, Striani, E, Strickman, Ms, Strong, Aw, Suson, Dj, Tajima, H, Takahashi, H, Takahashi, T, Tanaka, T, Thayer, Jb, Thayer, Jg, Theureau, G, Thompson, Dj, Thorsett, Se, Tibaldo, L, Tibolla, O, Torres, Df, Tosti, G, Tramacere, A, Uchiyama, Y, Usher, Tl, Van Etten, A, Vasileiou, V, Venter, C, Vilchez, N, Vitale, V, Waite, Ap, Wang, P, Wang, N, Watters, K, Weltevrede, P, Winer, Bl, Wood, Ks, Ylinen, T, Ziegler, M., Abdo, A. A., Ackermann, M., Ajello, M., Atwood, W. B., Axelsson, M., Baldini, L., Ballet, J., Barbiellini, G., Baring, M. G., Bastieri, D., Baughman, B. M., Bechtol, K., Bellazzini, R., Berenji, B., Blandford, R. D., Bloom, E. D., Bonamente, E., Borgland, A. W., Bregeon, J., Brez, A., Brigida, M., Bruel, P., Burnett, T. H., Buson, S., Caliandro, G. A., Cameron, R. A., Camilo, F., Caraveo, P. A., Casandjian, J. M., Cecchi, C., Celik, Oe., Charles, E., Chekhtman, A., Cheung, C. C., Chiang, J., Ciprini, S., Claus, R., Cognard, I., Cohen-Tanugi, J., Cominsky, L. R., Conrad, J., Corbet, R., Cutini, S., den Hartog, P. R., Dermer, C. D., de Angelis, A., de Luca, A., de Palma, F., Digel, S. W., Dormody, M., do Couto e Silva, E., Drell, P. S., Dubois, R., Dumora, D., Espinoza, C., Farnier, C., Favuzzi, C., Fegan, S. J., Ferrara, E. C., Focke, W. B., Fortin, P., Frailis, M., Freire, P. C. C., Fukazawa, Y., Funk, S., Fusco, P., Gargano, F., Gasparrini, D., Gehrels, N., Germani, S., Giavitto, G., Giebels, B., Giglietto, N., Giommi, P., Giordano, F., Glanzman, T., Godfrey, G., Gotthelf, E. V., Grenier, I. A., Grondin, M. -H., Grove, J. E., Guillemot, L., Guiriec, S., Gwon, C., Hanabata, Y., Harding, A. K., Hayashida, M., Hays, E., Hughes, R. E., Jackson, M. S., Johannesson, G., Johnson, A. S., Johnson, R. P., Johnson, T. J., Johnson, W. N., Johnston, S., Kamae, T., Kanbach, G., Kaspi, V. M., Katagiri, H., Kataoka, J., Kawai, N., Kerr, M., Knoedlseder, J., Kocian, M. L., Kramer, M., Kuss, M., Lande, J., Latronico, L., Lemoine-Goumard, M., Livingstone, M., Longo, F., Loparco, F., Lott, B., Lovellette, M. N., Lubrano, P., Lyne, A. G., Madejski, G. M., Makeev, A., Manchester, R. N., Marelli, M., Mazziotta, M. N., Mcconville, W., Mcenery, J. E., Mcglynn, S., Meurer, C., Michelson, P. F., Mineo, T., Mitthumsiri, W., Mizuno, T., Moiseev, A. A., Monte, C., Monzani, M. E., Morselli, A., Moskalenko, I. V., Murgia, S., Nakamori, T., Nolan, P. L., Norris, J. P., Noutsos, A., Nuss, E., Ohsugi, T., Omodei, N., Orlando, E, Ormes, J. F., Ozaki, M., Paneque, D., Panetta, J. H., Parent, D., Pelassa, V., Pepe, M., Pesce-Rollins, M., Piron, F., Porter, T. A., Raino, S., Rando, R., Ransom, S. M., Ray, P. S., Razzano, M., Rea, N., Reimer, A., Reimer, O., Reposeur, T., Ritz, S., Rodriguez, A. Y., Romani, R. W., Roth, M., Ryde, F., Sadrozinski, H. F. -W., Sanchez, D., Sander, A., Parkinson P. M., Saz, Scargle, J. D., Schalk, T. L., Sellerholm, A., Sgro, C., Siskind, E. J., Smith, D. A., Smith, P. D., Spandre, G., Spinelli, P., Stappers, B. W., Starck, J. -L., Striani, E., Strickman, M. S., Strong, A. W., Suson, D. J., Tajima, H., Takahashi, H., Takahashi, T., Tanaka, T., Thayer, J. B., Thayer, J. G., Theureau, G., Thompson, D. J., Thorsett, S. E., Tibaldo, L., Tibolla, O., Torres, D. F., Tosti, G., Tramacere, A., Uchiyama, Y., Usher, T. L., Van Etten, A., Vasileiou, V., Venter, C., Vilchez, N., Vitale, V., Waite, A. P., Wang, P., Wang, N., Watters, K., Weltevrede, P., Winer, B. L., Wood, K. S., Ylinen, T., and Ziegler, M.
Published: 2011

8. ERRATUM: THE FIRST FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS (vol 187, pg 460, 2010)

Author: Abdo, Aa, Ackermann, M, Ajello, M, Atwood, Wb, Axelsson, M, Baldini, L, Ballet, J, Barbiellini, G, Baring, Mg, Bastieri, Denis, Baughman, Bm, Bechtol, K, Bellazzini, R, Berenji, B, Blandford, Rd, Bloom, Ed, Bonamente, E, Borgland, Aw, Bregeon, J, Brez, A, Brigida, M, Bruel, P, Burnett, Th, Buson, Sara, Caliandro, Ga, Cameron, Ra, Camilo, F, Caraveo, Pa, Casandjian, Jm, Cecchi, C, Celik, O, Charles, E, Chekhtman, A, Cheung, Cc, Chiang, J, Ciprini, S, Claus, R, Cognard, I, COHEN TANUGI, J, Cominsky, Lr, Conrad, J, Corbet, R, Cutini, S, DEN HARTOG PR, Dermer, Cd, DE ANGELIS, A, DE LUCA, A, DE PALMA, F, Digel, Sw, Dormody, M, SILVA E, DOCOUTO E., Drell, Ps, Dubois, R, Dumora, D, Espinoza, C, Farnier, C, Favuzzi, C, Fegan, Sj, Ferrara, Ec, Focke, Wb, Fortin, P, Frailis, M, Freire, Pcc, Fukazawa, Y, Funk, S, Fusco, P, Gargano, F, Gasparrini, D, Gehrels, N, Germani, S, Giavitto, G, Giebels, B, Giglietto, N, Giommi, P, Giordano, F, Glanzman, T, Godfrey, G, Gotthelf, Ev, Grenier, Ia, Grondin, Mh, Grove, Je, Guillemot, L, Guiriec, S, Gwon, C, Hanabata, Y, Harding, Ak, Hayashida, M, Hays, E, Hughes, Re, Jackson, Ms, Johannesson, G, Johnson, As, Johnson, Rp, Johnson, Tj, Johnson, Wn, Johnston, S, Kamae, T, Kanbach, G, Kaspi, Vm, Katagiri, H, Kataoka, J, Kawai, N, Kerr, M, Knoedlseder, J, Kocian, Ml, Kramer, M, Kuss, M, Lande, J, Latronico, L, LEMOINE GOUMARD, M, Livingstone, M, Longo, F, Loparco, F, Lott, B, Lovellette, Mn, Lubrano, P, Lyne, Ag, Madejski, Gm, Makeev, A, Manchester, Rn, Marelli, M, Mazziotta, Mn, Mcconville, W, Mcenery, Je, Mcglynn, S, Meurer, C, Michelson, Pf, Mineo, T, Mitthumsiri, W, Mizuno, T, Moiseev, Aa, Monte, C, Monzani, Me, Morselli, A, Moskalenko, Iv, Murgia, S, Nakamori, T, Nolan, Pl, Norris, Jp, Noutsos, A, Nuss, E, Ohsugi, T, Omodei, N, Orlando, E, Ormes, Jf, Ozaki, M, Paneque, D, Panetta, Jh, Parent, D, Pelassa, V, Pepe, M, PESCE ROLLINS, M, Piron, F, Porter, Ta, Raino, S, Rando, Riccardo, Ransom, Sm, Ray, Ps, Razzano, M, Rea, N, Reimer, A, Reimer, O, Reposeur, T, Ritz, S, Rodriguez, Ay, Romani, Rw, Roth, M, Ryde, F, Sadrozinski, Hfw, Sanchez, D, Sander, A, SAZ PARKINSON PM, Scargle, Jd, Schalk, Tl, Sellerholm, A, Sgro, C, Siskind, Ej, Smith, Da, Smith, Pd, Spandre, G, Spinelli, P, Stappers, Bw, Starck, Jl, Striani, E, Strickman, Ms, Strong, Aw, Suson, Dj, Tajima, H, Takahashi, H, Takahashi, T, Tanaka, T, Thayer, Jb, Thayer, Jg, Theureau, G, Thompson, Dj, Thorsett, Se, Tibaldo, Luigi, Tibolla, O, Torres, Df, Tosti, G, Tramacere, A, Uchiyama, Y, Usher, Tl, VAN ETTEN, A, Vasileiou, V, Venter, C, Vilchez, N, Vitale, V, Waite, Ap, Wang, P, Wang, N, Watters, K, Weltevrede, P, Winer, Bl, Wood, Ks, Ylinen, T, and Ziegler, M.
Published: 2011

