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Items where Person is "Giodini-S"

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Number of items: 8.

Velander, Malin and van Uitert, Edo and Hoekstra, Henk et al. (2014) CFHTLenS: the relation between galaxy dark matter haloes and baryons from weak gravitational lensing. Monthly Notices of the Royal Astronomical Society, 437 (3). pp. 2111-2136. ISSN 0035-8711.

Giodini, S. and Finoguenov, A. and Pierini, D. et al. (2012) The galaxy stellar mass function of X-ray detected groups. Environmental dependence of galaxy evolution in the COSMOS survey. Astronomy and Astrophysics, 538 . Art. No. A104. ISSN 0004-6361.

Pierini, D. and Giodini, S. and Finoguenov, A. et al. (2011) Two fossil groups of galaxies at z ≈ 0.4 in the Cosmic Evolution Survey: accelerated stellar-mass build-up, different progenitors. Monthly Notices of the Royal Astronomical Society, 417 (4). pp. 2927-2937. ISSN 0035-8711.

Giodini, S. and Smolčić, V. and Finoguenov, A. et al. (2010) Radio Galaxy Feedback in X-ray-selected Groups from COSMOS: The Effect on the Intracluster Medium. Astrophysical Journal, 714 (1). pp. 218-228. ISSN 0004-637X.

Oklopčić, A. and Smolčić, V. and Giodini, S. et al. (2010) Identifying Dynamically Young Galaxy Groups Via Wide-angle Tail Galaxies: A Case Study in the COSMOS Field at z = 0.53. Astrophysical Journal, 713 (1). pp. 484-490. ISSN 0004-637X.

Leauthaud, Alexei and Finoguenov, Alexis and Kneib, Jean-Paul et al. (2010) A Weak Lensing Study of X-ray Groups in the Cosmos Survey: Form and Evolution of the Mass-Luminosity Relation. Astrophysical Journal, 709 (1). pp. 97-114. ISSN 0004-637X.

Giodini, S. and Pierini, D. and Finoguenov, A. et al. (2009) Stellar and Total Baryon Mass Fractions in Groups and Clusters Since Redshift 1. Astrophysical Journal, 703 (1). pp. 982-993. ISSN 0004-637X.

Finoguenov, A. and Guzzo, L. and Hasinger, G. et al. (2007) The XMM-Newton Wide-Field Survey in the COSMOS Field: Statistical Properties of Clusters of Galaxies. Astrophysical Journal Supplement Series, 172 (1). pp. 182-195. ISSN 0067-0049.

This list was generated on Tue Jan 19 05:34:44 2021 PST.