Optical and Radio Observations of the Afterglow from GRB990510: Evidence for a Jet

Autor: Harrison, F. A., Bloom, J. S., Frail, D. A., Sari, R., Kulkarni, S. R., Djorgovski, S. G., Axelrod, T., Mould, J., Schmidt, B. P., Wieringa, M. H., Wark, R. M., Subrahmanyan, R., McConnell, D., McCarthy, P. J., Schaefer, B. E., Markze, R. G. McMahon R. O., Firth, E., Soffitta, P., Amati, L.

Publikováno v: Astrophys.J.523:L121-L124,1999

We present multi-color optical and two-frequency radio observations of the bright SAX event, GRB 990510. The well-sampled optical decay, together with the radio observations are inconsistent with simple spherical afterglow models. The achromatic opti

Externí odkaz: http://arxiv.org/abs/astro-ph/9905306

The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models

Autor: P. S. Cowperthwaite, E. Berger, V. A. Villar, B. D. Metzger, M. Nicholl, R. Chornock, P. K. Blanchard, W. Fong, R. Margutti, M. Soares-Santos, K. D. Alexander, S. Allam, J. Annis, D. Brout, D. A. Brown, R. E. Butler, H.-Y. Chen, H. T. Diehl, Z. Doctor, M. R. Drout, T. Eftekhari, B. Farr, D. A. Finley, R. J. Foley, J. A. Frieman, C. L. Fryer, J. García-Bellido, M. S. S. Gill, J. Guillochon, K. Herner, D. E. Holz, D. Kasen, R. Kessler, J. Marriner, T. Matheson, E. H. Neilsen, E. Quataert, A. Palmese, A. Rest, M. Sako, D. M. Scolnic, N. Smith, D. L. Tucker, P. K. G. Williams, E. Balbinot, J. L. Carlin, E. R. Cook, F. Durret, T. S. Li, P. A. A. Lopes, A. C. C. Lourenço, J. L. Marshall, G. E. Medina, J. Muir, R. R. Muñoz, M. Sauseda, D. J. Schlegel, L. F. Secco, A. K. Vivas, W. Wester, A. Zenteno, Y. Zhang, T. M. C. Abbott, M. Banerji, K. Bechtol, A. Benoit-Lévy, E. Bertin, E. Buckley-Geer, D. L. Burke, D. Capozzi, A. Carnero Rosell, M. Carrasco Kind, F. J. Castander, M. Crocce, C. E. Cunha, C. B. D’Andrea, L. N. da Costa, C. Davis, D. L. DePoy, S. Desai, J. P. Dietrich, A. Drlica-Wagner, T. F. Eifler, A. E. Evrard, E. Fernandez, B. Flaugher, P. Fosalba, E. Gaztanaga, D. W. Gerdes, T. Giannantonio, D. A. Goldstein, D. Gruen, R. A. Gruendl, G. Gutierrez, K. Honscheid, B. Jain, D. J. James, T. Jeltema, M. W. G. Johnson, M. D. Johnson, S. Kent, E. Krause, R. Kron, K. Kuehn, N. Nuropatkin, O. Lahav, M. Lima, H. Lin, M. A. G. Maia, M. March, P. Martini, R. G. McMahon, F. Menanteau, C. J. Miller, R. Miquel, J. J. Mohr, E. Neilsen, R. C. Nichol, R. L. C. Ogando, A. A. Plazas, N. Roe, A. K. Romer, A. Roodman, E. S. Rykoff, E. Sanchez, V. Scarpine, R. Schindler, M. Schubnell, I. Sevilla-Noarbe, M. Smith, R. C. Smith, F. Sobreira, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, R. C. Thomas, M. A. Troxel, V. Vikram, A. R. Walker, R. H. Wechsler, J. Weller, B. Yanny, J. Zuntz

