Publications (48)
Synthesis models in the VO framework
M. Cervino, E. Terlevich, R. Terlevich +4
Using population synthesis of massive stars to study the interstellar medium near OB associations
R. Voss, R. Diehl, D. H. Hartmann +5
Evolutionary synthesis models of starbursts IV. Soft X-ray emission
M. Cervino, J. M. Mas-Hesse, D. Kunth
On emission-line spectra obtained from evolutionary synthesis models I. Dispersion in the ionising flux and Lowest Luminosity Limits
M. Cervino, V. Luridiana, E. Perez +2
A multiwavelength vision of star forming regions: What does lambda_1 know about lambda_2?
M. Cervino
New estimates of the contribution of Wolf--Rayet stellar winds to the Galactic 26Al
A. Palacios, G. Meynet, C. Vuissoz +4
Gamma-ray line emission from OB associations and young open clusters. II. The Cygnus region
J. Knodlseder, M. Cervino, J. -M. Le Duigou +3
Stellar Population Challenge: analysis of M67 with the VO
M. Cervino, R. Gutierrez, E. Solano
Physical conditions in NGC 6543 from ISO and HST data and the pitfalls of temperature maps
V. Luridiana, E. Perez, M. Cervino
Statistics and multiwavelength synthesis models: towards a new generation of synthesis models
M. Cervino
On the effect of discrete numbers of stars in chemical evolution models
M. Cervino, M. Molla
Results of an analysis of SDSS galaxies in the VO
W. Schoenell, M. Cervino, R. Cid Fernandes +6
Revisiting and assessing uncertainties in stellar populations synthesis models
M. Cervino, V. Luridiana
Progress report: probabilistic and statistical bases of surface brightness fluctuations
M. Cervino, V. Luridiana, L. Jamet
Statistical Synthesis Models
M. Cervino, V. Luridiana
Sampling effects in the emission line spectra of HII regions
M. Villaverde, V. Luridiana, M. Cervino
Physical limits to the validity of synthesis models: The Lowest Luminosity Limit
M. Cervino, V. Luridiana
The Cygnus X region: a nucleosynthesis laboratory for INTEGRAL
J. Knodlseder, M. Cervino, D. Schaerer +2
Confidence levels of evolutionary synthesis models III: On sampling and Poissonian fluctuations
M. Cervino, D. Valls-Gabaud, V. Luridiana +1
On surface brightness fluctuations: probabilistic and statistical bases I: Stellar population and theoretical SBF
M. Cervino, V. Luridiana, L. Jamet
Resolved and unresolved populations: statistics and synthesis models
M. Cervino
Near-IR Galaxy Counts and Evolution from the Wide-Field ALHAMBRA survey
D. Cristobal-Hornillos, J. A. L. Aguerri, M. Moles +19
On the self-consistency of evolutionary synthesis models
M. Cervino
The ALHAMBRA photometric system
T. Aparicio Villegas, E. J. Alfaro, J. Cabrera-Cano +20
From deterministic to probabilistic population synthesis (why synthesis models are not what we thought they were, and how they can be much more than that)
V. Luridiana, M. Cervino
Optimal filter systems for photometric redshift estimation
N. Benitez, M. Moles, J. A. L. Aguerri +18
Confidence limits of SN, Kinetic Energy and chemical yields in evolutionary synthesis models
M. Cervino, V. Luridiana
On biases in the predictions of stellar population synthesis models
M. Cervino, D. Valls--Gabaud
Local anti-correlation between star-formation rate and gas-phase metallicity in disk galaxies
J. Sanchez Almeida, N. Caon, C. Munoz-Tunon +2
Confidence limits of evolutionary synthesis models. IV Moving forward to a probabilistic formulation
M. Cervino, V. Luridiana, N. Cervino-Luridiana
Confidence Limits of Evolutionary Synthesis Models
M. Cervino, V. Luridiana
On some Uncertainties in Evolutionary Synthesis Models
M. Cervino, D. Valls--Gabaud
On the distribution of initial masses of stellar clusters inferred from synthesis models
M. Cervino, D. Valls-Gabaud
Hard X-ray-to-radio energy distributions in starburst galaxies
M. Cervino, J. M. Mas-Hesse
Herschel FIR counterparts of selected Ly-alpha emitters at z~2.2. Fast evolution since z~3 or missed obscured AGNs?
A. Bongiovanni, I. Oteo, J. Cepa +58
Physical conditions in the O++ zone from ISO and HST data. NGC 6543 revisited
V. Luridiana, E. Perez, M. Cervino
Can stellar winds account for temperature fluctuations in H II regions? The case of NGC 2363
V. Luridiana, M. Cervino, L. Binette
Confidence levels of evolutionary synthesis models
M. Cervino, V. Luridiana, F. J. Castander
How to use the SEDs produced by synthesis models (inside and outside the VO)?
M. Cervino, V. luridiana
A probabilistic formulation of evolutionary synthesis models: implications for SED fittings
M. Cervino, V. Luridiana
The effect of collisional enhancement of Balmer lines on the determination of the primordial helium abundance
V. Luridiana, A. Peimbert, M. Peimbert +1
Star cluster versus field star formation in the nucleus of the prototype starburst galaxy M82
S. Barker, R. de Grijs, M. Cervino
Confidence limits of evolutionary synthesis models III. On time-integrated quantities
M. Cervino, M. A. Gomez-Flechoso, F. J. Castander +4
Gamma-ray line emission from OB associations and young open clusters: I. Evolutionary synthesis models
M. Cervino, J. Knodlseder, D. Schaerer +2
Evolutionary population synthesis: the effect of binary systems
J. M. Mas-Hesse, M. Cervino
Fluorescent excitation of Balmer lines in gaseous nebulae: case D
V. Luridiana, S. Simon-Diaz, M. Cervino +3
26Al yields from rotating Wolf--Rayet star models
C. Vuissoz, G. Meynet, J. Knoedlseder +4
Diffuse gamma-ray line emission from multiple OB Associations in Cygnus
S. Plueschke, M. Cervino, R. Diehl +3