The Japanese space gravitational wave antenna; DECIGO

DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. DECIGO is expected to open a new window of observation for gravitational wave astronomy especially between 0.1 Hz and 10 Hz, revealing various mysteries of the universe such as dark energy, formation mechanism of supermassive black holes, and inflation of the universe. The pre-conceptual design of DECIGO consists of three drag-free spacecraft, whose relative displacements are measured by a differential Fabry– Perot Michelson interferometer. We plan to launch two missions, DECIGO pathfinder and pre- DECIGO first and finally DECIGO in 2024

DECIGO pathfinder

DECIGO pathfinder (DPF) is a milestone satellite mission for DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) which is a future space gravitational wave antenna. DECIGO is expected to provide us fruitful insights into the universe, in particular about dark energy, a formation mechanism of supermassive black holes, and the inflation of the universe. Since DECIGO will be an extremely large mission which will formed by three drag-free spacecraft with 1000m separation, it is significant to gain the technical feasibility of DECIGO before its planned launch in 2024. Thus, we are planning to launch two milestone missions: DPF and pre-DECIGO. The conceptual design and current status of the first milestone mission, DPF, are reviewed in this article

The status of DECIGO

DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) is the planned Japanese space gravitational wave antenna, aiming to detect gravitational waves from astrophysically and cosmologically significant sources mainly between 0.1 Hz and 10 Hz and thus to open a new window for gravitational wave astronomy and for the universe. DECIGO will consists of three drag-free spacecraft arranged in an equilateral triangle with 1000 km arm lengths whose relative displacements are measured by a differential Fabry-Perot interferometer, and four units of triangular Fabry-Perot interferometers are arranged on heliocentric orbit around the sun. DECIGO is vary ambitious mission, we plan to launch DECIGO in era of 2030s after precursor satellite mission, B-DECIGO. B-DECIGO is essentially smaller version of DECIGO: B-DECIGO consists of three spacecraft arranged in an triangle with 100 km arm lengths orbiting 2000 km above the surface of the earth. It is hoped that the launch date will be late 2020s for the present

Phase I and II Trials of Vinorelbine With Carboplatin for Patients 75 Years of Age or Older With Previously Untreated Non–Small-Cell Lung Cancer

The safety and efficacy of platinum-based combination chemotherapy for elderly patients with advanced Non-Small-cell lung cancer (NSCLC) remains unclear. We conducted phase I and phase II trials of a combination of vinorelbine and carboplatin for patients <75 years of age and with advanced NSCLC. Previously untreated patients (<75 years of age) with stage IIIB or IV NSCLC were enrolled. Based on a 4-week cycle, vinorelbine was given on days 1 and 8, and carboplatin was given on day 1. Dose-limiting toxicity was defined as grade 4 hematologic toxicity that lasted 4 days or more, febrile neutropenia; grade 3 or worse nonhematologic toxicities; or the omission of vinorelbine administration on day 8 in the first cycle. Thirteen patients were enrolled in phase I. dose-limiting toxicity was grade 4 neutropenia that lasted 4 days or more, observed in 2 of 4 patients at level 4. Phase II study used the dose of level 3 (20 mg/m 2 vinorelbine, area under the curve of 4 mg/mL/min carboplatin). Forty-two patients were enrolled. The response rate was 14.6% of 41 assessable patients (95% CI, 3.8-25.4). The median time to progression was 98 days (95% CI, 61-135 days), and the median survival time was 366 days (95% CI, 321-411 days). All toxicities were mild and manageable. Use of 20 mg/m 2 vinorelbine on days 1 and 8, followed by carboplatin area under the curve of 4 mg/mL/min on day 1 every 4 weeks warrants a phase III study for elderly patients with advanced NSCLC

The Japanese space gravitational wave antenna---DECIGO

International audienceDECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. It aims at detecting various kinds of gravitational waves between 1 mHz and 100 Hz frequently enough to open a new window of observation for gravitational wave astronomy. The pre-conceptual design of DECIGO consists of three drag-free satellites, 1000 km apart from each other, whose relative displacements are measured by a Fabry-Perot Michelson interferometer. We plan to launch DECIGO in 2024 after a long and intense development phase, including two pathfinder missions for verification of required technologies