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 BLOWOUT SHELL 2 312.2035 28.7297 311.67582 28.543644 325.497444 44.382569 72.14669544 -9.39669734 48.0881 55361.263599537 2010-06-14 06:19:35 55362.5155439815 2010-06-15 12:22:23 505056010 52.0698 50 52.0698 52.0698 0 52.0698 2 2 0 2 1 0 0 46.0827 46.0827 108.1558 1 PROCESSED 57552.3493634259 2016-06-13 08:23:05 55741 2011-06-29 00:00:00 55375.7627893518 2010-06-28 18:18:25 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 050088 The Cygnus Loop is a typical shell-like middle-aged SNR. The origin of this SNR is considered to be a cavity explosion. Many previous studies show the abundance of the Cygnus Loop's shell is wholly low (0.2 solar) while that of the ambient medium is typically 0.5 solar. Based on our previous observations, we found some shell regions show 0.5 solar abundances which are consistent with that of the ISM. To explain this result, we formed a hypothesis that the cavity wall density is low in such region and that the forward shock is now propagating outside the cavity, interacting with the ambient medium. In order to verify this hypothesis, we propose to observe the shell of the blowout region which originates from a large break of the cavity wall. We propose to observe two regions for 100ks. GALACTIC DIFFUSE EMISSION 5 B HIROYUKI UCHIDA JAP 5 AO5 X-RAY OBSERVATION OF THE CYGNUS LOOP BLOWOUT REGION XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505056010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '505056010'

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