@inProceedings{
 title = {Experimental XPM, SPM, FWM Penalty Evaluation in Very Dense WDM Optical Systems},
 type = {inProceedings},
 year = {2005},
 identifiers = {[object Object]},
 pages = {1339-1341},
 volume = {2},
 websites = {http://www.scopus.com/inward/record.url?eid=2-s2.0-84899152631&partnerID=tZOtx3y1,http://www.scopus.com/inward/record.url?eid=2-s2.0-30944460383&partnerID=tZOtx3y1,http://www.scopus.com/inward/record.url?eid=2-s2.0-84899117001&partnerID=tZOtx3y1},
 publisher = {Optical Society of America},
 id = {e009052b-548b-3cf0-a5c9-ae49de719026},
 created = {2016-04-12T13:14:33.000Z},
 file_attached = {false},
 profile_id = {d636df8b-dbd7-349c-8172-9f253b58c3e8},
 group_id = {1e8503e9-5fe7-398e-b5b0-831268375e5f},
 last_modified = {2016-04-12T13:14:33.000Z},
 read = {false},
 starred = {false},
 authored = {false},
 confirmed = {true},
 hidden = {false},
 citation_key = {Paradisol2005},
 abstract = {Experimental SPM, FWM and XPM contributions are separately measured. Evaluation of Q penalties is performed on a 2000-km, 33-GHz, 66-GHz and 100-GHz-spaced DWDM system. XPM is found to be the major constrain. © 2005 Optical Society of America.},
 bibtype = {inProceedings},
 author = {Paradisol, Livio and Boffil, Pierpaolo and Marazzil, Lucia and Vecchia, Nicola Dalla and Arfiglia, Massimo},
 booktitle = {Optics InfoBase Conference Papers}
}

{"_id":"ubMLbxkpSXTsjQWt6","bibbaseid":"paradisol-boffil-marazzil-vecchia-arfiglia-experimentalxpmspmfwmpenaltyevaluationinverydensewdmopticalsystems-2005","downloads":0,"creationDate":"2016-04-12T13:10:53.235Z","title":"Experimental XPM, SPM, FWM Penalty Evaluation in Very Dense WDM Optical Systems","author_short":["Paradisol, L.","Boffil, P.","Marazzil, L.","Vecchia, N., D.","Arfiglia, M."],"year":2005,"bibtype":"inProceedings","biburl":null,"bibdata":{"title":"Experimental XPM, SPM, FWM Penalty Evaluation in Very Dense WDM Optical Systems","type":"inProceedings","year":"2005","identifiers":"[object Object]","pages":"1339-1341","volume":"2","websites":"http://www.scopus.com/inward/record.url?eid=2-s2.0-84899152631&partnerID=tZOtx3y1,http://www.scopus.com/inward/record.url?eid=2-s2.0-30944460383&partnerID=tZOtx3y1,http://www.scopus.com/inward/record.url?eid=2-s2.0-84899117001&partnerID=tZOtx3y1","publisher":"Optical Society of America","id":"e009052b-548b-3cf0-a5c9-ae49de719026","created":"2016-04-12T13:14:33.000Z","file_attached":false,"profile_id":"d636df8b-dbd7-349c-8172-9f253b58c3e8","group_id":"1e8503e9-5fe7-398e-b5b0-831268375e5f","last_modified":"2016-04-12T13:14:33.000Z","read":false,"starred":false,"authored":false,"confirmed":"true","hidden":false,"citation_key":"Paradisol2005","abstract":"Experimental SPM, FWM and XPM contributions are separately measured. Evaluation of Q penalties is performed on a 2000-km, 33-GHz, 66-GHz and 100-GHz-spaced DWDM system. XPM is found to be the major constrain. © 2005 Optical Society of America.","bibtype":"inProceedings","author":"Paradisol, Livio and Boffil, Pierpaolo and Marazzil, Lucia and Vecchia, Nicola Dalla and Arfiglia, Massimo","booktitle":"Optics InfoBase Conference Papers","bibtex":"@inProceedings{\n title = {Experimental XPM, SPM, FWM Penalty Evaluation in Very Dense WDM Optical Systems},\n type = {inProceedings},\n year = {2005},\n identifiers = {[object Object]},\n pages = {1339-1341},\n volume = {2},\n websites = {http://www.scopus.com/inward/record.url?eid=2-s2.0-84899152631&partnerID=tZOtx3y1,http://www.scopus.com/inward/record.url?eid=2-s2.0-30944460383&partnerID=tZOtx3y1,http://www.scopus.com/inward/record.url?eid=2-s2.0-84899117001&partnerID=tZOtx3y1},\n publisher = {Optical Society of America},\n id = {e009052b-548b-3cf0-a5c9-ae49de719026},\n created = {2016-04-12T13:14:33.000Z},\n file_attached = {false},\n profile_id = {d636df8b-dbd7-349c-8172-9f253b58c3e8},\n group_id = {1e8503e9-5fe7-398e-b5b0-831268375e5f},\n last_modified = {2016-04-12T13:14:33.000Z},\n read = {false},\n starred = {false},\n authored = {false},\n confirmed = {true},\n hidden = {false},\n citation_key = {Paradisol2005},\n abstract = {Experimental SPM, FWM and XPM contributions are separately measured. Evaluation of Q penalties is performed on a 2000-km, 33-GHz, 66-GHz and 100-GHz-spaced DWDM system. XPM is found to be the major constrain. © 2005 Optical Society of America.},\n bibtype = {inProceedings},\n author = {Paradisol, Livio and Boffil, Pierpaolo and Marazzil, Lucia and Vecchia, Nicola Dalla and Arfiglia, Massimo},\n booktitle = {Optics InfoBase Conference Papers}\n}","author_short":["Paradisol, L.","Boffil, P.","Marazzil, L.","Vecchia, N., D.","Arfiglia, M."],"urls":{"Website":"http://www.scopus.com/inward/record.url?eid=2-s2.0-84899152631&partnerID=tZOtx3y1,http://www.scopus.com/inward/record.url?eid=2-s2.0-30944460383&partnerID=tZOtx3y1,http://www.scopus.com/inward/record.url?eid=2-s2.0-84899117001&partnerID=tZOtx3y1"},"bibbaseid":"paradisol-boffil-marazzil-vecchia-arfiglia-experimentalxpmspmfwmpenaltyevaluationinverydensewdmopticalsystems-2005","role":"author","downloads":0},"search_terms":["experimental","xpm","spm","fwm","penalty","evaluation","very","dense","wdm","optical","systems","paradisol","boffil","marazzil","vecchia","arfiglia"],"keywords":[],"authorIDs":[]}