Zobrazeno 1 - 10
of 130
pro vyhledávání: '"Methods: data analysi"'
Autor:
Delli , Veneri Michele, Tychoniec Łukasz, Guglielmetti Fabrizia, Longo Giuseppe, Villard Eric
We present a deep learning (DL) pipeline developed for the detection and characterization of astronomical sources within simulated Atacama Large Millimeter/submillimeter Array (ALMA) data cubes. The pipeline is composed of six DL models: a convolutio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5ef59ad93773851d175659af0ccdedc5
https://hdl.handle.net/11588/907387
https://hdl.handle.net/11588/907387
Autor:
Oleksandra Razim, Giuseppe Riccio, Stefano Cavuoti, Giuseppe Longo, Massimo Brescia, Mara Salvato
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 507:5034-5052
In order to answer the open questions of modern cosmology and galaxy evolution theory, robust algorithms for calculating photometric redshifts (photo-z) for very large samples of galaxies are needed. Correct estimation of the various photo-z algorith
Autor:
M. S. Cagliari, B. R. Granett, L. Guzzo, M. Bolzonella, L. Pozzetti, I. Tutusaus, S. Camera, A. Amara, N. Auricchio, R. Bender, C. Bodendorf, D. Bonino, E. Branchini, M. Brescia, V. Capobianco, C. Carbone, J. Carretero, F. J. Castander, M. Castellano, S. Cavuoti, A. Cimatti, R. Cledassou, G. Congedo, C. J. Conselice, L. Conversi, Y. Copin, L. Corcione, M. Cropper, H. Degaudenzi, M. Douspis, F. Dubath, S. Dusini, A. Ealet, S. Ferriol, N. Fourmanoit, M. Frailis, E. Franceschi, P. Franzetti, B. Garilli, C. Giocoli, A. Grazian, F. Grupp, S. V. H. Haugan, H. Hoekstra, W. Holmes, F. Hormuth, P. Hudelot, K. Jahnke, S. Kermiche, A. Kiessling, M. Kilbinger, T. Kitching, M. Kümmel, M. Kunz, H. Kurki-Suonio, S. Ligori, P. B. Lilje, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovic, R. Massey, M. Meneghetti, E. Merlin, G. Meylan, M. Moresco, L. Moscardini, S. M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, W. J. Percival, V. Pettorino, S. Pires, M. Poncet, L. Popa, F. Raison, R. Rebolo, J. Rhodes, H.-W. Rix, M. Roncarelli, E. Rossetti, R. Saglia, R. Scaramella, P. Schneider, M. Scodeggio, A. Secroun, G. Seidel, S. Serrano, C. Sirignano, G. Sirri, D. Tavagnacco, A. N. Taylor, I. Tereno, R. Toledo-Moreo, E. A. Valentijn, L. Valenziano, Y. Wang, N. Welikala, J. Weller, G. Zamorani, J. Zoubian, M. Baldi, R. Farinelli, E. Medinaceli, S. Mei, G. Polenta, E. Romelli, T. Vassallo, A. Humphrey
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 660, pp.A9. ⟨10.1051/0004-6361/202142224⟩
