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 1A1742-294(GC_BGD_1) 266.5264 -29.516 265.728429 -29.497192 266.950822 -6.111628 359.56008755 -0.392308 264.8664 53637.463287037 2005-09-24 11:07:08 53637.527962963 2005-09-24 12:40:16 100027030 2.0663 5 2.0663 2.0663 2.0663 2.0663 1 1 1 1 1 0 0 1.8877 1.8877 5.584 0 PROCESSED 57527.4000462963 2016-05-19 09:36:04 54247 2007-05-27 00:00:00 54035.4639583333 2006-10-27 11:08:06 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000027 We propose to obtain high quality spectra from 6 positions near the GC. The objective is to resolve 6.4 , 6.7 and 6.9 keV line and determine the high energy tail from each positions and/or from the sub-structures in each position. Combining all the results, we can see which sub-sub-structure is X-ray reflection from Sgr A* ( 6.4 keV line+ 7.1 keV edge + high energy tail), thermal plasma (6.7+6.9 keV lines, with no hard X-ray tail), non thermal emission (e.g. line but hard X-ray tail). Unexpected spectral feature could be also found, depending on the real origin. CALIBRATION 1 A SWG JAP 0 SWG Suzaku Observation of Galactic Center Region N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100027030/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '100027030'

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