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 TV COL 82.3326 -32.8641 81.870324 -32.902382 78.445337 -55.999473 236.83580562 -30.63495041 295.9146 54573.7555555556 2008-04-17 18:08:00 54574.6668634259 2008-04-18 16:00:17 403023010 35.8367 40 35.8367 35.8367 0 35.8367 2 2 0 2 1 0 0 30.1023 30.1023 78.7299 0 PROCESSED 57542.3393055556 2016-06-03 08:08:36 54953 2009-05-02 00:00:00 54587.0666550926 2008-05-01 01:35:59 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030107 We propose observations of 5 Intermediate Polars, a subcategory of magnetic CVs, as the first step toward establishment of an averaged hard X-ray spectrum of IPs that exist near the Solar system.The averaged spectrum should be compared with that of the Galactic Diffese X-ray Emssion (GDXE), to investigate the claimed spectral resemblance between them in energies above 10 keV. If the averaged IP spectrum shows any discrepancy with that of the GDXE, the "point-source origin" explanation for the GDXE would face a lack of appropriate hard X-ray source populations. This in turn is expected to strengthen the competing "truly diffuse origin"explanation, which attributes the GDXE hard X-rays to non thermal emission from electrons being accelerated in the interstellar space. GALACTIC POINT SOURCES 4 C TAKAYUKI YUASA JAP 3 AO3 SURVEY OBSERVATION OF INTERMEDIATE POLARS HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403023010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403023010'

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