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32 results on '"Rich, J. A."'

1. Optical Spectroscopy of Type Ia Supernovae by the Carnegie Supernova Projects I and II

Author

Morrell, N., primary, Phillips, M. M., additional, Folatelli, G., additional, Stritzinger, M. D., additional, Hamuy, M., additional, Suntzeff, N. B., additional, Hsiao, E. Y., additional, Taddia, F., additional, Burns, C. R., additional, Hoeflich, P., additional, Ashall, C., additional, Contreras, C., additional, Galbany, L., additional, Lu, J., additional, Piro, A. L., additional, Anais, J., additional, Baron, E., additional, Burrow, A., additional, Busta, L., additional, Campillay, A., additional, Castellón, S., additional, Corco, C., additional, Diamond, T., additional, Freedman, W. L., additional, Gonzalez, C., additional, Krisciunas, K., additional, Kumar, S., additional, Persson, S. E., additional, Serón, J., additional, Shahbandeh, M., additional, Torres, S., additional, Uddin, S. A., additional, Anderson, J. P., additional, Baltay, C., additional, Gall, C., additional, Goobar, A., additional, Hadjiyska, E., additional, Holmbo, S., additional, Kasliwal, M., additional, Lidman, C., additional, Marion, G. H., additional, Mazzali, P. A., additional, Nugent, P., additional, Perlmutter, S., additional, Pignata, G., additional, Rabinowitz, D., additional, Roth, M., additional, Ryder, S. D., additional, Shappee, B. J., additional, Vinkó, J., additional, Wheeler, J. C., additional, de Jaeger, T., additional, Lira, P., additional, Ruiz, M. T., additional, Rich, J. A., additional, Prieto, J. L., additional, Di Mille, F., additional, Osip, D., additional, Blanc, G., additional, and Palunas, P., additional

Published
2024
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2. Improved Cosmological Constraints from New, Old, and Combined Supernova Data Sets

Author

Kowalski, M, Rubin, D, Aldering, G, Agostinho, RJ, Amadon, A, Amanullah, R, Balland, C, Barbary, K, Blanc, G, Challis, PJ, Conley, A, Connolly, NV, Covarrubias, R, Dawson, KS, Deustua, SE, Ellis, R, Fabbro, S, Fadeyev, V, Fan, X, Farris, B, Folatelli, G, Frye, BL, Garavini, G, Gates, EL, Germany, L, Goldhaber, G, Goldman, B, Goobar, A, Groom, DE, Haissinski, J, Hardin, D, Hook, I, Kent, S, Kim, AG, Knop, RA, Lidman, C, Linder, EV, Mendez, J, Meyers, J, Miller, GJ, Moniez, M, Mourão, AM, Newberg, H, Nobili, S, Nugent, PE, Pain, R, Perdereau, O, Perlmutter, S, Phillips, MM, Prasad, V, Quimby, R, Regnault, N, Rich, J, Rubenstein, EP, Ruiz-Lapuente, P, Santos, FD, Schaefer, BE, Schommer, RA, Smith, RC, Soderberg, AM, Spadafora, AL, Strolger, L-G, Strovink, M, Suntzeff, NB, Suzuki, N, Thomas, RC, Walton, NA, Wang, L, Wood-Vasey, WM, and Yun, JL

Subjects
Particle and High Energy Physics, Physical Sciences, cosmological parameters, cosmology: observations, supernovae: general, astro-ph, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics, Space sciences
Abstract

