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 | IRAS 19254-7245 | 292.8508 | -72.6492 | 291.381636 | -72.754038 | 280.373528 | -50.031737 | 322.5078751 | -28.76929596 | 279.8892 | 54041.9830208333 | 2006-11-02 23:35:33 | 54044.5967476852 | 2006-11-05 14:19:19 | 701052010 | 113.5123 | 120 | 113.5203 | 113.5203 | 113.5123 | 113.5203 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 151.9778 | 151.9778 | 225.8099 | 1 | PROCESSED | 57536.068125 | 2016-05-28 01:38:06 | 54455 | 2007-12-21 00:00:00 | 54088.8285185185 | 2006-12-19 19:53:04 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 011342 | We propose a 120 ksec Suzaku exposure of the ULIRG IRAS19254-7245. A previous XMM-Newton observation revealed the presence of a strong iron emission line and a flat continuum, both suggesting that this source hosts a Compton-thick AGN. In this scenario, the 2-10 keV luminosity of IRAS19254-7245 could be greater than 10e44 erg/s. However since no direct continuum is visible in the XMM bandpass, a direct measure of the absorbing column density was not feasible, thus the intrinsic X-ray luminosity of this source was derived only through indirect arguments. The unique bandpass and sensititvity of Suzaku above 10 keV will allow us to confirm the Compton-thick nature of this source and to measure for the first time the intrinsic X-ray luminosity of the AGN hosted in IRAS 19254-7245. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | VALENTINA BRAITO | USA | 1 | AO1 | ASSESSING THE ENERGETIC BUDGET IN THE SUPERANTENNAE | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701052010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '701052010'
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