9. Search for hadronic decays of a light Higgs boson in the radiative decay Upsilon --> gamma A0

Author: Lees, J. P., Poireau, V., Tisserand, V., Garra Tico, J., Grauges, E., Martinelli, M., Milanes, D. A., Palano, A., Pappagallo, M., Eigen, G., Stugu, B., Brown, D. N., Kerth, L. T., Kolomensky, Y. u. G., Lynch, G., Koch, H., Schroeder, T., Asgeirsson, D. J., Hearty, C., Mattison, T. S., Mckenna, J. A., R. Y., So, Khan, A., Blinov, V. E., Buzykaev, A. R., Druzhinin, V. P., Golubev, V. B., Kravchenko, E. A., Onuchin, A. P., Serednyakov, S. I., Skovpen, Y. u. I., Solodov, E. P., Todyshev, K. Y. u., Yushkov, A. N., Bondioli, M., Kirkby, D., Lankford, A. J., Mandelkern, M., Stoker, D. P., Atmacan, H., Gary, J. W., Liu, F., Long, O., Vitug, G. M., Campagnari, C., Hong, T. M., Kovalskyi, D., Richman, J. D., West, C. A., Eisner, A. M., Kroseberg, J., Lockman, W. S., Martinez, A. J., Schalk, T., Schumm, B. A., Seiden, A., Cheng, C. H., Doll, D. A., Echenard, B., Flood, K. T., Hitlin, D. G., Ongmongkolkul, P., Porter, F. C., Rakitin, A. Y., Andreassen, R., Dubrovin, M. S., Huard, Z., Meadows, B. T., Sokoloff, M. D., Sun, L., Bloom, P. C., Ford, W. T., Gaz, A., Nagel, M., Nauenberg, U., Smith, J. G., Wagner, S. R., Ayad, R., Toki, W. H., Spaan, B., Kobel, M. J., Schubert, K. R., Schwierz, R., Bernard, D., Verderi, M., Clark, P. J., Playfer, S., Bettoni, D., Bozzi, C., Calabrese, R., Cibinetto, G., Fioravanti, E., Garzia, I., Luppi, E., Munerato, M., Negrini, M., Piemontese, L., Santoro, V., Baldini Ferroli, R., Calcaterra, A., de Sangro, R., Finocchiaro, G., Nicolaci, M., Patteri, P., Peruzzi, I. M., Piccolo, M., Rama, M., Zallo, A., Contri, R., Guido, E., Lo Vetere, M., Monge, M. R., Passaggio, S., Patrignani, C., Robutti, E., Bhuyan, B., Prasad, V., Lee, C. L., Morii, M., Edwards, A. J., Adametz, A., Marks, J., Uwer, U., Bernlochner, F. U., Ebert, M., Lacker, H. M., Lueck, T., Dauncey, P. D., Tibbetts, M., Behera, P. K., Mallik, U., Chen, C., Cochran, J., Meyer, W. T., Prell, S., Rosenberg, E. I., Rubin, A. E., Gritsan, A. V., Guo, Z. J., Arnaud, N., Davier, M., Grosdidier, G., Le Diberder, F., Lutz, A. M., Malaescu, B., Roudeau, P., Schune, M. H., Stocchi, A., Wormser, G., Lange, D. J., Wright, D. M., Bingham, I., Chavez, C. A., Coleman, J. P., Fry, J. R., Gabathuler, E., Hutchcroft, D. E., Payne, D. J., Touramanis, C., Bevan, A. J., Di Lodovico, F., Sacco, R., Sigamani, M., Cowan, G., Davis, C. L., Denig, A. G., Fritsch, M., Gradl, W., Hafner, A., Prencipe, E., Alwyn, K. E., Bailey, D., Barlow, R. J., Jackson, G., Lafferty, G. D., Behn, E., Cenci, R., Hamilton, B., Jawahery, A., Roberts, D. A., Simi, G., Dallapiccola, C., Cowan, R., Dujmic, D., Sciolla, G., Lindemann, D., Patel, P. M., Robertson, S. H., Schram, M., Biassoni, P., Lazzaro, A., Lombardo, V., Neri, N., Palombo, F., Stracka, S., Cremaldi, L., Godang, R., Kroeger, R., Sonnek, P., Summers, D. J., Nguyen, X., Taras, P., De Nardo, G., Monorchio, D., Onorato, G., Sciacca, C., Raven, G., Snoek, H. L., Jessop, C. P., Knoepfel, K. J., Losecco, J. M., Wang, W. F., Honscheid, K., Kass, R., Brau, J., Frey, R., Sinev, N. B., Strom, D., Torrence, E., Feltresi, E., Gagliardi, N., Margoni, M., Morandin, M., Posocco, M., Rotondo, M., Simonetto, F., Stroili, R., Akar, S., Ben Haim, E., Bomben, M., Bonneaud, G. R., Briand, H., Calderini, Giovanni, Chauveau, J., Hamon, O., Leruste, P. h., Marchiori, G., Ocariz, J., Sitt, S., Biasini, M., Manoni, E., Pacetti, S., Rossi, A., Angelini, Carlo, Batignani, Giovanni, Bettarini, Stefano, Carpinelli, M., Casarosa, G., Cervelli, A., Forti, Francesco, Giorgi, Marcello, Lusiani, A., Oberhof, B., Paoloni, Eugenio, Perez, A., Rizzo, Giuliana, Walsh, J. J., Lopes, Pegna D., Lu, C., Olsen, J., Smith, A. J. S., Telnov, A. V., Anulli, F., Cavoto, G., Faccini, R., Ferrarotto, F., Ferroni, F., Gaspero, M., Gioi L., Li, Mazzoni, M. A., Piredda, G., Nger C., Bu, Gruenberg, O., Hartmann, T., Leddig, T., Schroeder, H., Waldi, R., Adye, T., Olaiya, E. O., Wilson, F. F., Emery, S., Hamel, de Monchenault G., Vasseur, G., Yeche, C. h., Aston, D., Bard, D. J., Bartoldus, R., Benitez, J. F., Cartaro, C., Convery, M. R., Dorfan, J., Dubois Felsmann, G. P., Dunwoodie, W., Field, R. C., Franco, Sevilla M., Fulsom, B. G., Gabareen, A. M., Graham, M. T., Grenier, P., Hast, C., Innes, W. R., Kelsey, M. H., Kim, H., Kim, P., Kocian, M. L., Leith, D. W. G. S., Lewis, P., Li, S., Lindquist, B., Luitz, S., Luth, V., Lynch, H. L., Macfarlane, D. B., Muller, D. R., Neal, H., Nelson, S., Ofte, I., Perl, M., Pulliam, T., Ratcliff, B. N., Roodman, A., Salnikov, A. A., Schindler, R. H., Snyder, A., Su, D., Sullivan, M. K., Va'Vra, J., Wagner, A. P., Weaver, M., Wisniewski, W. J., Wittgen, M., Wright, D. H., Wulsin, H. W., Yarritu, A. K., Young, C. C., Ziegler, V., Park, W., Purohit, M. V., White, R. M., Wilson, J. R., Randle Conde, A., Sekula, S. J., Bellis, M., Burchat, P. R., Miyashita, T. S., Alam, M. S., Ernst, J. A., Gorodeisky, R., Guttman, N., Peimer, D. R., Soffer, A., Lund, P., Spanier, S. M., Eckmann, R., Ritchie, J. L., Ruland, A. M., Schilling, C. J., Schwitters, R. F., Wray, B. C., Izen, J. M., Lou, X. C., Bianchi, F., Gamba, D., Lanceri, L., Vitale, L., Martinez Vidal, F., Oyanguren, A., Ahmed, H., Albert, J., Banerjee, S. w., Choi, H. H. F., King, G. J., Kowalewski, R., Lewczuk, M. J., Nugent, I. M., Roney, J. M., Sobie, R. J., Tasneem, N., Gershon, T. J., Harrison, P. F., Latham, T. E., Puccio, E. M. T., Band, H. R., Dasu, S., Pan, Y., Prepost, R., S. L. . J., Wu, Ahmed, S., Pan, B., Saeed, M. A., Zain, S. B., Pelliccioni, M., Lopez March, N., Hamano, K., Vuosalo, C. O., S. L. O., Wu, Yu SS, Wu S. L., Yun, Jc, Zanetti, A, Zeng, Y, Zucchelli, S, Ruggi, P, Russell, P, Ryan, K, Sakata, S, Salemi, F, de la Jordana LS, Sandberg, V, Sannibale, V, Santamaria, L, Saraf, S, Sarin, P, Sassolas, B, Sathyaprakash, Bs, Sato, S, Satterthwaite, M, Saulson, Pr, Savage, R, Savov, P, Scanlan, M, Schilling, R, Schnabel, R, Schofield, R, Schulz, B, Schutz, Bf, Schwinberg, P, Scott, J, Scott, Sm, Searle, Ac, Sears, B, Seifert, F, Sellers, D, Sengupta, As, Sentenac, D, Sergeev, A, Shapiro, B, Shawhan, P, Shoemaker, Dh, Sibley, A, Siemens, X, Sigg, D, Sinha, S, Sintes, Am, Slagmolen, Bjj, Slutsky, J, Smith, Jr, Smith, Mr, Smith, Nd, Somiya, K, Sorazu, B, Stein, A, Stein, Lc, Steplewski, S, Stochino, A, Stone, R, Strain, Ka, Strigin, S, Stroeer, A, Sturani, R, Stuver, Al, Summerscales, Tz, Sun, Kx, Sung, M, Sutton, Pj, Swinkels, B, Szokoly, Gp, Talukder, D, Tang, L, Tanner, Db, Tarabrin, Sp, Taylor, Jr, Taylor, R, Terenzi, R, Thacker, J, Thorne, Ka, Thorne, Ks, Thuring, A, Tokmakov, Kv, Toncelli, A, Tonelli, M, Torres, C, Torrie, C, Tournefier, E, Travasso, F, Traylor, G, Trias, M, Trummer, J, Ugolini, D, Ulmen, J, Urbanek, K, Vahlbruch, H, Vajente, G, Vallisneri, M, van den Brand JFJ, Van Den Broeck, C, van der Putten, S, van der Sluys MV, van Veggel AA, Vass, S, Vaulin, R, Vavoulidis, M, Vecchio, A, Vedovato, G, Veitch, J, Veitch, P, Veltkamp, C, Verkindt, D, Vetrano, F, Vicere, A, Villar, A, Vinet, Jy, Vocca, H, Vorvick, C, Vyachanin, Sp, Waldman, Sj, Wallace, L, Ward, Rl, Was, M, Weidner, A, Weinert, M, Weinstein, Aj, Weiss, R, Wen, L, Wen, S, Wette, K, Whelan, Jt, Whitcomb, Se, Whiting, Bf, Wilkinson, C, Willems, Pa, Williams, Hr, Williams, L, Willke, B, Wilmut, I, Winkelmann, L, Winkler, W, Wipf, Cc, Wiseman, Ag, Woan, G, Wooley, R, Worden, J, Wu, W, Yakushin, I, Yamamoto, H, Yan, Z, Yoshida, S, Yvert, M, Zanolin, M, Zhang, J, Zhang, L, Zhao, C, Zotov, N, Zucker, Me, zur Muhlen, H, Zweizig Jrongiu, A, D'Amico, N, Freire, Pcc, Hessels, Jwt, Hobbs, Gb, Kramer, M, Lyne, Ag, Manchester, Rn, Marshall, Fe, Middleditch, J, Possenti, A, Ransom, Sm, Stairs, Ih, Stappers Bl, T, White, Dj, Yamamoto, K, Yeaton Massey, D, Yu, Pp, Zhang, Z, Zweizig, J., Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, BABAR, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], light higgs boson, High Energy Physics - Experiment, 14.80.Da, 14.40.Pq, 13.20.Gd, 12.60.Fr, 12.15.Ji, 12.60.Jv
Abstract: We search for hadronic decays of a light Higgs boson (A0) produced in radiative decays of an Upsilon(2S) or Upsilon(3S) meson, Upsilon --> gamma A0. The data have been recorded by the BABAR experiment at the Upsilon(3S) and Upsilon(2S) center of mass energies, and include (121.3 \pm 1.2) x 10^6 Upsilon(3S) and (98.3 \pm 0.9) x 10^6 Upsilon(2S) mesons. No significant signal is observed. We set 90% confidence level upper limits on the product branching fractions B(Upsilon(nS)-->gamma A0) x B(A0-->hadrons) (n=2 or 3) that range from 1 x 10^{-6} for an A0 mass of 0.3 GeV/c^2 to 8 x 10^{-5} at 7 GeV/c^2., Comment: 7 pages, 5 postscript figures, submitted to Physical Review Letters
Published: 2011

