total 1

No. target_name center_ra center_dec center_ra_b1950 center_dec_b1950 center_ecliptic_lon center_ecliptic_lat center_galactic_lon center_galactic_lat roll_angle observation_start_time_mjd observation_start_time observation_end_time_mjd observation_end_time observation_id exposure proposal_exposure xis0_exposure xis1_exposure xis2_exposure xis3_exposure xis0_observation_mode xis1_observation_mode xis2_observation_mode xis3_observation_mode hxd_observation_mode hxd_coarse_clock_rate_exposure hxd_first_clock_rate_exposure hxd_normal_clock_rate_exposure hxd_all_clock_rate_exposure hxd_wam_exposure hxd_burst_num processing_status processing_end_time_mjd processing_end_time public_date_mjd public_date distribute_start_date_mjd distribute_start_date processing_version processing_quantity processing_software proposal_id proposal_abstract proposal_category proposal_category_code proposal_priority pi_name co_pi_name proposal_affiliated_country proposal_cycle_count observation_type proposal_title main_detector xis_injection_flag data_access_url ql_access_url ql_image_url
1 BZ UMA 133.4243 57.801 132.45894 57.99062 117.906758 38.491504 159.01672768 38.83001001 307.4767 54549.9926388889 2008-03-24 23:49:24 54550.4446064815 2008-03-25 10:40:14 402046010 29.7466 20 29.7546 29.7546 0 29.7466 2 2 0 2 1 0 0 24.9212 24.9212 39.0459 0 PROCESSED 57541.9622106482 2016-06-02 23:05:35 54933 2009-04-12 00:00:00 54566.2225231482 2008-04-10 05:20:26 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021105 Dwarf Novae, the most numerous subclass of cataclysmic variables, are important contributors to the unresolved X-ray emissions from the Galactic disk and the bulge. However, current estimates of the integrated X-ray luminosity of dwarf novae are highly uncertain and are based on samples that may contain significant biases. We need to obtain an unbiased X-ray luminosity function of dwarf novae to estimate the true contribution of dwarf novae to the unresolved Galactic X-ray emission. Here we propose short Suzaku observations of dwarf novae with secure, parallax-based distance estimates that have not been the subject of pointed, imaging, X-ray observations in the 0.5-10 keV band. This will be an important check of potential biases in earlier studies. GALACTIC POINT SOURCES 4 C KOJI MUKAI USA 2 AO2 BUILDING UP AN UNBIASED X-RAY LUMINOSITY FUNCTION OF DWARF NOVAE: A PARALLAX SELECTED SAMPLE XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/402046010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402046010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