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 IW ERIDANI 66.4802 -19.763 65.931423 -19.87535 60.255555 -40.808034 216.43667954 -40.61449502 63.2719 56870.0005092593 2014-08-01 00:00:44 56870.9730902778 2014-08-01 23:21:15 409030010 39.4581 40 39.4581 39.8021 0 39.8341 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57616.4481134259 2016-08-16 10:45:17 57270 2015-09-05 00:00:00 56902.7186574074 2014-09-02 17:14:52 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 091211 Cataclysmic variables (CVs) detected in the INTEGRAL and Swift BAT hard X-ray surveys are predominantly magnetic systems of the intermediate polar subtype. However, as the survey sensitivity improves, an increasing number of polars are also detected as hard X-ray sources, even though the majority of polars are soft X-ray bright and hard X-ray faint. Over the long term, we hope to understand why most polars are soft X-ray dominated, and why a subset is hard X-ray bright. Here we propose Suzaku observations of four poorly studied BAT-detected polars, 1RXS J032540.0-081442, Swift J2319.4+2619, IW Eri, and IGR J14536-5522, supported by ground-based observations including optical polarimetry, to determine their system parameters. GALACTIC POINT SOURCES 4 A KOJI MUKAI USA 9 AO9 HARD X-RAY BRIGHT POLARS: WHY ARE THEY DIFFERENT? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/409030010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '409030010'

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