10. RADIO AND gamma-RAY CONSTRAINTS ON THE EMISSION GEOMETRY AND BIRTHPLACE OF PSR J2043+2740 RID G-6769-2011

Author: Noutsos, A, Abdo, Aa, Ackermann, M, Ajello, M, Ballet, J, Barbiellini, G, Baring, Mg, Bastieri, Denis, Bechtol, K, Bellazzini, R, Berenji, B, Bonamente, E, Borgland, Aw, Bregeon, J, Brez, A, Brigida, M, Bruel, P, Buehler, R, Busetto, Giovanni, Caliandro, Ga, Cameron, Ra, Camilo, F, Caraveo, Pa, Casandjian, Jm, Cecchi, C, Celik, O, Chaty, S, Chekhtman, A, Chiang, J, Ciprini, S, Claus, R, Cognard, I, Cohen Tanugi, J, Colafrancesco, S, Cutini, S, Dermer, Cd, de Palma, F, Drell, Ps, Dumora, D, Ea, Cm, Favuzzi, C, Ferrara, Ec, Focke, Wb, Frailis, M, Freire, Pcc, Fukazawa, Y, Funk, S, Fusco, P, Gargano, F, Germani, S, Giglietto, N, Giordano, F, Giroletti, M, Godfrey, G, Grandi, P, Grenier, Ia, Grove, Je, Guillemot, L, Guiriec, S, Harding, Ak, Hughes, Re, Jackson, Ms, Johannesson, G, Johnson, As, Johnson, Tj, Johnson, Wn, Johnston, S, Kamae, T, Katagiri, H, Kataoka, J, Knodlseder, J, Kramer, M, Kuss, M, Lande, J, Lee, Sh, Longo, F, Loparco, F, Lovellette, Mn, Lubrano, P, Lyne, Ag, Makeev, A, Marelli, M, Mazziotta, Mn, Mcenery, Je, Mehault, J, Michelson, Pf, Mizuno, T, Monte, C, Monzani, Me, Morselli, A, Moskalenko, Iv, Murgia, S, Naumann Godo, M, Nolan, Pl, Nuss, E, Ohsugi, T, Okumura, A, Omodei, N, Orlando, E, Ormes, Jf, Panetta, Jh, Parent, D, Pelassa, V, Pepe, M, Persic, M, Pesce Rollins, M, Piron, F, Porter, Ta, Raino, S, Ray, Ps, Razzano, M, Reimer, A, Reimer, O, Reposeur, T, Romani, Rw, Sadrozinski, Hfw, Sander, A, Parkinson, Pms, Sgro, C, Siskind, Ej, Smith, Da, Smith, Pd, Spandre, G, Spinelli, P, Stappers, Bw, Strickman, Ms, Suson, Dj, Takahashi, H, Tanaka, T, Theureau, G, Thompson, Dj, Thorsett, Se, Tibolla, O, Torres, Df, Tramacere, A, Usher, Tl, Vandenbroucke, J, Vianello, G, Vilchez, N, Villata, M, Vitale, V, von Kienlin, A, Waite, Ap, Wang, P, Watters, K, Weltevrede, P, Winer, Bl, Wood, Ks, and Ziegler, M.
Published: 2011

11. The nature of the PSR J2051-0827 eclipses

Author: Stappers, BW, Bailes, M, Lyne, AG, Camilo, F, Manchester, RN, Sandhu, JS, Toscano, M, Bell, JF, Stappers, BW, Bailes, M, Lyne, AG, Camilo, F, Manchester, RN, Sandhu, JS, Toscano, M, and Bell, JF
Published: 2001

12. BIRTH-RATE OF MILLISECOND PULSARS

Author: LORIMER, DR, LYNE, AG, FESTIN, L, NICASTRO, L, LORIMER, DR, LYNE, AG, FESTIN, L, and NICASTRO, L
Abstract: Addresses: LORIMER DR, UNIV MANCHESTER, NUFFIELD RADIO ASTRON LABS, JODRELL BANK, MACCLESFIELD SK11 9DL, CHESHIRE, ENGLAND. ASTRON OBSERV, S-75120 UPPSALA, SWEDEN. CNR, IST TECNOL & STUDIE RADIASIONI EXTRATERR, I-40129 BOLOGNA, ITALY.
Published: 1995

13. An unusual blastocyst stage of the marsupial Isoodon macrourus

Author: Lyne, AG and Hollis, DE
Abstract: Four blastocysts, identical in size (diameter 1.1 mm) and appearance, were obtained from one uterus of a short-nosed bandicoot I. macrourus and examined by light and electron microscopy. These blastocysts were unusual in that each one had a conspicuous region of protoderm about 0.3-0.5 mm in width and mostly more than one cell thick. The remainder of the protoderm was thin and unilaminar. Cell divisions were more numerous in the thickened region than in the remainder of the protoderm. Some entire cells and blebs of cytoplasm had been shed or were being shed from the thickened region into the blastocoele. The egg membranes were similzr to those of bilaminar blastocysts, the shell membranes being intact and about 1.0 um thick, and the mucoid coat and zona pellucida being discontinuous.
Published: 1977
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14. Endodermal formation in blastocytes of the marsupials Isoodon macrousus and Perameles nasuta

Author: Hollis, DE and Lyne, AG
Abstract: Eleven embryos, ranging from partly to fully bilaminar blastocysts, were obtained from the bandicoots I. macrourus and P. nasuta and were examined by light and electron microscopy. The morphological changes which occurred during the differentiation of the endoderm and ectoderm are described. The shell membrane was thinner than it was in unilaminar blastocysts and had a deposit of material of irregular thickness on its outer surface. The mucoid coat and zona pellucida were absent or discontinuous. Endoderm formation was first observed in blastocysts about 1.0 mm in diameter. Cells migrated inwards from regions of thickened protoderm to form a continuous layer of similar flattened cells - the endoderm - beneath the protoderm, which then became the ectoderm. The blastocysts were fully bilaminar when they were 1.5-1.9 mm in diameter. At this stage the ectoderm was composed of two distinct regions, an embryonic region of cuboidal cells and a non-embryonic region of flattened cells resembling the cells of the endoderm. The formation of the endoderm in bandicoots closely resembles that described in other marsupials, except the American opossum Didelphis virginiana in which endoderm cells are released into the blastocoele before they form a continuous layer.
Published: 1977
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15. Observations on oetrus and the oestrous cycle in the marsupials Isoodon Macrourus and Perameles nasuta

Author: Lyne, AG
Abstract: Observations have been made on oestrus and the oestrous cycle in the bandicoots I. macrourus and P. nasuta caged indoors. Oestrus was diagnosed from a number of criteria, particularly the sexual behaviour of the males. Attempted matings, non-fertile matings and matings leading to pregnancy were restricted to one day of the oestrous cycle, except on one occasion when a male I. macrourus attempted to mate on two consecutive days. The lips of the urogenital opening of the female were usually greatly swollen at oestrus but pouch changes at this time were not detected. Vaginal smears at oestrus usually showed an increase in the number of partly and fully cornified epithelial cells and few, if any, polymorphonuclear leucocytes. During the winter and spring of 1972 and spring of 1973, over 1000 vaginal smears were taken from 29 P. nasuta and about 700 smears were taken from 21 I. macrourus. Information on the length of the oestrous cycle in P. nasuta, using all criteria, was obtained from only nine cycles in eight animals. The cycle length averaged 21 days but the range was from 10 to 34 days. Considerably more information on the length of the cycle was obtained from the smaller number of I. macrourus; the average length of 39 cycles in 15 animals was 20 days, the range being 9-34 days.
Published: 1976
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16. Early embryology af the marsupials Isoodon macrourus and Perameles nasuta

Author: Lyne, AG and Hollis, DE
Abstract: Twelve embryos, ranging from a four-celled stage to late unilaminar blastocysts, were obtained from the bandicoots I. macrourus and P. nasuta and examined by light and electron microscopy. These early stages covered at least one-quarter of the 12.5-day gestation period. The three non-cellular egg membranes characteristic of marsupials (zona pellucida, mucoid coat and shell membrane) were present, although the zona was sometimes absent or discontinuous in the intermediate and late unilaminar blastocysts examined. At the four-celled stage the blastomeres were close to the zona, but they had lost contact with each other, probably due to the extrusion of yolk, a phenomenon which has been described in other marsupials. The embryo did not increase in diameter until it was composed of at least 75 contiguous cells, which were in contact with the zona. In several of the larger blastocysts the protoderm cells had lost contact with the zona. Subsequently, the number of cells increased considerably and they were flattened against the egg membranes to form the late unilaminar blastocyst stage. Electron microscopy of the protoderm cells revealed the presence of numerous microvilli, particularly on the outer surface, and a range of other structures as great as those found in eutherian mammals. Remnants of spindle bridges were common in one 75-celled embryo. The yolk material in the blastocoele was also composed of a variety of structures, including small crystalloid inclusions composed of hexagonal units about 8-10 nm in diameter. Similar crystalloids have been described in the cells of early mouse and rabbit embryos and in egg and embryonic cells of various amphibians.
Published: 1976
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17. Innervation of vibrissa follicles in the marsupial Trichosurus vulpecula

Author: Hollis, DE and Lyne, AG
Abstract: The innervation of the mystacial vibrissa follicles in the adult brush-tailed possum, T. vulpecula, has been studied by light and electron microscopy. One to five large nerve trunks penetrate the lower part of the follicle capsule and divide many times as they ascend and completely envelop the con- nective tissue sheath of the follicle. As many as 500 myelinated nerves have been observed in the mid region of the largest follicles. Above the mid region, most of the nerves move closer to the centre of the follicle and finally terminate within or near the outer layer of epithelial cells. Four main types of nerve endings have been observed: (1) Sensory receptor cells, called Merkel cells, with their associated neurites are numerous within the outer layer of epithelial cells. (2) Palisade endings, which are less common than the Merkel cell-neurite complexes, surround the upper part of the glassy membrane of the follicle. In transverse section each palisade ending appears as a flattened central neurite partially enveloped on either side by Schwann cell processes. (3) Bulbous endings occur in both the connective tissue sheath and in the outer layer of follicle epithelial cells. They are larger than types (1) and (2) and their ultrastructure varies markedly. (4) Compound endings occur within the connective tissue sheath of the follicle. They are uncommon but large and are composed of a chain of bulbous units joined by nerves; the entire ending may be encapsulated. Within each unit there is a tangle of nerve fibres. The Merkel cell-neurite complexes and the palisade endings in T. vulpecula are remarkably similar to those of eutherian mammals, suggesting that such sensory structures were features of primitive mammals.
Published: 1974
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18. Observations on the structure of vibrissa follicles in the marsupial Trichosurus vulpecula, with special reference to Keratinization

