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 | 4 DRA | 187.5655 | 69.216 | 187.018636 | 69.492063 | 136.915856 | 61.202296 | 125.72551845 | 47.79722512 | 145.5318 | 55874.1707291667 | 2011-11-09 04:05:51 | 55875.0619328704 | 2011-11-10 01:29:11 | 406041010 | 42.258 | 40 | 42.258 | 42.258 | 0 | 42.258 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 39.7925 | 39.7925 | 76.998 | 2 | PROCESSED | 57603.7210532407 | 2016-08-03 17:18:19 | 56260 | 2012-11-29 00:00:00 | 55890.6961458333 | 2011-11-25 16:42:27 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 061212 | 4 Dra is a weakly symbiotic star that exhibited strong variability in ROSAT observations. Our Suzaku Cycle 5 observation confirms it to be an absorbed hard X-ray source, powered by accretion. It is thus a nearby, lower accretion rate analogue of the hard X-ray bright symbiotic stars such as T CrB and CH Cyg. During Suzaku Cycle 6, 4 Dra is near apastron and near the inferior conjunction of the accreting white dwarf: both these should reduce the absorption due to the M giant, while absorption by the accretion flow near the white dwarf should remain roughly comparable. We therefore propose a second Suzaku observation of 4 Dra to constrain the relative contributions of these two X-ray absorbers, and to obtain a high signal-to-noise spectrum of a symbiotic star boundary layer near 1 keV. | GALACTIC POINT SOURCES | 4 | C | KOJI MUKAI | USA | 6 | AO6 | A SUZAKU OBSERVATION OF 4 DRA NEAR INFERIOR CONJUNCTION | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406041010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '406041010'
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