Some further comments on the paper "biparametric scale adaptive filter design" for the detection of compact sources as proposed by M. Lopez-Caniego et. al 2005, MNRAS 359, 993
| dc.creator | Vio, R. | |
| dc.creator | Andreani, P. | |
| dc.date | 2005-10-17 | |
| dc.date.accessioned | 2026-07-07T06:43:55Z | |
| dc.date.available | 2026-07-07T06:43:55Z | |
| dc.description | In this note we re-propose the arguments presented in Vio (2005) examining the superiority of the 'bi-parametric scale adaptive filter' (BSAF) when dealing with source detection as claimed by (Lopez-Caniego 2005a) and confirmed in Lopez-Caniego (2005b). We suggest here that the dispute can be easily solved if these authors provide the community with a detailed derivation of a basic equation. | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0510477 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0510477 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/102599 | |
| dc.subject | Astrophysics | |
| dc.title | Some further comments on the paper "biparametric scale adaptive filter design" for the detection of compact sources as proposed by M. Lopez-Caniego et. al 2005, MNRAS 359, 993 | |
| dc.type | text |