Luciola hypertelescope space observatory: versatile, upgradable high-resolution imaging, from stars to deep-field cosmology
نویسندگان
چکیده
منابع مشابه
Observations of the Hubble Deep Field with the Infrared Space Observatory - IV. Association of sources with Hubble Deep Field galaxies
We discuss the identification of sources detected by the Infrared Space Observatory (ISO) at 6.7 and 15 11m in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existing optical and near-infrared HDF catalogues using the likelihood ratio method, confirming these results (and, in one case, clarifying them) with independent visual searches. We find 15 ISO...
متن کاملObservations of the Hubble Deep Field with the Infrared Space Observatory - lYe Association of sources with Hubble Deep Field galaxies
We discuss the identification of sources detected by the Infrared Space Observatory (ISO) at 6.7 and 15 11m in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existing optical and near-infrared HDF catalogues using the likelihood ratio method, confirming these results (and, in one case, clarifying them) with independent visual searches. We find 15 ISO...
متن کاملHigh Resolution Imaging of Molecular Outflows in Massive Young Stars
We present high angular resolution observations toward two massive star forming regions IRAS 18264-1152 and IRAS 23151+5912 with the Plateau de Bure Interferometer (PdBI) in the SiO (J=2-1) and HCO (J=1-0) lines and at 1.3 mm and 3.4 mm continuum, and with the Very Large Array (VLA) in the NH3 (J,K)=(1,1), (2,2) lines. The NH3 (1,1) and (2,2) emission is detected toward IRAS 18264-1152 only. Fo...
متن کاملObservations of the Hubble Deep Field with the Infrared Space Observatory - II. Source detection and photometry
Goldschmidt, P.; Oliver, S. J.; Serjeant, S. B. G.; Baker, A.; Eaton, N.; Efstathiou, A.; Gruppioni, C.; Mann, R. G.; Mobasher, B.; Rowan-Robinson, M.; Sumner, T. J.; Danese, L.; Elbaz, D.; Franceschini, A.; Egami, E.; Kontizas, M.; Lawrence, A.; McMahon, R.; Norgaard-Nielsen, H. U.; Perez-Fournon, I. and Gonzalez-Serrano, J. I. (1997). Observations of the Hubble Deep Field with the Infrared Sp...
متن کامل- Poor Stars . Viii . High - Resolution , High - Signal - to - Noise Analysis
High-resolution, high-signal-to-noise (〈S/N〉 = 85) spectra have been obtained for five stars – CD–2417504, CD–38245, CS 22172–002, CS 22885–096, and CS 22949–037 – having [Fe/H] . –3.5 according to previous lower S/N material. LTE model-atmosphere techniques are used to determine [Fe/H] and relative abundances, or their limits, for some 18 elements, and to constrain more tightly the early enric...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Experimental Astronomy
سال: 2008
ISSN: 0922-6435,1572-9508
DOI: 10.1007/s10686-008-9123-8