Minor Planet Observations [809 European Southern Observatory, La Silla]
Not Available
Tholen, D. J. et al.
Advertised on:
3
2008
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Minor Planet Observations [304 Las Campanas Observatory]Not AvailableSheppard, S. S. et al.
Advertised on:
32008 -
Massive galaxies in Extended Groth Strip (Trujillo+, 2007)We use the Palomar Observatory Wide-field Infrared (POWIR)/DEEP-2 survey (Davis et al., 2003, SPIE, Vol. 4834, p. 161; Bundy et al., 2006ApJ...651..120B ; Conselice et al., 2007ApJ...660L..55C, 2007MNRAS.381..962C) to define a sample of 831 galaxies with masses larger than 1011h70-2M{sun} located over ~710arcmin2 in the Extended Groth Strip (EGS)Trujillo, I. et al.
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32008 -
Massive galaxies in Extended Groth Strip (Trujillo+, 2007)We use the Palomar Observatory Wide-field Infrared (POWIR)/DEEP-2 survey (Davis et al., 2003, SPIE, Vol. 4834, p. 161; Bundy et al., 2006ApJ...651..120B ; Conselice et al., 2007ApJ...660L..55C, 2007MNRAS.381..962C) to define a sample of 831 galaxies with masses larger than 1011h70-2M{sun} located over ~710arcmin2 in the Extended Groth Strip (EGS)Trujillo, I. et al.
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32008 -
MAGIC Observations of the Unidentified γ-Ray Source TeV J2032+4130We observed the first known very high energy (VHE) γ-ray-emitting unidentified source, TeV J2032+4130, for 94 hr with the MAGIC telescope. The source was detected with a significance of 5.6 σ. The flux, position, and angular extension are compatible with the previous ones measured by the HEGRA telescope system 5 years ago. The integral flux amountsAlbert, J. et al.
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Lupus-TR-3b: A Low-Mass Transiting Hot Jupiter in the Galactic Plane?We present a strong case for a transiting hot Jupiter planet identified during a single-field transit survey toward the Lupus Galactic plane. The object, Lupus-TR-3b, transits a V=17.4 K1 V host star every 3.91405 days. Spectroscopy and stellar colors indicate a host star with effective temperature 5000 +/- 150 K, with a stellar mass and radius ofWeldrake, David T. F. et al.
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32008