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 SNR HB3 SE-C 36.0358 62.4578 35.086232 62.23139 58.169094 44.855041 133.42083063 1.4890972 247.4994 56323.7716666667 2013-01-31 18:31:12 56324.1585532407 2013-02-01 03:48:19 507058010 24.142 20 24.1616 24.142 0 24.1696 2 2 0 2 1 0 0 23.4547 23.4547 33.4239 0 PROCESSED 57608.6786342593 2016-08-08 16:17:14 56711 2014-02-23 00:00:00 56345.4779976852 2013-02-22 11:28:19 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 071316 We propose to study the large SNR HB3, which is classified as the mixed-morphology SNRs. The Fermi LAT revealed recently bright gamma-ray emissions adjacent to the southeastern shell of HB3, indicating the gamma rays originate in shocked molecular clouds associated with the nearby HII region W3/W4. However it is difficult to determine the gamma-ray origins since the HII regions are dominant in all energy bands except for X-ray. Our aim is to obtain the spatial structure and the temperature of thermal X-ray emissions at this site. These information will help us to understand whether HB3 interacts with molecular clouds. For this purpose, we require high sensitivities and the wide field of view to cover the southeastern shell. Suzaku is an ideal X-ray observatory to achieve this objective. GALACTIC DIFFUSE EMISSION 5 C JUNICHIRO KATSUTA USA 7 AO7 SUZAKU OBSERVATION OF A GAMMA-RAY EMISSION SNR, HB3 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/507058010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '507058010'

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