Publikováno v: Astrophys.J.
Astrophys.J., 2017, 848 (2), pp.L17. 〈10.3847/2041-8213/aa8fc7〉
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2017, 848 (2), pp.L17. ⟨10.3847/2041-8213/aa8fc7⟩
Astrophys.J., 2017, 848 (2), pp.L17. ⟨10.3847/2041-8213/aa8fc7⟩
NASA Astrophysics Data System
Cowperthwaite, P S, Berger, E, Villar, V A, Metzger, B D, Nicholl, M, Chornock, R, Blanchard, P K, Fong, W, Margutti, R, Soares-Santos, M, Alexander, K D, Allam, S, Annis, J, Brout, D, Brown, D A, Butler, R E, Chen, H-Y, Diehl, H T, Doctor, Z, Drout, M R, Eftekhari, T, Farr, B, Finley, D A, Foley, R J, Frieman, J A, Fryer, C L, García-Bellido, J, Gill, M S S, Guillochon, J, Herner, K, Holz, D E, Kasen, D, Kessler, R, Marriner, J, Matheson, T, E. H. Neilsen, J, Quataert, E, Palmese, A, Rest, A, Sako, M, Scolnic, D M, Smith, N, Tucker, D L, Williams, P K G, Balbinot, E, Carlin, J L, Cook, E R, Durret, F, Li, T S, Lopes, P A A, Lourenço, A C C, Marshall, J L, Medina, G E, Muir, J, Muñoz, R R, Sauseda, M, Schlegel, D J, Secco, L F, Vivas, A K, Wester, W, Zenteno, A, Zhang, Y, Abbott, T M C, Banerji, M, Bechtol, K, Benoit-Lévy, A, Bertin, E, Buckley-Geer, E, Burke, D L, Capozzi, D, Rosell, A C, Kind, M C, Castander, F J, Crocce, M, Cunha, C E, D'Andrea, C B, Costa, L N D, Davis, C, DePoy, D L, Desai, S, Dietrich, J P, Drlica-Wagner, A, Eifler, T F, Evrard, A E, Fernandez, E, Flaugher, B, Fosalba, P, Gaztanaga, E, Gerdes, D W, Giannantonio, T, Goldstein, D A, Gruen, D, Gruendl, R A, Gutierrez, G, Honscheid, K, Jain, B, James, D J, Jeltema, T, Johnson, M W G, Johnson, M D, Kent, S, Krause, E, Kron, R, Kuehn, K, Kuropatkin, N, Lahav, O, Lima, M, Lin, H, Maia, M A G, March, M, Martini, P, McMahon, R G, Menanteau, F, Miller, C J, Miquel, R, Mohr, J J, Neilsen, E, Nichol, R C, Ogando, R L C, Plazas, A A, Roe, N, Romer, A K, Roodman, A, Rykoff, E S, Sanchez, E, Scarpine, V, Schindler, R, Schubnell, M, Sevilla-Noarbe, I, Smith, M, Smith, R C, Sobreira, F, Suchyta, E, Swanson, M E C, Tarle, G, Thomas, D, Thomas, R C, Troxel, M A, Vikram, V, Walker, A R, Wechsler, R H, Weller, J, Yanny, B & Zuntz, J 2017, ' The electromagnetic counterpart of the binary neutron star merger LIGO/VIRGO GW170817. II. UV, optical, and near-IR light curves and comparison to kilonova models ', Astrophysical Journal Letters, vol. 848, no. 2 . https://doi.org/10.3847/2041-8213/aa8fc7

We present UV, optical, and NIR photometry of the first electromagnetic counterpart to a gravitational wave source from Advanced LIGO/Virgo, the binary neutron star merger GW170817. Our data set extends from the discovery of the optical counterpart a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d0676037e50c0a51918a7cc2d26b651
https://hal.archives-ouvertes.fr/hal-01669860

The XMM-Newton serendipitous survey

Autor: X. Barcons, F. J. Carrera, M. T. Ceballos, M. J. Page, J. Bussons-Gordo, A. Corral, J. Ebrero, S. Mateos, J. A. Tedds, M. G. Watson, D. Baskill, M. Birkinshaw, T. Boller, N. Borisov, M. Bremer, G. E. Bromage, H. Brunner, A. Caccianiga, C. S. Crawford, M. S. Cropper, R. Della Ceca, P. Derry, A. C. Fabian, P. Guillout, Y. Hashimoto, G. Hasinger, B. J. M. Hassall, G. Lamer, N. S. Loaring, T. Maccacaro, K. O. Mason, R. G. McMahon, L. Mirioni, J. P. D. Mittaz, C. Motch, I. Negueruela, J. P. Osborne, F. Panessa, I. Pérez-Fournon, J. P. Pye, T. P. Roberts, S. Rosen, N. Schartel, N. Schurch, A. Schwope, P. Severgnini, R. Sharp, G. C. Stewart, G. Szokoly, A. Ullán, M. J. Ward, R. S. Warwick, P. J. Wheatley, N. A. Webb, D. Worrall, W. Yuan, H. Ziaeepour

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2007, 476 (3), pp.1191-1203. ⟨10.1051/0004-6361:20077606⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & astrophysics, 2007, Vol.476(3), pp.1191-1203 [Peer Reviewed Journal]

[Aims] X-ray sources at intermediate fluxes (a few x 10-14 erg cm-2 s-1) with a sky density of ~100 deg-2 are responsible for a significant fraction of the cosmic X-ray background at various energies below 10 keV. The aim of this paper is to provide

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f403877ea7c9c491409e5c4f7e194a2a
https://doi.org/10.1051/0004-6361:20077606

The European Large AreaISOSurvey: optical identifications of 15-μm and 1.4-GHz sources in N1 and N2

Autor: Steve Serjeant, S. J. Oliver, E. A. Gonzalez-Solares, Carlo Lari, Chris J. Willott, Michael G. Irwin, Paolo Ciliegi, S. T. Hodgkin, Michael Rowan-Robinson, Mattia Vaccari, I. Perez-Fournon, R. G. McMahon

Publikováno v: Monthly Notices of the Royal Astronomical Society. 358:333-340

We present the optical identification of mid-IR and radio sources detected in the European Large Area ISO Survey (ELAIS) areas N1 and N2. Using the r' band optical data from the Wide Field Survey we apply a likelihood ratio method to search for the c

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1e2751b5a305ed78b63e66a3458e9d51
https://doi.org/10.1111/j.1365-2966.2005.08725.x

A homogeneous sample of sub-damped Lyman alpha systems - I. Construction of the sample and chemical abundance measurements

Autor: Tae-Sun Kim, Celine Peroux, Sandro D'Odorico, Miroslava Dessauges-Zavadsky, R. G. McMahon

Publikováno v: Monthly Notices of the Royal Astronomical Society. 345:447-479

In this first paper of a series, we report on the use of quasar spectra obtained with the UVES high resolution spectrograph and available through the ESO VLT archive to build the first sample of sub-DLA systems, absorbers with HI column densities > 1

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::d1aed6fa891a2ed37fee44c217250f75
https://doi.org/10.1046/j.1365-8711.2003.06949.x