Author: Hollis, DE and Lyne, AG
Abstract: The structure of active and resting vibrissa follicles from adult brush-tailed possums, T. vulpecula, has been examined with the light and the electron microscope. Particular attention is given to the structural changes which occur during keratinization of the vibrissa and hardening of the inner root sheath, and these changes are compared with those of pelage follicles in eutherian mammals. Keratinization in the various follicle layers is similar in these two follicle types. However, the stages of keratinization in vibrissa follicles are better defined than they are in the smaller pelage follicles of other species. A transition phase of hardening has been observed in the inner root sheath cells of vibrissa follicles. This phase appears to be very short-lived and has not been previously described in other follicles.
Published: 1975
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19. Gestation period and birth in the marsupial Isoodon macrourus

Author: Lyne, AG
Abstract: The birth of a litter of two short-nosed bandicoots, I. macvourus, was witnessed and photographed. As mating (between litter mates) had also been observed the length of the gestation period was known. It was between 12 days 8 h and 12 days 11 h-the shortest gestation recorded for any mammal. In the 2 h preceding parturition, when the female was watched continuously, she was not seen to lick the pouch or the urogenital opening. However, just before the first young was suddenly expelled, vigorous licking of the urogenital opening began, the mother being on her side with one hind leg raised. The second young was born about 2 min later. The young appeared to be born free of membranes but had intact allantoic stalks. Although the mother did not lick a path in the hair leading to the pouch she continuously licked around the young as they crawled towards the pouch. The allantoic stalks and the deciduous claws on the fore feet anchored the young to the mother during this journey.
Published: 1974
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20. Growth of vibrissae in the marsupial Trichosurus vulpecula

Author: Lyne, AG, Downes, AM, and Chase, HB
Abstract: The autoradiographic technique was used to study the growth of the vibrissae in the mystacial, genal, and supraorbital regions of three brush-tailed possums. During the first cycle there were well-marked gradients in length within and between the rows of mystacial vibrissae. The length growth rates of the corresponding vibrissae on the left and right sides of the body were almost identical at any particular time, although the growth rates varied throughout the cycle. The variations in the final lengths of the vibrissae were due to variations in both the growth rate and the length of the cycle. The diameters increased continuously throughout the cycle. The rate of regrowth after plucking vibrissae from active and resting follicles was also studied. The new vibrissa in a particular follicle initially grew at a much faster rate than either the corres- ponding undisturbed vibrissa on the other side of the head or the vibrissa which had just been plucked. The subsequent rate of growth decreased progressively throughout the cycle. In spite of differences in growth rates during the first and later cycles, the overall dimensions of the successive vibrissae from a particular follicle were very similar. The normal retention of vibrissae was studied in one animal. At least some vibrissae were retained for more than a year after they had stopped growing. The results demonstrate that the vibrissae of T. vulgecula provide an excellent model for studies of the factors controlling follicle activity.
Published: 1974
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21. Activity Rhythms in the Marsupials Isoodon macrourus and Perameles nasuta in Captivity

Author: Lyne, AG
Abstract: Exercise wheels and closed-circuit television were used to record the activity rhythms of 34 1. macrourus and 32 P, nasuta (1) outdoors; (2) indoors with natural light; (3) indoors with artificial light in which the phases of night and day were normal; (4) same as (3) but with the phases of night and day reversed; (5) continuous dark; (6) continuous light. In tests (3)-(6) a faint red light was on continuously. These tests were made on animals caged singly or in pairs and lasted for periods of from 8 to 357 days. When a male and a female of different body weights were tested together, the animal using the wheel was identified by its weight. Five I. macrourus and 23 P. nasuta exposed to normal phases of night and day were active mainly during the dark periods. The daily activity pattern varied considerably but was fairly constant for individuals. When the phases of night and day were reversed, the animals continued to be active during the dark periods and, in many of them, the pattern of activity was similar to that under normal phases of night and day. They were, therefore, entrained to the artificial lighting system. However, in 17 out of 31 P. nasuta and 5 out of 31 1. macrourus exposed to reversed lighting conditions, activity started later each day. When the trigger for exercise began to fall close to the beginning of a light period, no activity was taken; the animals did not run in the wheel or take other exercise for 2-5 days, feeding and drinking were greatly reduced and some animals did not leave the nest box for 1-2 days. After this pause, exercise began again at the beginning of a dark period. In 10 I. macrourus exposed to continuous dark the period of the endogenous rhythm was either more than or less than 24 h, and in continuous light (four animals), the wheel-running activity was greatly reduced.
Published: 1981
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22. Ultrastructure of Luteal Cells in Fully Formed and Regressing Corpora Lutea During Pregnancy and Lactation in the Marsupials Isoodon Macrourus and Perameles Nasuta.

Author: Hollis, DE and Lyne, AG
Abstract: Corpora lutea (CL) collected from 23 bandicoots (I. macrourus and P. nasuta), from day 5 of pregnancy (gestation 12.5 days) to day 53 of lactation (lactation c. 60 days), were examined with the electron microscope. The luteal cells of fully formed CL (from day 5 of pregnancy to day 44 of lactation) were large and contained spherical nuclei with distinct nucleoli. The amount of heterochromatin increased during the latter part of this period. The cytoplasm contained numerous lipid droplets and abundant smooth endoplasmic reticulum (SER). Granular endoplasmic reticulum (GER) was less common. Mitochondria were most numerous from day 16 to day 44 of lactation and some of them contained large osmiophilic inclusions. Several types of granules and inclusions were present in the cytoplasm. During pregnancy, small dense-cored granules were common in P. nasuta and sparse in I. macrourus. They were still present in small numbers during early lactation in P. nasuta but were absent throughout lactation in I. macrourus. A special type of cell junction associated with endoplasmic reticulum was present between the luteal cells in P. nasuta but not in I. macrourus. The luteal cells of regressing CL on days 48, 50 and 53 of lactation were markedly reduced in size, with small irregularly shaped nuclei containing clumps of heterochromatin and indistinct nucleoli. The cells still contained numerous lipid droplets, and osmiophilic inclusions were still present in some of the mitochondria, which were reduced in number (and absent in the animal at day 50). Lancet-shaped spaces, which probably initially contained cholesterol crystals extracted by solvents during processing, were present in some of the regressing luteal cells. Organelles, including SER and GER, were either sparse or unrecognizable in luteal cells at advanced stages of regression. In general, the ultrastructural features of the luteal cells in fully formed and regressing CL of bandicoots were similar to those described in active and regressing CL of eutherian mammals.
Published: 1980
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23. Observations on the corpus luteum during pregnancy and lactation in the marsupials Isooson macrous and Perameles nasuta

Author: Lyne, AG and Hollis, DE
Abstract: Ovaries from the bandicoots I. macrourus and P. nasuta, collected during pregnancy and lactation, were examined macroscopically and with the light microscope. The mean number of corpora lutea (CL) was greater in I. macrourus (5.13) than in P. nasuta (3.31). This difference in ovulation rate was reflected in the mean number of embryos and the mean number of pouch young respectively (I. macrourus 4.05, 3.07; P. nasuta 2.63, 2.65). During the first few days of pregnancy, the transformation of follicle granulosa cells into luteal cells was accompanied by the intrusion of the theca, which produced a network of blood vessels and connective tissue. A conspicuous feature of the developing CL was the presence of pools of blood between the luteal cells. By 5-6 days of pregnancy, the CL was a fully formed structure, the central cavity having been filled in by hypertrophy of the luteal cells and an increase in the connective tissue which formed a central core. The luteal cells had almost reached their maximum size and they contained numerous lipid droplets. Mitoses of luteal cells were not evident at any stage in the formation of the CL or later, though some of the luteal cells had two or more nuclei. The structure of the CL and the diameter of the luteal cells and their nuclei remained almost constant until regression occurred after the 45th day of the 60-day lactation period. Regression of the CL was characterized by a marked reduction in the size of the luteal cells and their nuclei as well as an increase in the connective tissue component. Diameters and volumes of the CL were similar in the two species, reaching maxima during the second half of pregnancy and changing very little until the 45th day of lactation, after which they decreased rapidly. This decline occurred whether or not the animals subsequently ovulated during the last quarter of the lactation period.
Published: 1979
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24. Effect of adverse nutrition on the skin and wool follicles in Merino sheep

Author: Lyne, AG
Abstract: The effect of adverse nutrition on the body weight, skin thickness, and wool follicles of five groups of five Merino wethers has been observed over a period of 64 months in an experiment on the utilization of low quality roughage. All animals on the poorest diet (roughage containing 2.6% crude protein, ad lib.) were transferred to a recovery ration of lucerne chaff, wheat, linseed meal, and meat meal (33 : 33 : 20 : 13) at 6–9 weeks after the commencement of the experiment. Only three animals on the better diets needed this recovery ration. In general, changes in skin thickness paralleled changes in body weight. A marked increase in skin thickness which followed shearing was probably due to cold stress. Fibre shedding was a major feature of the reaction of the follicle population to adverse nutrition, but all afflicted follicles regenerated their fibres when the recovery ration was given. Primary (P) and secondary (S) follicles responded differently to adverse nutrition. Approximately 20 000 P follicles and 155 000 S follicles were examined. 1.4% of the P follicles and 9.%% of the S follicles showed evidence of shedding.
Published: 1964
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25. Development of horns in merino sheep

Author: Lyne, AG and Hollis, DE
Abstract: Development of horns has been studied in 20 foetuses ranging in age from 55 to 144 days of gestation, and in 16 lambs, ranging in age from birth to 42 days. Samples from one adult have also been examined. An increase in the thickness of the epidermis appears to be the first indication of horn development, recognizable in a 75-day-old male foetus and in an 84-day-old female foetus. Primary hair follicles develop in the horn region and produce emerging hairs, but these follicles later degenerate and disappear. The sweat glands and sebaceous glands formed in association with these follicles also degenerate, usually after hair growth has ceased. Fusion of primary follicles is a common feature in the horn growing skin, particularly before hair formation; a common connective tissue sheath surrounds the lower parts of these fused follicles. No secondary follicles are formed in the horn region but some branching of the primary follicles has been observed. By 118 days of gestation the epidermis in the horn region becomes greatly thickened, with very long dermal papillae which are well vascularized and innervated. Medulla-like columns of cells are formed above each dermal papilla and these cells keratinize later than the cells between the columns. These medullary cells remain in contact with each other longer than do the other cells of the horny sheath. Numerous arteriovenous anastomoses, which develop at two levels in the dermis of the horn region, are in continuity with capillaries which enter the dermal papillae of the epidermis. An outgrowth of bone from the frontal region of the skull, which later becomes the bony core of the horn, is first seen in a male foetus at 118 days. Acetylcholinesterase-positive branched cells (Langerhans cells), present in the lower part of the thick epidermis of developing horns, are not discernible in fully formed horns.
Published: 1973
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26. The development, structure, and function of the submandibular cutaneous (chin) glands in the rabbit.

