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 | VICINITY_4U1957+11 | 300.5977 | 12.1307 | 300.008296 | 11.990222 | 305.849194 | 31.842544 | 52.0534723 | -9.74567764 | 252.1551 | 55499.6275578704 | 2010-10-30 15:03:41 | 55501.8265625 | 2010-11-01 19:50:15 | 505057010 | 80.5839 | 80 | 80.5839 | 80.5839 | 0 | 80.5839 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 59.2042 | 59.2042 | 189.9759 | 2 | PROCESSED | 57553.9949305556 | 2016-06-14 23:52:42 | 55882 | 2011-11-17 00:00:00 | 55515.3752083333 | 2010-11-15 09:00:18 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050090 | We propose for an observation of the vicinity of 4U 1957+11, in order to study the Galactic low-latitude hot gas. Recently, detection of OVII and NeIX aborption lines was reported in the spectrum of 4U 1957+11 (Yao et al. 2008). By combining a Suzaku observation of diffuse hot plasma around the object with the reported absorption line equivalnet widths, we will constrain the temperature, line-of-sight length, density of the hot plasma of the direction. Not only to understand the Galactic gas, but also to understand feedback mechanism from a galaxy to the intergalactic space will our study play an important role. | GALACTIC DIFFUSE EMISSION | 5 | B | YOH TAKEI | JAP | 5 | AO5 | EMISSION/ABSORPTION COMBINATION STUDY OF GALACTIC LOW-LATITUDE HOT GAS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505057010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '505057010'
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