DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
object_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
awarded_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
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
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://data.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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