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_G0.9+0.1 266.9332 -28.1474 266.1438 -28.130586 267.277369 -4.735296 0.91503767 0.01290063 105.8953 54536.2637152778 2008-03-11 06:19:45 54540.229375 2008-03-15 05:30:18 502051010 138.7614 133 138.7614 138.7614 0 138.7614 2 2 0 2 1 0 0 122.2214 122.2214 342.5768 1 PROCESSED 57541.9299305556 2016-06-02 22:19:06 54919 2009-03-29 00:00:00 54550.6988078704 2008-03-25 16:46:17 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020071 The Suzaku PV observations found that the diffuse X-rays (6.7 and 6.9 keV-lines) from the GC region can well be explained by a thermal emission from hot plasma (6-7 keV). The most plausible energy injection source is multiple SNe. The huge thermal energy (10^54 ergs) and short timescale (10^5 yr) of the hot plasma suggest that the GC region harbors at least 10 young SNRs. To confirm this scenario, we propose to observe the shell of G0.9+0.1 and the connecting region of Sgr B and D. The first objective is to detect a thermal emission from the shell of G0.9+0.1 and the second is to discover new SNRs. GALACTIC DIFFUSE EMISSION 5 A KATSUJI KOYAMA JAP 2 AO2 SNR G0.9+0.1 AND THE CONNECTING REGION OF SGR B AND D XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502051010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '502051010'

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