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 | MKN 335 | 1.5767 | 20.2085 | 0.933785 | 19.930185 | 9.740922 | 17.859652 | 108.75946317 | -41.41793251 | 71.5257 | 56454.1494907407 | 2013-06-11 03:35:16 | 56457.9792824074 | 2013-06-14 23:30:10 | 708016010 | 143.995 | 300 | 144.027 | 143.995 | 0 | 144.027 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 129.5529 | 129.5529 | 330.8674 | 3 | PROCESSED | 57611.6156828704 | 2016-08-11 14:46:35 | 56383 | 2013-04-01 00:00:00 | 56470.7662037037 | 2013-06-27 18:23:20 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 081411 | The idea of this proposal is trigger a 300ks observation with Suzaku of the Narrow Line Seyfert 1 Galaxy Mkn 335 during one of its low X-ray flux states. The goal here is to measure its underlying broad-band continuum with Suzaku during a low state and compare it with the 2006 high-state observations. Mkn 335 is one of the best examples of an AGN that went into a deep minimum X-ray flux state. Two competing models can explain these extreme low states: reflection models and partial covering absorber models. Both models still require a variable underlying intrinsic continuum. The science driver is to find out what is causing these low X-ray flux states that have been observed in several NLS1s. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | DIRK GRUPE | USA | 8 | AO8-TOO | INTRINSIC LOW-STATE X-RAY LUMINOSITY OF THE NLS1 MKN 335 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/708016010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '708016010'
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