Esta web estará fuera de servicio por mantenimiento el lunes 6 de mayo de 7:30 a 8:00.

VRIJHK photometry of SN 2002cv (Elias-Rosa+, 2008)

Bibcode
2008yCat..73840107E
Elias-Rosa, N.; Benetti, S.; Turatto, M.; Cappellaro, E.; Valenti, S.; Arkharov, A. A.; Beckman, J. E.; Paola, A. D.; Dolci, M.; Filippenko, A. V.; Foley, R. J.; Krisciunas, K.; Larionov, V. M.; Li, W.; Meikle, W. P. S.; Pastorello, A.; Valentini, G.; Hillebrandt, W.
Referencia bibliográfica

VizieR On-line Data Catalog: J/MNRAS/384/107. Originally published in: 2008MNRAS.384..107E

Fecha de publicación:
5
2008
Número de autores
18
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
The fact that another SN Ia, SN 2002bo, exploded in the same galaxy a few months before SN 2002cv, makes available pre-discovery optical and near-IR (NIR) data and hence templates for photometric measurements via image subtraction. SN 2002cv was observed for seven months, from day 10.7 to +205.9 relative to I-band maximum light. Here, we present the data collected by four different teams: University of California, Berkeley (USA), Imperial College (UK), Padova Observatory (INAF, Italy) and Teramo Observatory (INAF, Italy). (4 data files).
Tipo
Sin árbitro
Supernovas
Fotometría

Te puede interesar

  • Sin árbitro
    A machine learning method to infer clusters of galaxies mass radial profiles from mock Sunyaev-Zel'dovich maps with The Three Hundred clusters
    Our study introduces a new machine learning algorithm for estimating 3D cumulative radial profiles of total and gas mass in galaxy clusters from thermal Sunyaev-Zel'dovich (SZ) effect maps. We generate mock images from 2522 simulated clusters, employing an autoencoder and random forest in our approach. Notably, our model makes no prior assumptions
    Ferragamo, A. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300019F
    Número de citas
    0
  • Sin árbitro
    The European Low Frequency Survey. Observing the radio sky to understand the beginning of the Universe
    In this paper we present the European Low Frequency Survey (ELFS), a project that will enable the detection of primordial B-mode polarization by measuring the Galactic and extra-Galactic foregrounds in the 5- 120 GHz frequency window. Indeed, the main difficulty in measuring the Bmode polarization comes not just from its sheer faintness, but from
    Mennella, A. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300031M
    Número de citas
    0
  • Sin árbitro
    Estimation of the hydrostatic-to-lensing mass bias from resolved cluster masses
    We present a study on the bias of hydrostatic masses with respect to lensing mass estimates for a sample of 53 clusters in a redshift range between z = 0.05 and 1.07. The M 500 mass for each cluster was inferred from X-ray and lensing data, without using a priori observable-mass scaling relations. Cluster masses of our reference analysis were
    Muñoz-Echeverría, M. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300033M
    Número de citas
    0