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 SWIFT J2319.4+2619 349.8819 26.2473 349.265885 25.973522 2.029717 27.934963 98.48369948 -32.22425134 253.9963 56633.8796875 2013-12-07 21:06:45 56634.8786111111 2013-12-08 21:05:12 408030010 41.2758 40 41.2758 41.2758 0 41.2758 1 1 0 1 1 0 0 38.149 38.149 86.2879 2 PROCESSED 57613.5369328704 2016-08-13 12:53:11 57039 2015-01-17 00:00:00 56672.6300578704 2014-01-15 15:07:17 3.0.22.44 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 081213 Polars are a subclass of magnetic cataclysmic variables in which a strongly magnetic white dwarf accretes matter from a late-type, Roche-lobe filling mass donor. They are usually soft X-ray bright and hard X-ray dim, due to either buried shocks or strong cyclotron cooling, depending on system parameters. However, a small subset of polars have been detected as bright hard X-ray sources in INTEGRAL and Swift BAT surveys. As a part of an effort to understand the hard-to-soft X-ray luminosity ratios of polars in general, and specifically to understand what combination of parameters make some polars hard X-ray bright, we propose Suzaku observations of two poorly studied BAT polars, Swift J2319.4+2619 and IW Eri, supported by ground-based observations including optical polarimetry. GALACTIC POINT SOURCES 4 C KOJI MUKAI USA 8 AO8 THE HARD X-RAY BRIGHT POLARS SWIFT J2319.4+2619 AND IW ERI XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/408030010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '408030010'

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