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 | 187.4841 | 69.1938 | 186.936079 | 69.469913 | 136.91907 | 61.165888 | 125.77229084 | 47.81569563 | 339.9969 | 55304.8913773148 | 2010-04-18 21:23:35 | 55305.8557291667 | 2010-04-19 20:32:15 | 405035010 | 42.2602 | 40 | 42.2682 | 42.2682 | 0 | 42.2602 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 43.792 | 43.792 | 83.2778 | 1 | PROCESSED | 57551.2555439815 | 2016-06-12 06:07:59 | 55693 | 2011-05-12 00:00:00 | 55327.2173958333 | 2010-05-11 05:13:03 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 051212 | The symbiotic star, 4 Dra, has been poorly studied in X-rays. Based on the ROSAT data, we argue that it is a nearby, lower accretion rate analogue of the hard X-ray bright symibiotic stars that have been detected above 10 keV. We propose the first pointed observation of 4 Dra that covers the entire 0.4-10 keV band to test our interpretation: we expect it to be bright above 2 keV, with an optically thin thermal spectrum, likely with a strong and complex intrinsic absorber. If confirmed, 4 Dra may turn out to be a key object in the study of hard X-ray emitting symbiotic stars. | GALACTIC POINT SOURCES | 4 | B | KOJI MUKAI | USA | 5 | AO5 | THE FIRST LOOK AT THE SYMBIOTIC STAR 4 DRA ABOVE 2 KEV | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/405035010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '405035010'
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