Author: Lyne, AG, Molyneux, GS, Mykytowycz, R, and Parakkal, PF
Abstract: Embryological, histological, and histochemical features of the chin glands in the rabbit, Oryctolagus cuniculus (L.), are described. The glands are modified sweat glands which develop as appendages of the first hair follicles of the pelage. All the secretory cells are of the merocrine type, although some secrete in the typical apocrine manner. In the adult, the glands are much better developed in males than in females. Two main types of secretory cells were clearly seen in most animals, particularly adult males. Cells which stained heavily with osmium tetroxide (dark cells) were also present. No other mammalian cutaneous gland is so complex. Histochemical techniques to demonstrate enzymes revealed that particular glandular components contained large amounts of alkaline phosphatase and the whole gland was well supplied with nerves containing cholinesterases. The function of the secretion from these glands in marking territories is outlined.
Published: 1964
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27. Observations on the breeding and growth of the marsupial Perameles nasuta Geoffroy, with notes on other bandicoots.

Author: Lyne, AG
Abstract: A study has been made of 521 bandicoots (Perameles nasuta, 324; P. gunnii, 111 ; Isoodon obesulus, 86). Near Sydney, P. nasuta breeds all the year round with no indication of any peaks of breeding activity. Limited observations on P. gunnii and I. obesulus in Tasmania also suggest that births occur in every season of the year. Parturition of a single individual of P. nasuta was witnessed. Fifteen new-born specimens of this species were measured and body weight records were obtained for five of them. The average dimensions of these specimens, and consecutive measurements of three specimens born in captivity and of known age, were used to age pouch young of unknown age. Age changes in the appearance of P. nasuta are described and illustrated. Hair emerges on the trunk at about 40 days after birth and at 2 months the coat is similar to that of the adult. The rate of body growth is extremely rapid just prior to the opening of the eyes (usually at 45-48 days), and the young first appear outside the pouch several days later. The pouch contains eight teats, and the mean litter sizes were: P. nasuta, 2.44 (52 litters); P. gunnii, 2.23 (22 litters); I. obesulus, 2.33 (9 litters). In 47 litters of P. nasuta, 73 young were on teats of the left side compared with 46 on the right side of the pouch. The sexes were equally represented in the pouch young of the three species examined. In P. nasuta, sexual maturity is reached at about 450 g in females and about 650 g in males. The linear equivalence (cube root of the body weight) is used as an overall measure of size with which the parts of the body are compared.
Published: 1964
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28. Effects of Grafting the Skin in Merino Sheep, With Special Reference to the Growth of Wool and Hair

Author: Lyne, AG, primary and Hollis, DE, additional
Published: 1980
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29. Studies on the Development of Wool Follicles in Tissue Culture

Author: H Hardy, Margaret, primary and Lyne, AG, additional
Published: 1956
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30. Observations on the surface structure of the hairs of Tasmanian monotremes and marsupials

Author: Lyne, AG, primary
Published: 1950
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31. Studies on the Rate of Wool Growth Using [35s]Cystine

Author: Downes, AM, primary and Lyne, AG, additional
Published: 1961
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32. Selection for Constancy of Expression of the Tabby Gene in the Mouse

Author: Lyne, AG, primary, Henrikson, RC, additional, and Hollis, DE, additional
Published: 1970
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33. Effects of Freezing the Skin and Plucking the Fibres in Sheep, With Special Reference to Pigmentation

Author: Lyne, AG, primary and Hollis, DE, additional
Published: 1968
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34. The Pre-Natal Development of Skin and Hair in Cattle II. Bos Indicus l. X B. Taurus l.

Author: Lyne, AG, primary and J Heideman, Margaret, additional
Published: 1960
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35. Neogenesis of Wool Follicles

Author: Lyne, AG, primary and Brook, AH, additional
Published: 1964
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36. Syndactyly in the manus of a Marsupial

Author: Lyne, AG, primary
Published: 1953
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37. The Postnatal Development of Wool Follicles, Shedding, and Skin Thickness in Inbred Merino and Southdown-Merino Crossbred Sheep

Author: Lyne, AG, primary
Published: 1961
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38. Radioautographic Studies of the Incorporation of [35s]Cystine into Wool

Author: Downes, AM, primary, Lyne, AG, additional, and Clarke, WH, additional
Published: 1962
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39. Effect of Subdermal Pressure on the Skin and Its Appendages in the Sheep

Author: Jolly, M, primary and Lyne, AG, additional
Published: 1969
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40. The Melanocyte Population in the Skin During Development of the Marsupial Trichosurus Vulpecula

Author: Lyne, AG, primary
Published: 1970
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41. The Skin of the Sheep: a Comparision of Body Regions

Author: Lyne, AG, primary and Hollis, DE, additional
Published: 1968
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42. Studies on Experimental Dermal Cysts in Sheep

Author: Molyneux, GS, primary and Lyne, AG, additional
Published: 1961
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43. The Development of the Epidermis and hair Canals in the Merino Sheep Foetus

Author: Lyne, AG, primary
Published: 1957
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44. The Pre-Natal Development of Skin and hair in Cattle (Bos Taurus L.)

Author: Lyne, AG, primary and J Heideman, Margaret, additional
Published: 1959
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45. The Development and Replacement of Pelage Hairs in the Bandicoot Perameleb Nasuta Geoffroy (Marsupialia : Peramelidae)

Author: Lyne, AG, primary
Published: 1957
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46. The Pre-Natal Development of Wool Follicles in Merino Sheep

Author: H Hardy, Margaret, primary and Lyne, AG, additional
Published: 1956
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47. The Development of Hair Follicles in the Marsupial Trichosurus Vulpecula

Author: Lyne, AG, primary
Published: 1970
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48. Gravitational-wave Constraints on the Equatorial Ellipticity of Millisecond Pulsars

