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 | 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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