Cagliari, M S, Granett, B R, Guzzo, L, Bolzonella, M, Pozzetti, L, Tutusaus, I, Camera, S, Amara, A, Auricchio, N, Bender, R, Bodendorf, C, Bonino, D, Branchini, E, Brescia, M, Capobianco, V, Carbone, C, Carretero, J, Castander, F J, Castellano, M, Cavuoti, S, Cimatti, A, Cledassou, R, Congedo, G, Conselice, C J, Conversi, L, Copin, Y, Corcione, L, Cropper, M, Degaudenzi, H, Douspis, M, Dubath, F, Dusini, S, Ealet, A, Ferriol, S, Fourmanoit, N, Frailis, M, Franceschi, E, Franzetti, P, Garilli, B, Giocoli, C, Grazian, A, Grupp, F, Haugan, S V H, Hoekstra, H, Holmes, W, Hormuth, F, Hudelot, P, Jahnke, K, Kermiche, S, Kiessling, A, Kilbinger, M, Kitching, T, Kümmel, M, Kunz, M, Kurki-Suonio, H, Ligori, S, Lilje, P B, Lloro, I, Maiorano, E, Mansutti, O, Marggraf, O, Markovic, K, Massey, R, Meneghetti, M, Merlin, E, Meylan, G, Moresco, M, Moscardini, L, Niemi, S M, Padilla, C, Paltani, S, Pasian, F, Pedersen, K, Percival, W J, Pettorino, V, Pires, S, Poncet, M, Popa, L, Raison, F, Rebolo, R, Rhodes, J, Rix, H W, Roncarelli, M, Rossetti, E, Saglia, R, Scaramella, R, Schneider, P, Scodeggio, M, Secroun, A, Seidel, G, Serrano, S, Sirignano, C, Sirri, G, Tavagnacco, D, Taylor, A N, Tereno, I, Toledo-Moreo, R, Valentijn, E A, Valenziano, L, Wang, Y, Welikala, N, Weller, J, Zamorani, G, Zoubian, J, Baldi, M, Farinelli, R, Medinaceli, E, Mei, S, Polenta, G, Romelli, E, Vassallo, T & Humphrey, A 2022, ' Euclid : Constraining ensemble photometric redshift distributions with stacked spectroscopy ', Astronomy and Astrophysics, vol. 660, A9 . https://doi.org/10.1051/0004-6361/202142224
Astronomy & Astrophysics, 660, A9
Astronomy and Astrophysics-A&A, 2022, 660, pp.A9. ⟨10.1051/0004-6361/202142224⟩
Cagliari, M S, Granett, B R, Guzzo, L, Bolzonella, M, Pozzetti, L, Tutusaus, I, Camera, S, Amara, A, Auricchio, N, Bender, R, Bodendorf, C, Bonino, D, Branchini, E, Brescia, M, Capobianco, V, Carbone, C, Carretero, J, Castander, F J, Castellano, M, Cavuoti, S, Cimatti, A, Cledassou, R, Congedo, G, Conselice, C J, Conversi, L, Copin, Y, Corcione, L, Cropper, M, Degaudenzi, H, Douspis, M, Dubath, F, Dusini, S, Ealet, A, Ferriol, S, Fourmanoit, N, Frailis, M, Franceschi, E, Franzetti, P, Garilli, B, Giocoli, C, Grazian, A, Grupp, F, Haugan, S V H, Hoekstra, H, Holmes, W, Hormuth, F, Hudelot, P, Jahnke, K, Kermiche, S, Kiessling, A, Kilbinger, M, Kitching, T, Kümmel, M, Kunz, M, Kurki-Suonio, H, Ligori, S, Lilje, P B, Lloro, I, Maiorano, E, Mansutti, O, Marggraf, O, Markovic, K, Massey, R, Meneghetti, M, Merlin, E, Meylan, G, Moresco, M, Moscardini, L, Niemi, S M, Padilla, C, Paltani, S, Pasian, F, Pedersen, K, Percival, W J, Pettorino, V, Pires, S, Poncet, M, Popa, L, Raison, F, Rebolo, R, Rhodes, J, Rix, H W, Roncarelli, M, Rossetti, E, Saglia, R, Scaramella, R, Schneider, P, Scodeggio, M, Secroun, A, Seidel, G, Serrano, S, Sirignano, C, Sirri, G, Tavagnacco, D, Taylor, A N, Tereno, I, Toledo-Moreo, R, Valentijn, E A, Valenziano, L, Wang, Y, Welikala, N, Weller, J, Zamorani, G, Zoubian, J, Baldi, M, Farinelli, R, Medinaceli, E, Mei, S, Polenta, G, Romelli, E, Vassallo, T & Humphrey, A 2022, ' Euclid : Constraining ensemble photometric redshift distributions with stacked spectroscopy ', Astronomy and Astrophysics, vol. 660, A9 . https://doi.org/10.1051/0004-6361/202142224
Astronomy & Astrophysics, 660, A9
Euclid Consortium: M. S. Cagliari et al.