Author: D. Rosińska, Patrice Hello, I. M. Pinto, Stephane Perries, I. La Rosa, Jean-René Cudell, S. Ponrathnam, Chunnong Zhao, G. Pagliaroli, W. Z. Korth, Torrey Cullen, S. H. Huttner, F. Garufi, Rakesh Kumar, Gor Oganesyan, O. Schwarm, Bernard F. Whiting, R. L. Savage, M. Laxen, Anchal Gupta, S. Hochheim, N. A. Robertson, A. F. Brooks, P. J. Quinonez, Andrew Melatos, M. Lorenzini, Surendra Nadh Somala, David Jones, David H. Shoemaker, J. D. Callaghan, Angela Trapananti, H. Rafferty, I. Dorrington, I. Di Palma, J. G. Bartlett, Yu Huang, Geert Raaijmakers, F. Y. Khalili, Q. Chu, J. H. Briggs, Mark Hannam, Marco Cavaglia, Subroto Mukherjee, David Jonathan Hofman, Lindsay DeMarchi, H. Sun, V. JaberianHamedan, Liam Cunningham, V. Kringel, I. M. Romero-Shaw, R. Tso, Jonathan Blackman, Frances Hellman, I. Molina, Jürgen Heinze, P. J. Sutton, Tyson Littenberg, G. Valdes, A. Adams, Laura Cadonati, Ken K. Y. Ng, K. Toland, T. D. Creighton, S. Barnum, R. Kirchhoff, S. P. Jadhav, V. Fafone, Kendall Ackley, R. K. Nayak, H. Y. Chia, A. Strunk, D. Petterson, Pablo Cerdá-Durán, Vivien Raymond, B. Edelman, G. Stolle-McAllister, M. Was, Giacomo Bruno, Sheelu Abraham, J. D. Bentley, I. C. F. Wong, Peter Aufmuth, Tania Regimbau, A. J. Tanasijczuk, L. Mereni, Patrick M. Koch, S. Banagiri, T. L. Lam, José A. Font, Tomasz Bulik, N. Singh, S. B. Anderson, J. Gais, Maya Fishbach, Tim Dietrich, Manel Molina-Ruiz, S. B. Coughlin, M. Mateu-Lucena, Jessica Steinlechner, M. Kolstein, A. Neunzert, D. Fiorucci, C. L. Chan, M. Heurs, A. K. Prajapati, A. R. Wade, M. Patel, Benjamin Stappers, W. Kastaun, H. Qi, J. H. Romie, G. Kuehn, F. J. Raab, Zachariah B. Etienne, N. Mukund, Jennifer Watchi, L. Kleybolte, Daniel R. George, Susan M. Scott, E. K. Porter, V. B. Adya, T. P. Downes, C. Horst, M. Pedraza, F. Muciaccia, A. Lockwood, F. Cavalier, A. Bals, G. Baltus, Karl Gill, V. Srivastava, M. Fays, Santosh Roy, A. Allocca, A. M. Farah, M. F. Carney, A. F. Helmling-Cornell, Ajay Kumar, C. Whittle, A. K. Divakarla, M. Mondin, M. M. Hanke, H. Vocca, L. Xiao, C. M. Mow-Lowry, Sergey P. Vyatchanin, L. Aiello, R. Green, V. Sequino, C. J. Richardson, Alberto Vecchio, Geoffrey Mo, J. M. Fishner, Will M. Farr, M. Montani, Nancy Aggarwal, Anupam Sharma, Lionel London, P. Kumar, A. Singha, Matteo Breschi, László Á. Gergely, Terry G. McRae, L. G. Prokhorov, Alessandro Longo, Richard J. Oram, D. D'Urso, François Bondu, Reed Essick, S. Kandhasamy, B. Sorazu, Lili Yang, M. Branchesi, D. Y. T. Pong, R. Gustafson, P. Barneo, A. F. Vargas, Chad Hanna, A. Bramley, C. Kimball, J. Oberling, M. Pirello, Fiodor Sorrentino, A. Di Lieto, M. Saleem, Matthew Bailes, M. Vasúth, A. Malik, S. Gaudio, G. R. Johns, Michael Williams, Moritz Mehmet, C. Darsow-Fromm, A. L. Stuver, T. J. Slaven-Blair, R. S. Bankar, M. C. Milovich-Goff, J. L. Wright, S. Bagnasco, P. Fulda, D. Hoyland, J. Casanueva Diaz, V. M. Bedakihale, P. Schale, C. Van Den Broeck, J. L. Willis, M. Eisenmann, E. Sowell, Ofek Birnholtz, J. Smetana, I. Dave, B. Hughey, P. Couvares, B. Idzkowski, V. Loriette, V. Skliris, S. T. Countryman, Surabhi Sachdev, Christopher J. Moore, Alec Mishkin, R. Cavalieri, A. K. Srivastava, A. E. Pace, A. Basti, Ryan N. Lang, Krzysztof Piotrzkowski, A. E. Tolley, J.-P. Coulon, E. A. Chase, Z. Frei, A. Macquet, Daichi Tsuna, D. L. Ferguson, M. J. Szczepańczyk, Denis Martynov, Marco Bazzan, C. Ingram, L. Pinard, Charalampos Markakis, F. Badaracco, T. T. Nguyen, Andrea Chincarini, Minkyun Noh, T. Z. Summerscales, E. Payne, T. Sadecki, M. Piendibene, S. Grunewald, R. Prasanna, Alessandra Corsi, D. Laghi, E. J. Daw, Maurizio Canepa, P. H. Nguyen, Antonio Marquina, Eric Hennes, A. S. Ubhi, T. A. Ferreira, K. D. Giardina, E. M. Santos, J. K. Wofford, M. A. Page, P. W. F. Forsyth, J. S. Lange, B. E. Ewing, M. C. Tringali, E. Massera, Y. Asali, S. Raja, S. Maliakal, C. Di Giorgio, J. Bidler, R. Dean, H. J. Bulten, D. B. Tanner, K. Rose, M. Pracchia, S. E. Gossan, Albert Lazzarini, Samaya Nissanke, A. T. Tran, M. A. Bizouard, B. K. Berger, V. V. Frolov, N. V. Krishnendu, A. Singhal, Kentaro Komori, Silvia Corezzi, J.-D. Fournier, Philip F. Hopkins, Oscar Blanch, Shaon Ghosh, F. Hernandez Vivanco, S. Leavey, Hai-Ping Cheng, A. Iess, Shawn Rosofsky, T. Di Girolamo, Archisman Ghosh, A. Balsamo, S. Khadka, C. I. Torrie, Jan Harms, A. S. Sengupta, Zhihui Du, G. Ciani, S. S. Eikenberry, James Healy, P. Brockill, Y. K. Lecoeuche, G. M. Harry, K. Venkateswara, R. Cotesta, Yuri Levin, S. X. Rail, Alessandro Nagar, Nicolas Sanchis-Gual, T. Hardwick, D. Steinmeyer, J. Liu, A. Pasqualetti, M. Tse, D. S. Tsai, D. Moraru, Edward Seidel, J. Woehler, T. H. Pang, J. Zweizig, F. Nocera, Alicia M. Sintes, M. Curyło, Kun Li, E. Floden, Gianpietro Cagnoli, Kevin M. Ryan, C. Difronzo, M. Korobko, Rosa Poggiani, F. Travasso, Michał Bejger, Giuseppe Intini, A. K. Y. Li, J. Jiang, G. Vajente, S. M. Gaebel, Benno Willke, A. Grado, C. Cahillane, J. Hennig, S. Bae, E. Coccia, M. E. Zucker, B. A. Weaver, J. G. Rollins, E. Hofgard, L.-W. Wei, Irene Fiori, G. Vedovato, L. E. H. Datrier, D. B. Kozak, A. Grimaldi, P. J. King, E. L. Merilh, C. Vorvick, Bruno Giacomazzo, Yang Yang, Xing-Jiang Zhu, Alena Ananyeva, Stanislav Babak, B. D. Lackey, Bala R. Iyer, S. McCormick, P. Grassia, Kipp Cannon, M. Steinke, S. G. Crowder, D. M. Macleod, T. D. Ramirez, Carl-Johan Haster, C. Pluchar, B. L. Swinkels, F. Cleva, G. Bergmann, M. P. Ross, T. B. Edo, S. Chung, M. Pichot, Maximiliano Isi, T. C. Pechsiri, M. Boldrini, Luigi D'Onofrio, F. Vetrano, J. Brooks, V. Gayathri, S. Walsh, Miriam Cabero, Alessandra Buonanno, M. Bischi, F. Frasconi, X. Liu, Kiran Prasai, D. Bankar, A. Poverman, M. Khursheed, F. Brighenti, F. Bergamin, B. R. Becher, J. Feicht, Satya Mohapatra, Sascha Husa, G. Venugopalan, S. R. Mohite, D.B. DeBra, A. Ain, R. D. Rodriguez-Soto, Doğa Veske, J. P. Zendri, J. G. Guerrero, R. Jaume, R. A. Eisenstein, B. J. J. Slagmolen, Hee-Suk Cho, Jishnu Suresh, G. D. Meadors, V. Frey, S. Farinon, A. Pele, M. Constancio, L. K. Nuttall, T. Zelenova, Riccardo Bassiri, Magnus Manske, R. Macas, G. Billingsley, D. M. Wilken, Sebastian Steinlechner, C. A. Rose, D. Ugolini, Roberto Chierici, F. Magaña-Sandoval, O. A. Hannuksela, L. Rolland, V. Hui, A. Perreca, Fabrizio Barone, G. Gemme, M. Drago, Mairi Sakellariadou, M. T. Hübner, Guenakh Mitselmakher, V. Tiwari, N. Man, Haocun Yu, Yann Bouffanais, M. Croquette, E. M. Gretarsson, Ying Guo, S. E. Dwyer, David Keitel, V. Savant, P. Raffai, E. Goetz, Peter Fritschel, Wenxiao Wang, V. Valsan, M. Masso-Reid, S. Karki, Francesco Chiadini, G. Pillant, S. H. R. Yuen, R. Metzdorff, S. J. Cooper, J. Junker, A. Lartaux-Vollard, Gabrielle Allen, Suvadeep Bose, L. Errico, C. Olivetto, J. Glanzer, W. G. Anderson, G. Cella, Vuk Mandic, Alessandro Bertolini, R. P. Udall, H. Estelles, S. J. Rowlinson, Joey Shapiro Key, O. Edy, J. R. Sanders, Stefan Grimm, P. Chanial, Z. J. Holmes, Podila Satya Venkata Narasimha Sharma, E. K. Gustafson, S. V. Angelova, E. Maros, E. J. Fauchon-Jones, A. Yoon, M. Lormand, Piotr Jaranowski, A. S. Hines, Paul Hill, Binlei Ding, S. Sudhagar, P. Puppo, Javier M. Antelis, S. J. Kapadia, K. Haughian, G. L. Mansell, R. Gouaty, A. V. Bhandari, Z. Márka, J. Betzwieser, J. Petermann, V. Dattilo, M. Ball, D. Singh, M. Merzougui, O. de Varona, S. Appert, Y. Setyawati, G. Cho, P. Shawhan, I. Ferrante, J. N. Hohmann, S. D'Antonio, Marta Colleoni, C. Nguyen, B. A. Boom, A. M. Sergeev, H. M. Lee, Chris A. Collins, G. Mendell, Antoine Heidmann, R. Flaminio, I. Belahcene, M. C. Heintze, D. A. Melchor, F. Marion, D. Buskulic, R. Fittipaldi, Francesco Pannarale, Soichiro Morisaki, K. Merfeld, J. A. Giaime, D. Corre, Y. M. Kim, K. A. Thorne, Jonathan E. Thompson, F. Carbognani, J.