We present a new compilation of Type Ia supernovae (SNe Ia), a new data set of low-redshift nearby-Hubble-flow SNe, and new analysis procedures to work with these heterogeneous compilations. This "Union" compilation of 414 SNe Ia, which reduces to 307 SNe after selection cuts, includes the recent large samples of SNe Ia from the Supernova Legacy Survey and ESSENCE Survey, the older data sets, as well as the recently extended data set of distant supernovae observed with the Hubble Space Telescope (HST). A single, consistent, and blind analysis procedure is used for all the various SN Ia subsamples, and a new procedure is implemented that consistently weights the heterogeneous data sets and rejects outliers. We present the latest results from this Union compilation and discuss the cosmological constraints from this new compilation and its combination with other cosmological measurements (CMB and BAO). The constraint we obtain from supernovae on the dark energy density isΩΛ = 0.713-0.029+0.027(stat) -0.039+0.036(sys), for a flat, ACDM universe. Assuming a constant equation of state parameter, w, the combined constraints from SNe, BAO, and CMB give w = -0.969-0.063+0.059(stat) -0.066+0.063(sys). While our results are consistent with a cosmological constant, we obtain only relatively weak constraints on a w that varies with redshift. In particular, the current SN data do not yet significantly constrain w at z > 1. With the addition of our new nearby Hubble-flow SNe Ia, these resulting cosmological constraints are currently the tightest available. © 2008. The American Astronomical Society. All rights reserved.

Published
2008

3. Rates and Properties of Type Ia Supernovae as a Function of Mass and Star Formation in Their Host Galaxies

Author

Sullivan, M, Le Borgne, D, Pritchet, CJ, Hodsman, A, Neill, JD, Howell, DA, Carlberg, RG, Astier, P, Aubourg, E, Balam, D, Basa, S, Conley, A, Fabbro, S, Fouchez, D, Guy, J, Hook, I, Pain, R, Palanque-Delabrouille, N, Perrett, K, Regnault, N, Rich, J, Taillet, R, Baumont, S, Bronder, J, Ellis, RS, Filiol, M, Lusset, V, Perlmutter, S, Ripoche, P, and Tao, C

Subjects
distance scale, galaxies : evolution, supernovae : general, surveys, astro-ph, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

We show that Type Ia supernovae (SNe Ia) are formed within both very young and old stellar populations, with observed rates that depend on the stellar mass and mean star formation rates (SFRs) of their host galaxies. Models in which the SN Ia rate depends solely on host galaxy stellar mass are ruled out with >99% confidence. Our analysis is based on 100 spectroscopically confirmed SNe Ia, plus 24 photometrically classified events, all from the Supernova Legacy Survey (SNLS) and distributed over 0.2 < z < 0.75. We estimate stellar masses and SFRs for the SN Ia host galaxies by fitting their broadband spectral energy distributions with the galaxy spectral synthesis code PÉGASE.2. We show that the SN Ia rate per unit mass is proportional to the specific SFR of the parent galaxies - more vigorously star-forming galaxies host more SNe Ia per unit stellar mass, broadly equivalent to the trend of increasing SN Ia rate in later type galaxies seen in the local universe. Following earlier suggestions for a simple "two-component" model approximating the SN Ia rate, we find bivariate linear dependencies of the SN Ia rate on both the stellar masses and the mean SFRs of the host systems. We find that the SN Ia rate can be well represented as the sum of 5.3 ± 1.1 × 10-14 SNe yr -1M⊙-1 and 3.9 ± 0.7 × 10-4 SNe yr-1 (M⊙ yr-1) -1 of star formation. We also demonstrate a dependence of distant SN Ia light-curve shapes on star formation in the host galaxy, similar to trends observed locally. Passive galaxies, with no star formation, preferentially host faster declining/dimmer SNe Ia, while brighter events are found in systems with ongoing star formation. © 2006. The American Astronomical Society. All rights reserved.

Published
2006

4. Metallicity, Ionization Parameter, and Pressure Variations of H ii Regions in the TYPHOON Spiral Galaxies: NGC 1566, NGC 2835, NGC 3521, NGC 5068, NGC 5236, and NGC 7793

Author

Grasha, K., primary, Chen, Q. H., additional, Battisti, A. J., additional, Acharyya, A., additional, Ridolfo, S., additional, Poehler, E., additional, Mably, S., additional, Verma, A. A., additional, Hayward, K. L., additional, Kharbanda, A., additional, Poetrodjojo, H., additional, Seibert, M., additional, Rich, J. A., additional, Madore, B. F., additional, and Kewley, L. J., additional

