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 N11 SB 74.1823 -66.412 74.156384 -66.487992 354.048784 -83.709745 277.1886014 -36.07081942 146.432 54046.4407291667 2006-11-07 10:34:39 54047.232037037 2006-11-08 05:34:08 501091010 30.452 30 30.452 30.452 30.452 30.452 2 2 2 2 1 0 0 26.405 26.405 68.3659 0 PROCESSED 57536.0384953704 2016-05-28 00:55:26 54455 2007-12-21 00:00:00 54088.5643287037 2006-12-19 13:32:38 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011251 Clusters of massive stars, through their stellar winds and supernovae, form large diffuse structures known as superbubbles (SBs), which play an essential role in shaping the local interstellar medium. Most SB models indicate that these objects should be dominated by thermal plasma processes. However, observations of 2 SBs have detected significant nonthermal contributions to their X-ray emission, which raises many questions. Is it generated by synchrotron, inverse-Compton, or nonthermal Bremsstrahlung processes? Are colliding stellar winds or internal supernova remnants responsible? We therefore propose to examine the X-ray emission from 4 X-ray bright SBs, to search for nonthermal X-ray emission, and if possible place strong constraints on the source of this emission. GALACTIC DIFFUSE EMISSION 5 C ROSA WILLIAMS USA 1 AO1 A SEARCH FOR NONTHERMAL X-RAY EMISSION FROM SUPERBUBBLES XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501091010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501091010'

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