[Context] The ESA Euclid mission will produce photometric galaxy samples over 15 000 square degrees of the sky that will be rich for clustering and weak lensing statistics. The accuracy of the cosmologica
[Context] The ESA Euclid mission will produce photometric galaxy samples over 15 000 square degrees of the sky that will be rich for clustering and weak lensing statistics. The accuracy of the cosmologica
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a8c6cae2116123d9df0ac1e956f91516
https://u-paris.hal.science/hal-03664785/document
https://u-paris.hal.science/hal-03664785/document
Autor:
Thorold Tronrud, Patricia B Tissera, Facundo A Gómez, Robert J J Grand, Ruediger Pakmor, Federico Marinacci, Christine M Simpson
We develop a method ('Galactic Archaeology Neural Network', GANN) based on neural network models (NNMs) to identify accreted stars in galactic discs by only their chemical fingerprint and age, using a suite of simulated galaxies from the Auriga Proje
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6f63d22983408839dddadf4d7989d781
https://doi.org/10.48550/arxiv.2207.06586
https://doi.org/10.48550/arxiv.2207.06586
Autor:
N. Hamaus, M. Aubert, A. Pisani, S. Contarini, G. Verza, M.-C. Cousinou, S. Escoffier, A. Hawken, G. Lavaux, G. Pollina, B. D. Wandelt, J. Weller, M. Bonici, C. Carbone, L. Guzzo, A. Kovacs, F. Marulli, E. Massara, L. Moscardini, P. Ntelis, W. J. Percival, S. Radinović, M. Sahlén, Z. Sakr, A. G. Sánchez, H. A. Winther, N. Auricchio, S. Awan, R. Bender, C. Bodendorf, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, V. Capobianco, J. Carretero, F. J. Castander, M. Castellano, S. Cavuoti, A. Cimatti, R. Cledassou, G. Congedo, L. Conversi, Y. Copin, L. Corcione, M. Cropper, A. Da Silva, H. Degaudenzi, M. Douspis, F. Dubath, C. A. J. Duncan, X. Dupac, S. Dusini, A. Ealet, S. Ferriol, P. Fosalba, M. Frailis, E. Franceschi, P. Franzetti, M. Fumana, B. Garilli, B. Gillis, C. Giocoli, A. Grazian, F. Grupp, S. V. H. Haugan, W. Holmes, F. Hormuth, K. Jahnke, S. Kermiche, A. Kiessling, M. Kilbinger, T. Kitching, M. Kümmel, M. Kunz, H. Kurki-Suonio, S. Ligori, P. B. Lilje, I. Lloro, E. Maiorano, O. Marggraf, K. Markovic, R. Massey, S. Maurogordato, M. Melchior, M. Meneghetti, G. Meylan, M. Moresco, E. Munari, S. M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, V. Pettorino, S. Pires, M. Poncet, L. Popa, L. Pozzetti, R. Rebolo, J. Rhodes, H. Rix, M. Roncarelli, E. Rossetti, R. Saglia, P. Schneider, A. Secroun, G. Seidel, S. Serrano, C. Sirignano, G. Sirri, J.-L. Starck, P. Tallada-Crespí, D. Tavagnacco, A. N. Taylor, I. Tereno, R. Toledo-Moreo, F. Torradeflot, E. A. Valentijn, L. Valenziano, Y. Wang, N. Welikala, G. Zamorani, J. Zoubian, S. Andreon, M. Baldi, S. Camera, S. Mei, C. Neissner, E. Romelli
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 658, pp.A20. ⟨10.1051/0004-6361/202142073⟩
Astronomy & Astrophysics, 2022, Vol.658, pp.A20 [Peer Reviewed Journal]
Hamaus, N, Aubert, M, Pisani, A, Contarini, S, Verza, G, Cousinou, M C, Escoffier, S, Hawken, A, Lavaux, G, Pollina, G, Wandelt, B D, Weller, J, Bonici, M, Carbone, C, Guzzo, L, Kovacs, A, Marulli, F, Massara, E, Moscardini, L, Ntelis, P, Percival, W J, Radinović, S, Sahlén, M, Sakr, Z, Sánchez, A G, Winther, H A, Auricchio, N, Awan, S, Bender, R, Bodendorf, C, Bonino, D, Branchini, E, Brescia, M, Brinchmann, J, Capobianco, V, Carretero, J, Castander, F J, Castellano, M, Cavuoti, S, Cimatti, A, Cledassou, R, Congedo, G, Conversi, L, Copin, Y, Corcione, L, Cropper, M, Da Silva, A, Degaudenzi, H, Douspis, M, Dubath, F, Duncan, C A J, Dupac, X, Dusini, S, Ealet, A, Ferriol, S, Fosalba, P, Frailis, M, Franceschi, E, Franzetti, P, Fumana, M, Garilli, B, Gillis, B, Giocoli, C, Grazian, A, Grupp, F, Haugan, S V H, Holmes, W, Hormuth, F, Jahnke, K, Kermiche, S, Kiessling, A, Kilbinger, M, Kitching, T, Kümmel, M, Kunz, M, Kurki-Suonio, H, Ligori, S, Lilje, P B, Lloro, I, Maiorano, E, Marggraf, O, Markovic, K, Massey, R, Maurogordato, S, Melchior, M, Meneghetti, M, Meylan, G, Moresco, M, Munari, E, Niemi, S M, Padilla, C, Paltani, S, Pasian, F, Pedersen, K, Pettorino, V, Pires, S, Poncet, M, Popa, L, Pozzetti, L, Rebolo, R, Rhodes, J, Rix, H, Roncarelli, M, Rossetti, E, Saglia, R, Schneider, P, Secroun, A, Seidel, G, Serrano, S, Sirignano, C, Sirri, G, Starck, J L, Tallada-Crespí, P, Tavagnacco, D, Taylor, A N, Tereno, I, Toledo-Moreo, R, Torradeflot, F, Valentijn, E A, Valenziano, L, Wang, Y, Welikala, N, Zamorani, G, Zoubian, J, Andreon, S, Baldi, M, Camera, S, Mei, S, Neissner, C & Romelli, E 2022, ' Euclid : Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids ', Astronomy and Astrophysics, vol. 658, A20 . https://doi.org/10.1051/0004-6361/202142073
