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 BF ERI 69.8754 -4.5962 69.256008 -4.693413 67.473114 -26.478101 201.0367912 -31.29845078 262.0133 56350.9190625 2013-02-27 22:03:27 56351.6253009259 2013-02-28 15:00:26 407045010 32.8177 30 32.8177 32.8177 0 32.8178 3 3 0 3 1 0 0 32.0161 32.0161 61.0099 1 PROCESSED 57610.6930092593 2016-08-10 16:37:56 56738 2014-03-22 00:00:00 56372.5138773148 2013-03-21 12:19:59 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 071212 The mass of an accreting white dwarf is a key parameter governing its X-ray emission. We expect that the higher the mass, the higher the temperature and luminosity. Existing data appear consistent with this expectation, given the considerable uncertainties usually associated with the white dwarf masses of individual systems. Here we propose Suzaku observations of 5 dwarf novae for which very high or very low white dwarf mass estimates have been published. These targets provide the best opportunity of further establishing the mass-temperature correlation. Moreover, if the mass estimates are reliable, these targets are of interest from evolutionary considerations - how did these systems form with such high/low mass white dwarfs, and what are their ultimate fates? GALACTIC POINT SOURCES 4 C KOJI MUKAI USA 7 AO7 DWARF NOVAE WITH EXTREME WHITE DWARF MASSES XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407045010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '407045010'

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