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119
for query "
P. Andreani
". (0.00 sec.)
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1.
Digital Deblurring of CMB Maps II: Asymmetric Point Spread Function
R. Vio
;
J.G. Nagy
;
L. Tenorio
;
P. Andreani
;
C. Baccigalupi W. Wamsteker
;
4 Sep 2003
/ Astron.Astrophys. 408 (2003) 835-844
2.
Millimetric Properties of IRAS Galaxies (III): Luminosity Functions and Contributions to the Sub-Mm Sky Background
A. Franceschini
;
P. Andreani
;
L. Danese
;
3 Jun 1997
3.
Search for sub-mm, mm and radio continuum emission from Extremely Red Objects
Niruj R. Mohan
;
A. Cimatti
;
H.J.A. Roettgering
;
P. Andreani
;
P. Severgnini
;
R.P.J. Tilanus
;
C.L. Carilli
;
S.A. Stanford ( RRI
;
India
;
IISc
;
India
;
OA Arcetri
;
Sterrewacht
;
Leiden
;
MPIfEP Garching
;
OA Padova
;
Univ. Firenze
;
JACH
;
Hawaii
;
NRAO
;
14 Dec 2001
4.
The enhancement and decrement of the Sunyaev-Zeldovich effect towards the ROSAT Cluster RXJ0658-5557
P. Andreani
;
H. Boehringer G. Dall'Oglio
;
L. Martinis
;
P. Shaver R. Lemke
;
L.-AA. Nyman
;
R. Booth
;
L. Pizzo
;
N. Whyborn
;
Y. Tanaka
;
H. Liang
;
5 Nov 1998
5.
The Sunyaev-Zeldovich Effect at 1 and 2 mm towards ROSAT Clusters
P.Andreani
;
G.Dall'Oglio
;
L.Pizzo
;
L.Martinis
;
P.Shaver
;
H.Boehringer
;
R. Lemke
;
L.-A.Nyman
;
R.Booth
;
N.Whyborn
;
28 Aug 1996
6.
Looking for the S-Z Effect towards Distant ROSAT Clusters of Galaxies
P.Andreani
;
L.Pizzo
;
G.Dall'Oglio
;
N.Whyborn
;
H.Boehringer
;
P.Shaver
;
R. Lemke
;
A.Otarola
;
L.-A.Nyman
;
R.Booth
;
2 Feb 1996
7.
Digital Deblurring of CMB Maps: Performance and Efficient Implementation
R. Vio
;
J.G. Nagy
;
L. Tenorio
;
P. Andreani
;
C. Baccigalupi
;
W. Wamsteker
;
24 Dec 2002
/ Astron.Astrophys. 401 (2003) 389
8.
New Clues on the Nature of Extremely Red Galaxies
A. Cimatti
;
E. Daddi
;
S. di Serego Alighieri
;
L. Pozzetti
;
F. Mannucci
;
A. Renzini
;
E. Oliva
;
G. Zamorani
;
P. Andreani
;
H.J.A. Röttgering
;
8 Oct 1999
9.
The evolution of the clustering of QSOs
F. La Franca
;
P. Andreani
;
S. Cristiani
;
22 Feb 1998
10.
Numerical Simulation of Non-Gaussian Random Fields with Prescribed Correlation Structure
Roberto Vio
;
Paola Andreani
;
Willem Wamsteker
;
7 May 2001
11.
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
R. Vio & P. Andreani
;
17 Oct 2005
12.
Some comments on the note "Some comments on the paper 'Filter design for the detection of compact sources based on the Neyman-Pearson detector' by M. Lopez-Caniego et. al (2005, MNRAS 359, 993)" by R. Vio and P. Andreani (astroph/0509394)
M. Lopez-Caniego
;
D. Herranz
;
R.B. Barreiro
;
J.L. Sanz
;
23 Sep 2005
13.
Some comments on the paper "Filter design for the detection of compact sources based on the Neyman-Pearson detector" by M. Lopez-Caniego et. al (2005, MNRAS 359, 993)
R. Vio
;
P. Andreani
;
14 Sep 2005
14.
Far-IR and MM Properties of Quasars
P. Andreani A. Franceschini G.L. Granato
;
26 May 1997
15.
1.25 mm Observations of a Complete Sample of IRAS Galaxies: (II) Dust Properties
P.Andreani
;
A.Franceschini
;
4 Jun 1996
16.
MM Observations of IRAS Galaxies: Dust Properties, Luminosity Functions and Contributions to the Sub-MM Background
P. Andreani
;
A. Franceschini
;
3 Jun 1996
17.
THE CLUSTERING OF QUASARS
P. Andreani
;
S. Cristiani
;
F. La Franca
;
29 May 1995
18.
CO, HI and cold dust in a sample of IRAS galaxies
Paola Andreani
;
Fabienne Casoli
;
Maryvonne Gerin
;
5 Dec 1994
19.
Building the cosmic infrared background brick by brick with Herschel/PEP
S. Berta
;
B. Magnelli
;
R. Nordon
;
D. Lutz
;
S. Wuyts
;
B. Altieri
;
P. Andreani
;
H. Aussel
;
H. Castaneda
;
J. Cepa
;
A. Cimatti
;
E. Daddi
;
D. Elbaz
;
N.M. Foerster Schreiber
;
R. Genzel
;
E. Le Floc'h
;
R. Maiolino
;
I. Perez-Fournon
;
A. Poglitsch
;
P. Popesso
;
F. Pozzi
;
L. Riguccini
;
G. Rodighiero
;
M. Sanchez-Portal
;
E. Sturm
;
L.J. Tacconi
;
I. Valtchanov
;
15 Jun 2011
20.
Global Convergence of Algorithms Under Constant Rank Conditions for Nonlinear Second-Order Cone Programming
Roberto Andreani
;
Gabriel Haeser
;
Héctor Ramírez C.
;
Leonardo M. Mito
;
Thiago P. Silveira
;
22 Oct 2021
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