Astronomy & astrophysics, 658:A20. EDP Sciences
Astronomy and Astrophysics-A&A, 2022, 658, pp.A20. ⟨10.1051/0004-6361/202142073⟩
Astronomy & Astrophysics, 2022, Vol.658, pp.A20 [Peer Reviewed Journal]
Hamaus, N, Aubert, M, Pisani, A, Contarini, S, Verza, G, Cousinou, M C, Escoffier, S, Hawken, A, Lavaux, G, Pollina, G, Wandelt, B D, Weller, J, Bonici, M, Carbone, C, Guzzo, L, Kovacs, A, Marulli, F, Massara, E, Moscardini, L, Ntelis, P, Percival, W J, Radinović, S, Sahlén, M, Sakr, Z, Sánchez, A G, Winther, H A, Auricchio, N, Awan, S, Bender, R, Bodendorf, C, Bonino, D, Branchini, E, Brescia, M, Brinchmann, J, Capobianco, V, Carretero, J, Castander, F J, Castellano, M, Cavuoti, S, Cimatti, A, Cledassou, R, Congedo, G, Conversi, L, Copin, Y, Corcione, L, Cropper, M, Da Silva, A, Degaudenzi, H, Douspis, M, Dubath, F, Duncan, C A J, Dupac, X, Dusini, S, Ealet, A, Ferriol, S, Fosalba, P, Frailis, M, Franceschi, E, Franzetti, P, Fumana, M, Garilli, B, Gillis, B, Giocoli, C, Grazian, A, Grupp, F, Haugan, S V H, Holmes, W, Hormuth, F, Jahnke, K, Kermiche, S, Kiessling, A, Kilbinger, M, Kitching, T, Kümmel, M, Kunz, M, Kurki-Suonio, H, Ligori, S, Lilje, P B, Lloro, I, Maiorano, E, Marggraf, O, Markovic, K, Massey, R, Maurogordato, S, Melchior, M, Meneghetti, M, Meylan, G, Moresco, M, Munari, E, Niemi, S M, Padilla, C, Paltani, S, Pasian, F, Pedersen, K, Pettorino, V, Pires, S, Poncet, M, Popa, L, Pozzetti, L, Rebolo, R, Rhodes, J, Rix, H, Roncarelli, M, Rossetti, E, Saglia, R, Schneider, P, Secroun, A, Seidel, G, Serrano, S, Sirignano, C, Sirri, G, Starck, J L, Tallada-Crespí, P, Tavagnacco, D, Taylor, A N, Tereno, I, Toledo-Moreo, R, Torradeflot, F, Valentijn, E A, Valenziano, L, Wang, Y, Welikala, N, Zamorani, G, Zoubian, J, Andreon, S, Baldi, M, Camera, S, Mei, S, Neissner, C & Romelli, E 2022, ' Euclid : Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids ', Astronomy and Astrophysics, vol. 658, A20 . https://doi.org/10.1051/0004-6361/202142073
Astronomy & astrophysics, 658:A20. EDP Sciences
Euclid Consortium: N. Hamaus et al.
Euclid is poised to survey galaxies across a cosmological volume of unprecedented size, providing observations of more than a billion objects distributed over a third of the full sky. Approximately 20 million
Euclid is poised to survey galaxies across a cosmological volume of unprecedented size, providing observations of more than a billion objects distributed over a third of the full sky. Approximately 20 million
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ff36b5d550032f9f08ec755d6bad134
https://hdl.handle.net/11588/900371
https://hdl.handle.net/11588/900371
Autor:
Keihanen, E., Lindholm, V., Monaco, P., Blot, L., Carbone, C., Kiiveri, K., Sánchez, A. G., Viitanen, A., Valiviita, J., Amara, A., Auricchio, N., Baldi, M., Bonino, D., Branchini, E., Brescia, M., Brinchmann, J., Camera, S., Capobianco, V., Carretero, J., Castellano, M., Cavuoti, S., Cimatti, A., Cledassou, R., Congedo, G., Conversi, L., Copin, Y., Corcione, L., Cropper, M., Da Silva, A., Degaudenzi, H., Douspis, M., Dubath, F., Duncan, C. A. J., Dupac, X., Dusini, S., Ealet, A., Farrens, S., Ferriol, S., Frailis, M., Franceschi, E., Fumana, M., Gillis, B., Giocoli, C., Grazian, A., Grupp, F., Guzzo, L., Haugan, S. V. H., Hoekstra, H., Holmes, W., Hormuth, F., Jahnke, K., Kümmel, M., Kermiche, S., Kiessling, A., Kitching, T., Kunz, M., Kurki-Suonio, H., Ligori, S., Lilje, P. B., Lloro, I., Maiorano, E., Mansutti, O., Marggraf, O., Marulli, F., Massey, R., Melchior, M., Meneghetti, M., Meylan, G., Moresco, M., Morin, B., Moscardini, L., Munari, E., Niemi, S. M., Padilla, C., Paltani, S., Pasian, F., Pedersen, K., Pettorino, V., Pires, S., Polenta, G., Poncet, M., Popa, L., Raison, F., Renzi, A., Rhodes, J., Romelli, E., Saglia, R., Sartoris, B., Schneider, P., Schrabback, T., Secroun, A., Seidel, G., Sirignano, C., Sirri, G., Stanco, L., Surace, C., Tallada-Crespí, P., Tavagnacco, D., Taylor, A. N., Tereno, I., Toledo-Moreo, R., Torradeflot, F., Valentijn, E. A., Valenziano, L., Vassallo, T., Wang, Y., Weller, J., Zamorani, G., Zoubian, J., Andreon, S., Maino, D., de la Torre, S.
