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
|
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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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