DARTS Astro

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 KT PER 24.2933 50.9468 23.514247 50.69234 43.593687 37.546222 130.24865907 -11.27406186 260.9001 54843.8957060185 2009-01-12 21:29:49 54844.5334953704 2009-01-13 12:48:14 403041010 29.1957 20 29.1957 29.1957 0 29.1957 2 2 0 2 1 0 0 28.1658 28.1658 55.0899 0 PROCESSED 57545.1649537037 2016-06-06 03:57:32 55328 2010-05-12 00:00:00 54854.0547916667 2009-01-23 01:18:54 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031144 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 to continue our ongoing program to observe dwarf novae with secure, parallax-based distance estimates. GALACTIC POINT SOURCES 4 C KOJI MUKAI USA 3 AO3 BUILDING UP AND UNBIASED X-RAY LUMINOSITY FUNCTION OF DWARF NOVAE: A CONTINUATION IN SUZAKU CYCLE 3 XIS Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/403041010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403041010'

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