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 666, pp.A129. ⟨10.1051/0004-6361/202244065⟩
Astronomy and astrophysics, 666:A129. EDP Sciences
Astronomy & Astrophysics, 666, A129
Astronomy and Astrophysics-A&A, 2022, 666, pp.A129. ⟨10.1051/0004-6361/202244065⟩
Astronomy and astrophysics, 666:A129. EDP Sciences
Astronomy & Astrophysics, 666, A129
We present a method for fast evaluation of the covariance matrix for a two-point galaxy correlation function (2PCF) measured with the Landy-Szalay estimator. The standard way of evaluating the covariance matrix consists in running the estimator on a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::726089e54577f2daa91e1cdf804e556b
https://hal.science/hal-03691688
https://hal.science/hal-03691688
Autor:
J Antoniadis, Z Arzoumanian, S Babak, M Bailes, A-S Bak Nielsen, P T Baker, C G Bassa, B Bécsy, A Berthereau, M Bonetti, A Brazier, P R Brook, M Burgay, S Burke-Spolaor, R N Caballero, J A Casey-Clyde, A Chalumeau, D J Champion, M Charisi, S Chatterjee, S Chen, I Cognard, J M Cordes, N J Cornish, F Crawford, H T Cromartie, K Crowter, S Dai, M E DeCesar, P B Demorest, G Desvignes, T Dolch, B Drachler, M Falxa, E C Ferrara, W Fiore, E Fonseca, J R Gair, N Garver-Daniels, B Goncharov, D C Good, E Graikou, L Guillemot, Y J Guo, J S Hazboun, G Hobbs, H Hu, K Islo, G H Janssen, R J Jennings, A D Johnson, M L Jones, A R Kaiser, D L Kaplan, R Karuppusamy, M J Keith, L Z Kelley, M Kerr, J S Key, M Kramer, M T Lam, W G Lamb, T J W Lazio, K J Lee, L Lentati, K Liu, J Luo, R S Lynch, A G Lyne, D R Madison, R A Main, R N Manchester, A McEwen, J W McKee, M A McLaughlin, M B Mickaliger, C M F Mingarelli, C Ng, D J Nice, S Osłowski, A Parthasarathy, T T Pennucci, B B P Perera, D Perrodin, A Petiteau, N S Pol, N K Porayko, A Possenti, S M Ransom, P S Ray, D J Reardon, C J Russell, A Samajdar, L M Sampson, S Sanidas, J M Sarkissian, K Schmitz, L Schult, A Sesana, G Shaifullah, R M Shannon, B J Shapiro-Albert, X Siemens, J Simon, T L Smith, L Speri, R Spiewak, I H Stairs, B W Stappers, D R Stinebring, J K Swiggum, S R Taylor, G Theureau, C Tiburzi, M Vallisneri, E van der Wateren, A Vecchio, J P W Verbiest, S J Vigeland, H Wahl, J B Wang, J Wang, L Wang, C A Witt, S Zhang, X J Zhu
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Antoniadis, J, Arzoumanian, Z, Babak, S, Bailes, M, Bak nielsen, A, Baker, P T, Bassa, C G, Bécsy, B, Berthereau, A, Bonetti, M, Brazier, A, Brook, P R, Burgay, M, Burke-spolaor, S, Caballero, R N, Casey-clyde, J A, Chalumeau, A, Champion, D J, Charisi, M, Chatterjee, S, Chen, S, Cognard, I, Cordes, J M, Cornish, N J, Crawford, F, Cromartie, H T, Crowter, K, Dai, S, Decesar, M E, Demorest, P B, Desvignes, G, Dolch, T, Drachler, B, Falxa, M, Ferrara, E C, Fiore, W, Fonseca, E, Gair, J R, Garver-daniels, N, Goncharov, B, Good, D C, Graikou, E, Guillemot, L, Guo, Y J, Hazboun, J S, Hobbs, G, Hu, H, Islo, K, Janssen, G H, Jennings, R J, Johnson, A D, Jones, M L, Kaiser, A R, Kaplan, D L, Karuppusamy, R, Keith, M J, Kelley, L Z, Kerr, M, Key, J S, Kramer, M, Lam, M T, Lamb, W G, Lazio, T J W, Lee, K J, Lentati, L, Liu, K, Luo, J, Lynch, R S, Lyne, A G, Madison, D R, Main, R A, Manchester, R N, Mcewen, A, Mckee, J W, Mclaughlin, M