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 GAMMA CASSIOPEIAE 14.1598 60.7356 13.401441 60.465287 43.939726 48.837698 123.56796459 -2.12972511 72.5084 55755.0038888889 2011-07-13 00:05:36 55756.333587963 2011-07-14 08:00:22 406040010 55.394 50 55.394 55.394 0 55.394 2 2 0 2 1 0 0 56.2164 56.2164 114.8778 0 PROCESSED 57602.6019791667 2016-08-02 14:26:51 56183 2012-09-13 00:00:00 55816.6655208333 2011-09-12 15:58:21 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 061207 We propose a 50 ks Suzaku observation to obtain for the first time the hard X-ray spectrum of the classical Be star Gamma Cas. This star is a prototype of the "Gamma Cas stars" class, whose nature is not yet understood. Earlier XMM-Newton and Swift BAT observations gave a hint of the presence of the hard X-ray emission above 10 keV. The broadband Suzaku spectrum will allow to establish its X-ray emission mechanism - non-thermal emission or reflection of thermal emission from a neutral surface. On this basis, we will be able to discriminate the mechanisms between the magnetic disk dynamo and the accretion on a compact star. These new data will be pivotal in solving the enigma of Gamma Cas and revealing the true nature of this astrophysically important object. GALACTIC POINT SOURCES 4 C KENJI HAMAGUCHI USA 6 AO6 SUZAKU'S HARD LOOK AT GAMMA CASSIOPEIAE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406040010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '406040010'

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