-G. Ducoin, C. Affeldt, S. Meshkov, Seog Oh, A. M. Holgado, K. G. Arun, M. Fitz-Axen, R. Gray, Isabel Cordero-Carrión, Ll. M. Mir, S. Vass, R. Coyne, J. Calderón Bustillo, J. A. Rocha, P. J. Veitch, Fabrice Matichard, R. K. Lanza, P. Dupej, Eric B. Flynn, B. Gateley, Howard Pan, S. J. Jadhav, Rico K. L. Lo, A. R. Williamson, Felipe Guzman, E. A. Huerta, R. Goetz, Stefano Ansoldi, D. D. White, S. C. Tait, A. Paolone, R. J. Trudeau, Tarun Souradeep, N. A. Didio, M. A. Okada, Shubhanshu Tiwari, A. Rocchi, B. Goncharov, R. Birney, V. Villa-Ortega, W. Katzman, L. E. Sanchez, D. Hartwig, Umakant D. Rapol, E. N. Clark, Ellen S. Howell, Aldo Ejlli, R. C. Walet, V. P. Mitrofanov, Fabrizio Bobba, M. Diaz-Ortiz, R. Taylor, Giovanni Carapella, A. Chiummo, G. S. Davies, H. Overmier, Astrid Lamberts, David A. Williams, I. W. Harry, W. Del Pozzo, P. F. Cohadon, Daniel E. Holz, Vincenzo Fiumara, Edoardo Milotti, B. Lantz, E. Lalande, H. Heitmann, D. Sawant, S. Wang, Matteo Pegoraro, Piero Rettegno, E. Cesarini, Aaron Buikema, C. C. Wipf, M. J. Cowart, C. Osthelder, Michela Mapelli, J. Li, N. Radulesco, D. J. Stops, J. S. H. Lee, T. 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Hansen, Sanjeev Dhurandhar, R. M. S. Schofield, S. Sayah, N. A. Holland, Sebastiano Bernuzzi, Simone Mozzon, O. Halim, Odylio D. Aguiar, S. G. Gaonkar, Nicholas Demos, J. D. Lough, N. Sennett, Sebastien Clesse, N. Bode, Haixing Miao, Kenneth A. Strain, Jimin George, Otto A. Hannuksela, Albino Perego, Soma Mukherjee, G. A. Prodi, R. DeSalvo, B. F. Neil, P. Gupta, S. Ronchini, H. S. Chen, D. Sellers, Anuradha Gupta, F. Robinet, Fausto Acernese, K. Kuns, M. Cieślar, Valérie Martinez, Shreya Anand, M. Bitossi, C. Périgois, Cesare Barbieri, Walter Winkler, J. O'Dell, S. Katsanevas, Madeline Wade, Dániel Barta, E. Fenyvesi, Lucy E Clarke, C. Gray, G. H. Ogin, T. J. Shaffer, M. K. M. Bader, Xin Chen, R. M. Martin, Matthias H. Hennig, K. W. Tsang, H. Ohta, S. L. Danilishin, F. Di Giovanni, G. Bogaert, M. Sieniawska, A. C. Utina, Gregory Ashton, K. Chakravarti, K. L. Dooley, A. Romero, Sung-Po Chao, Fabio Marchesoni, T. Etzel, Patrick Weltevrede, A. S. Markosyan, K. Wette, M. Mantovani, E. 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Knowles, Aykutlu Dana, Martin M. Fejer, J. R. Smith, R. Bork, S. Ghonge, K. AultONeal, Marica Valentini, H. Radkins, S. Biscoveanu, P. Figura, Archana Pai, J. Sadiq, Antonios Kontos, J. D. Jones, K.S.J. Rao, D. Schaetzl, F. Paoletti, D. P. Kapasi, B. Mours, R. Cummings, D. W. Yeeles, Deep Jariwala, Fabrizio Giulio Luca Pilo, J. McIver, L. M. DaneshgaranBajastani, V. Avendano, D. Mukherjee, O. Durante, E. A. Muñiz, S. Brunett, M. C. Araya, Robert Bruntz, A. Bozzi, G. J. Kim, S. Choate, L. van der Schaaf, S. A. Pai, R. Huxford, D. Sentenac, Patrick Brady, H. Hansen, P. Ruggi, A. Puecher, Srishti Tiwari, Karsten Danzmann, Andrea H. Tapia, A. Mullavey, T. J. N. Nelson, Javier Sánchez, P. Oppermann, Filip Morawski, M. Davier, E. Schwartz, C. De Rossi, M. Punturo, Leopoldo Milano, A. R. Guimaraes, R. Mittleman, Junwei Cao, A. Bisht, Kim Janssens, Y. Boetzel, S. M. Koehlenbeck, Jonathan R. Gair, Jordan Camp, D. Tao, C. Lazzaro, G. Guixé, Xiaohui Fan, B. Ratto, Richard O'Shaughnessy, B. 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Ramirez, Td, Rapol, Ud, Reardon, Dj, Reitze, Dh, Richardson, Cj, Richardson, Jw, Ricker, Pm, Robertson, Na, Rocha, Ja, Rodriguez-Soto, Rd, Rollins, Jg, Roma, Vj, Romel, Cl, Romero-Shaw, Im, Romie, Jh, Rose, Ca, Rosofsky, Sg, Ross, Mp, Rowlinson, Sj, Sanchez, Ej, Sanchez, Jh, Sanchez, Le, Sanders, Jr, Santiago, Ka, Saravanan, Tr, Savage, Rl, Schofield, Rm, Schulte, Bw, Schutz, Bf, Scott, Sm, Shoemaker, Dh, Shoemaker, Dm, Singer, Lp, Sintes, Am, Slagmolen, Bjj, Slaven-Blair, Tj, Smith, Jr, Smith, Rje, Somala, Sn, Son, Ej, Spencer, Ap, Srivastava, Ak, Steer, Da, Stolle-McAllister, G, Stops, Dj, Strain, Ka, Stuver, Al, Summerscales, Tz, Sutton, Pj, Swinkels, Bl, Tait, Sc, Tanasijczuk, Aj, Tanner, Db, San Martin, Ent, Tasson, Jd, Thirugnanasambandam, Mp, Thompson, Je, Thondapu, Sr, Thorne, Ka, Tolley, Ae, Torrie, Ci, Melo, Ite, Tran, At, Tringali, Mc, Trudeau, Rj, Tsang, Kw, Udall, Rp, Urban, Al, Usman, Sa, Utina, Ac, van Bakel, N, van Beuzekom, M, van den Brand, Jfj, Van den Broeck, C, 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V. van, Vasúth, M., Viceré, A., Weßels, P., Yu, Hang, Yu, Haocun, Zadrożny, A., RS: FSE Grav. waves and fundamental physics, Grav. waves and fundamental physics, Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Collège de France (CdF (institution)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Joseph Louis LAGRANGE (LAGRANGE), Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), LIGO Scientific, Virgo, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF (institution))-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut des Hautes Études Scientifiques (IHES), The LIGO Scientific Collaboration, The Virgo Collaboration, and Van Swinderen Institute for Particle Physics and G
Subjects: Gravitational waves, Neutron stars, Pulsars, Gravitational wave sources, 010504 meteorology & atmospheric sciences, Astronomy, Astrophysics, Vela, 01 natural sciences, General Relativity and Quantum Cosmology, [SPI]Engineering Sciences [physics], neutron, Millisecond pulsar, emission, 010303 astronomy & astrophysics, QC, QB, Settore FIS/01, Physics, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), [PHYS]Physics [physics], Astrophysics::Instrumentation and Methods for Astrophysics, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Astrophysics - High Energy Astrophysical Phenomena, Gravitational-Waves, Pulsars, Neutron Stars, Gravitational wave, PROPER MOTION, Proper motion, gr-qc, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Neutron star, General Relativity and Quantum Cosmology (gr-qc), Gravitational-Waves, SEARCHES, Settore FIS/05 - Astronomia e Astrofisica, Pulsar, 0103 physical sciences, [CHIM]Chemical Sciences, Astrophysique, STFC, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, crab pulsar, Crab Pulsar, RCUK, Astronomy and Astrophysics, Neutron Stars, Gravitational waves, Neutron stars, Pulsars, Gravitational wave sources, LIGO, Space and Planetary Science, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: We present a search for continuous gravitational waves from five radio pulsars, comprising three recycled pulsars (PSR J0437-4715, PSR J0711-6830, and PSR J0737-3039A) and two young pulsars: the Crab pulsar (J0534+2200) and the Vela pulsar (J0835-4510). We use data from the third observing run of Advanced LIGO and Virgo combined with data from their first and second observing runs. For the first time, we are able to match (for PSR J0437-4715) or surpass (for PSR J0711-6830) the indirect limits on gravitational-wave emission from recycled pulsars inferred from their observed spin-downs, and constrain their equatorial ellipticities to be less than 10-8. For each of the five pulsars, we perform targeted searches that assume a tight coupling between the gravitational-wave and electromagnetic signal phase evolution. We also present constraints on PSR J0711-6830, the Crab pulsar, and the Vela pulsar from a search that relaxes this assumption, allowing the gravitational-wave signal to vary from the electromagnetic expectation within a narrow band of frequencies and frequency derivatives., 0, info:eu-repo/semantics/published
Published: 2020