Published
2022
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5. Massive Star Cluster Formation and Destruction in Luminous Infrared Galaxies in GOALS. II. An ACS/WFC3 Survey of Nearby LIRGs

Author

Linden, S. T., primary, Evans, A. S., additional, Larson, K., additional, Privon, G. C., additional, Armus, L., additional, Rich, J., additional, Díaz-Santos, T., additional, Murphy, E. J., additional, Song, Y., additional, Barcos-Muñoz, L., additional, Howell, J., additional, Charmandaris, V., additional, Inami, H., additional, U, V., additional, Surace, J. A., additional, Mazzarella, J. M., additional, and Calzetti, D., additional

Published
2021
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6. Star-forming Clumps in Local Luminous Infrared Galaxies

Author

Larson, K. L., primary, Díaz-Santos, T., additional, Armus, L., additional, Privon, G. C., additional, Linden, S. T., additional, Evans, A. S., additional, Howell, J., additional, Charmandaris, V., additional, U, V., additional, Sanders, D. B., additional, Stierwalt, S., additional, Barcos-Muñoz, L., additional, Rich, J., additional, Medling, A., additional, Cook, D., additional, Oklopĉić, A., additional, Murphy, E. J., additional, and Bonfini, P., additional

Published
2020
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7. A Spectacular Radio Flare from XRF 050416a at 40 Days and Implications for the Nature of X-Ray Flashes

Author

Soderberg, A. M, Nakar, E, Cenko, S. B, Cameron, P. B, Frail, D. A, Kulkarni, S. R, Fox, D. B, Berger, E, Gal-Yam, A, Moon, D-S, Price, P. A, Anderson, G, Schmidt, B. P, Salvo, M, Rich, J, Rau, A, Ofek, E. O, Chevalier, R. A, Hamuy, M, Harrison, F. A, Kumar, P, MacFadyen, A, McCarthy, P. J, Park, H. S, and Peterson, B. A

Subjects
Astronomy
Abstract

We present detailed optical, near-infrared, and radio observations of the X-ray flash 050416a obtained with Palomar and Siding Springs Observatories as well as HST and the VLA, placing this event among the best-studied X-ray flashes to date. In addition, we present an optical spectrum from Keck LRIS from which we measure the redshift of the burst, Z=0.6528. At this redshift the isotropic-equivalent prompt energy release was about 10(exp 51) erg, and using a standard afterglow synchrotron model we find that the blastwave kinetic energy is a factor of 10 larger, E-K,iso approximately equals 10 (exp 52) erg. The lack of an observed jet break to t - 20 days indicates that the opening angle is larger than 7 deg and the total beaming-corrected relativistic energy is larger than 10 exp (50) erg. We further show that the burst produced a strong radio flare at t is similar to 40 days accompanied by an observed flattening in the X-ray band which we attribute to an abrupt circumburst density jump or an episode of energy injection (either from a refreshed shock or off-axis ejecta). Late-time observations with HST show evidence for an associated supernova with peak optical luminosity roughly comparable to that of SN 1998bw. Next, we show that the host galaxy of XRF 050416a is actively forming stars at a rate of at least 2 M-solar per year with a luminosity of L-B is similar to 0.5L* and metallicity of Z is similar to 0.2-0.8 Z-solar. Finally, we discuss the nature of XRF 050416a in the context of short-hard gamma-ray bursts and under the framework of off-axis and dirty fireball models for X-ray flashes.

Published
2007
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9. Massive Star Cluster Formation and Destruction in Luminous Infrared Galaxies in GOALS

Author

Linden, S. T., primary, Evans, A. S., additional, Rich, J., additional, Larson, K. L., additional, Armus, L., additional, Díaz-Santos, T., additional, Privon, G. C., additional, Howell, J., additional, Inami, H., additional, Kim, D.-C., additional, Chien, L.-H., additional, Vavilkin, T., additional, Mazzarella, J. M., additional, Modica, F., additional, Surace, J. A., additional, Manning, S., additional, Abdullah, A., additional, Blake, A., additional, Yarber, A., additional, and Lambert, T., additional

Published
2017
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10. STAR FORMATION SUPPRESSION IN COMPACT GROUP GALAXIES: A NEW PATH TO QUENCHING?

