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 G298.6-0.0 183.3899 -62.6356 182.720759 -62.35751 219.490154 -53.509251 298.59488766 -0.08324812 319.8129 56150.8519097222 2012-08-11 20:26:45 56152.08625 2012-08-13 02:04:12 507037010 17.2388 50 17.2388 17.2388 0 17.2388 1 1 0 1 1 0 0 19.1746 19.1746 106.616 0 PROCESSED 57606.8422222222 2016-08-06 20:12:48 56721 2014-03-05 00:00:00 56291.7215162037 2012-12-30 17:18:59 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070047 A key element to untangle the Galactic origin of the cosmic-ray is the acceleration of high energy particles that occurs in the shocks of the supernova remnants (SNRs). Recent Fermi surveys revealed that particles are more efficiently escaping from the acceleration system when the SNRs get older. However what is still unknown is the plasma condition environment that makes the mechanism more efficient. X-ray observations are an excellent tool to understand the plasma condition but there has not been a systematic X-ray follow-up observations of these Fermi SNRs. The Suzaku Observatory is ideal for such X-ray systematic study because of his low background. We propose here X-ray observations of 4 SNRs detected by Fermi to solve cosmic-ray escape problem. GALACTIC DIFFUSE EMISSION 5 B AYA BAMBA JAP 7 AO7 SUZAKU SYSTEMATIC STUDY OF FERMI DETECTED SNRS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/507037010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '507037010'

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