A, Mickaliger, M B, Mingarelli, C M F, Nice, D J, Osłowski, S, Parthasarathy, A, Pennucci, T T, Perera, B B P, Perrodin, D, Petiteau, A, Pol, N S, Porayko, N K, Possenti, A, Ransom, S M, Ray, P S, Reardon, D J, Russell, C J, Samajdar, A, Sampson, L M, Sanidas, S, Sarkissian, J M, Schmitz, K, Schult, L, Sesana, A, Shaifullah, G, Shannon, R M, Shapiro-albert, B J, Siemens, X, Simon, J, Smith, T L, Speri, L, Spiewak, R, Stairs, I H, Stappers, B W, Stinebring, D R, Swiggum, J K, Taylor, S R, Theureau, G, Tiburzi, C, Vallisneri, M, Van der wateren, E, Vecchio, A, Verbiest, J P W, Vigeland, S J, Wahl, H, Wang, J, Wang, J, Wang, L, Witt, C A, Zhang, S, Zhu, X J & Ng, C 2022, ' The International Pulsar Timing Array second data release: Search for an isotropic gravitational wave background ', Monthly Notices of the Royal Astronomical Society, vol. 510, no. 4, pp. 4873-4887 . https://doi.org/10.1093/mnras/stab3418
Monthly Notices of the Royal Astronomical Society, 2022, 510, pp.4873-4887. ⟨10.1093/mnras/stab3418⟩
Monthly Notices of the Royal Astronomical Society, 510, pp. 4873-4887
Monthly Notices of the Royal Astronomical Society, 510, 4873-4887
Antoniadis, J, Arzoumanian, Z, Babak, S, Bailes, M, Bak nielsen, A, Baker, P T, Bassa, C G, Bécsy, B, Berthereau, A, Bonetti, M, Brazier, A, Brook, P R, Burgay, M, Burke-spolaor, S, Caballero, R N, Casey-clyde, J A, Chalumeau, A, Champion, D J, Charisi, M, Chatterjee, S, Chen, S, Cognard, I, Cordes, J M, Cornish, N J, Crawford, F, Cromartie, H T, Crowter, K, Dai, S, Decesar, M E, Demorest, P B, Desvignes, G, Dolch, T, Drachler, B, Falxa, M, Ferrara, E C, Fiore, W, Fonseca, E, Gair, J R, Garver-daniels, N, Goncharov, B, Good, D C, Graikou, E, Guillemot, L, Guo, Y J, Hazboun, J S, Hobbs, G, Hu, H, Islo, K, Janssen, G H, Jennings, R J, Johnson, A D, Jones, M L, Kaiser, A R, Kaplan, D L, Karuppusamy, R, Keith, M J, Kelley, L Z, Kerr, M, Key, J S, Kramer, M, Lam, M T, Lamb, W G, Lazio, T J W, Lee, K J, Lentati, L, Liu, K, Luo, J, Lynch, R S, Lyne, A G, Madison, D R, Main, R A, Manchester, R N, Mcewen, A, Mckee, J W, Mclaughlin, M A, Mickaliger, M B, Mingarelli, C M F, Nice, D J, Osłowski, S, Parthasarathy, A, Pennucci, T T, Perera, B B P, Perrodin, D, Petiteau, A, Pol, N S, Porayko, N K, Possenti, A, Ransom, S M, Ray, P S, Reardon, D J, Russell, C J, Samajdar, A, Sampson, L M, Sanidas, S, Sarkissian, J M, Schmitz, K, Schult, L, Sesana, A, Shaifullah, G, Shannon, R M, Shapiro-albert, B J, Siemens, X, Simon, J, Smith, T L, Speri, L, Spiewak, R, Stairs, I H, Stappers, B W, Stinebring, D R, Swiggum, J K, Taylor, S R, Theureau, G, Tiburzi, C, Vallisneri, M, Van der wateren, E, Vecchio, A, Verbiest, J P W, Vigeland, S J, Wahl, H, Wang, J, Wang, J, Wang, L, Witt, C A, Zhang, S, Zhu, X J & Ng, C 2022, ' The International Pulsar Timing Array second data release: Search for an isotropic gravitational wave background ', Monthly Notices of the Royal Astronomical Society, vol. 510, no. 4, pp. 4873-4887 . https://doi.org/10.1093/mnras/stab3418
Monthly Notices of the Royal Astronomical Society, 2022, 510, pp.4873-4887. ⟨10.1093/mnras/stab3418⟩
Monthly Notices of the Royal Astronomical Society, 510, pp. 4873-4887
Monthly Notices of the Royal Astronomical Society, 510, 4873-4887