Author

Alatalo, K., primary, Appleton, P. N., additional, Lisenfeld, U., additional, Bitsakis, T., additional, Lanz, L., additional, Lacy, M., additional, Charmandaris, V., additional, Cluver, M., additional, Dopita, M. A., additional, Guillard, P., additional, Jarrett, T., additional, Kewley, L. J., additional, Nyland, K., additional, Ogle, P. M., additional, Rasmussen, J., additional, Rich, J. A., additional, Verdes-Montenegro, L., additional, Xu, C. K., additional, and Yun, M., additional

Published
2015
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11. ON THE DISTANCE OF THE GLOBULAR CLUSTER M4 (NGC 6121) USING RR LYRAE STARS. I. OPTICAL AND NEAR-INFRARED PERIOD-LUMINOSITY AND PERIOD-WESENHEIT RELATIONS

Author

Braga, V. F., primary, Dall'Ora, M., additional, Bono, G., additional, Stetson, P. B., additional, Ferraro, I., additional, Iannicola, G., additional, Marengo, M., additional, Neeley, J., additional, Persson, S. E., additional, Buonanno, R., additional, Coppola, G., additional, Freedman, W., additional, Madore, B. F., additional, Marconi, M., additional, Matsunaga, N., additional, Monson, A., additional, Rich, J., additional, Scowcroft, V., additional, and Seibert, M., additional

Published
2015
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12. STRONG FAR-INFRARED COOLING LINES, PECULIAR CO KINEMATICS, AND POSSIBLE STAR-FORMATION SUPPRESSION IN HICKSON COMPACT GROUP 57

Author

Alatalo, K., primary, Appleton, P. N., additional, Lisenfeld, U., additional, Bitsakis, T., additional, Guillard, P., additional, Charmandaris, V., additional, Cluver, M., additional, Dopita, M. A., additional, Freeland, E., additional, Jarrett, T., additional, Kewley, L. J., additional, Ogle, P. M., additional, Rasmussen, J., additional, Rich, J. A., additional, Verdes-Montenegro, L., additional, Xu, C. K., additional, and Yun, M., additional

Published
2014
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13. MID-INFRARED PROPERTIES OF LUMINOUS INFRARED GALAXIES. II. PROBING THE DUST AND GAS PHYSICS OF THE GOALS SAMPLE

Author

Stierwalt, S., primary, Armus, L., additional, Charmandaris, V., additional, Diaz-Santos, T., additional, Marshall, J., additional, Evans, A. S., additional, Haan, S., additional, Howell, J., additional, Iwasawa, K., additional, Kim, D. C., additional, Murphy, E. J., additional, Rich, J. A., additional, Spoon, H. W. W., additional, Inami, H., additional, Petric, A. O., additional, and U, V., additional

Published
2014
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14. THE ALLWISE MOTION SURVEY AND THE QUEST FOR COLD SUBDWARFS

Author

Kirkpatrick, J. Davy, primary, Schneider, Adam, additional, Fajardo-Acosta, Sergio, additional, Gelino, Christopher R., additional, Mace, Gregory N., additional, Wright, Edward L., additional, Logsdon, Sarah E., additional, McLean, Ian S., additional, Cushing, Michael C., additional, Skrutskie, Michael F., additional, Eisenhardt, Peter R., additional, Stern, Daniel, additional, Baloković, Mislav, additional, Burgasser, Adam J., additional, Faherty, Jacqueline K., additional, Lansbury, George B., additional, Rich, J. A., additional, Skrzypek, Nathalie, additional, Fowler, John W., additional, Cutri, Roc M., additional, Masci, Frank J., additional, Conrow, Tim, additional, Grillmair, Carl J., additional, McCallon, Howard L., additional, Beichman, Charles A., additional, and Marsh, Kenneth A., additional

