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 | 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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