We searched for an isotropic stochastic gravitational wave background in the second data release of the International Pulsar Timing Array, a global collaboration synthesizing decadal-length pulsar-timing campaigns in North America, Europe, and Austra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54e36387eca2a575908de1126f17275f
http://hdl.handle.net/10281/362277
http://hdl.handle.net/10281/362277
Autor:
A Samajdar, G Shaifullah, A Sesana, J Antoniadis, M Burgay, S Chen, I Cognard, L Guillemot, M Kramer, J W McKee, M B Mickaliger, G Theureau, E Van , derundefined Wateren
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 517, 1, pp. 1460-1468
Monthly Notices of the Royal Astronomical Society, 517, 1460-1468
Monthly Notices of the Royal Astronomical Society, 517, 1460-1468
Recently, global pulsar timing arrays have released results from searching for a nano-Hertz gravitational wave background signal. Although there has not been any definite evidence of the presence of such a signal in residuals of pulsar timing data ye
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a1f731dedd8f79e5447263b78c6f374
Autor:
J. Wang, G. M. Shaifullah, J. P. W. Verbiest, C. Tiburzi, D. J. Champion, I. Cognard, M. Gaikwad, E. Graikou, L. Guillemot, H. Hu, R. Karuppusamy, M. J. Keith, M. Kramer, Y. Liu, A. G. Lyne, M. B. Mickaliger, B. W. Stappers, G. Theureau
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 cros
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6b5c12b82801245a6ffadf90a3ece415
http://hdl.handle.net/10281/363426
http://hdl.handle.net/10281/363426
Euclid::Constraining dark energy coupled to electromagnetism using astrophysical and laboratory data
Autor:
Martinelli M., Martins C. J. A. P., Nesseris S., Tutusaus I., Blanchard A., Camera S., Carbone C., Casas S., Pettorino V., Sakr Z., Yankelevich V., Sapone D., Amara A., Auricchio N., Bodendorf C., Bonino D., Branchini E., Capobianco V., Carretero J., Castellano M., Cavuoti S., Cimatti A., Cledassou R., Corcione L., Costille A., Degaudenzi H., Douspis M., Dubath F., Dusini S., Ealet A., Ferriol S., Frailis M., Franceschi E., Garilli B., Giocoli C., Grazian A., Grupp F., Haugan S. V. H., Holmes W., Hormuth F., Jahnke K., Kiessling A., Kummel M., Kunz M., Kurki-Suonio H., Ligori S., Lilje P. B., Lloro I., Mansutti O., Marggraf O., Markovic K., Massey R., Meneghetti M., Meylan G., Moscardini L., Niemi S. M., Padilla C., Paltani S., Pasian F., Pedersen K., Pires S., Poncet M., Popa L., Raison F., Rebolo R., Rhodes J., Roncarelli M., Rossetti E., Saglia R., Secroun A., Seidel G., Serrano S., Sirignano C., Sirri G., Starck J. -L., Tavagnacco D., Taylor A. N., Tereno I., Toledo-Moreo R., Valenziano L., Wang Y., Zamorani G., Zoubian J., Baldi M., Brescia M., Congedo G., Conversi L., Copin Y., Fabbian G., Farinelli R., Medinaceli E., Mei S., Polenta G., Romelli E., Vassallo T.
Publikováno v:
2021, ' Euclid: Constraining dark energy coupled to electromagnetism using astrophysical and laboratory data ', Astronomy and Astrophysics, vol. 654, A148, pp. 1-14 . https://doi.org/10.1051/0004-6361/202141353
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 654, pp.A148. ⟨10.1051/0004-6361/202141353⟩
Astron.Astrophys.