Published
2014
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16. TWO SUPERLUMINOUS SUPERNOVAE FROM THE EARLY UNIVERSE DISCOVERED BY THE SUPERNOVA LEGACY SURVEY

Author

Howell, D. A., primary, Kasen, D., additional, Lidman, C., additional, Sullivan, M., additional, Conley, A., additional, Astier, P., additional, Balland, C., additional, Carlberg, R. G., additional, Fouchez, D., additional, Guy, J., additional, Hardin, D., additional, Pain, R., additional, Palanque-Delabrouille, N., additional, Perrett, K., additional, Pritchet, C. J., additional, Regnault, N., additional, Rich, J., additional, and Ruhlmann-Kleider, V., additional

Published
2013
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17. MID-INFRARED ATOMIC FINE-STRUCTURE EMISSION-LINE SPECTRA OF LUMINOUS INFRARED GALAXIES:SPITZER/IRS SPECTRA OF THE GOALS SAMPLE

Author

Inami, H., primary, Armus, L., additional, Charmandaris, V., additional, Groves, B., additional, Kewley, L., additional, Petric, A., additional, Stierwalt, S., additional, Díaz-Santos, T., additional, Surace, J., additional, Rich, J., additional, Haan, S., additional, Howell, J., additional, Evans, A. S., additional, Mazzarella, J., additional, Marshall, J., additional, Appleton, P., additional, Lord, S., additional, Spoon, H., additional, Frayer, D., additional, Matsuhara, H., additional, and Veilleux, S., additional

Published
2013
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18. SPECTROSCOPIC OBSERVATIONS OF SN 2012fr: A LUMINOUS, NORMAL TYPE Ia SUPERNOVA WITH EARLY HIGH-VELOCITY FEATURES AND A LATE VELOCITY PLATEAU

Author

Childress, M. J., primary, Scalzo, R. A., additional, Sim, S. A., additional, Tucker, B. E., additional, Yuan, F., additional, Schmidt, B. P., additional, Cenko, S. B., additional, Silverman, J. M., additional, Contreras, C., additional, Hsiao, E. Y., additional, Phillips, M., additional, Morrell, N., additional, Jha, S. W., additional, McCully, C., additional, Filippenko, A. V., additional, Anderson, J. P., additional, Benetti, S., additional, Bufano, F., additional, de Jaeger, T., additional, Forster, F., additional, Gal-Yam, A., additional, Le Guillou, L., additional, Maguire, K., additional, Maund, J., additional, Mazzali, P. A., additional, Pignata, G., additional, Smartt, S., additional, Spyromilio, J., additional, Sullivan, M., additional, Taddia, F., additional, Valenti, S., additional, Bayliss, D. D. R., additional, Bessell, M., additional, Blanc, G. A., additional, Carson, D. J., additional, Clubb, K. I., additional, de Burgh-Day, C., additional, Desjardins, T. D., additional, Fang, J. J., additional, Fox, O. D., additional, Gates, E. L., additional, Ho, I.-T., additional, Keller, S., additional, Kelly, P. L., additional, Lidman, C., additional, Loaring, N. S., additional, Mould, J. R., additional, Owers, M., additional, Ozbilgen, S., additional, Pei, L., additional, Pickering, T., additional, Pracy, M. B., additional, Rich, J. A., additional, Schaefer, B. E., additional, Scott, N., additional, Stritzinger, M., additional, Vogt, F. P. A., additional, and Zhou, G., additional

Published
2013
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21. THE RISE TIME OF NORMAL AND SUBLUMINOUS TYPE Ia SUPERNOVAE

Author

González-Gaitán, S., primary, Conley, A., additional, Bianco, F. B., additional, Howell, D. A., additional, Sullivan, M., additional, Perrett, K., additional, Carlberg, R., additional, Astier, P., additional, Balam, D., additional, Balland, C., additional, Basa, S., additional, Fouchez, D., additional, Fourmanoit, N., additional, Graham, M. L., additional, Guy, J., additional, Hardin, D., additional, Hook, I. M., additional, Lidman, C., additional, Pain, R., additional, Palanque-Delabrouille, N., additional, Pritchet, C. J., additional, Regnault, N., additional, Rich, J., additional, and Ruhlmann-Kleider, V., additional

