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 | AX J1714.1-3912 | 258.5249 | -39.1972 | 257.66219 | -39.139743 | 260.755226 | -16.122974 | 347.85266774 | -0.22742448 | 85.6964 | 55608.0538078704 | 2011-02-16 01:17:29 | 55608.9654050926 | 2011-02-16 23:10:11 | 505076010 | 32.6017 | 30 | 32.6017 | 32.6017 | 0 | 32.6017 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 28.3362 | 28.3362 | 78.7579 | 1 | PROCESSED | 57600.9625115741 | 2016-07-31 23:06:01 | 55988 | 2012-03-02 00:00:00 | 55621.1409027778 | 2011-03-01 03:22:54 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 052012 | Molecular clouds are predicted to emit strong non-thermal X-rays when they are close to particle-accelerating SNRs, but this emission has not been confirmed yet. We propose to observe the non-thermal X-ray source AX J1714.1-3912 to investigate its relationship with the SNR RX J1713.7-3946. ASCA observations have shown that the hard spectrum of the source may be associated with bremsstrahlung emission from particles accelerated in the SNR and diffusing in a nearby molecular cloud. This emission has never been observed in other SNRs. However, the association of the source with the remnant is still controversial and the ASCA data do not allow us to constrain the spectral properties. We aim at verifying the association with the remnant and at investigating the physical origin of the emission. | GALACTIC DIFFUSE EMISSION | 5 | A | MARCO MICELI | EUR | 5 | AO5 | INVESTIGATING THE PHYSICAL ORIGIN OF AX J1714.1-3912 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505076010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '505076010'
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