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 | MONOGEM RING W1 | 100.4191 | 15.2834 | 99.703498 | 15.332031 | 100.143287 | -7.791413 | 198.20484712 | 4.79777248 | 269.9998 | 55998.5603356482 | 2012-03-12 13:26:53 | 56000.0002314815 | 2012-03-14 00:00:20 | 506053010 | 61.1266 | 60 | 61.1267 | 61.1266 | 0 | 61.1266 | 3 | 2 | 0 | 2 | 1 | 0 | 0 | 59.074 | 59.074 | 124.3739 | 1 | PROCESSED | 57604.899849537 | 2016-08-04 21:35:47 | 56382 | 2013-03-31 00:00:00 | 56016.6737152778 | 2012-03-30 16:10:09 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 061316 | We propose to observe the oldest, nearby SNR, the Monogem Ring, with the Suzaku XIS to study the plasma conditions in two locations which are near the Galactic plane and where there is evidence of a significant interaction with cooler (10^4 - 10^5 K), denser material. We chose one pointing where the turbulent mixing of hot and cooler gas should be large, and an adjacent pointing where the mixing should be small. From our previous Suzaku observation at a region far from the plane, we derived an ionization timescale for the non-equilibrium plasma which is apparently inconsistent with the age of the SNR. Our proposed observations will allow a detailed comparison of the plasma conditions in these regions with very different histories, and initial and current conditions. | GALACTIC DIFFUSE EMISSION | 5 | C | PAUL PLUCINSKY | USA | 6 | AO6 | STUDYING THE PLASMA EVOLUTION IN THE MONOGEM RING | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506053010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '506053010'
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