Published
2011
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22. CONSTRAINING TYPE Ia SUPERNOVAE PROGENITORS FROM THREE YEARS OF SUPERNOVA LEGACY SURVEY DATA

Author

Bianco, F. B., primary, Howell, D. A., additional, Sullivan, M., additional, Conley, A., additional, Kasen, D., additional, González-Gaitán, S., additional, Guy, J., additional, Astier, P., additional, Balland, C., additional, Carlberg, R. G., additional, Fouchez, D., additional, Fourmanoit, N., additional, Hardin, D., additional, Hook, I., additional, Lidman, C., additional, Pain, R., additional, Palanque-Delabrouille, N., additional, Perlmutter, S., additional, Perrett, K. M., additional, Pritchet, C. J., additional, Regnault, N., additional, Rich, J., additional, and Ruhlmann-Kleider, V., additional

Published
2011
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23. SNLS3: CONSTRAINTS ON DARK ENERGY COMBINING THE SUPERNOVA LEGACY SURVEY THREE-YEAR DATA WITH OTHER PROBES

Author

Sullivan, M., primary, Guy, J., additional, Conley, A., additional, Regnault, N., additional, Astier, P., additional, Balland, C., additional, Basa, S., additional, Carlberg, R. G., additional, Fouchez, D., additional, Hardin, D., additional, Hook, I. M., additional, Howell, D. A., additional, Pain, R., additional, Palanque-Delabrouille, N., additional, Perrett, K. M., additional, Pritchet, C. J., additional, Rich, J., additional, Ruhlmann-Kleider, V., additional, Balam, D., additional, Baumont, S., additional, Ellis, R. S., additional, Fabbro, S., additional, Fakhouri, H. K., additional, Fourmanoit, N., additional, González-Gaitán, S., additional, Graham, M. L., additional, Hudson, M. J., additional, Hsiao, E., additional, Kronborg, T., additional, Lidman, C., additional, Mourao, A. M., additional, Neill, J. D., additional, Perlmutter, S., additional, Ripoche, P., additional, Suzuki, N., additional, and Walker, E. S., additional

Published
2011
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25. SUBLUMINOUS TYPE Ia SUPERNOVAE AT HIGH REDSHIFT FROM THE SUPERNOVA LEGACY SURVEY

Author

González-Gaitán, S., primary, Perrett, K., additional, Sullivan, M., additional, Conley, A., additional, Howell, D. A., additional, Carlberg, R. G., additional, Astier, P., additional, Balam, D., additional, Balland, C., additional, Basa, S., additional, Fouchez, D., additional, Guy, J., additional, Hardin, D., additional, Hook., I. M., additional, Pain, R., additional, Pritchet, C. J., additional, Regnault, N., additional, Rich, J., additional, and Lidman, C., additional

Published
2011
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27. Clustering of Supernova Ia Host Galaxies

Author

Carlberg, R. G., primary, Sullivan, M., additional, Le Borgne, D., additional, Conley, A., additional, Howell, D. A., additional, Perrett, K., additional, Astier, P., additional, Balam, D., additional, Balland, C., additional, Basa, S., additional, Hardin, D., additional, Fouchez, D., additional, Guy, J., additional, Hook, I., additional, Pain, R., additional, Pritchet, C. J., additional, Regnault, N., additional, Rich, J., additional, and Perlmutter, S., additional

Published
2008
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28. AnHSTStudy of the Supernovae Accompanying GRB 040924 and GRB 041006