49. The Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

Author: G. Busetto, Brian L Winer, John J. Ruan, A. A. Moiseev, Eric Charles, Steven Ritz, D. J. Suson, Luca Baldini, Simon Johnston, F. Loparco, N. Renault, W. Mitthumsiri, Na Wang, Sylvain Guiriec, I. A. Grenier, James Chiang, Jeffrey D. Scargle, Roger W. Romani, Jürgen Knödlseder, S. Germani, K. S. Wood, P. Lubrano, M. Marelli, Jayashree Roy, R. Buehler, Jun Kataoka, Gloria Spandre, Ronaldo Bellazzini, A. S. Johnson, S. Cutini, Michael Kramer, T. Ohsugi, Eleonora Troja, Miranda Jackson, Maura McLaughlin, T. Reposeur, Peter F. Michelson, Marcello Giroletti, Francesco Longo, R. C. G. Chaves, Yasunobu Uchiyama, Johann Cohen-Tanugi, M. Orienti, Alex Drlica-Wagner, Dario Gasparrini, M. Hayashida, Sylvain Chaty, Nanda Rea, E. D. Bloom, Jean Ballet, A. Morselli, Xian Hou, V. Vitale, T. Jogler, Charles D. Dermer, R. N. Manchester, D. Parent, M. E. Monzani, Andrea Belfiore, Stefano Ciprini, Bhaswati Bhattacharyya, Gemma H. Janssen, R. Rousseau, J. Lande, Scott M. Ransom, Michael Keith, Luca Latronico, P. R. den Hartog, Gino Tosti, M. Mayer, Francesco Massaro, R. E. Hughes, A. W. Chen, A. B. Hill, L. R. Cominsky, Igor V. Moskalenko, Melissa Pesce-Rollins, J. G. Thayer, M. Burgay, Elisabetta Bissaldi, Olaf Reimer, Paul S. Ray, Holger J. Pletsch, M. Tinivella, T. L. Usher, M. E. DeCesar, Jason W. T. Hessels, Paulo C. C. Freire, G. A. Caliandro, Jan Conrad, Elizabeth C. Ferrara, Takeshi Nakamori, J. M. Casandjian, Terri Brandt, Hiromitsu Takahashi, André Schulz, Patrick Weltevrede, Andrew W. Strong, M. N. Mazziotta, D. Dumora, C. Favuzzi, J. Mehault, Christo Venter, A. De Angelis, P. Fusco, L. Guillemot, D. J. Thompson, T. H. Burnett, Diego F. Torres, A. A. Abdo, E. Orlando, Gregory Desvignes, W. N. Johnson, Gilles Theureau, L. Tibaldo, S. Murgia, M. T. Wolff, C. Cecchi, Alberto Sartori, T. Glanzman, F. Piron, Rodrigo Nemmen, Matthew Kerr, Matthew G. Baring, D. Horan, Giacomo Vianello, Fernando Camilo, L. Di Venere, Gudlaugur Johannesson, O. Tibolla, Masanori Ohno, D. L. Wood, E. Hays, Y. Hanabata, G. Pivato, M. Roth, F. Gargano, Alice K. Harding, Ismaël Cognard, Benjamin Stappers, Justin Vandenbroucke, Emanuele Bonamente, J. F. Ormes, Eugenio Bottacini, T. A. Porter, Guido Barbiellini, E. J. Siskind, David A. Smith, L. Falletti, Denis Bastieri, R. Claus, Marianne Lemoine-Goumard, Johan Bregeon, D. Hadasch, Ryan Shannon, A. Possenti, A. Reimer, J. H. Panetta, M. Razzano, S. Rainò, Eric V. Gotthelf, Tsunefumi Mizuno, Filippo D'Ammando, Julie McEnery, T. Kamae, M. Brigida, Stephen E. Thorsett, R. P. Johnson, G. Chiaro, J. E. Grove, P. M. Saz Parkinson, J. S. Perkins, Paolo Giommi, Marco Ajello, J. B. Thayer, S. Larsson, S. Buson, Nicola Giglietto, A. De Luca, M. N. Lovellette, P. A. Caraveo, Persis S. Drell, Alice Allafort, Roberto Mignani, Tyrel J. Johnson, R. A. Cameron, A. Chekhtman, R. Dubois, W. B. Focke, P. Spinelli, Seth Digel, Francesco Giordano, John W. Hewitt, P. Bruel, V. Vasileiou, Matthew Wood, G. Godfrey, F. de Palma, Andrew Lyne, M.-H. Grondin, Robert R. Rando, M. Pierbattista, Cristobal M. Espinoza, Omer Celik, A. Franckowiak, Stefan Funk, Zhenwei Yang, Carmelo Sgrò, E. Nuss, David Paneque, M. Kuss, Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), PSL Research University (PSL)-PSL Research University (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), FERMI, Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Istituto Nazionale di Fisica Nucleare, sezione di Bari (INFN, sezione di Bari), National Institute for Nuclear Physics (INFN), IEEC-CSIC, Universitat Autònoma de Barcelona [Barcelona] (UAB), Laboratoire d'Astrophysique de Grenoble (LAOG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Particules de Montpellier (LUPM), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Fermi-LAT, High Energy Astrophys. & Astropart. Phys (API, FNWI), Abdo AA, Ajello M, Allafort A, Baldini L, Ballet J, Barbiellini G, Baring MG, Bastieri D, Belfiore A, Bellazzini R, Bhattacharyya B, Bissaldi E, Bloom ED, Bonamente E, Bottacini E, Brandt TJ, Bregeon J, Brigida M, Bruel P, Buehler R, Burgay M, Burnett TH, Busetto G, Buson S, Caliandro GA, Cameron RA, Camilo F, Caraveo PA, Casandjian JM, Cecchi C, Celik O, Charles E, Chaty S, Chaves RCG, Chekhtman A, Chen AW, Chiang J, Chiaro G, Ciprini S, Claus R, Cognard I, Cohen-Tanugi J, Cominsky LR, Conrad J, Cutini S, DAmmando F, De Angelis A, DeCesar ME, De Luca A, Den Hartog PR, De Palma F, Dermer CD, Desvignes G, Digel SW, Di Venere L, Drell PS, Drlica-Wagner A, Dubois R, Dumora D, Espinoza CM, Falletti L, Favuzzi C, Ferrara EC, Focke WB, Franckowiak A, Freire PCC, Funk S, Fusco P, Gargano F, Gasparrini D, Germani S, Giglietto N, Giommi P, Giordano F, Giroletti M, Glanzman T, Godfrey G, Gotthelf EV, Grenier IA, Grondin MH, Grove JE, Guillemot L, Guiriec S, Hadasch D, Hanabata Y, Harding AK, Hayashida M, Hays E, Hessels J, Hewitt J, Hill AB, Horan D, Hou X, Hughes RE, Jackson MS, Janssen GH, Jogler T, Johannesson G, Johnson RP, Johnson AS, Johnson TJ, Johnson WN, Johnston S, Kamae T, Kataoka J, Keith M, Kerr M, Knodlseder J, Kramer M, Kuss M, Lande J, Larsson S, Latronico L, Lemoine-Goumard M, Longo F, Loparco F, Lovellette MN, Lubrano P, Lyne AG, Manchester RN, Marelli M, Massaro F, Mayer M, Mazziotta MN, McEnery JE, McLaughlin MA, Mehault J, Michelson PF, Mignani RP, Mitthumsiri W, Mizuno T, Moiseev AA, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nakamori T, Nemmen R, Nuss E, Ohno M, Ohsugi T, Orienti M, Orlando E, Ormes JF, Paneque D, Panetta JH, Parent D, Perkins JS, Pesce-Rollins M, Pierbattista M, Piron F, Pivato G, Pletsch HJ, Porter TA, Possenti A, Raino S, Rando R, Ransom SM, Ray PS, Razzano M, Rea N, Reimer A, Reimer O, Renault N, Reposeur T, Ritz S, Romani RW, Roth M, Rousseau R, Roy J, Ruan J, Sartori A, Parkinson PMS, Scargle JD, Schulz A, Sgro C, Shannon R, Siskind EJ, Smith DA, Spandre G, Spinelli P, Stappers BW, Strong AW, Suson DJ, Takahashi H, Thayer JG, Thayer JB, Theureau G, Thompson DJ, Thorsett SE, Tibaldo L, Tibolla O, Tinivella M, Torres DF, Tosti G, Troja E, Uchiyama Y, Usher TL, Vandenbroucke J, Vasileiou V, Venter C, Vianello G, Vitale V, Wang N, Weltevrede P, Winer BL, Wolff MT, Wood DL, Wood KS, Wood M, Yang Z, Abdo, A. A., Ajello, M., Allafort, A., Baldini, L., Ballet, J., BARBIELLINI AMIDEI, Guido, Baring, M. G., Bastieri, D., Belfiore, A., Bellazzini, R., Bhattacharyya, B., Bissaldi, Elisabetta, Bloom, E. D., Bonamente, E., Bottacini, E., Brandt, T. J., Bregeon, J., Brigida, M., Bruel, P., Buehle, R., Burgay, M., Burnett, T. H., Busetto, G., Buson, S., Caliandro, G. A., Cameron, R. A., Camilo, F., Caraveo, P. A., Casandjian, J. M., Cecchi, C., Çelik, Ö., Charles, E., Chaty, S., Chaves, R. C. G., Chekhtman, A., Chen, A. W., Chiang, J., Chiaro, G., Ciprini, S., Claus, R., Cognard, I., Cohen Tanugi, J., Cominsky, L. R., Conrad, J., Cutini, S., D'Ammando, F., de Angelis, A., Decesar, M. E., De Luca, A., den Hartog, P. R., de Palma, F., Dermer, C. D., Desvignes, G., Digel, S. W., Di Venere, L., Drell, P. S., Drlica Wagner, A., Dubois, R., Dumora, D., Espinoza, C. M., Falletti, L., Favuzzi, C., Ferrara, E. C., Focke, W. B., Franckowiak, A., Freire, P. C. C., Funk, S., Fusco, P., Gargano, F., Gasparrini, D., Germani, S., Giglietto, N., Giommi, P., Giordano, F., Giroletti, M., Glanzman, T., Godfrey, G., Gotthelf, E. V., Grenier, I. A., Grondin, M. H., Grove, J. E., Guillemot, L., Guiriec, S., Hadasch, D., Hanabata, Y., Harding, A. K., Hayashida, M., Hays, E., Hessels, J., Hewitt, J., Hill, A. B., Horan, D., Hou, X., Hughes, R. E., Jackson, M. S., Janssen, G. H., Jogler, T., Jóhannesson, G., Johnson, R. P., Johnson, A. S., Johnson, T. J., Johnson, W. N., Johnston, S., Kamae, T., Kataoka, J., Keith, M., Kerr, M., Knödlseder, J., Kramer, M., Kuss, M., Lande, J., Larsson, S., Latronico, L., Lemoine Goumard, M., Longo, Francesco, Loparco, F., Lovellette, M. N., Lubrano, P., Lyne, A. G., Manchester, R. N., Marelli, M., Massaro, F., Mayer, M., Mazziotta, M. N., Mcenery, J. E., Mclaughlin, M. A., Mehault, J., Michelson, P. F., Mignani, R. P., Mitthumsiri, W., Mizuno, T., Moiseev, A. A., Monzani, M. E., Morselli, A., Moskalenko, I. V., Murgia, S., Nakamori, T., Nemmen, R., Nuss, E., Ohno, M., Ohsugi, T., Orienti, M., Orlando, E., Ormes, J. F., Paneque, D., Panetta, J. H., Parent, D., Perkins, J. S., Pesce Rollins, M., Pierbattista, M., Piron, F., Pivato, G., Pletsch, H. J., Porter, T. A., Possenti, A., Rainò, S., Rando, R., Ransom, S. M., Ray, P. S., Razzano, M., Rea, N., Reimer, A., Reimer, O., Renault, N., Reposeur, T., Ritz, S., Romani, R. W., Roth, M., Rousseau, R., Roy, J., Ruan, J., Sartori, A., Saz Parkinson, P. M., Scargle, J. D., Schulz, A., Sgrò, C., Shannon, R., Siskind, E. J., Smith, D. A., Spandre, G., Spinelli, P., Stappers, B. W., Strong, A. W., Suson, D. J., Takahashi, H., Thayer, J. G., Thayer, J. B., Theureau, G., Thompson, D. J., Thorsett, S. E., Tibaldo, L., Tibolla, O., Tinivella, M., Torres, D. F., Tosti, G., Troja, E., Uchiyama, Y., Usher, T. L., Vandenbroucke, J., Vasileiou, V., Venter, C., Vianello, G., Vitale, V., Wang, N., Weltevrede, P., Winer, B. L., Wolff, M. T., Wood, D. L., Wood, K. S., Wood, M., and Yang, Z.
Subjects: Catalogs pulsars, general stars, neutron, catalog, CRAB PULSAR, Astrophysics, 01 natural sciences, Pulsar wind nebula, general [pulsars], law.invention, neutron, Millisecond pulsar, law, catalogs, pulsars: general, stars: neutron, 010303 astronomy & astrophysics, general stars, Physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::Instrumentation and Methods for Astrophysics, WIND NEBULA, SUPERNOVA REMNANT G21.5-0.9, Astrophysics - High Energy Astrophysical Phenomena, PHOTON IMAGING CAMERA, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], WHITE-DWARF COMPANION, MIDDLE-AGED PULSAR, DEEP OPTICAL OBSERVATIONS, NANCAY RADIO TELESCOPE, MILLISECOND PULSARS, LIGHT CURVES, Astrophysics::High Energy Astrophysical Phenomena, Catalogs pulsars, Astrophysics::Cosmology and Extragalactic Astrophysics, catalogs , pulsars: general , stars: neutron, Telescope, neutron [stars], Pulsar, 0103 physical sciences, Astrophysics::Galaxy Astrophysics, 010308 nuclear & particles physics, Crab Pulsar, catalogs – pulsars: general – stars: neutron, Astronomy, Astronomy and Astrophysics, Neutron star, Space and Planetary Science, ddc:520, X-ray pulsar, Fermi Gamma-ray Space Telescope
Abstract: This catalog summarizes 117 high-confidence > 0.1 GeV gamma-ray pulsar detections using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite. Half are neutron stars discovered using LAT data, through periodicity searches in gamma-ray and radio data around LAT unassociated source positions. The 117 pulsars are evenly divided into three groups: millisecond pulsars, young radio-loud pulsars, and young radio-quiet pulsars. We characterize the pulse profiles and energy spectra and derive luminosities when distance information exists. Spectral analysis of the off-peak phase intervals indicates probable pulsar wind nebula emission for four pulsars, and off-peak magnetospheric emission for several young and millisecond pulsars. We compare the gamma-ray properties with those in the radio, optical, and X-ray bands. We provide flux limits for pulsars with no observed gamma-ray emission, highlighting a small number of gamma-faint, radio-loud pulsars. The large, varied gamma-ray pulsar sample constrains emission models. Fermi's selection biases complement those of radio surveys, enhancing comparisons with predicted population distributions., Comment: 145 pages. Online files at http://fermi.gsfc.nasa.gov/ssc/data/access/lat/2nd_PSR_catalog/ A typo in the value of the photon flux for CTA 1 (PSR J0007+7303) has been corrected in Table 9. NASA ADS at http://cdsads.u-strasbg.fr/abs/2013ApJS..208...17A
Published: 2013

50. Observation of the Crab pulsar, PSR 0531 + 21, at 0.2-6.0 MeV with the FIGARO II experiment

Author: J. L. Masnou, E. Barouch, Livio Scarsi, Bruno Sacco, M. Salvati, Gaetano Gerardi, Enrico Costa, M. Niel, B. Parlier, B. Agrinier, Teresa Mineo, P. Mandrou, C. Hote, Enrico Massaro, P. M. Mcculloch, Agrinier, B, Masnou, Jl, Parlier, B, Niel, M, Mandrou, P, Vedrenne, G, Gerardi, G, Mineo, T, Sacco, B, Scarsi, L, Costa, E, Massaro, E, Matt, Giorgio, Salvati, M, and Lyne, Ag
Subjects: Physics, Crab Nebula, Pulsar, Space and Planetary Science, Crab Pulsar, Astrophysics::High Energy Astrophysical Phenomena, Astronomy and Astrophysics, Astrophysics, Gamma-ray astronomy, Light curve, Electromagnetic radiation, Radio wave, Luminosity
Abstract: Observations of the Crab pulsar (PSR 0531 + 21) in the energy range 0.2-6 MeV have been made with the balloon-borne Figaro II experiment. The gross appearance of the light curve is characterized by the well-known double-peak structure with a phase separation of 0.4. The data confirm that the second pulse is the dominant feature, and the interpulse region is more luminous than in other energy ranges. Above about 0.5 MeV, an extra structure was detected in the light curve, with two features at a phase lag of 0.4 as the main one. Phase-resolved spectroscopy indicates that the first peak spectrum is concave upward, and the second one is concave downward, while the averaged spectrum is well represented by a single power law with slope 2.2. The good timing accuracy of Figaro made it possible to measure a delay between gamma rays and radio waves of 300 + or - 70 microsec, that if produced by dispersion, implies a value of DM fitting very well the radio measurements 2 months before and after the observation. 29 refs.
Published: 1990

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