Can we use GRB to probe high redshift star formation?

F. Fiore; D. Guetta; S. Piranomonte; V. D'Elia; L. A. Antonelli

doi:10.1393/ncb/i2007-10267-0

Can we use GRB to probe high redshift star formation?

F. Fiore
, D. Guetta
, S. Piranomonte
, V. D'Elia
, L. A. Antonelli

نتاج البحث: نشر في مجلة › مقالة › مراجعة النظراء

ملخص

We present a detailed analysis of the selection effects that plague GRB observations. We find that these effects may partially explain the different redshift distributions between BeppoSax/HETE2 and Swift bursts. It is mandatory to consider these effects to determine the redshift evolution of GRBs.

اللغة الأصلية	الإنجليزيّة
الصفحات (من إلى)	1395-1402
عدد الصفحات	8
دورية	NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS
مستوى الصوت	121
رقم الإصدار	10-11
المعرِّفات الرقمية للأشياء	https://doi.org/10.1393/ncb/i2007-10267-0
حالة النشر	نُشِر - 2006
منشور خارجيًا	نعم

الوصول إلى المستند

10.1393/ncb/i2007-10267-0

الملفات والروابط الأخرى

Link to publication in Scopus

قم بذكر هذا

@article{cabaa8b8526d4f0fae9d69b8e695c220,

title = "Can we use GRB to probe high redshift star formation?",

abstract = "We present a detailed analysis of the selection effects that plague GRB observations. We find that these effects may partially explain the different redshift distributions between BeppoSax/HETE2 and Swift bursts. It is mandatory to consider these effects to determine the redshift evolution of GRBs.",

author = "F. Fiore and D. Guetta and S. Piranomonte and V. D'Elia and Antonelli, \{L. A.\}",

year = "2006",

doi = "10.1393/ncb/i2007-10267-0",

language = "אנגלית",

volume = "121",

pages = "1395--1402",

journal = "NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS",

issn = "1594-9982",

publisher = "Editrice Compositori s.r.l.",

number = "10-11",

}

Can we use GRB to probe high redshift star formation? / Fiore, F.; Guetta, D.; Piranomonte, S. وآخرون.
في: NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS, المجلد 121, رقم 10-11, 2006, صفحة 1395-1402.