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(0,-1.6) 268.0544 -29.7594 267.254612 -29.748002 268.29113 -6.329868 0.03481768 -1.65633011 65.7488 54899.6540509259 2009-03-09 15:41:50 54900.8168865741 2009-03-10 19:36:19 503081010 59.2233 50 59.2233 59.2233 0 59.2233 2 2 0 2 1 0 0 57.6018 57.6018 100.4538 1 PROCESSED 57545.7843402778 2016-06-06 18:49:27 55330 2010-05-14 00:00:00 54916.3813194444 2009-03-26 09:09:06 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 030131 We propose a 50 ksec observation of very enigmatic diffuse structure at 1.6 degree south from the Galactic center. We first discovered this structure with ROSAT. Then with ASCA, we found that the spectrum exhibits thin thermal emission accompanied with a hard tail which may be nonthermal radiation from high energy electrons. These results imply presence of a strong shock in this region, possibly due to a jet from Sgr A*. The diffuse emission may be a fossil of the past activities. With the observation of Suzaku, we obtain the richest statistics ever achieved. Then we will reveal the shock front from the image, and verify the past activities of the massive blackhole. GALACTIC DIFFUSE EMISSION 5 B HIROSHI MURAKAMI JAP 3 AO3 NEW EVIDENCE OF THE PAST ACTIVITY IN THE GALACTIC CENTER REGION XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503081010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '503081010'

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