Astron.Astrophys., 2021, 654, pp.A148. ⟨10.1051/0004-6361/202141353⟩
Astronomy & astrophysics, 2021, Vol.654, pp.A148 [Peer Reviewed Journal]
Digital.CSIC. Repositorio Institucional del CSIC
instname
Martinelli, M, Martins, C J A P, Nesseris, S, Tutusaus, I, Blanchard, A, Camera, S, Carbone, C, Casas, S, Pettorino, V, Sakr, Z, Yankelevich, V, Sapone, D, Amara, A, Auricchio, N, Bodendorf, C, Bonino, D, Branchini, E, Capobianco, V, Carretero, J, Castellano, M, Cavuoti, S, Cimatti, A, Cledassou, R, Corcione, L, Costille, A, Degaudenzi, H, Douspis, M, Dubath, F, Dusini, S, Ealet, A, Ferriol, S, Frailis, M, Franceschi, E, Garilli, B, Giocoli, C, Grazian, A, Grupp, F, Haugan, S V H, Holmes, W, Hormuth, F, Jahnke, K, Kiessling, A, Kümmel, M, Kunz, M, Kurki-Suonio, H, Ligori, S, Lilje, P B, Lloro, I, Mansutti, O, Marggraf, O, Markovic, K, Massey, R, Meneghetti, M, Meylan, G, Moscardini, L, Niemi, S M, Padilla, C, Paltani, S, Pasian, F, Pedersen, K, Pires, S, Poncet, M, Popa, L, Raison, F, Rebolo, R, Rhodes, J, Roncarelli, M, Rossetti, E, Saglia, R, Secroun, A, Seidel, G, Serrano, S, Sirignano, C, Sirri, G, Starck, J L, Tavagnacco, D, Taylor, A N, Tereno, I, Toledo-Moreo, R, Valenziano, L, Wang, Y, Zamorani, G, Zoubian, J, Baldi, M, Brescia, M, Congedo, G, Conversi, L, Copin, Y, Fabbian, G, Farinelli, R, Medinaceli, E, Mei, S, Polenta, G, Romelli, E & Vassallo, T 2021, ' Euclid : Constraining dark energy coupled to electromagnetism using astrophysical and laboratory data ', Astronomy and Astrophysics, vol. 654, A148 . https://doi.org/10.1051/0004-6361/202141353
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 654, pp.A148. ⟨10.1051/0004-6361/202141353⟩
Astron.Astrophys.
Astron.Astrophys., 2021, 654, pp.A148. ⟨10.1051/0004-6361/202141353⟩
Astronomy & astrophysics, 2021, Vol.654, pp.A148 [Peer Reviewed Journal]
Digital.CSIC. Repositorio Institucional del CSIC
instname
Martinelli, M, Martins, C J A P, Nesseris, S, Tutusaus, I, Blanchard, A, Camera, S, Carbone, C, Casas, S, Pettorino, V, Sakr, Z, Yankelevich, V, Sapone, D, Amara, A, Auricchio, N, Bodendorf, C, Bonino, D, Branchini, E, Capobianco, V, Carretero, J, Castellano, M, Cavuoti, S, Cimatti, A, Cledassou, R, Corcione, L, Costille, A, Degaudenzi, H, Douspis, M, Dubath, F, Dusini, S, Ealet, A, Ferriol, S, Frailis, M, Franceschi, E, Garilli, B, Giocoli, C, Grazian, A, Grupp, F, Haugan, S V H, Holmes, W, Hormuth, F, Jahnke, K, Kiessling, A, Kümmel, M, Kunz, M, Kurki-Suonio, H, Ligori, S, Lilje, P B, Lloro, I, Mansutti, O, Marggraf, O, Markovic, K, Massey, R, Meneghetti, M, Meylan, G, Moscardini, L, Niemi, S M, Padilla, C, Paltani, S, Pasian, F, Pedersen, K, Pires, S, Poncet, M, Popa, L, Raison, F, Rebolo, R, Rhodes, J, Roncarelli, M, Rossetti, E, Saglia, R, Secroun, A, Seidel, G, Serrano, S, Sirignano, C, Sirri, G, Starck, J L, Tavagnacco, D, Taylor, A N, Tereno, I, Toledo-Moreo, R, Valenziano, L, Wang, Y, Zamorani, G, Zoubian, J, Baldi, M, Brescia, M, Congedo, G, Conversi, L, Copin, Y, Fabbian, G, Farinelli, R, Medinaceli, E, Mei, S, Polenta, G, Romelli, E & Vassallo, T 2021, ' Euclid : Constraining dark energy coupled to electromagnetism using astrophysical and laboratory data ', Astronomy and Astrophysics, vol. 654, A148 . https://doi.org/10.1051/0004-6361/202141353
Astronomy & Astrophysics
Martinelli, M., et al.
In physically realistic, scalar-field-based dynamical dark energy models (including, e.g., quintessence), one naturally expects the scalar field to couple to the rest of the model's degrees of freedom. In particular, a cou
In physically realistic, scalar-field-based dynamical dark energy models (including, e.g., quintessence), one naturally expects the scalar field to couple to the rest of the model's degrees of freedom. In particular, a cou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f553abee5f33e35c2146e3aba7c0da6f
https://hdl.handle.net/20.500.11820/b92256b5-fe34-407b-8526-d30a021ca95e
https://hdl.handle.net/20.500.11820/b92256b5-fe34-407b-8526-d30a021ca95e