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 GC_SGR_B_EAST 267.0203 -28.3518 266.229607 -28.335406 267.358668 -4.938031 0.77973231 -0.1584432 71.8708 54162.5141203704 2007-03-03 12:20:20 54164.5273726852 2007-03-05 12:39:25 501039010 96.4018 100 96.4018 96.4018 0 96.4018 2 2 0 2 1 0 0 91.0829 91.0829 173.9318 3 PROCESSED 57537.6522800926 2016-05-29 15:39:17 54736 2008-09-27 00:00:00 54171.4429050926 2007-03-12 10:37:47 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010060 We detected discrete structures of 6.4-keV and 6.7-keV line with the deep observation of Sgr B. These structures are candidate of X-ray reflection nebula and supernova remnant, respectively. Both targets imply the past activities in the Galactic center region: AGN, star burst, or something else. To verify these origin, we propose extensional observation around the Sgr B region. We also investigate metal abundances in the Galactic center by using line intensity ratio at the SNR. GALACTIC DIFFUSE EMISSION 5 B KATSUJI KOYAMA JAP 1 AO1 OBSERVATIONS OF SNR/XRN CANDIDATES NEAR THE SGR B REGION XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501039010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501039010'

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