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
|
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1 | G298.6-0.0 | 183.3873 | -62.6234 | 182.718198 | -62.34531 | 219.474963 | -53.500968 | 298.59191859 | -0.0713547 | 133.8706 | 56341.7597222222 | 2013-02-18 18:14:00 | 56342.6981712963 | 2013-02-19 16:45:22 | 507037020 | 39.7247 | 35 | 39.7247 | 39.7247 | 0 | 39.7247 | 3 | 2 | 0 | 2 | 1 | 0 | 0 | 36.2621 | 36.2621 | 81.0699 | 0 | PROCESSED | 57610.644849537 | 2016-08-10 15:28:35 | 56721 | 2014-03-05 00:00:00 | 56362.8029861111 | 2013-03-11 19:16:18 | 3.0.22.44 | 4 | 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/ver3.0/507037020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '507037020'
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