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 | CYGNUS LOOP BLOWOUT1 | 312.1499 | 29.2487 | 311.624762 | 29.062833 | 325.710057 | 44.881262 | 72.53069275 | -9.03908096 | 78.1532 | 55686.7775578704 | 2011-05-05 18:39:41 | 55687.8494907407 | 2011-05-06 20:23:16 | 506011010 | 48.5641 | 50 | 48.5641 | 48.5641 | 0 | 48.5641 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 42.0429 | 42.0429 | 92.5799 | 1 | PROCESSED | 57601.954224537 | 2016-08-01 22:54:05 | 56066 | 2012-05-19 00:00:00 | 55698.3278472222 | 2011-05-17 07:52:06 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060053 | The Cygnus Loop is a prototypical middle-aged SNR. Based on the previous observation, the shell region shows relatively low temperature with low metal abundance while the interior shows high temperature with high metal abundance. The plasma in the interior is the fossil of the progenitor star. Recently, we found a strong Si-K line emission from the southernmost blowout region where the shell is very thin. The complete observation of this region will reveal a pure ejecta of this remnant. We may also be able to reveal a whole picture of an asymmetric ejecta distribution of the Cygnus Loop. We propose 6-pointing observation of the Cygnus Loop's blowout region for 240ks. | GALACTIC DIFFUSE EMISSION | 5 | A | HIROYUKI UCHIDA | JAP | 6 | AO6 | MEASUREMENT OF ABUNDANCES INSIDE THE SOUTHERNMOST PART OF THE CYGNUS LOOP, BLOWOUT REGION | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506011010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '506011010'
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