Author

Soderberg, A. M., primary, Kulkarni, S. R., additional, Price, P. A., additional, Fox, D. B., additional, Berger, E., additional, Moon, D.‐S., additional, Cenko, S. B., additional, Gal‐Yam, A., additional, Frail, D. A., additional, Chevalier, R. A., additional, Cowie, L., additional, Da Costa, G. S., additional, MacFadyen, A., additional, McCarthy, P. J., additional, Noel, N., additional, Park, H. S., additional, Peterson, B. A., additional, Phillips, M. M., additional, Rauch, M., additional, Rest, A., additional, Rich, J., additional, Roth, K., additional, Roth, M., additional, Schmidt, B. P., additional, Smith, R. C., additional, and Wood, P. R., additional

Published
2006
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29. Gemini Spectroscopy of Supernovae from the Supernova Legacy Survey: Improving High‐Redshift Supernova Selection and Classification

Author

Howell, D. A., primary, Sullivan, M., additional, Perrett, K., additional, Bronder, T. J., additional, Hook, I. M., additional, Astier, P., additional, Aubourg, E., additional, Balam, D., additional, Basa, S., additional, Carlberg, R. G., additional, Fabbro, S., additional, Fouchez, D., additional, Guy, J., additional, Lafoux, H., additional, Neill, J. D., additional, Pain, R., additional, Palanque‐Delabrouille, N., additional, Pritchet, C. J., additional, Regnault, N., additional, Rich, J., additional, Taillet, R., additional, Knop, R., additional, McMahon, R. G., additional, Perlmutter, S., additional, and Walton, N. A., additional

Published
2005
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30. Afterglows, Redshifts, and Properties ofSwiftGamma‐Ray Bursts

Author

Berger, E., primary, Kulkarni, S. R., additional, Fox, D. B., additional, Soderberg, A. M., additional, Harrison, F. A., additional, Nakar, E., additional, Kelson, D. D., additional, Gladders, M. D., additional, Mulchaey, J. S., additional, Oemler, A., additional, Dressler, A., additional, Cenko, S. B., additional, Price, P. A., additional, Schmidt, B. P., additional, Frail, D. A., additional, Morrell, N., additional, Gonzalez, S., additional, Krzeminski, W., additional, Sari, R., additional, Gal‐Yam, A., additional, Moon, D.‐S., additional, Penprase, B. E., additional, Jayawardhana, R., additional, Scholz, A., additional, Rich, J., additional, Peterson, B. A., additional, Anderson, G., additional, McNaught, R., additional, Minezaki, T., additional, Yoshii, Y., additional, Cowie, L. L., additional, and Pimbblet, K., additional

Published
2005
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31. EROS and MACHO Combined Limits on Planetary-Mass Dark Matter in the Galactic Halo

Author

Alcock, C., primary, Allsman, R. A., additional, Alves, D., additional, Ansari, R., additional, Aubourg, É., additional, Axelrod, T. S., additional, Bareyre, P., additional, Beaulieu, J.-Ph., additional, Becker, A. C., additional, Bennett, D. P., additional, Brehin, S., additional, Cavalier, F., additional, Char, S., additional, Cook, K. H., additional, Ferlet, R., additional, Fernandez, J., additional, Freeman, K. C., additional, Griest, K., additional, Grison, Ph., additional, Gros, M., additional, Gry, C., additional, Guibert, J., additional, Lachièze-Rey, M., additional, Laurent, B., additional, Lehner, M. J., additional, Lesquoy, É., additional, Magneville, C., additional, Marshall, S. L., additional, Maurice, É., additional, Milsztajn, A., additional, Minniti, D., additional, Moniez, M., additional, Moreau, O., additional, Moscoso, L., additional, Palanque-Delabrouille, N., additional, Peterson, B. A., additional, Pratt, M. R., additional, Prévôt, L., additional, Queinnec, F., additional, Quinn, P. J., additional, Renault, C., additional, Rich, J., additional, Spiro, M., additional, Stubbs, C. W., additional, Sutherland, W., additional, Tomaney, A., additional, Vandehei, T., additional, Vidal-Madjar, A., additional, Vigroux, L., additional, and Zylberajch, S., additional

Published
1998
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